Math Formulas: Complete List by Topic, With Examples

#Formula
TL;DR
A math formula is a rule written in symbols that connects quantities, so you can calculate an unknown. This page lists 1,400+ math formulas by topic, each with its meaning and a worked example.
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Bhanzu TeamLast updated on September 30, 2026284 min read

What Is A Math Formula?

A math formula is a rule, written with symbols, that shows exactly how one quantity depends on others. The area of a circle, $A = \pi r^{2}$, is a formula: give it the radius and it returns the area, every time.

A formula is not quite the same as an equation or an identity, and the difference matters when you use one.

  • Formula: a rule for calculating one quantity from others, such as $A = \pi r^{2}$ or simple interest $I = \frac{PRT}{100}$.

  • Equation: a statement that two expressions are equal, often true only for certain values, such as $2x + 3 = 11$, which holds only when $x = 4$.

  • Identity: an equation that is true for every value of its variables, such as $(a + b)^{2} = a^{2} + 2ab + b^{2}$.

94% of 15,687 consultation responses on the maths question backed formulae sheets for GCSE maths, and England's exam regulator, Ofqual, made the sheets compulsory for the 2025, 2026 and 2027 exams. Ofqual decision, updated 13 November 2024

How Do You Use This Math Formula List?

Jump to a branch: Basic math · Commercial math · Algebra · Advanced algebra · Geometry · Coordinate geometry and vectors · Trigonometry · Calculus · Statistics and probability

  • Each table has three columns. The name of the formula, the formula itself, and what every letter means, including any condition such as $a \neq 0$.

  • Each subtopic ends with a worked example. Real numbers go through the formula, so you can check that you are reading it the right way.

  • Linked names open a full lesson. A linked formula leads to a page with the derivation, more examples and common mistakes.

Which Math Formulas Should You Learn First?

Learn the formulas for the chapter you are studying now, in the order your course uses them. The table shows where the most-used formulas usually appear.

School stage

Formulas to know well

Why they come first

Grades 6 to 8

area and perimeter of rectangles, triangles and circles, simple interest, percent change, laws of exponents, $(a + b)^{2}$ and $(a - b)^{2}$

every later chapter reuses them

Grades 9 to 10

Pythagorean theorem, quadratic formula, distance and midpoint formulas, surface area and volume, AP $n$th term and sum, basic trig ratios, mean of grouped data

board exams test them directly

Grades 11 to 12

trig identities, binomial theorem, $^{n}C_{r}$, limits and derivatives, standard integrals, conic sections, probability rules

entrance exams such as JEE and the SAT build on them

Which Math Formulas Are Most Often Written Wrong?

A formula copied with one symbol out of place gives a confident wrong answer. These are the slips that show up again and again in homework and in quick-reference lists.

  • Slope without brackets. Writing $m = y_{2} - y_{1} / x_{2} - x_{1}$ divides only $y_{1}$ by $x_{2}$. The slope is $m = \frac{y_{2} - y_{1}}{x_{2} - x_{1}}$.

  • The quadratic formula's $2a$. The $2a$ divides the whole top, $x = \frac{-b \pm \sqrt{b^{2} - 4ac}}{2a}$, not just the square root.

  • Squaring a sum. $(a + b)^{2}$ is $a^{2} + 2ab + b^{2}$. Leaving out $2ab$ is the most common algebra error of all.

  • Logs of a sum. $\log(a + b)$ does not split. Only products do: $\log(ab) = \log a + \log b$.

  • The $-1$ in trigonometry. $\sin^{-1} x$ means the inverse sine, the angle whose sine is $x$. It is not $\frac{1}{\sin x}$, which is $\csc x$.

  • The integral of $\frac{1}{x}$. It is $\ln\lvert x \rvert + C$. The absolute value keeps it valid for negative $x$, and the $+ C$ is part of every indefinite integral.

  • Sample standard deviation. A sample divides by $n - 1$, a whole population by $n$. Calculators show both, so pick the one your question asks for.

  • Compound interest per period. With interest compounded quarterly, the rate per period is $\frac{r}{4}$ and the number of periods is $4t$. Using the yearly rate with quarterly periods inflates the answer.

  • BODMAS taken letter by letter. BODMAS lists D before M, but division and multiplication have equal rank and go left to right. So $12 \div 3 \times 2 = 8$, not 2.

Which Exams Give You A Formula Sheet?

It depends on the exam, and it changes, so check the official rules for yours.

  • SAT: yes. College Board says a reference sheet of commonly used formulas appears on every test with math questions in its Bluebook testing app.

  • GCSE maths (England): yes for the 2025, 2026 and 2027 exams, including the November sittings, under the Ofqual decision above.

  • Most school board and entrance exams: usually no. Plan to know the formulas for your syllabus by heart.

A reference sheet does not remove the need to understand a formula. You still have to recognise which formula fits the question, and that comes from practice.

How Do You Remember Math Formulas?

Understand where a formula comes from, then use it until you no longer need to look it up.

  • Derive it once. The area of a triangle is half a rectangle. The sum of an AP pairs the first and last terms. A formula you can rebuild is a formula you cannot forget for long.

  • Learn formulas in families. Keep area, perimeter and volume of the same shape together, and the six trig ratios together, so each one reminds you of the next.

  • Say the letters in words. "Area equals pi times radius squared" sticks better than a string of symbols.

  • Write your own sheet. Rewriting the formulas for a chapter from memory, then checking them, shows you exactly which ones have not stuck yet.

  • Use it on a real problem. Students who memorise the formula for the sum of an AP often mix up $n$ and $a_{n}$ until they have worked five problems with it. After that, the letters mean something.

Basic Math Formulas: Arithmetic And Numbers

These are the number rules that every later topic depends on: order of operations, fractions, decimals, percentages, ratios, averages, factors, divisibility and sums of number patterns. Students from Grade 6 onward use them daily, and aptitude sections of competitive exams test them for speed.

Order Of Operations (BODMAS And PEMDAS)

BODMAS (used in India and the UK) and PEMDAS (used in the US) describe the same order, only the letters differ.

Formula

Expression

What it means

Brackets or parentheses first

$2 \times (3 + 4) = 2 \times 7 = 14$

Simplify whatever is inside brackets before anything else, starting with the innermost pair and working outward.

Nested brackets

$\lbrace 2 + [3 \times (5 - 1)]\rbrace = \lbrace 2 + 12\rbrace = 14$

Clear round brackets ( ) first, then square brackets [ ], then curly braces { }, from the inside out.

Orders or exponents

$3 + 2^{3} = 3 + 8 = 11$

Powers and roots come next. BODMAS calls them Orders and PEMDAS calls them Exponents.

"Of" means multiply

$\frac{1}{2} \text{ of } 10 = \frac{1}{2} \times 10 = 5$

The word "of" between a fraction or percent and a number means multiplication, as in half of 10.

Division and multiplication, left to right

$12 \div 3 \times 2 = 4 \times 2 = 8$

These two share the same rank, so work them in the order they appear from left to right, not division first.

Addition and subtraction, left to right

$10 - 4 + 3 = 6 + 3 = 9$

These also share one rank and are done last, again strictly from left to right.

Fraction bar as a bracket

$\frac{6 + 4}{7 - 2} = \frac{10}{5} = 2$

A fraction bar groups its numerator and its denominator, so simplify each one fully before dividing.

Minus sign and powers

$-3^{2} = -9$

The exponent binds only to the 3, so square first and apply the minus after. Compare $(-3)^{2} = 9$.

Example: $8 + 12 \div 4 \times 3 - 2^{2} = 8 + 3 \times 3 - 4 = 8 + 9 - 4 = 13$.

Fraction Formulas

Formula

Expression

What it means

Adding like fractions

$\frac{a}{c} + \frac{b}{c} = \frac{a + b}{c}$

When the denominators are equal, add the numerators and keep the common denominator $c$, where $c \neq 0$.

Subtracting like fractions

$\frac{a}{c} - \frac{b}{c} = \frac{a - b}{c}$

Subtract the numerators and keep the common denominator $c$, with $c \neq 0$.

Adding unlike fractions

$\frac{a}{b} + \frac{c}{d} = \frac{ad + bc}{bd}$

Rewrite both over the common denominator $bd$, with $b, d \neq 0$. Using the LCM of $b$ and $d$ keeps numbers smaller.

Subtracting unlike fractions

$\frac{a}{b} - \frac{c}{d} = \frac{ad - bc}{bd}$

Same method as addition, subtract the cross products over $bd$, then reduce to lowest terms.

Multiplying fractions

$\frac{a}{b} \times \frac{c}{d} = \frac{ac}{bd}$

Multiply numerator by numerator and denominator by denominator, with $b, d \neq 0$. Cancel common factors first to save work.

Dividing fractions

$\frac{a}{b} \div \frac{c}{d} = \frac{a}{b} \times \frac{d}{c} = \frac{ad}{bc}$

Keep the first fraction, flip the second and multiply. Needs $b, c, d \neq 0$ because you cannot divide by zero.

Reciprocal of a fraction

$\frac{a}{b} \to \frac{b}{a}$

Swap numerator and denominator, valid when $a \neq 0$. A number times its reciprocal always equals 1.

Mixed number to improper fraction

$a\frac{b}{c} = \frac{ac + b}{c}$

Multiply the whole number $a$ by the denominator $c$, add the numerator $b$ and keep $c$ as the denominator.

Improper fraction to mixed number

$\frac{p}{q} = Q\frac{R}{q}$

Divide $p$ by $q$. The quotient $Q$ is the whole part and the remainder $R$ is the new numerator over $q$.

Equivalent fractions

$\frac{a}{b} = \frac{a \times k}{b \times k}$

Multiplying or dividing top and bottom by the same nonzero number $k$ gives the same value in a different form.

Simplest form

$\frac{a}{b} = \frac{a \div h}{b \div h}$

Divide numerator and denominator by $h$, the HCF of $a$ and $b$, to reduce the fraction to lowest terms.

Comparing fractions

$\frac{a}{b} > \frac{c}{d} \iff ad > bc$

Cross-multiply to compare two fractions without finding a common denominator. Valid when $b$ and $d$ are both positive.

Fraction of a quantity

$\frac{a}{b} \text{ of } N = \frac{a \times N}{b}$

To find a fraction of an amount $N$, multiply $N$ by the numerator and divide by the denominator.

Example: $\frac{2}{3} + \frac{3}{4} = \frac{2 \times 4 + 3 \times 3}{12} = \frac{17}{12} = 1\frac{5}{12}$.

Decimal, Fraction And Percent Conversion Formulas

Formula

Expression

What it means

Percent as a fraction

$p% = \frac{p}{100}$

Percent means "per hundred", so $p$ percent is $p$ parts out of 100. For example $35% = 0.35$.

Fraction to percent

$\frac{a}{b} = \left(\frac{a}{b} \times 100\right)%$

Multiply a fraction by 100 to express it as a percent, with $b \neq 0$.

Decimal to percent

$d = (100d)%$

Move the decimal point two places to the right and add the percent sign, so $0.075 = 7.5%$.

Terminating decimal to fraction

$0.d_{1}d_{2}\ldots d_{k} = \frac{d_{1}d_{2}\ldots d_{k}}{10^{k}}$

Write the $k$ digits after the point over $10^{k}$, then simplify. For example $0.125 = \frac{125}{1000} = \frac{1}{8}$.

Pure recurring decimal to fraction

$0.\overline{d_{1}d_{2}\ldots d_{k}} = \frac{d_{1}d_{2}\ldots d_{k}}{10^{k} - 1}$

A block of $k$ digits that repeats forever equals that block over $k$ nines, so $0.\overline{7} = \frac{7}{9}$.

Mixed recurring decimal to fraction

$0.a\overline{b} = \frac{ab - a}{90}$

Here $ab$ is the two-digit number formed by the digits. One non-repeating digit $a$ is followed by a repeating digit $b$, so $0.1\overline{6} = \frac{15}{90} = \frac{1}{6}$.

Multiplying by a power of 10

$x \times 10^{n}$

Shift the decimal point of $x$ by $n$ places to the right. Dividing by $10^{n}$ shifts it $n$ places to the left.

Decimal places in a product

$\text{places in } (x \times y) = \text{places in } x + \text{places in } y$

Multiply as whole numbers, then place the point so the answer has as many decimal places as both factors together.

Scientific notation

$N = a \times 10^{n}$

Write any number with $1 \leq a < 10$ and integer $n$. Large numbers get positive $n$ and small numbers negative $n$.

Example: $0.\overline{36} = \frac{36}{99} = \frac{4}{11}$, and as a percent $\frac{4}{11} \times 100 \approx 36.36%$.

Percentage Formulas

Formula

Expression

What it means

Percent of a number

$p% \text{ of } N = \frac{p}{100} \times N$

Convert the percent to a fraction of 100 and multiply by the amount $N$.

What percent A is of B

$\frac{A}{B} \times 100%$

Gives $A$ as a percent of the whole $B$, with $B \neq 0$. Used for marks, shares and proportions of a total.

Percentage change

$\frac{\text{new} - \text{old}}{\text{old}} \times 100%$

A positive result is an increase and a negative result is a decrease. Always divide by the original (old) value.

Percentage increase

$\frac{\text{increase}}{\text{original}} \times 100%$

The rise in value as a percent of the starting value, where increase equals new minus original.

Percentage decrease

$\frac{\text{decrease}}{\text{original}} \times 100%$

The fall in value as a percent of the starting value, where decrease equals original minus new.

Increasing by p%

$N \times \left(1 + \frac{p}{100}\right)$

Multiplies $N$ by a single factor to give the value after a $p$ percent rise, so a 20 percent rise means times 1.2.

Decreasing by p%

$N \times \left(1 - \frac{p}{100}\right)$

Gives the value after a $p$ percent fall, so a 15 percent fall means multiplying by 0.85.

Reverse percentage after an increase

$\text{original} = \frac{\text{final}}{1 + \frac{p}{100}}$

Finds the starting value when you know the value after a $p$ percent increase. Divide, do not subtract $p$ percent of the final value.

Reverse percentage after a decrease

$\text{original} = \frac{\text{final}}{1 - \frac{p}{100}}$

Finds the starting value from the value after a $p$ percent decrease, with $p < 100$.

Two successive percentage changes

$\text{net change} = a + b + \frac{ab}{100}$

Net percent change after changes of $a$ percent then $b$ percent. Write a decrease as a negative number.

Percent error

$\frac{\lvert \text{measured} - \text{actual} \rvert}{\text{actual}} \times 100%$

How far a measured or estimated value is from the true value, as a percent of the true value.

Example: A price rises from 250 to 300, so the change is $\frac{300 - 250}{250} \times 100% = 20%$. If a price is 360 after a 20% rise, the original was $\frac{360}{1.2} = 300$.

Ratio And Proportion Formulas

Formula

Expression

What it means

Ratio formula

$a : b = \frac{a}{b}$

Compares two quantities in the same unit by division, read "a to b", with $b \neq 0$.

Simplest form of a ratio

$a : b = \frac{a}{h} : \frac{b}{h}$

Divide both terms by $h$, their HCF, so the terms have no common factor other than 1.

Proportion and cross-multiplication

$a : b = c : d \iff ad = bc$

Two ratios are equal when the product of the extremes $a, d$ equals the product of the means $b, c$.

Fourth proportional

$x = \frac{bc}{a}$

The value $x$ that completes $a : b = c : x$, found by cross-multiplication with $a \neq 0$.

Third proportional

$x = \frac{b^{2}}{a}$

The value $x$ in $a : b = b : x$, where the middle term is repeated.

Mean proportional

$x = \sqrt{ab}$

The value $x$ in $a : x = x : b$ for positive $a$ and $b$. It is the geometric mean of the two numbers.

Direct proportion

$\frac{y_{1}}{x_{1}} = \frac{y_{2}}{x_{2}}$

When $y = kx$, both quantities rise or fall together and their ratio stays fixed at the constant $k$.

Inverse proportion

$x_{1}y_{1} = x_{2}y_{2}$

When $y = \frac{k}{x}$, one quantity rises as the other falls and their product stays fixed. Typical case: workers and days.

Dividing N in the ratio a : b

$\frac{a}{a + b} \times N$ and $\frac{b}{a + b} \times N$

Each share is its ratio part over the total number of parts, multiplied by the amount $N$ being shared.

Dividing N in the ratio a : b : c

$\frac{a}{a + b + c} \times N$

The first share of three. Replace the numerator by $b$ or $c$ for the other two shares.

Combining two ratios

$a : b : c = pr : qr : qs$

Joins $a : b = p : q$ and $b : c = r : s$ by making the shared term $b$ equal in both.

Compound ratio

$(a : b) \times (c : d) = ac : bd$

Multiply the first terms together and the second terms together to combine two ratios into one.

Componendo and dividendo

$\frac{a + b}{a - b} = \frac{c + d}{c - d}$

Follows from $\frac{a}{b} = \frac{c}{d}$ when $a \neq b$ and $c \neq d$. Useful for solving ratio equations quickly.

Example: Divide 360 in the ratio $4 : 5$. There are 9 parts, so the shares are $\frac{4}{9} \times 360 = 160$ and $\frac{5}{9} \times 360 = 200$.

Average Formulas

Formula

Expression

What it means

Average formula (arithmetic mean)

$\bar{x} = \frac{x_{1} + x_{2} + \cdots + x_{n}}{n}$

Add all $n$ values and divide by how many there are. This is the everyday meaning of "average".

Total from the average

$\text{sum} = \bar{x} \times n$

Rearranged mean formula. Most average word problems are solved by converting averages back to totals first.

Weighted average

$\bar{x}{w} = \frac{\sum{i=1}^{n} w_{i}x_{i}}{\sum_{i=1}^{n} w_{i}}$

Each value $x_{i}$ counts $w_{i}$ times, for example credits or marks weightage. Weights must not sum to zero.

Combined average of two groups

$\bar{x} = \frac{n_{1}\bar{x}{1} + n{2}\bar{x}{2}}{n{1} + n_{2}}$

Merges groups of sizes $n_{1}$ and $n_{2}$ with means $\bar{x}{1}$ and $\bar{x}{2}$. Do not simply average the two means.

Average of equally spaced numbers

$\bar{x} = \frac{\text{first} + \text{last}}{2}$

For any list with a constant gap, such as consecutive integers or an AP, the mean is the midpoint of the ends.

Average of the first n natural numbers

$\frac{n + 1}{2}$

The mean of $1, 2, \ldots, n$. For 1 to 100 it is 50.5.

Average of the first n even numbers

$n + 1$

The mean of $2, 4, \ldots, 2n$. For the first 10 even numbers it is 11.

Average of the first n odd numbers

$n$

The mean of the odd numbers $1, 3, \ldots, 2n - 1$ is simply $n$, so the first 8 odd numbers average 8.

New average after adding one value

$\bar{x}_{\text{new}} = \frac{n\bar{x} + a}{n + 1}$

When a value $a$ joins $n$ values with mean $\bar{x}$, rebuild the total and divide by the new count.

New average after replacing one value

$\bar{x}_{\text{new}} = \bar{x} + \frac{\text{new} - \text{old}}{n}$

Swapping one of $n$ values shifts the mean by the difference spread over all $n$ values.

Example: Class A has 30 students with mean 72 and class B has 20 with mean 80, so the combined mean is $\frac{30 \times 72 + 20 \times 80}{50} = \frac{3760}{50} = 75.2$.

HCF And LCM Formulas

HCF (highest common factor) is also called GCD or GCF, and LCM is the least common multiple. The formulas below are for positive integers.

Formula

Expression

What it means

HCF by prime factorisation

$\text{HCF} = \prod p_{i}^{\min(a_{i}, b_{i})}$

Write both numbers as products of primes $p_{i}$ and multiply each common prime raised to its lowest power.

LCM by prime factorisation

$\text{LCM} = \prod p_{i}^{\max(a_{i}, b_{i})}$

Multiply every prime that appears in either number, each raised to its highest power.

HCF times LCM

$\text{HCF}(a, b) \times \text{LCM}(a, b) = a \times b$

True for any pair of positive integers $a$ and $b$. It does not hold for three or more numbers in general.

LCM from the HCF

$\text{LCM}(a, b) = \frac{a \times b}{\text{HCF}(a, b)}$

The quickest way to find an LCM when the HCF is known or easy to find.

Co-prime numbers

$\text{HCF}(a, b) = 1 \Rightarrow \text{LCM}(a, b) = ab$

Two numbers with no common factor except 1 have their product as their LCM, for example 8 and 15.

Euclid's division algorithm

$\text{HCF}(a, b) = \text{HCF}(b, r)$

Here $r$ is the remainder when $a$ is divided by $b$. Repeat until the remainder is 0, and the last divisor is the HCF.

HCF of fractions

$\text{HCF}\left(\frac{a}{b}, \frac{c}{d}\right) = \frac{\text{HCF}(a, c)}{\text{LCM}(b, d)}$

For fractions in lowest terms, take the HCF of the numerators over the LCM of the denominators.

LCM of fractions

$\text{LCM}\left(\frac{a}{b}, \frac{c}{d}\right) = \frac{\text{LCM}(a, c)}{\text{HCF}(b, d)}$

For fractions in lowest terms, take the LCM of the numerators over the HCF of the denominators.

Greatest common factor divides the difference

$\text{HCF}(a, b) \mid (a - b)$

Any common factor of two numbers also divides their difference, which helps narrow down the HCF quickly.

Example: $12 = 2^{2} \times 3$ and $18 = 2 \times 3^{2}$, so $\text{HCF} = 2 \times 3 = 6$ and $\text{LCM} = 2^{2} \times 3^{2} = 36$. Check: $6 \times 36 = 216 = 12 \times 18$.

Prime Factorisation And Factor Count Formulas

Each row assumes $N = p_{1}^{a_{1}} p_{2}^{a_{2}} \cdots p_{k}^{a_{k}}$, where the $p_{i}$ are distinct primes and each $a_{i} \geq 1$.

Formula

Expression

What it means

Prime factorisation

$N = p_{1}^{a_{1}} p_{2}^{a_{2}} \cdots p_{k}^{a_{k}}$

Every integer greater than 1 can be written as a product of prime powers in exactly one way, apart from order.

Number of factors

$d(N) = (a_{1} + 1)(a_{2} + 1)\cdots(a_{k} + 1)$

Add 1 to each exponent and multiply. The count includes 1 and $N$ itself.

Sum of factors

$\sigma(N) = \frac{p_{1}^{a_{1}+1} - 1}{p_{1} - 1} \times \cdots \times \frac{p_{k}^{a_{k}+1} - 1}{p_{k} - 1}$

Multiply one geometric-series sum per prime. The total includes 1 and $N$.

Product of all factors

$N^{d(N)/2}$

Factors pair up to multiply to $N$, so the product of all $d(N)$ factors is $N$ raised to half that count.

Number of odd factors

$(a_{2} + 1)(a_{3} + 1)\cdots(a_{k} + 1)$

For even $N$, take $p_{1} = 2$ and ignore its exponent, since odd factors cannot contain the prime 2. If $N$ is odd, every factor is odd.

Number of even factors

$d(N) - \text{odd factors}$

All factors minus the odd ones. Equivalently $a_{1}(a_{2} + 1)\cdots(a_{k} + 1)$ when $p_{1} = 2$.

Factor count of a perfect square

$d(N)$ is odd

A number has an odd number of factors exactly when it is a perfect square, because its square root pairs with itself.

Example: $360 = 2^{3} \times 3^{2} \times 5$, so $d(360) = 4 \times 3 \times 2 = 24$ factors and $\sigma(360) = 15 \times 13 \times 6 = 1170$.

Divisibility Rules

In this table $d_{0}$ is the units digit of $N$ and $a \mid N$ means $a$ divides $N$ with no remainder.

Formula

Expression

What it means

Divisibility by 2

$2 \mid N \iff d_{0} \in \lbrace 0, 2, 4, 6, 8\rbrace$

A number is divisible by 2 when its last digit is even.

Divisibility by 3

$3 \mid N \iff 3 \mid (\text{sum of digits})$

Add all the digits. If that sum is a multiple of 3, so is the number.

Divisibility by 4

$4 \mid N \iff 4 \mid (\text{last two digits})$

Only the number formed by the tens and units digits matters, because 100 is a multiple of 4.

Divisibility by 5

$5 \mid N \iff d_{0} \in \lbrace 0, 5\rbrace$

A number is divisible by 5 when it ends in 0 or 5.

Divisibility by 6

$6 \mid N \iff 2 \mid N \text{ and } 3 \mid N$

The number must pass both the test for 2 and the test for 3, since 2 and 3 are co-prime.

Divisibility by 7

$7 \mid N \iff 7 \mid (\text{rest} - 2d_{0})$

Remove the units digit, double it and subtract from the remaining number. Repeat until the result is small.

Divisibility by 8

$8 \mid N \iff 8 \mid (\text{last three digits})$

Only the last three digits matter, because 1000 is a multiple of 8.

Divisibility by 9

$9 \mid N \iff 9 \mid (\text{sum of digits})$

If the digit sum is a multiple of 9, the number is too. The remainder on division by 9 equals the digit-sum remainder.

Divisibility by 10

$10 \mid N \iff d_{0} = 0$

A number is divisible by 10 when its last digit is 0.

Divisibility by 11

$11 \mid N \iff 11 \mid (S_{\text{odd}} - S_{\text{even}})$

Sum the digits in odd places and in even places counting from the right. A difference of 0 or a multiple of 11 passes.

Divisibility by 12

$12 \mid N \iff 3 \mid N \text{ and } 4 \mid N$

The number must pass the tests for both 3 and 4.

Divisibility by 25

$25 \mid N \iff \text{last two digits} \in \lbrace 00, 25, 50, 75\rbrace$

Only the last two digits matter, because 100 is a multiple of 25.

Co-prime divisors rule

$a \mid N \text{ and } b \mid N \Rightarrow ab \mid N$

Holds when $\text{HCF}(a, b) = 1$. This is why tests for 6, 12, 15 and 18 combine two simpler tests.

Example: For 7392 the digit sum is 21, so $3 \mid 7392$, and the last two digits give $4 \mid 92$, so $7392 \div 12 = 616$ exactly.

Squares, Cubes And Roots

Formula

Expression

What it means

Square of a number

$n^{2} = n \times n$

A number multiplied by itself. The square of any real number is never negative.

Perfect squares

$N = k^{2}$

$N$ is a perfect square when $k$ is an integer. Perfect squares end in 0, 1, 4, 5, 6 or 9, never in 2, 3, 7 or 8.

Cube of a number

$n^{3} = n \times n \times n$

A number used three times as a factor. The cube keeps the sign of the number, so $(-2)^{3} = -8$.

Perfect cube

$N = k^{3}$

$N$ is a perfect cube when $k$ is an integer, as in 1, 8, 27, 64 and 125.

Square root

$\sqrt{N} = k \iff k^{2} = N$

The principal square root is the non-negative value $k$, defined for real numbers only when $N \geq 0$.

Cube root

$\sqrt[3]{N} = k \iff k^{3} = N$

Defined for every real $N$, including negatives, so $\sqrt[3]{-27} = -3$.

Square root of a square

$\sqrt{x^{2}} = \lvert x \rvert$

The result is the absolute value of $x$, since a principal square root is never negative.

Product rule for roots

$\sqrt{ab} = \sqrt{a} \times \sqrt{b}$

Valid for $a \geq 0$ and $b \geq 0$. Used to simplify roots by pulling out perfect-square factors.

Quotient rule for roots

$\sqrt{\frac{a}{b}} = \frac{\sqrt{a}}{\sqrt{b}}$

Valid for $a \geq 0$ and $b > 0$. The root of a fraction is the root of the top over the root of the bottom.

Simplifying a square root

$\sqrt{a^{2}b} = a\sqrt{b}$

For $a \geq 0$ and $b \geq 0$, move a perfect-square factor $a^{2}$ outside the root as $a$.

Squaring a number ending in 5

$(10a + 5)^{2} = 100a(a + 1) + 25$

Multiply the leading part $a$ by the next integer and write 25 after it, so $35^{2} = 1225$.

Gap between consecutive squares

$(n + 1)^{2} - n^{2} = 2n + 1$

Consecutive squares differ by consecutive odd numbers, so $n^{2}$ to $(n + 1)^{2}$ always steps by $2n + 1$.

Pythagorean triples

$(m^{2} - n^{2}, \ 2mn, \ m^{2} + n^{2})$

For integers $m > n > 0$ these three numbers always satisfy $a^{2} + b^{2} = c^{2}$. $m = 2, n = 1$ gives 3, 4, 5.

Example: $\sqrt{72} = \sqrt{36 \times 2} = 6\sqrt{2} \approx 6 \times 1.41421 \approx 8.4853$.

Sum Formulas For Natural Numbers

Formula

Expression

What it means

Sum of natural numbers formula

$1 + 2 + 3 + \cdots + n = \frac{n(n + 1)}{2}$

Adds the first $n$ counting numbers. Pairing the first and last terms gives $n$ halves of $n + 1$.

Sum of even numbers formula

$2 + 4 + 6 + \cdots + 2n = n(n + 1)$

Adds the first $n$ even numbers. It is twice the sum of the first $n$ natural numbers.

Sum of odd numbers

$1 + 3 + 5 + \cdots + (2n - 1) = n^{2}$

The first $n$ odd numbers always add to a perfect square, for example $1 + 3 + 5 = 9$.

Sum of squares

$1^{2} + 2^{2} + \cdots + n^{2} = \frac{n(n + 1)(2n + 1)}{6}$

Adds the squares of the first $n$ natural numbers. The answer is always a whole number.

Sum of cubes of n natural numbers

$1^{3} + 2^{3} + \cdots + n^{3} = \left[\frac{n(n + 1)}{2}\right]^{2}$

The sum of the first $n$ cubes equals the square of the sum of the first $n$ natural numbers.

Sum of squares of the first n even numbers

$2^{2} + 4^{2} + \cdots + (2n)^{2} = \frac{2n(n + 1)(2n + 1)}{3}$

Four times the sum of the first $n$ squares, because each term is $4k^{2}$.

Sum of squares of the first n odd numbers

$1^{2} + 3^{2} + \cdots + (2n - 1)^{2} = \frac{n(2n - 1)(2n + 1)}{3}$

Adds the squares of the first $n$ odd numbers, for example $1 + 9 + 25 = 35$ when $n = 3$.

Sum of consecutive integers from a to b

$a + (a + 1) + \cdots + b = \frac{(b - a + 1)(a + b)}{2}$

Number of terms times the average of the first and last terms, for integers $a \leq b$.

Sum of multiples of k up to N

$k \times \frac{m(m + 1)}{2}$

Here $m = \left\lfloor \frac{N}{k} \right\rfloor$ is the number of multiples of $k$ from 1 to $N$.

Example: $1^{2} + 2^{2} + \cdots + 10^{2} = \frac{10 \times 11 \times 21}{6} = \frac{2310}{6} = 385$.

Division Algorithm Formulas

Formula

Expression

What it means

Dividend, divisor, quotient and remainder

$a = bq + r, \quad 0 \leq r < b$

Dividend $a$ equals divisor $b$ times quotient $q$ plus remainder $r$, for integers with $b > 0$. The remainder is always smaller than the divisor.

Finding the divisor

$b = \frac{a - r}{q}$

Rearranges the division algorithm when the dividend, quotient and remainder are known, with $q \neq 0$.

Finding the quotient

$q = \left\lfloor \frac{a}{b} \right\rfloor$

The quotient is the whole-number part of $a \div b$, found by rounding down, for positive $a$ and $b$.

Exact division

$r = 0 \iff b \mid a$

A zero remainder means $b$ is a factor of $a$ and $a$ is a multiple of $b$.

Same remainder test

$a \equiv c \pmod{m} \iff m \mid (a - c)$

Two integers leave the same remainder on division by $m$ exactly when $m$ divides their difference.

Remainder of a sum

$(a + c) \bmod m = [(a \bmod m) + (c \bmod m)] \bmod m$

Find each remainder first, add them, then take the remainder again. Saves work with large numbers.

Remainder of a product

$(a \times c) \bmod m = [(a \bmod m) \times (c \bmod m)] \bmod m$

Multiply the separate remainders and reduce again. Used to find remainders of large products and powers.

Division involving zero

$\frac{0}{a} = 0$

Zero divided by any nonzero $a$ is 0, but $\frac{a}{0}$ is undefined for every number $a$.

Example: Dividing 257 by 12 gives $q = 21$ and $r = 257 - 12 \times 21 = 5$, so $257 = 12 \times 21 + 5$.

Counting Integers And Even Or Odd Rules

Formula

Expression

What it means

Integers from a to b, both included

$b - a + 1$

Counts every integer in the closed range from $a$ to $b$, where $a \leq b$. From 15 to 40 there are 26.

Integers from a to b, both excluded

$b - a - 1$

Counts only the integers strictly between $a$ and $b$, where $a < b$.

Integers from a to b, one end included

$b - a$

Counts the integers when exactly one of the two endpoints is part of the range.

Multiples of k from 1 to N

$\left\lfloor \frac{N}{k} \right\rfloor$

Divide $N$ by $k$ and drop the decimal part, for positive integers $N$ and $k$.

Multiples of k from a to b

$\left\lfloor \frac{b}{k} \right\rfloor - \left\lfloor \frac{a - 1}{k} \right\rfloor$

Multiples up to $b$ minus multiples below $a$, for positive integers $a \leq b$.

Terms in an equally spaced list

$\frac{\text{last} - \text{first}}{d} + 1$

Counts the numbers in a list with constant gap $d$, such as $7, 11, 15, \ldots, 99$.

Even number

$2k$

Any integer of the form $2k$, where $k$ is an integer, is even. Zero is even.

Odd numbers

$2k + 1$

Any integer of the form $2k + 1$, where $k$ is an integer, is odd. It leaves remainder 1 when divided by 2.

Sum of two evens or two odds

$2m + 2n = 2(m + n)$

Even plus even is even, and odd plus odd is also even, since $(2m + 1) + (2n + 1) = 2(m + n + 1)$.

Sum of an even and an odd

$2m + (2n + 1) = 2(m + n) + 1$

Adding or subtracting an even and an odd number always gives an odd number.

Products of evens and odds

$(2m + 1)(2n + 1) = 2(2mn + m + n) + 1$

Odd times odd is odd. If at least one factor is even, the product is even.

Consecutive integers

$n, \ n + 1, \ n + 2, \ \ldots$

Integers one apart. Consecutive even or odd integers step by 2, as in $n, \ n + 2, \ n + 4$.

Product of consecutive integers

$n(n + 1)$ is even

Any two consecutive integers include an even number, and any three consecutive integers have a product divisible by 6.

Example: The multiples of 7 from 10 to 50 number $\left\lfloor \frac{50}{7} \right\rfloor - \left\lfloor \frac{9}{7} \right\rfloor = 7 - 1 = 6$, namely 14, 21, 28, 35, 42 and 49.

Commercial Math And Measurement Formulas

These formulas cover money problems (interest, profit and loss, discounts, tax), motion and work problems, and conversions between units of length, area, volume, mass, temperature and time. They are used from Grade 6 arithmetic up to the aptitude sections of competitive exams.

Simple Interest

Formula

Expression

What it means

Simple interest

$SI = \frac{P \times R \times T}{100}$

$P$ is the principal, $R$ the rate in percent per year and $T$ the time in years. Interest is charged only on the original principal.

Amount

$A = P + SI$

The total repaid or received at the end of the period is the principal plus the interest.

Amount in one step

$A = P\left(1 + \frac{RT}{100}\right)$

Gives the final amount directly without finding the interest first. $P$, $R$ and $T$ mean the same as above.

Principal

$P = \frac{100 \times SI}{R \times T}$

Rearranged form used when the interest, rate and time are known and the sum lent is unknown.

Rate

$R = \frac{100 \times SI}{P \times T}$

Finds the yearly rate in percent from the interest, the principal and the time in years.

Time period

$T = \frac{100 \times SI}{P \times R}$

Finds the number of years needed to earn a given interest on principal $P$ at $R%$ per year.

Interest with a decimal rate

$I = Prt$

The same formula with $r$ written as a decimal (8% becomes 0.08) and $t$ in years, as in US textbooks.

Time in months or days

$T = \frac{m}{12}$ or $T = \frac{d}{365}$

Change $m$ months or $d$ days into years before putting $T$ into the simple interest formula.

Time for a sum to become k times

$T = \frac{100(k - 1)}{R}$

Years needed at simple interest for the amount to reach $k$ times the principal at a rate of $R%$ per year.

Example: For $P = 5000$, $R = 8$ and $T = 3$, $SI = \frac{5000 \times 8 \times 3}{100} = 1200$, so the amount is $5000 + 1200 = 6200$ rupees.

Compound Interest

In this table $R$ is the yearly rate in percent and $n$ is the number of years, unless a row says otherwise.

Formula

Expression

What it means

Amount, compounded annually

$A = P\left(1 + \frac{R}{100}\right)^{n}$

$P$ is the principal. Interest is added once a year, and each year's interest also earns interest after that.

Compound interest

$CI = A - P$

The compound interest earned is the final amount minus the principal that was invested.

Compounded half-yearly

$A = P\left(1 + \frac{R}{200}\right)^{2n}$

Interest is added every six months, so the rate per period is halved and the number of periods doubles.

Compounded quarterly

$A = P\left(1 + \frac{R}{400}\right)^{4n}$

Interest is added four times a year, so each quarter uses $\frac{R}{4}%$ and there are $4n$ periods.

Compounded n times a year

$A = P\left(1 + \frac{r}{n}\right)^{nt}$

General form. Here $r$ is the annual rate as a decimal, $n$ the compounding periods per year and $t$ the years. Monthly uses $n = 12$, daily $n = 365$.

Compounded continuously

$A = Pe^{rt}$

$e \approx 2.71828$, $r$ is the annual rate as a decimal and $t$ the time in years. It is the limit of compounding ever more often.

Different rates in successive years

$A = P\left(1 + \frac{R_{1}}{100}\right)\left(1 + \frac{R_{2}}{100}\right)\left(1 + \frac{R_{3}}{100}\right)$

Used when the rate changes each year, with $R_{1}%$ in the first year, $R_{2}%$ in the second and so on.

Fractional number of years

$A = P\left(1 + \frac{R}{100}\right)^{n}\left(1 + \frac{fR}{100}\right)$

For $n$ whole years plus a fraction $f$ of a year, with simple interest on the part year. For 2.5 years, $n = 2$ and $f = \frac{1}{2}$.

CI minus SI for 2 years

$CI - SI = P\left(\frac{R}{100}\right)^{2}$

The extra interest over two years caused by the first year's interest earning interest. Assumes annual compounding.

CI minus SI for 3 years

$CI - SI = P\left(\frac{R}{100}\right)^{2}\left(3 + \frac{R}{100}\right)$

The gap between compound and simple interest over three years on the same principal at the same annual rate.

Rule of 72

$t \approx \frac{72}{R}$

A quick estimate of the years needed for money to double at $R%$ compounded yearly. It is most accurate near 8%.

Example: 10000 rupees at 8% per year compounded quarterly for 1 year gives $A = 10000\left(1 + \frac{8}{400}\right)^{4} = 10000 \times 1.02^{4} \approx 10824.32$, so $CI \approx 824.32$ rupees.

Effective Annual Rate, Present Value And Loans

Formula

Expression

What it means

Effective annual rate

$EAR = \left(1 + \frac{r}{n}\right)^{n} - 1$

The true yearly growth when a nominal decimal rate $r$ is compounded $n$ times a year. Used to compare savings or loan offers.

EAR with continuous compounding

$EAR = e^{r} - 1$

The effective yearly rate when the nominal decimal rate $r$ is compounded continuously.

Nominal rate from EAR

$r = n\left[(1 + EAR)^{\frac{1}{n}} - 1\right]$

Turns an effective annual rate back into the nominal rate that is compounded $n$ times per year.

Present value

$PV = \frac{A}{\left(1 + \frac{r}{n}\right)^{nt}}$

The sum to invest today to reach amount $A$ after $t$ years at nominal rate $r$ compounded $n$ times a year.

Compound annual growth rate

$CAGR = \left(\frac{V_{f}}{V_{i}}\right)^{\frac{1}{t}} - 1$

The steady yearly growth rate, as a decimal, that takes a starting value $V_{i}$ to a final value $V_{f}$ in $t$ years.

Loan EMI

$EMI = \frac{P \cdot i \cdot (1 + i)^{N}}{(1 + i)^{N} - 1}$

Equal monthly instalment on a loan $P$, where $i$ is the monthly rate as a decimal (annual rate divided by 12) and $N$ the number of months.

Example: A nominal rate of 12% compounded monthly has $EAR = \left(1 + \frac{0.12}{12}\right)^{12} - 1 = 1.01^{12} - 1 \approx 0.1268$, which is about 12.68% per year.

Appreciation And Depreciation

Formula

Expression

What it means

Appreciation

$V = V_{0}\left(1 + \frac{R}{100}\right)^{n}$

Value after $n$ years when an asset worth $V_{0}$ gains $R%$ of its current value every year, such as land.

Depreciation

$V = V_{0}\left(1 - \frac{R}{100}\right)^{n}$

Value after $n$ years when an item worth $V_{0}$ loses $R%$ of its current value every year, such as a car.

Original value from depreciated value

$V_{0} = \frac{V}{\left(1 - \frac{R}{100}\right)^{n}}$

Works backward from today's value $V$ to the value $n$ years ago under yearly depreciation at $R%$.

Population growth

$P_{n} = P_{0}\left(1 + \frac{R}{100}\right)^{n}$

Population after $n$ years when it grows by $R%$ a year from $P_{0}$. Use a minus sign for a yearly decline.

Population n years ago

$P_{0} = \frac{P_{n}}{\left(1 + \frac{R}{100}\right)^{n}}$

Finds the earlier population from the present one $P_{n}$ when the growth rate $R%$ has stayed constant.

Growth then decline

$V = V_{0}\left(1 + \frac{R_{1}}{100}\right)\left(1 - \frac{R_{2}}{100}\right)$

A rise of $R_{1}%$ in one year followed by a fall of $R_{2}%$ the next. Add one factor for each extra year.

Straight-line depreciation

$D = \frac{C - S}{n}$

Equal yearly depreciation $D$ for an asset that costs $C$ and has scrap value $S$ after a useful life of $n$ years.

Example: A machine bought for 50000 rupees depreciates at 10% a year, so after 2 years it is worth $50000 \times 0.9^{2} = 50000 \times 0.81 = 40500$ rupees.

Profit And Loss

Formula

Expression

What it means

Profit

$\text{Profit} = SP - CP$

A profit is made when the selling price $SP$ is more than the cost price $CP$.

Loss

$\text{Loss} = CP - SP$

A loss is made when the cost price $CP$ is more than the selling price $SP$.

Profit percentage

$\text{Profit},% = \frac{\text{Profit}}{CP} \times 100$

Profit written as a percent of the cost price. Profit and loss percents are based on $CP$ unless a question says otherwise.

Loss percentage

$\text{Loss},% = \frac{\text{Loss}}{CP} \times 100$

Loss written as a percent of the cost price $CP$, used to compare losses on items of different prices.

Selling price at a profit

$SP = CP \times \frac{100 + P%}{100}$

Finds the selling price when the cost price and the wanted profit percent $P%$ are known.

Selling price at a loss

$SP = CP \times \frac{100 - L%}{100}$

Finds the selling price when an item is sold at a loss of $L%$ on its cost price.

Cost price from SP and profit

$CP = \frac{100 \times SP}{100 + P%}$

Works back to the cost price when the selling price and the profit percent are given.

Cost price from SP and loss

$CP = \frac{100 \times SP}{100 - L%}$

Works back to the cost price when the selling price and the loss percent are given.

Profit margin

$\text{Margin},% = \frac{\text{Profit}}{SP} \times 100$

Profit as a percent of the selling price, common in business. It is smaller than the profit percent on cost whenever there is a profit.

Same SP with equal gain and loss

$\text{Net loss},% = \frac{x^{2}}{100}$

Two items sold at the same price, one at an $x%$ gain and one at an $x%$ loss, always give an overall loss of this percent.

Gain with a false weight

$\text{Gain},% = \frac{\text{True weight} - \text{False weight}}{\text{False weight}} \times 100$

A seller who charges the cost price but hands over less than the true weight makes this percent profit.

Partnership profit share

$\text{Share}{A} : \text{Share}{B} = C_{A}T_{A} : C_{B}T_{B}$

Partners divide profit in the ratio of each capital $C$ multiplied by the time $T$ for which it was invested.

Example: An item costing 800 rupees is sold at a 20% profit, so $SP = 800 \times \frac{120}{100} = 960$ rupees and the profit is $960 - 800 = 160$ rupees.

Discount And Marked Price

The marked price (list price) is the price printed on the item, and a discount is always worked out on it.

Formula

Expression

What it means

Discount

$D = MP - SP$

Discount is the reduction from the marked price $MP$ to the selling price $SP$ that the buyer actually pays.

Discount percentage

$D% = \frac{D}{MP} \times 100$

Discount written as a percent of the marked price, never of the cost price.

Selling price after discount

$SP = MP\left(1 - \frac{d}{100}\right)$

The price paid after a discount of $d%$ is taken off the marked price $MP$.

Marked price from SP

$MP = \frac{100 \times SP}{100 - d}$

Finds the list price when the selling price and the discount rate $d%$ are known.

Markup

$MP = CP\left(1 + \frac{m}{100}\right)$

A seller who marks goods $m%$ above the cost price $CP$ sets the marked price this way.

Marked price for a target profit

$MP = CP \times \frac{100 + P%}{100 - d%}$

The marked price that still leaves a profit of $P%$ on cost after a discount of $d%$ is given.

Profit after markup and discount

$\text{Profit},% = m - d - \frac{md}{100}$

Net profit percent on cost when goods are marked $m%$ above cost and then sold at a $d%$ discount.

Buy x get y free

$\text{Discount},% = \frac{y}{x + y} \times 100$

The effective discount when a customer pays for $x$ items and takes home $x + y$ items.

Example: To make a 20% profit on a cost of 1000 rupees while giving a 10% discount, $MP = 1000 \times \frac{120}{90} \approx 1333.33$ rupees.

Successive Discounts And Percentage Changes

Formula

Expression

What it means

Two successive discounts

$d = d_{1} + d_{2} - \frac{d_{1}d_{2}}{100}$

The single discount equal to $d_{1}%$ followed by $d_{2}%$. The second discount applies to the already reduced price.

Price after successive discounts

$SP = MP\left(1 - \frac{d_{1}}{100}\right)\left(1 - \frac{d_{2}}{100}\right)\left(1 - \frac{d_{3}}{100}\right)$

Multiply one factor for each discount. The order does not matter, but the discounts cannot simply be added.

Two successive changes

$\text{Net change},% = a + b + \frac{ab}{100}$

Net percent change after a change of $a%$ and then $b%$. Use positive values for increases and negative values for decreases.

Rise and fall by the same percent

$\text{Net change},% = -\frac{x^{2}}{100}$

An increase of $x%$ and a decrease of $x%$, in either order, always end in a net decrease.

Fixed spending after a price rise

$\text{Cut},% = \frac{r}{100 + r} \times 100$

How much consumption must drop when the price rises by $r%$ so that total spending stays the same.

Fixed spending after a price fall

$\text{Increase},% = \frac{r}{100 - r} \times 100$

How much consumption can grow when the price falls by $r%$ while total spending stays the same.

Example: Discounts of 20% and 10% equal a single discount of $20 + 10 - \frac{20 \times 10}{100} = 28%$, so an item marked 2000 rupees sells for $2000 \times 0.8 \times 0.9 = 1440$ rupees.

GST And Sales Tax

Formula

Expression

What it means

Tax amount

$\text{Tax} = \frac{t}{100} \times P$

Tax on a pre-tax price $P$ at a rate of $t%$. The same formula works for GST, VAT and US sales tax.

Price including tax

$P_{\text{incl}} = P\left(1 + \frac{t}{100}\right)$

The final bill when tax at $t%$ is added to the pre-tax price $P$.

Pre-tax price from inclusive price

$P = \frac{100 \times P_{\text{incl}}}{100 + t}$

Removes the tax from a tax-inclusive price. Subtracting $t%$ of the inclusive price gives the wrong answer.

Tax inside an inclusive price

$\text{Tax} = P_{\text{incl}} \times \frac{t}{100 + t}$

The tax portion contained in a price that already includes tax at $t%$.

CGST and SGST split

$\text{CGST} = \text{SGST} = \frac{\text{GST}}{2}$

For a sale within one Indian state, the GST is split equally between the central and the state government.

IGST

$\text{IGST} = \text{GST}$

For a sale between two Indian states, the full GST is charged as one integrated tax.

Net GST payable

$\text{GST payable} = \text{Output GST} - \text{Input tax credit}$

A business pays the tax collected on its sales minus the tax it already paid on its purchases.

Discount then tax

$P_{\text{final}} = MP\left(1 - \frac{d}{100}\right)\left(1 + \frac{t}{100}\right)$

Tax is charged on the price after discount, so apply the discount factor first and then the tax factor.

Example: An item priced at 2000 rupees with 18% GST carries $\text{Tax} = \frac{18}{100} \times 2000 = 360$, so the bill is 2360 rupees, with 180 rupees each of CGST and SGST for a sale within one state.

Speed, Distance And Time

Formula

Expression

What it means

Speed

$S = \frac{D}{T}$

Speed $S$ is the distance $D$ covered per unit of time $T$. Keep units matched, such as km with hours.

Distance

$D = S \times T$

Distance travelled when moving at a constant speed $S$ for a time $T$.

Time

$T = \frac{D}{S}$

Time taken to cover a distance $D$ at a constant speed $S$.

km/h to m/s

$v_{\text{m/s}} = v_{\text{km/h}} \times \frac{5}{18}$

Multiply by $\frac{5}{18}$ because 1 km is 1000 m and 1 hour is 3600 seconds.

m/s to km/h

$v_{\text{km/h}} = v_{\text{m/s}} \times \frac{18}{5}$

The reverse conversion. For example, a speed of 10 m/s equals 36 km/h.

Average speed

$\text{Average speed} = \frac{\text{Total distance}}{\text{Total time}}$

Always divide total distance by total time. Taking the plain mean of the speeds is wrong when the times differ.

Average speed over two equal distances

$\bar{v} = \frac{2xy}{x + y}$

Average speed when two equal distances are covered at speeds $x$ and $y$. It is the harmonic mean of the two speeds.

Average speed over three equal distances

$\bar{v} = \frac{3xyz}{xy + yz + zx}$

Average speed when three equal distances are covered at speeds $x$, $y$ and $z$.

Average speed over equal times

$\bar{v} = \frac{x + y}{2}$

When the same amount of time is spent at speeds $x$ and $y$, the ordinary mean of the two speeds is correct.

Speed and time for a fixed distance

$\frac{S_{1}}{S_{2}} = \frac{T_{2}}{T_{1}}$

Over the same distance, speed and time are inversely proportional, so doubling the speed halves the time.

Distance from late and early arrival

$D = \frac{S_{1}S_{2}(t_{1} + t_{2})}{S_{2} - S_{1}}$

At the slower speed $S_{1}$ a traveller arrives $t_{1}$ late and at the faster speed $S_{2}$ arrives $t_{2}$ early. Times in hours.

Example: A car drives 120 km at 40 km/h and returns at 60 km/h, so its average speed is $\frac{2 \times 40 \times 60}{40 + 60} = 48,\text{km/h}$ (240 km in 5 hours).

Relative Speed, Trains, Boats And Streams

Formula

Expression

What it means

Relative speed, same direction

$S_{r} = \lvert u - v \rvert$

When two objects move the same way at speeds $u$ and $v$, the gap between them changes at the difference.

Relative speed, opposite directions

$S_{r} = u + v$

When two objects move towards or away from each other at speeds $u$ and $v$, the speeds add.

Time to meet

$T = \frac{d}{u + v}$

Time for two objects $d$ apart, moving towards each other at speeds $u$ and $v$, to meet.

Time to catch up

$T = \frac{d}{u - v}$

Time for a faster object at speed $u$ to close a gap $d$ on a slower one at $v$ going the same way, with $u > v$.

Train passing a pole or person

$T = \frac{L}{S}$

A train of length $L$ moving at speed $S$ must cover its own length to pass a point object.

Train passing a platform or bridge

$T = \frac{L + P}{S}$

The train must cover its own length $L$ plus the length $P$ of the platform or bridge.

Two trains crossing, opposite directions

$T = \frac{L_{1} + L_{2}}{u + v}$

Time for trains of lengths $L_{1}$ and $L_{2}$, moving towards each other at speeds $u$ and $v$, to pass completely.

Two trains crossing, same direction

$T = \frac{L_{1} + L_{2}}{u - v}$

Time for the faster train at speed $u$ to fully overtake the slower train at speed $v$, with $u > v$.

Downstream speed

$v_{d} = b + s$

A boat with speed $b$ in still water moves along with a current of speed $s$, so the speeds add.

Upstream speed

$v_{u} = b - s$

Moving against the current, the boat's speed is its still-water speed $b$ minus the stream speed $s$.

Speed in still water

$b = \frac{v_{d} + v_{u}}{2}$

The boat's still-water speed is the mean of its downstream speed $v_{d}$ and upstream speed $v_{u}$.

Speed of the stream

$s = \frac{v_{d} - v_{u}}{2}$

The speed of the current is half the difference between the downstream and upstream speeds.

Example: A 200 m train at $72,\text{km/h} = 72 \times \frac{5}{18} = 20,\text{m/s}$ crosses a 300 m platform in $\frac{200 + 300}{20} = 25$ seconds.

Time And Work

These rows assume that each worker or pipe keeps a constant rate.

Formula

Expression

What it means

Work rate

$\text{Rate} = \frac{1}{n}$

A worker who finishes a whole job in $n$ days completes $\frac{1}{n}$ of the job each day.

Work done

$W = \text{Rate} \times T$

The fraction of the job finished equals the work rate multiplied by the time $T$ spent working.

Combined rate

$\frac{1}{T} = \frac{1}{a} + \frac{1}{b}$

When workers who take $a$ and $b$ days alone work together, their daily rates add. $T$ is the joint time.

Two workers together

$T = \frac{ab}{a + b}$

Time for two workers, who need $a$ and $b$ days alone, to finish the job together.

Three workers together

$T = \frac{abc}{ab + bc + ca}$

Joint time for three workers who need $a$, $b$ and $c$ days alone.

One worker alone from the joint time

$T_{B} = \frac{aT}{a - T}$

If A alone takes $a$ days and A and B together take $T$ days, B alone takes this long. Needs $a > T$.

Work equivalence

$\frac{M_{1}D_{1}H_{1}}{W_{1}} = \frac{M_{2}D_{2}H_{2}}{W_{2}}$

$M$ is workers, $D$ days, $H$ hours per day and $W$ the amount of work. Used to rescale a job to a new team.

Efficiency and time

$\frac{E_{A}}{E_{B}} = \frac{T_{B}}{T_{A}}$

Efficiency and time for the same job are inversely proportional, so a worker twice as efficient takes half the time.

Pipe filling with a leak

$T = \frac{ab}{b - a}$

A pipe fills a tank in $a$ hours and a leak empties it in $b$ hours, with $b > a$. $T$ is the net filling time.

Net rate of several pipes

$\frac{1}{T} = \sum \frac{1}{f_{i}} - \sum \frac{1}{e_{j}}$

Add the rates of the filling pipes (times $f_{i}$) and subtract the rates of the emptying pipes (times $e_{j}$).

Sharing wages

$\text{Share}{A} : \text{Share}{B} = W_{A} : W_{B}$

Pay for a joint job is divided in the ratio of the work each person did, which is rate times time.

Example: If A finishes a job in 12 days and B in 6 days, together they need $\frac{12 \times 6}{12 + 6} = \frac{72}{18} = 4$ days.

Length Conversions

Formula

Expression

What it means

Kilometre to metre

$1,\text{km} = 1000,\text{m}$

Multiply kilometres by 1000 to get metres. Metric length units change by powers of 10.

Metre to centimetre

$1,\text{m} = 100,\text{cm}$

Multiply metres by 100 to get centimetres, and divide centimetres by 100 to get metres.

Centimetre to millimetre

$1,\text{cm} = 10,\text{mm}$

Multiply centimetres by 10 to get millimetres. One metre is 1000 millimetres.

Inch to centimetre

$1,\text{in} = 2.54,\text{cm}$

Exact by definition. Multiply inches by 2.54 for centimetres, or divide centimetres by 2.54 for inches.

Foot to inches

$1,\text{ft} = 12,\text{in}$

One foot is 12 inches, so multiply feet by 12 to get inches.

Foot to meters

$1,\text{ft} = 0.3048,\text{m}$

Exact value. Multiply feet by 0.3048 for metres. One metre is about 3.2808 feet.

Yard to metre

$1,\text{yd} = 3,\text{ft} = 0.9144,\text{m}$

One yard is three feet or 36 inches, which is exactly 0.9144 metres.

Miles to km

$1,\text{mile} = 1.609344,\text{km}$

Exact value. Multiply miles by 1.609344 (often rounded to 1.61) to get kilometres. One mile is 1760 yards.

Kilometres to miles

$1,\text{km} \approx 0.621371,\text{mile}$

Multiply kilometres by about 0.6214 to get miles, the reverse of the row above.

Nautical mile

$1,\text{nautical mile} = 1852,\text{m}$

Used at sea and in the air. A speed of one nautical mile per hour is called one knot.

Example: A 10 km race is $10 \times 0.621371 \approx 6.21$ miles, and a height of 6 ft is $6 \times 0.3048 = 1.8288,\text{m}$.

Mass And Capacity Conversions

Formula

Expression

What it means

Kilogram to gram

$1,\text{kg} = 1000,\text{g}$

Multiply kilograms by 1000 to get grams. One gram is 1000 milligrams.

Tonne to kilogram

$1,\text{t} = 1000,\text{kg}$

A metric tonne is 1000 kilograms. It differs from the US short ton of 2000 pounds.

Pound to kilogram

$1,\text{lb} = 0.45359237,\text{kg}$

Exact by definition. Multiply pounds by about 0.4536 to get kilograms.

Kilogram to pound

$1,\text{kg} \approx 2.20462,\text{lb}$

Multiply kilograms by about 2.2046 to get pounds.

Pound to ounce

$1,\text{lb} = 16,\text{oz}$

One pound is 16 ounces, and one ounce is about 28.35 grams.

Litre to millilitre

$1,\text{L} = 1000,\text{mL}$

Multiply litres by 1000 to get millilitres. One millilitre is the same volume as one cubic centimetre.

US gallon to litre

$1,\text{US gal} = 3.785411784,\text{L}$

Exact value, about 3.785 litres. This is the gallon used for fuel and milk in the United States.

UK gallon to litre

$1,\text{UK gal} = 4.54609,\text{L}$

The imperial gallon, exactly 4.54609 litres, is larger than the US gallon.

Example: A mass of 70 kg is $70 \times 2.20462 \approx 154.32$ pounds.

Area And Volume Unit Conversions

To convert an area, square the length factor, and to convert a volume, cube it.

Formula

Expression

What it means

Area conversion rule

$\text{Area factor} = k^{2}$

If one large unit of length equals $k$ small units, one square large unit equals $k^{2}$ square small units.

Volume conversion rule

$\text{Volume factor} = k^{3}$

If one large unit of length equals $k$ small units, one cubic large unit equals $k^{3}$ cubic small units.

Square centimetres to square metres

$1,\text{m}^{2} = 10000,\text{cm}^{2}$

Divide square centimetres by 10,000 to get square metres, because $100^{2} = 10000$.

Square kilometre to square metre

$1,\text{km}^{2} = 10^{6},\text{m}^{2}$

One square kilometre is one million square metres, since $1000^{2} = 10^{6}$.

Hectare

$1,\text{ha} = 10000,\text{m}^{2}$

A hectare is the area of a square 100 m on each side. One square kilometre is 100 hectares.

Acre

$1,\text{acre} = 4046.8564224,\text{m}^{2}$

Exact value, about 0.4047 hectare. One acre is also 43,560 square feet.

Square foot to square inches

$1,\text{ft}^{2} = 144,\text{in}^{2}$

Since one foot is 12 inches, one square foot is $12^{2} = 144$ square inches.

Square metre to square feet

$1,\text{m}^{2} \approx 10.7639,\text{ft}^{2}$

Multiply square metres by about 10.764 to get square feet, often used for room and flat sizes.

Cubic metre to cubic centimetre

$1,\text{m}^{3} = 10^{6},\text{cm}^{3}$

One cubic metre is one million cubic centimetres, since $100^{3} = 10^{6}$.

Cubic centimetre to millilitre

$1,\text{cm}^{3} = 1,\text{mL}$

Links volume to capacity. A 1 cm cube holds one millilitre, so 1000 cubic centimetres make one litre.

Cubic metre to litre

$1,\text{m}^{3} = 1000,\text{L}$

Used in tank and water-storage problems. Multiply cubic metres by 1000 to get litres.

Cubic foot to litre

$1,\text{ft}^{3} \approx 28.3168,\text{L}$

One cubic foot holds about 28.32 litres, found from $0.3048^{3},\text{m}^{3}$.

Example: A tank measuring 2 m by 1.5 m by 1 m has volume $2 \times 1.5 \times 1 = 3,\text{m}^{3}$, which holds $3 \times 1000 = 3000,\text{L}$ of water.

Temperature Conversions

Formula

Expression

What it means

Celsius to Fahrenheit

$F = \frac{9}{5}C + 32$

Multiply the Celsius reading $C$ by 1.8 and then add 32 to get the Fahrenheit reading $F$.

Fahrenheit to Celsius

$C = \frac{5}{9}(F - 32)$

Subtract 32 from the Fahrenheit reading first, then multiply the result by $\frac{5}{9}$.

Celsius to Kelvin

$K = C + 273.15$

Add 273.15 to the Celsius reading. Kelvin is written without a degree sign, and 0 K is absolute zero.

Kelvin to Celsius

$C = K - 273.15$

Subtract 273.15 from the kelvin value. Many school problems round this constant to 273.

Kelvin to Fahrenheit

$F = \frac{9}{5}(K - 273.15) + 32$

Changes kelvin to Celsius and then Celsius to Fahrenheit in a single step.

Fahrenheit to Kelvin

$K = \frac{5}{9}(F - 32) + 273.15$

Changes Fahrenheit to Celsius and then adds 273.15 to reach the kelvin value.

Temperature change

$\Delta F = \frac{9}{5}\Delta C$ and $\Delta K = \Delta C$

For a difference in temperature, do not add 32 or 273.15. A rise of 10 degrees Celsius is a rise of 18 degrees Fahrenheit.

Equal reading

$-40^{\circ}\text{C} = -40^{\circ}\text{F}$

The only temperature at which the Celsius and Fahrenheit scales show the same number.

Example: Normal body temperature of $37^{\circ}\text{C}$ is $\frac{9}{5} \times 37 + 32 = 66.6 + 32 = 98.6^{\circ}\text{F}$.

Time Conversions

Formula

Expression

What it means

Minute to seconds

$1,\text{min} = 60,\text{s}$

Multiply minutes by 60 to get seconds, and divide seconds by 60 to get minutes.

Hour to seconds

$1,\text{h} = 60,\text{min} = 3600,\text{s}$

Multiply hours by 3600 to get seconds. This factor is used when changing km/h into m/s.

Day

$1,\text{day} = 24,\text{h} = 1440,\text{min} = 86400,\text{s}$

The standard lengths used to change days into hours, minutes or seconds.

Week

$1,\text{week} = 7,\text{days} = 168,\text{h}$

Multiply weeks by 7 to get days, or by 168 to get hours.

Year

$1,\text{year} = 365,\text{days} = 52,\text{weeks} + 1,\text{day}$

A common year. A leap year has 366 days, which is 52 weeks and 2 days.

Leap year rule

$4 \mid y$, except when $100 \mid y$ and $400 \nmid y$

Year $y$ is a leap year if divisible by 4, but a century year must also be divisible by 400. So 2000 was a leap year and 1900 was not.

Decimal hours to minutes

$\text{Minutes} = \text{decimal part} \times 60$

Changes a time such as 2.75 hours into hours and minutes. The fractional part times 60 gives the minutes.

12-hour to 24-hour clock

$H_{24} = H_{12} + 12$

Add 12 to the hour for times from 1 pm to 11 pm. 12 am becomes 00 and 12 pm stays 12.

Angle between clock hands

$\theta = \lvert 30H - 5.5M \rvert$

Angle in degrees at $H$ hours and $M$ minutes, with $H$ read on a 12-hour clock. If the result is more than $180^{\circ}$, the smaller angle is $360^{\circ} - \theta$.

Example: A time of 2.75 hours is 2 hours and $0.75 \times 60 = 45$ minutes, which is $165 \times 60 = 9900$ seconds.

Algebra Formulas

This branch covers identities, exponents, surds, logarithms, straight lines, inequalities, quadratics, polynomials, variation, exponential change and functions. Students need it from Grade 7 onward, and it is the base for board exams, the SAT and JEE.

Algebraic Identities

Each identity below is true for every real value of $a$, $b$, $c$ and $x$.

Formula

Expression

What it means

Square of a sum (a + b whole square)

$(a+b)^{2} = a^{2} + 2ab + b^{2}$

The square of a sum equals both squares plus twice their product. Use it to expand brackets or square numbers like 103 mentally.

Square of a difference

$(a-b)^{2} = a^{2} - 2ab + b^{2}$

The square of a difference equals both squares minus twice their product. Handy for squares such as 98 or $(x-5)^{2}$.

Difference of squares

$a^{2} - b^{2} = (a+b)(a-b)$

A difference of two perfect squares always factors into their sum times their difference. Used in factoring and quick products like $51 \times 49$.

a square plus b square

$a^{2} + b^{2} = (a+b)^{2} - 2ab = (a-b)^{2} + 2ab$

Rewrites a sum of two squares using the sum or difference and the product. Use it when $a + b$ or $a - b$ and $ab$ are given.

Sum of the two binomial squares

$(a+b)^{2} + (a-b)^{2} = 2(a^{2} + b^{2})$

Adding the square of the sum and the square of the difference cancels the $2ab$ terms and doubles the squares.

Difference of the two binomial squares

$(a+b)^{2} - (a-b)^{2} = 4ab$

Subtracting the two squares leaves four times the product. Use it to find $ab$ from a known sum and difference.

Product with a common first term

$(x+a)(x+b) = x^{2} + (a+b)x + ab$

Multiplies two binomials that share $x$. The middle coefficient is the sum of $a$ and $b$ and the constant is their product.

Product of three binomials with a common term

$(x+a)(x+b)(x+c) = x^{3} + (a+b+c)x^{2} + (ab+bc+ca)x + abc$

Expands three brackets that share $x$. The coefficients are the sum, the sum of pairwise products and the product of $a$, $b$, $c$.

Cube of a sum

$(a+b)^{3} = a^{3} + 3a^{2}b + 3ab^{2} + b^{3} = a^{3} + b^{3} + 3ab(a+b)$

Cubes a binomial with coefficients 1, 3, 3, 1. The shorter second form is faster when $a + b$ and $ab$ are known.

Cube of a difference

$(a-b)^{3} = a^{3} - 3a^{2}b + 3ab^{2} - b^{3} = a^{3} - b^{3} - 3ab(a-b)$

Cubes a difference. The signs alternate, starting with plus, and the coefficients stay 1, 3, 3, 1.

a cube plus b cube

$a^{3} + b^{3} = (a+b)(a^{2} - ab + b^{2})$

Factors a sum of two cubes. The linear factor keeps the plus sign and the middle term of the quadratic factor is negative.

a cube minus b cube

$a^{3} - b^{3} = (a-b)(a^{2} + ab + b^{2})$

Factors a difference of two cubes. The linear factor has the minus sign and every term of the quadratic factor is positive.

Square of a trinomial

$(a+b+c)^{2} = a^{2} + b^{2} + c^{2} + 2ab + 2bc + 2ca$

The square of three terms is the sum of their squares plus twice each pairwise product.

a square plus b square plus c square

$a^{2} + b^{2} + c^{2} = (a+b+c)^{2} - 2(ab + bc + ca)$

Finds the sum of three squares when the total $a + b + c$ and the sum of pairwise products are known.

Sum of three cubes identity

$a^{3} + b^{3} + c^{3} - 3abc = (a+b+c)(a^{2} + b^{2} + c^{2} - ab - bc - ca)$

Factors this symmetric cubic expression into the sum of the terms times a quadratic factor. Common in Class 9 and JEE problems.

Three cubes with zero sum

$a^{3} + b^{3} + c^{3} = 3abc$ when $a + b + c = 0$

A special case of the previous identity. When the three numbers add to zero, the left factor vanishes.

Example: If $a + b = 7$ and $ab = 12$, then $a^{2} + b^{2} = 7^{2} - 2(12) = 49 - 24 = 25$.

Laws Of Exponents

Formula

Expression

What it means

Product rule

$a^{m} \cdot a^{n} = a^{m+n}$

When powers with the same base $a$ are multiplied, keep the base and add the exponents $m$ and $n$.

Quotient rule

$\frac{a^{m}}{a^{n}} = a^{m-n}$

When powers with the same nonzero base are divided, keep the base and subtract the bottom exponent from the top one. Needs $a \neq 0$.

Power of a power rule

$(a^{m})^{n} = a^{mn}$

Raising a power to another power multiplies the exponents. Do not confuse it with the product rule, which adds them.

Power of a product

$(ab)^{n} = a^{n}b^{n}$

An exponent outside brackets applies to every factor inside. It does not spread over addition, since $(a+b)^{2} \neq a^{2} + b^{2}$.

Power of a quotient

$\left(\frac{a}{b}\right)^{n} = \frac{a^{n}}{b^{n}}$

The exponent applies to both the numerator and the denominator. The denominator $b$ must be nonzero.

Zero exponent

$a^{0} = 1$

Any nonzero base raised to zero equals 1. The expression $0^{0}$ is left undefined in school algebra.

Negative exponent

$a^{-n} = \frac{1}{a^{n}}$

A negative exponent means the reciprocal of the positive power. The base $a$ must be nonzero.

Negative exponent of a fraction

$\left(\frac{a}{b}\right)^{-n} = \left(\frac{b}{a}\right)^{n}$

Flip the fraction and make the exponent positive. Both $a$ and $b$ must be nonzero.

Fractional exponent

$a^{\frac{1}{n}} = \sqrt[n]{a}$

An exponent of $\frac{1}{n}$ means the $n$th root. For even $n$ the base must satisfy $a \geq 0$ to give a real answer.

Rational exponent

$a^{\frac{m}{n}} = \sqrt[n]{a^{m}} = (\sqrt[n]{a})^{m}$

The denominator $n$ is the root and the numerator $m$ is the power. Taking the root first keeps the numbers small. Use $a > 0$.

Equal powers of the same base

$a^{m} = a^{n}$ implies $m = n$

For a base with $a > 0$ and $a \neq 1$, equal powers force equal exponents. This is how simple exponential equations are solved.

Example: $8^{\frac{2}{3}} \times 2^{-1} = (\sqrt[3]{8})^{2} \times \frac{1}{2} = 4 \times \frac{1}{2} = 2$.

Radicals And Surds

For even roots the rules below need the numbers under the root to be non-negative, and any denominator must be nonzero.

Formula

Expression

What it means

Definition of the nth root

$\sqrt[n]{a} = b$ means $b^{n} = a$

The $n$th root of $a$ is the number whose $n$th power is $a$. For even $n$ it is the non-negative root, with $a \geq 0$.

Square root of a square

$\sqrt{a^{2}} = \lvert a \rvert$

The square root of a square is the absolute value, not $a$ itself. For example, $\sqrt{(-3)^{2}} = 3$.

Product rule for roots

$\sqrt{a} \cdot \sqrt{b} = \sqrt{ab}$

Multiply the numbers under two square roots. Valid for $a \geq 0$ and $b \geq 0$.

Quotient rule for roots

$\frac{\sqrt{a}}{\sqrt{b}} = \sqrt{\frac{a}{b}}$

Divide the numbers under two square roots. Valid for $a \geq 0$ and $b > 0$.

Product rule for nth roots

$\sqrt[n]{a} \cdot \sqrt[n]{b} = \sqrt[n]{ab}$

Roots of the same order combine under one root sign. For even $n$, both $a$ and $b$ must be non-negative.

Root of a root

$\sqrt[m]{\sqrt[n]{a}} = \sqrt[mn]{a}$

Taking an $n$th root and then an $m$th root equals one root of order $mn$. For example, $\sqrt{\sqrt{16}} = \sqrt[4]{16} = 2$.

Simplifying a surd

$\sqrt{a^{2}b} = a\sqrt{b}$

Take a perfect-square factor $a^{2}$ out of the root, as in $\sqrt{72} = 6\sqrt{2}$. Needs $a \geq 0$ and $b \geq 0$.

Adding like surds

$p\sqrt{a} + q\sqrt{a} = (p+q)\sqrt{a}$

Only surds with the same number under the root combine. In general $\sqrt{a} + \sqrt{b} \neq \sqrt{a+b}$.

Rationalising a single surd

$\frac{1}{\sqrt{a}} = \frac{\sqrt{a}}{a}$

Multiply top and bottom by $\sqrt{a}$ to clear the root from the denominator. Needs $a > 0$.

Rationalising with the conjugate

$\frac{1}{\sqrt{a} + \sqrt{b}} = \frac{\sqrt{a} - \sqrt{b}}{a - b}$

Multiply by the conjugate $\sqrt{a} - \sqrt{b}$ so the denominator becomes a difference of squares. Needs $a, b \geq 0$ and $a \neq b$.

Rationalising a binomial surd

$\frac{1}{p + \sqrt{q}} = \frac{p - \sqrt{q}}{p^{2} - q}$

Same conjugate method when one term is rational. Here $q > 0$ and $p^{2} \neq q$.

Square root of a binomial surd

$\sqrt{a + b + 2\sqrt{ab}} = \sqrt{a} + \sqrt{b}$

Recognises a perfect square hidden under a root, as in $\sqrt{5 + 2\sqrt{6}} = \sqrt{3} + \sqrt{2}$. Needs $a, b \geq 0$.

Example: $\frac{1}{\sqrt{5} + \sqrt{2}} = \frac{\sqrt{5} - \sqrt{2}}{5 - 2} = \frac{\sqrt{5} - \sqrt{2}}{3} \approx \frac{2.2361 - 1.4142}{3} \approx 0.2740$.

Logarithms

Formula

Expression

What it means

Log to exponential form

$\log_{b} x = y$ means $b^{y} = x$

A logarithm is the exponent $y$ that turns base $b$ into $x$. Needs $b > 0$, $b \neq 1$ and argument $x > 0$.

Product rule

$\log_{b}(MN) = \log_{b} M + \log_{b} N$

The log of a product is the sum of the logs. Valid for $M > 0$, $N > 0$, $b > 0$ and $b \neq 1$.

Quotient rule

$\log_{b}\left(\frac{M}{N}\right) = \log_{b} M - \log_{b} N$

The log of a quotient is the log of the top minus the log of the bottom. Needs $M > 0$ and $N > 0$.

Power rule

$\log_{b}(M^{p}) = p\log_{b} M$

An exponent inside a log comes out as a multiplier. Valid for $M > 0$ and any real $p$.

Change of base

$\log_{b} M = \frac{\log_{k} M}{\log_{k} b}$

Converts a log to any new base $k$ with $k > 0$ and $k \neq 1$. Use base 10 or $e$ to evaluate on a calculator.

Reciprocal rule

$\log_{b} a = \frac{1}{\log_{a} b}$

Swapping the base and the argument gives the reciprocal. Needs $a, b > 0$ with $a \neq 1$ and $b \neq 1$.

Chain rule for bases

$\log_{a} b \cdot \log_{b} c = \log_{a} c$

The middle base cancels, like a chain of unit conversions. All bases must be positive and not equal to 1, and $c > 0$.

Power of the base

$\log_{b^{q}} M = \frac{1}{q}\log_{b} M$

A power on the base divides the log. Here $q \neq 0$ and $b^{q} \neq 1$. For example, $\log_{4} M = \frac{1}{2}\log_{2} M$.

Log of the base

$\log_{b} b = 1$

Any valid base raised to the power 1 is itself, so the log of the base is 1. For example, $\log_{10} 10 = 1$.

Log of one

$\log_{b} 1 = 0$

Any valid base raised to zero is 1, so the log of 1 is zero in every base.

Inverse properties

$b^{\log_{b} x} = x$ and $\log_{b}(b^{x}) = x$

Exponentials and logs of the same base undo each other. The first form needs $x > 0$, the second holds for all real $x$.

Exchange rule

$a^{\log_{b} c} = c^{\log_{b} a}$

The base-$a$ and the argument-$c$ positions can be swapped. Needs $a > 0$, $c > 0$, $b > 0$ and $b \neq 1$.

Common and natural logs

$\log x = \log_{10} x$ and $\ln x = \log_{e} x$

In school work, $\log$ with no base means base 10 and $\ln$ means base $e \approx 2.71828$. Both need $x > 0$.

Converting ln to log

$\ln x = \ln 10 \cdot \log_{10} x \approx 2.3026\log_{10} x$

A special case of change of base. Useful values are $\log_{10} 2 \approx 0.3010$ and $\log_{10} 3 \approx 0.4771$.

Example: $\log_{2} 80 = \log_{2}(16 \times 5) = \log_{2} 16 + \log_{2} 5 = 4 + \frac{\ln 5}{\ln 2} \approx 4 + 2.3219 = 6.3219$.

Linear Equations And Straight Lines

Formula

Expression

What it means

Linear equation in one variable

$ax + b = 0$ gives $x = -\frac{b}{a}$

A first-degree equation in one unknown has exactly one solution when the coefficient $a \neq 0$.

Slope formula

$m = \frac{y_{2} - y_{1}}{x_{2} - x_{1}}$

Slope $m$ is rise over run between points $(x_{1}, y_{1})$ and $(x_{2}, y_{2})$. Needs $x_{1} \neq x_{2}$, since a vertical line has undefined slope.

Slope from an angle

$m = \tan\theta$

$\theta$ is the angle the line makes with the positive $x$-axis, measured anticlockwise. Not defined when $\theta = 90^{\circ}$.

Slope intercept form

$y = mx + c$

$m$ is the slope and $c$ is the $y$-intercept. US textbooks write the same form as $y = mx + b$.

Point slope form

$y - y_{1} = m(x - x_{1})$

The line through the point $(x_{1}, y_{1})$ with slope $m$. Use it when one point and the slope are known.

Two-point form

$y - y_{1} = \frac{y_{2} - y_{1}}{x_{2} - x_{1}}(x - x_{1})$

The line through two known points. It is point-slope form with the slope formula substituted. Needs $x_{1} \neq x_{2}$.

Intercept form

$\frac{x}{a} + \frac{y}{b} = 1$

The line cutting the $x$-axis at $(a, 0)$ and the $y$-axis at $(0, b)$. Needs $a \neq 0$ and $b \neq 0$.

Standard form of linear equations

$Ax + By = C$

$A$, $B$, $C$ are constants with $A$ and $B$ not both zero. The slope is $-\frac{A}{B}$ when $B \neq 0$.

General form

$ax + by + c = 0$

The form used in Indian textbooks. Its slope is $-\frac{a}{b}$ and its $y$-intercept is $-\frac{c}{b}$, both needing $b \neq 0$.

X and y intercepts

$x = \frac{C}{A}$ and $y = \frac{C}{B}$ for $Ax + By = C$

Set $y = 0$ to find where the line meets the $x$-axis and $x = 0$ for the $y$-axis. Needs $A \neq 0$ and $B \neq 0$.

Slope of parallel lines

$m_{1} = m_{2}$

Two non-vertical lines are parallel exactly when their slopes are equal. All vertical lines are parallel to each other.

Slope of perpendicular lines

$m_{1} \cdot m_{2} = -1$

Two lines, neither vertical, are perpendicular when the product of slopes is $-1$, so $m_{2} = -\frac{1}{m_{1}}$.

Horizontal and vertical lines

$y = k$ and $x = h$

$y = k$ is parallel to the $x$-axis with slope 0. $x = h$ is parallel to the $y$-axis with undefined slope.

Unique solution test for two lines

$\frac{a_{1}}{a_{2}} \neq \frac{b_{1}}{b_{2}}$

For $a_{1}x + b_{1}y + c_{1} = 0$ and $a_{2}x + b_{2}y + c_{2} = 0$, the lines meet at exactly one point.

Parallel or coincident lines test

$\frac{a_{1}}{a_{2}} = \frac{b_{1}}{b_{2}}$

If this common ratio differs from $\frac{c_{1}}{c_{2}}$ the lines are parallel with no solution. If it equals $\frac{c_{1}}{c_{2}}$ there are infinitely many solutions.

Example: The line through $(1, 2)$ and $(3, 8)$ has $m = \frac{8 - 2}{3 - 1} = 3$, so $y - 2 = 3(x - 1)$, which simplifies to $y = 3x - 1$.

Linear Inequalities And Absolute Value

Multiplying or dividing both sides of an inequality by a negative number reverses the sign, and forgetting this causes most errors here.

Formula

Expression

What it means

Addition property

If $a < b$, then $a + c < b + c$

Adding or subtracting the same real number $c$ on both sides keeps the direction of the inequality.

Multiplying by a positive number

If $a < b$ and $c > 0$, then $ac < bc$

Multiplying or dividing both sides by a positive number keeps the direction of the inequality.

Multiplying by a negative number

If $a < b$ and $c < 0$, then $ac > bc$

Multiplying or dividing both sides by a negative number flips the inequality sign.

Reciprocal property

If $0 < a < b$, then $\frac{1}{a} > \frac{1}{b}$

Taking reciprocals of two positive numbers reverses the order. It also holds when both are negative, but not across zero.

Transitive property

If $a < b$ and $b < c$, then $a < c$

Inequalities in the same direction chain together. Used to join steps and to write compound inequalities.

Absolute value

$\lvert x \rvert = x$ if $x \geq 0$, and $\lvert x \rvert = -x$ if $x < 0$

The absolute value is the distance of $x$ from zero on the number line, so it is never negative.

Product and quotient of absolute values

$\lvert ab \rvert = \lvert a \rvert \lvert b \rvert$ and $\left\lvert \frac{a}{b} \right\rvert = \frac{\lvert a \rvert}{\lvert b \rvert}$

Absolute value splits over multiplication and division. The quotient form needs $b \neq 0$.

Absolute value equation

$\lvert x \rvert = a$ gives $x = \pm a$

For $a > 0$ there are two solutions, for $a = 0$ only $x = 0$, and for $a < 0$ there is no solution.

Less-than absolute inequality

$\lvert x \rvert < a$ is equivalent to $-a < x < a$

For $a > 0$, the solutions lie within $a$ units of zero, giving one bounded interval. No solution if $a \leq 0$.

Greater-than absolute inequality

$\lvert x \rvert > a$ is equivalent to $x < -a$ or $x > a$

For $a \geq 0$, the solutions lie more than $a$ units from zero, giving two separate rays.

Shifted absolute inequality

$\lvert x - h \rvert < a$ is equivalent to $h - a < x < h + a$

For $a > 0$, $x$ is within distance $a$ of the centre $h$. Use it for tolerance and error-bound problems.

Triangle inequality

$\lvert a + b \rvert \leq \lvert a \rvert + \lvert b \rvert$

The size of a sum never exceeds the sum of the sizes. Equality holds when $a$ and $b$ have the same sign or one is zero.

Reverse triangle inequality

$\lvert \lvert a \rvert - \lvert b \rvert \rvert \leq \lvert a - b \rvert$

The gap between two sizes is at most the distance between the numbers. Used to find lower bounds.

Example: To solve $\lvert 2x - 3 \rvert < 5$, write $-5 < 2x - 3 < 5$, then $-2 < 2x < 8$, which gives $-1 < x < 4$.

Quadratic Equations

Every row assumes the standard form below with real coefficients and $a \neq 0$. The roots are written $\alpha$ and $\beta$.

Formula

Expression

What it means

Standard form of a quadratic equation

$ax^{2} + bx + c = 0$

A second-degree equation in $x$ with constants $a$, $b$, $c$. If $a = 0$ it becomes linear, so $a \neq 0$ is required.

Quadratic formula

$x = \frac{-b \pm \sqrt{b^{2} - 4ac}}{2a}$

Gives both roots of any quadratic directly. Use it when the quadratic does not factor easily.

Discriminant

$D = b^{2} - 4ac$

The expression under the square root in the quadratic formula. Its sign tells you the nature of the roots before solving. Also written $\Delta$.

Two distinct real roots

$D > 0$

The parabola crosses the $x$-axis twice. If $a$, $b$, $c$ are rational and $D$ is a perfect square, both roots are rational.

Two equal real roots

$D = 0$ gives $x = -\frac{b}{2a}$

The quadratic is a perfect square and the parabola touches the $x$-axis at its vertex.

No real roots

$D < 0$

The parabola does not meet the $x$-axis. The two roots are complex conjugates $\frac{-b \pm i\sqrt{-D}}{2a}$.

Sum of roots

$\alpha + \beta = -\frac{b}{a}$

The two roots add to minus the $x$ coefficient divided by the $x^{2}$ coefficient. Holds for real and complex roots.

Product of roots

$\alpha\beta = \frac{c}{a}$

The two roots multiply to the constant term divided by the $x^{2}$ coefficient.

Difference of roots

$\lvert \alpha - \beta \rvert = \frac{\sqrt{D}}{\lvert a \rvert}$

The distance between two real roots, found without solving. Needs $D \geq 0$.

Quadratic from its roots

$x^{2} - (\alpha + \beta)x + \alpha\beta = 0$

Builds a quadratic with given roots from their sum and product. Multiply through by any nonzero constant to clear fractions.

Factored form

$ax^{2} + bx + c = a(x - \alpha)(x - \beta)$

Any quadratic can be written using its leading coefficient and its two roots. Links roots to $x$-intercepts.

Vertex of a parabola

$\left(-\frac{b}{2a}, -\frac{D}{4a}\right)$

The turning point of $y = ax^{2} + bx + c$. The $y$-value equals $c - \frac{b^{2}}{4a}$, the minimum if $a > 0$ and the maximum if $a < 0$.

Axis of symmetry

$x = -\frac{b}{2a}$

The vertical line through the vertex that splits the parabola into mirror halves. It lies midway between the two roots.

Vertex form

$y = a(x - h)^{2} + k$

$(h, k)$ is the vertex. The parabola opens up when $a > 0$ and down when $a < 0$.

Completing the square

$ax^{2} + bx + c = a\left(x + \frac{b}{2a}\right)^{2} - \frac{b^{2} - 4ac}{4a}$

Rewrites a quadratic in vertex form. It is the step that derives the quadratic formula and finds the vertex.

Example: For $2x^{2} - 7x + 3 = 0$, $D = 49 - 24 = 25$, so $x = \frac{7 \pm 5}{4}$, giving $x = 3$ or $x = \frac{1}{2}$.

Polynomials

Formula

Expression

What it means

General polynomial

$p(x) = a_{n}x^{n} + a_{n-1}x^{n-1} + \dots + a_{1}x + a_{0}$

A polynomial of degree $n$ with constant coefficients $a_{0}$ to $a_{n}$ and leading coefficient $a_{n} \neq 0$.

Division algorithm

$p(x) = g(x) \cdot q(x) + r(x)$

Dividing $p(x)$ by a nonzero $g(x)$ gives quotient $q(x)$ and remainder $r(x)$, where $r(x) = 0$ or its degree is less than that of $g(x)$.

Remainder theorem

Remainder of $p(x) \div (x - a)$ is $p(a)$

Substitute $x = a$ to find the remainder without long division. For a divisor $ax - b$ with $a \neq 0$, the remainder is $p\left(\frac{b}{a}\right)$.

Factor theorem

$(x - a)$ is a factor of $p(x)$ if and only if $p(a) = 0$

A value that makes the polynomial zero gives a linear factor. Use it to find the first factor of a cubic.

Rational root theorem

$x = \frac{p}{q}$ with $p \mid a_{0}$ and $q \mid a_{n}$

Any rational root in lowest terms has numerator dividing the constant term and denominator dividing the leading coefficient. Needs integer coefficients.

Sum of coefficients

$p(1) = a_{n} + a_{n-1} + \dots + a_{0}$

Substituting $x = 1$ adds all coefficients. If the sum is zero, then $x - 1$ is a factor.

Sum of roots of a cubic

$\alpha + \beta + \gamma = -\frac{b}{a}$

For $ax^{3} + bx^{2} + cx + d = 0$ with $a \neq 0$, the three roots add to minus $b$ over $a$.

Sum of pairwise products for a cubic

$\alpha\beta + \beta\gamma + \gamma\alpha = \frac{c}{a}$

For the same cubic, the products of the roots taken two at a time add to $c$ over $a$.

Product of roots of a cubic

$\alpha\beta\gamma = -\frac{d}{a}$

For the same cubic, the three roots multiply to minus the constant term over the leading coefficient.

Cubic from its roots

$x^{3} - (\alpha + \beta + \gamma)x^{2} + (\alpha\beta + \beta\gamma + \gamma\alpha)x - \alpha\beta\gamma = 0$

Builds a monic cubic with roots $\alpha$, $\beta$, $\gamma$. The signs alternate minus, plus, minus.

Roots of a degree n polynomial

Sum $= -\frac{a_{n-1}}{a_{n}}$ and product $= (-1)^{n}\frac{a_{0}}{a_{n}}$

Extends the quadratic and cubic relations to any degree $n$, counting complex and repeated roots.

Number of roots

Exactly $n$ roots in the complex numbers

A degree $n$ polynomial has $n$ roots counted with multiplicity, so at most $n$ real roots. Non-real roots of real polynomials come in conjugate pairs.

Example: For $p(x) = x^{3} - 4x^{2} + x + 6$, $p(2) = 8 - 16 + 2 + 6 = 0$, so $x - 2$ is a factor and the remainder on dividing by $x - 2$ is 0.

Direct, Inverse And Joint Variation

Formula

Expression

What it means

Direct variation

$y = kx$

$y$ varies directly as $x$ with a nonzero constant $k$. The ratio $\frac{y}{x}$ stays fixed and the graph is a line through the origin.

Direct variation between two pairs

$\frac{y_{1}}{x_{1}} = \frac{y_{2}}{x_{2}}$

Solves a direct variation problem without finding $k$. Both $x$ values must be nonzero.

Direct variation with a power

$y = kx^{n}$

$y$ varies as the $n$th power of $x$, as when the area of a circle varies as the square of its radius.

Inverse variation

$y = \frac{k}{x}$

$y$ varies inversely as $x$ with $k \neq 0$ and $x \neq 0$. The product $xy = k$ stays fixed and one grows as the other shrinks.

Inverse variation between two pairs

$x_{1}y_{1} = x_{2}y_{2}$

Solves an inverse variation problem, such as workers and days, without finding $k$ first.

Inverse square variation

$y = \frac{k}{x^{2}}$

$y$ varies inversely as the square of $x$. Doubling $x$ makes $y$ one quarter. Used for light intensity and gravity.

Joint variation

$z = kxy$

$z$ varies directly as the product of $x$ and $y$, with a nonzero constant $k$.

Combined variation

$z = \frac{kx}{y}$

$z$ varies directly as $x$ and inversely as $y$, with $k \neq 0$ and $y \neq 0$.

Example: If $y$ varies inversely as $x$ and $y = 12$ when $x = 3$, then $k = 36$, so when $x = 9$, $y = \frac{36}{9} = 4$.

Exponential Growth And Decay

Formula

Expression

What it means

Exponential function

$f(x) = a \cdot b^{x}$

$a \neq 0$ is the starting value and $b$ is the growth factor, with $b > 0$ and $b \neq 1$. Growth if $b > 1$, decay if $0 < b < 1$.

Growth at a fixed percent

$A = P(1 + r)^{t}$

$P$ grows by rate $r$, written as a decimal, for each of $t$ periods. Used for population and investment growth.

Decay at a fixed percent

$A = P(1 - r)^{t}$

$P$ shrinks by rate $r$ per period, with $0 < r < 1$. Used for falling values such as a car's price.

Continuous growth or decay

$A = Pe^{kt}$

$e \approx 2.71828$ and $k$ is the continuous rate per unit time. $k > 0$ gives growth and $k < 0$ gives decay.

Half-life form

$N = N_{0}\left(\frac{1}{2}\right)^{\frac{t}{T}}$

$N_{0}$ is the starting amount and $T$ is the half-life. After each interval $T$ the amount halves.

Half-life from a decay constant

$T = \frac{\ln 2}{k}$

For $N = N_{0}e^{-kt}$ with $k > 0$, this is the time to halve. Note $\ln 2 \approx 0.6931$.

Doubling time form

$N = N_{0} \cdot 2^{\frac{t}{T_{d}}}$

$T_{d}$ is the doubling time. The quantity doubles after every interval of length $T_{d}$.

Doubling time for continuous growth

$T_{d} = \frac{\ln 2}{k}$

For $N = N_{0}e^{kt}$ with $k > 0$, this is the time for the quantity to double.

Doubling time for percent growth

$T_{d} = \frac{\ln 2}{\ln(1 + r)}$

The exact number of periods to double at rate $r$ per period, with $r > 0$ written as a decimal.

Rule of 70

$T_{d} \approx \frac{70}{R}$

A quick estimate of doubling time when $R$ is the percent growth rate per period. Accurate for small rates.

Time to reach a value

$t = \frac{1}{k}\ln\left(\frac{A}{P}\right)$

Solves $A = Pe^{kt}$ for time. Needs $A > 0$, $P > 0$ and $k \neq 0$.

Example: A sample of 80 g with a half-life of 5 years leaves $N = 80\left(\frac{1}{2}\right)^{\frac{15}{5}} = 80 \times \frac{1}{8} = 10,\text{g}$ after 15 years.

Functions

Formula

Expression

What it means

Composition of functions

$(f \circ g)(x) = f(g(x))$

Apply $g$ first, then $f$. The input $x$ must be in the domain of $g$ and $g(x)$ in the domain of $f$.

Order matters in composition

$f \circ g \neq g \circ f$ in general

Changing the order of two functions usually changes the result, so always work from the inside out.

Composition is associative

$(f \circ g) \circ h = f \circ (g \circ h)$

Grouping does not matter for three functions applied in a fixed order, which is $h$, then $g$, then $f$.

Inverse functions

$f(f^{-1}(x)) = x$ and $f^{-1}(f(x)) = x$

$f^{-1}$ undoes $f$. It exists only when $f$ is one-to-one, and $f^{-1}(x)$ is not the same as $\frac{1}{f(x)}$.

Finding an inverse

$y = f(x)$, solve for $x$, then swap $x$ and $y$

The standard method to get $f^{-1}(x)$. The domain of $f^{-1}$ is the range of $f$.

Inverse of a linear function

$f(x) = ax + b$ gives $f^{-1}(x) = \frac{x - b}{a}$

Undo the operations in reverse order, subtract $b$ and then divide by $a$. Needs $a \neq 0$.

Inverse of a composition

$(f \circ g)^{-1} = g^{-1} \circ f^{-1}$

To undo $g$ then $f$, undo $f$ first and then $g$. Both functions must be invertible.

Graph of an inverse

Point $(a, b)$ on $f$ gives $(b, a)$ on $f^{-1}$

The graph of $f^{-1}$ is the reflection of the graph of $f$ in the line $y = x$.

Even function test

$f(-x) = f(x)$

A function is even if this holds for every $x$ in its domain. Its graph is symmetric about the $y$-axis, like $x^{2}$ or $\cos x$.

Odd function test

$f(-x) = -f(x)$

A function is odd if this holds for every $x$ in its domain. Its graph has symmetry about the origin, like $x^{3}$ or $\sin x$.

Products of even and odd functions

even times even is even, odd times odd is even, even times odd is odd

Combine these rules to test products quickly. Sums of two even functions are even and sums of two odd functions are odd.

Even and odd parts

$f(x) = \frac{f(x) + f(-x)}{2} + \frac{f(x) - f(-x)}{2}$

Any function on a domain symmetric about zero splits into an even part plus an odd part.

Graph transformations

$y = a \cdot f(x - h) + k$

Shifts the graph of $f$ right by $h$ and up by $k$, and stretches it vertically by a factor of $\lvert a \rvert$. A negative $a$ reflects it in the $x$-axis.

Average rate of change

$\frac{f(b) - f(a)}{b - a}$

The slope of the line joining $(a, f(a))$ and $(b, f(b))$ on the graph. Needs $a \neq b$.

Example: If $f(x) = 2x + 3$ and $g(x) = x^{2}$, then $(f \circ g)(3) = f(9) = 21$, while $(g \circ f)(3) = g(9) = 81$.

Advanced Algebra Formulas: Sequences, Counting, Complex Numbers And Matrices

This branch covers progressions, special sums, the binomial theorem, permutations and combinations, complex numbers, matrices and determinants, sets, and logic. It is core material for Grade 11 and 12, JEE, SAT Math Level 2 and A-level students.

Arithmetic Progression (AP)

Formula

Expression

What it means

Common difference

$d = a_{n} - a_{n-1}$

The fixed amount added to each term to get the next one. A positive $d$ gives an increasing AP and a negative $d$ a decreasing one.

nth term of an arithmetic sequence

$a_{n} = a + (n-1)d$

Gives the term in position $n$, where $a$ is the first term, $d$ the common difference and $n$ a positive integer.

nth term from the end

$l - (n-1)d$

Counts backwards from the last term $l$ of a finite AP to find the term in position $n$ from the end.

Number of terms

$n = \frac{l - a}{d} + 1$

Finds how many terms a finite AP has when you know the first term $a$, last term $l$ and common difference $d \neq 0$.

Sum of first n terms

$S_{n} = \frac{n}{2}[2a + (n-1)d]$

Adds the first $n$ terms of an AP using the first term $a$ and common difference $d$.

Sum using the last term

$S_{n} = \frac{n}{2}(a + l)$

The same sum written as the number of terms times the average of the first term $a$ and last term $l$.

nth term from the sums

$a_{n} = S_{n} - S_{n-1}$

Recovers any term from the sum formula for $n \geq 2$, with $a_{1} = S_{1}$. Works for any sequence, not only an AP.

Arithmetic mean of two numbers

$A = \frac{a + b}{2}$

The single number that makes $a$, $A$, $b$ an AP. It is the midpoint of $a$ and $b$.

Condition for three terms in AP

$2b = a + c$

Three numbers $a$, $b$, $c$ are in AP exactly when twice the middle one equals the sum of the outer two.

Inserting n arithmetic means

$d = \frac{b - a}{n + 1}$

Common difference needed to place $n$ equally spaced numbers between $a$ and $b$, giving $n + 2$ terms in total.

Convenient choice of terms

$a - d,\ a,\ a + d$ or $a - 3d,\ a - d,\ a + d,\ a + 3d$

Symmetric choices for three or four unknown terms in AP, used when their sum is given so that $d$ cancels.

Example: For the AP 3, 7, 11, and so on, $a = 3$ and $d = 4$, so $a_{20} = 3 + 19 \times 4 = 79$ and $S_{20} = \frac{20}{2}(3 + 79) = 820$.

Geometric Progression (GP)

Formula

Expression

What it means

Common ratio

$r = \frac{a_{n}}{a_{n-1}}$

The fixed factor each term is multiplied by to get the next one. All terms of a GP are nonzero.

Nth term of a GP

$a_{n} = ar^{n-1}$

Gives the term in position $n$, where $a$ is the first term and $r$ the common ratio.

nth term from the end

$\frac{l}{r^{n-1}}$

Term in position $n$ counted backwards from the last term $l$ of a finite GP with common ratio $r$.

Sum of first n terms of a GP

$S_{n} = \frac{a(r^{n} - 1)}{r - 1}$

Adds the first $n$ terms when $r \neq 1$. The equal form $\frac{a(1 - r^{n})}{1 - r}$ is easier to use when $r < 1$.

Sum when the ratio is 1

$S_{n} = na$

If $r = 1$ every term equals $a$, so the sum of $n$ terms is simply $n$ times $a$.

Sum using the last term

$S_{n} = \frac{lr - a}{r - 1}$

Sum of a finite GP from its first term $a$, last term $l$ and ratio $r \neq 1$.

Sum of an infinite GP

$S_{\infty} = \frac{a}{1 - r}$

The value the partial sums approach. It exists only when $\lvert r \rvert < 1$, otherwise the series diverges.

Geometric mean of two numbers

$G = \sqrt{ab}$

For positive $a$ and $b$, the number that makes $a$, $G$, $b$ a GP.

Condition for three terms in GP

$b^{2} = ac$

Three nonzero numbers $a$, $b$, $c$ are in GP exactly when the square of the middle one equals the product of the outer two.

Inserting n geometric means

$r = \left(\frac{b}{a}\right)^{\frac{1}{n+1}}$

Common ratio needed to place $n$ numbers between positive $a$ and $b$ so that all $n + 2$ numbers form a GP.

Product of first n terms

$P_{n} = a^{n}r^{\frac{n(n-1)}{2}}$

Multiplies the first $n$ terms of a GP, since the powers of $r$ add up to $0 + 1 + \cdots + (n-1)$.

Convenient choice of terms

$\frac{a}{r},\ a,\ ar$

Symmetric choice for three unknown terms in GP, used when their product is given so that $r$ cancels.

Example: For the GP 2, 6, 18, and so on, $a = 2$ and $r = 3$, so $a_{6} = 2 \times 3^{5} = 486$ and $S_{6} = \frac{2(3^{6} - 1)}{3 - 1} = 728$.

Harmonic Progression And Means

All the mean results in this table assume the numbers are positive.

Formula

Expression

What it means

Harmonic progression

$\frac{1}{a_{1}}, \frac{1}{a_{2}}, \frac{1}{a_{3}}, \ldots$ form an AP

A sequence of nonzero numbers is an HP when the reciprocals of its terms are in arithmetic progression.

nth term of an HP

$a_{n} = \frac{1}{\frac{1}{a} + (n-1)d}$

Here $a$ is the first term and $d = \frac{1}{a_{2}} - \frac{1}{a_{1}}$ is the common difference of the reciprocals.

Harmonic mean of two numbers

$H = \frac{2ab}{a + b}$

The number that makes $a$, $H$, $b$ an HP. Used for average speed over two equal distances.

Harmonic mean of n numbers

$H = \frac{n}{\frac{1}{x_{1}} + \frac{1}{x_{2}} + \cdots + \frac{1}{x_{n}}}$

The count of values divided by the sum of their reciprocals. Suits averages of rates.

Condition for three terms in HP

$b = \frac{2ac}{a + c}$

Three nonzero numbers $a$, $b$, $c$ are in HP when the middle one is the harmonic mean of the outer two.

AM, GM, HM inequality

$A \geq G \geq H$

For any set of positive numbers, the arithmetic mean is at least the geometric mean, which is at least the harmonic mean. Equality holds only when all numbers are equal.

AM-GM for n numbers

$\frac{x_{1} + x_{2} + \cdots + x_{n}}{n} \geq \sqrt[n]{x_{1}x_{2}\cdots x_{n}}$

Standard tool for finding the minimum of a sum or the maximum of a product of positive quantities.

Link between the three means

$G^{2} = AH$

For two positive numbers, the square of the geometric mean equals the product of the arithmetic and harmonic means.

Numbers from their means

$x^{2} - 2Ax + G^{2} = 0$

The two numbers whose AM is $A$ and GM is $G$ are the roots of this quadratic.

Example: For $a = 4$ and $b = 16$, $A = 10$, $G = \sqrt{64} = 8$ and $H = \frac{2 \times 4 \times 16}{20} = 6.4$, and indeed $G^{2} = 64 = 10 \times 6.4$.

Special Sums And Sigma Notation

Formula

Expression

What it means

Sum of first n natural numbers

$\sum_{k=1}^{n} k = \frac{n(n+1)}{2}$

Adds $1 + 2 + \cdots + n$ for a positive integer $n$. It is the AP sum with $a = 1$ and $d = 1$.

Sum of squares

$\sum_{k=1}^{n} k^{2} = \frac{n(n+1)(2n+1)}{6}$

Adds $1^{2} + 2^{2} + \cdots + n^{2}$ for a positive integer $n$. Needed when summing any quadratic expression in $k$.

Sum of cubes

$\sum_{k=1}^{n} k^{3} = \left[\frac{n(n+1)}{2}\right]^{2}$

Adds $1^{3} + 2^{3} + \cdots + n^{3}$. The result is the square of the sum of the first $n$ natural numbers.

Sum of fourth powers

$\sum_{k=1}^{n} k^{4} = \frac{n(n+1)(2n+1)(3n^{2} + 3n - 1)}{30}$

Adds $1^{4} + 2^{4} + \cdots + n^{4}$. Used less often, mainly in JEE series questions.

Sum of first n odd numbers

$\sum_{k=1}^{n} (2k - 1) = n^{2}$

Adds $1 + 3 + 5 + \cdots + (2n - 1)$, the first $n$ odd numbers. The total is always a perfect square.

Sum of first n even numbers

$\sum_{k=1}^{n} 2k = n(n+1)$

Adds $2 + 4 + 6 + \cdots + 2n$, the first $n$ even numbers. It is twice the sum of the first $n$ natural numbers.

Sum of a constant

$\sum_{k=1}^{n} c = nc$

Adding the same number $c$ a total of $n$ times gives $n$ times $c$.

Linearity of sigma notation

$\sum_{k=1}^{n} (p,u_{k} + q,v_{k}) = p\sum_{k=1}^{n} u_{k} + q\sum_{k=1}^{n} v_{k}$

Constants $p$ and $q$ come out of a sum, and a sum of terms splits into separate sums. Used to sum any polynomial in $k$.

Telescoping sum

$\sum_{k=1}^{n} \frac{1}{k(k+1)} = \frac{n}{n+1}$

Write $\frac{1}{k(k+1)} = \frac{1}{k} - \frac{1}{k+1}$ so that middle terms cancel in pairs.

Infinite arithmetico-geometric series

$S_{\infty} = \frac{a}{1 - r} + \frac{dr}{(1 - r)^{2}}$

Sum of $a + (a + d)r + (a + 2d)r^{2} + \cdots$, where each AP term is multiplied by a GP term. Needs $\lvert r \rvert < 1$.

Example: $1^{2} + 2^{2} + \cdots + 10^{2} = \frac{10 \times 11 \times 21}{6} = 385$ and $1^{3} + 2^{3} + \cdots + 10^{3} = 55^{2} = 3025$.

Binomial Theorem

Here $n$ is a positive integer unless the row says otherwise.

Formula

Expression

What it means

Binomial theorem

$(a + b)^{n} = \sum_{r=0}^{n} \binom{n}{r} a^{n-r}b^{r}$

Expands a power of a two-term sum. The powers of $a$ fall from $n$ to 0 while the powers of $b$ rise from 0 to $n$.

General term

$T_{r+1} = \binom{n}{r} a^{n-r}b^{r}$

Gives the term in position $r + 1$ directly, for $0 \leq r \leq n$, without writing the full expansion.

Number of terms

$n + 1$

The expansion of $(a + b)^{n}$ always has one more term than the power $n$.

Middle term, n even

$T_{\frac{n}{2} + 1}$

When $n$ is even there is a single middle term, in position $\frac{n}{2} + 1$.

Middle terms, n odd

$T_{\frac{n+1}{2}}$ and $T_{\frac{n+3}{2}}$

When $n$ is odd there are two middle terms, in positions $\frac{n+1}{2}$ and $\frac{n+3}{2}$.

rth term from the end

$T_{n - r + 2}$

The term in position $r$ counted from the end is the term in position $n - r + 2$ counted from the start.

Sum of binomial coefficients

$\binom{n}{0} + \binom{n}{1} + \cdots + \binom{n}{n} = 2^{n}$

Found by putting $a = b = 1$. For any polynomial $p(x)$, the sum of its coefficients is $p(1)$.

Alternating sum of coefficients

$\binom{n}{0} - \binom{n}{1} + \binom{n}{2} - \cdots + (-1)^{n}\binom{n}{n} = 0$

Found by putting $a = 1$ and $b = -1$, valid for $n \geq 1$.

Even and odd position coefficients

$\binom{n}{0} + \binom{n}{2} + \cdots = \binom{n}{1} + \binom{n}{3} + \cdots = 2^{n-1}$

The coefficients in odd positions and in even positions each add up to half of $2^{n}$, for $n \geq 1$.

Greatest binomial coefficient

$\binom{n}{\frac{n}{2}}$ for even $n$, $\binom{n}{\frac{n-1}{2}} = \binom{n}{\frac{n+1}{2}}$ for odd $n$

The largest coefficient sits in the middle of the expansion.

Term independent of x

Set the power of $x$ in $T_{r+1}$ equal to 0

Solve for $r$, then substitute it into the general term to get the constant term.

Binomial expansion of $(1 + x)^{n}$

$1 + nx + \frac{n(n-1)}{2!}x^{2} + \frac{n(n-1)(n-2)}{3!}x^{3} + \cdots$

Ends after $n + 1$ terms for a positive integer $n$. For any real $n$ it is an infinite series valid when $\lvert x \rvert < 1$.

Example: In $(x + 2)^{6}$, $n = 6$ is even, so the middle term is $T_{4} = \binom{6}{3}x^{3}(2)^{3} = 20 \times 8x^{3} = 160x^{3}$.

Factorials And Permutations

Formula

Expression

What it means

Factorial

$n! = n(n-1)(n-2)\cdots 2 \cdot 1$

The product of all positive integers up to $n$. By definition $0! = 1$.

Recursive factorial

$n! = n \times (n-1)!$

Each factorial is $n$ times the one before it, for $n \geq 1$. Useful for cancelling factorials in fractions.

nPr formula

$^{n}P_{r} = \frac{n!}{(n-r)!}$

Number of ordered arrangements of $r$ objects chosen from $n$ distinct objects, for $0 \leq r \leq n$.

Arranging all n objects

$^{n}P_{n} = n!$

Number of ways to line up $n$ distinct objects in a row.

Permutations with repetition allowed

$n^{r}$

Number of ordered arrangements of length $r$ when each place can be filled by any of $n$ objects again and again.

Permutations with identical objects

$\frac{n!}{p!,q!,s!}$

Arrangements of $n$ objects in which $p$ are alike of one kind, $q$ of another and $s$ of a third.

Circular permutations

$(n-1)!$

Ways to seat $n$ distinct people around a round table, where rotations of the same order count once.

Circular arrangements that can be flipped

$\frac{(n-1)!}{2}$

For beads on a necklace or flowers in a garland, clockwise and anticlockwise orders count once. Valid for $n \geq 3$.

Particular object always included

$r \cdot {}^{n-1}P_{r-1}$

Arrangements of $r$ out of $n$ distinct objects in which one chosen object must appear.

Particular object never included

$^{n-1}P_{r}$

Arrangements of $r$ out of $n$ distinct objects in which one chosen object is left out.

Derangements

$D_{n} = n!\left(1 - \frac{1}{1!} + \frac{1}{2!} - \frac{1}{3!} + \cdots + \frac{(-1)^{n}}{n!}\right)$

Number of ways to arrange $n$ objects so that none is in its original place. For example $D_{3} = 2$ and $D_{4} = 9$.

Power of a prime in n factorial

$\left\lfloor \frac{n}{p} \right\rfloor + \left\lfloor \frac{n}{p^{2}} \right\rfloor + \left\lfloor \frac{n}{p^{3}} \right\rfloor + \cdots$

Exponent of the prime $p$ in $n!$, where the brackets mean the greatest integer. Used to count trailing zeros with $p = 5$.

Example: The letters of BANANA have 3 As and 2 Ns among 6 letters, so they can be arranged in $\frac{6!}{3!,2!} = \frac{720}{12} = 60$ ways.

Combinations

Formula

Expression

What it means

nCr formula

$^{n}C_{r} = \binom{n}{r} = \frac{n!}{r!,(n-r)!}$

Number of ways to choose $r$ objects from $n$ distinct objects when order does not matter, for $0 \leq r \leq n$.

Link between nPr and nCr

$^{n}P_{r} = r! \times {}^{n}C_{r}$

Each selection of $r$ objects can be ordered in $r!$ ways, which turns a combination count into a permutation count.

Complementary selections

$^{n}C_{r} = {}^{n}C_{n-r}$

Choosing $r$ objects to take is the same as choosing $n - r$ objects to leave behind.

Special values

$^{n}C_{0} = {}^{n}C_{n} = 1$ and $^{n}C_{1} = n$

There is one way to choose nothing or everything, and $n$ ways to choose a single object.

Equal combinations

If $^{n}C_{x} = {}^{n}C_{y}$ then $x = y$ or $x + y = n$

Used to solve equations in which two combinations with the same $n$ are equal.

Pascal's rule

$^{n}C_{r} + {}^{n}C_{r-1} = {}^{n+1}C_{r}$

Two neighbouring entries in one row of Pascal's triangle add to the entry below them, for $1 \leq r \leq n$.

Ratio of consecutive terms

$\frac{{}^{n}C_{r}}{{}^{n}C_{r-1}} = \frac{n - r + 1}{r}$

Lets you get each coefficient from the previous one and find where the coefficients stop increasing.

Absorption identity

$r \cdot {}^{n}C_{r} = n \cdot {}^{n-1}C_{r-1}$

Moves a factor of $r$ inside a combination. Often used when summing $r\binom{n}{r}$ over $r$.

Selecting at least one

$^{n}C_{1} + {}^{n}C_{2} + \cdots + {}^{n}C_{n} = 2^{n} - 1$

Number of nonempty selections from $n$ distinct objects, since each object is either taken or not.

Identical objects into distinct groups

$^{n+r-1}C_{r-1}$

Ways to share $n$ identical objects among $r$ people when a person may get none, also called stars and bars.

Each group gets at least one

$^{n-1}C_{r-1}$

Ways to share $n$ identical objects among $r$ people when each person gets at least one, for $n \geq r$.

Lines and triangles from points

$^{n}C_{2}$ lines and $^{n}C_{3}$ triangles

Counts from $n$ points in a plane with no three collinear, because two points fix a line and three fix a triangle.

Example: A committee of 3 chosen from 8 people can be formed in $^{8}C_{3} = \frac{8 \times 7 \times 6}{3 \times 2 \times 1} = 56$ ways.

Complex Numbers: Standard Form And Operations

Formula

Expression

What it means

Imaginary unit

$i = \sqrt{-1}$, so $i^{2} = -1$

The number whose square is $-1$. It is also called iota in Indian textbooks.

Powers of i

$i^{4k} = 1$, $i^{4k+1} = i$, $i^{4k+2} = -1$, $i^{4k+3} = -i$

Powers of $i$ repeat every 4 steps, so divide the power by 4 and use the remainder. Here $k$ is an integer.

Standard form

$z = a + bi$

A complex number with real part $\text{Re}(z) = a$ and imaginary part $\text{Im}(z) = b$, where $a$ and $b$ are real.

Equality of complex numbers

$a + bi = c + di$ if and only if $a = c$ and $b = d$

Two complex numbers are equal only when both their real parts and their imaginary parts match.

Addition and subtraction

$(a + bi) \pm (c + di) = (a \pm c) + (b \pm d)i$

Add or subtract the real parts and the imaginary parts separately.

Multiplication

$(a + bi)(c + di) = (ac - bd) + (ad + bc)i$

Expand like two binomials and replace $i^{2}$ with $-1$.

Conjugate

$\bar{z} = a - bi$

Flips the sign of the imaginary part. Also $z + \bar{z} = 2a$ and $z\bar{z} = a^{2} + b^{2}$.

Modulus of a complex number

$\lvert z \rvert = \sqrt{a^{2} + b^{2}}$

The distance of the point $(a, b)$ from the origin in the Argand plane. It is never negative.

Division

$\frac{a + bi}{c + di} = \frac{(ac + bd) + (bc - ad)i}{c^{2} + d^{2}}$

Found by multiplying top and bottom by the conjugate $c - di$ of the denominator. Needs $c + di \neq 0$.

Reciprocal

$\frac{1}{z} = \frac{\bar{z}}{\lvert z \rvert^{2}}$

The multiplicative inverse of any nonzero complex number $z$.

Modulus rules

$\lvert z_{1}z_{2} \rvert = \lvert z_{1} \rvert \lvert z_{2} \rvert$ and $\left\lvert \frac{z_{1}}{z_{2}} \right\rvert = \frac{\lvert z_{1} \rvert}{\lvert z_{2} \rvert}$

The modulus of a product or quotient is the product or quotient of the moduli, with $z_{2} \neq 0$.

Conjugate rules

$\overline{z_{1} + z_{2}} = \overline{z_{1}} + \overline{z_{2}}$ and $\overline{z_{1}z_{2}} = \overline{z_{1}},\overline{z_{2}}$

Taking the conjugate can be done before or after adding or multiplying.

Triangle inequality

$\lvert z_{1} + z_{2} \rvert \leq \lvert z_{1} \rvert + \lvert z_{2} \rvert$

The length of one side of a triangle is at most the sum of the other two. Equality holds when $z_{1}$ and $z_{2}$ point the same way.

Distance between two points

$\lvert z_{1} - z_{2} \rvert$

The distance between the points $z_{1}$ and $z_{2}$ in the Argand plane.

Square root of a complex number

$\sqrt{a + bi} = \pm\left(\sqrt{\frac{\lvert z \rvert + a}{2}} + i,\frac{b}{\lvert b \rvert}\sqrt{\frac{\lvert z \rvert - a}{2}}\right)$

Both square roots of $z = a + bi$ with $b \neq 0$. The factor $\frac{b}{\lvert b \rvert}$ is just the sign of $b$.

Example: $\frac{3 + 4i}{1 - 2i} = \frac{(3 + 4i)(1 + 2i)}{1^{2} + 2^{2}} = \frac{3 + 10i + 8i^{2}}{5} = \frac{-5 + 10i}{5} = -1 + 2i$.

Complex Numbers: Polar Form, De Moivre's Theorem And Roots Of Unity

Angles in this table are in radians.

Formula

Expression

What it means

Argument

$\tan\theta = \frac{b}{a}$, with $-\pi < \theta \leq \pi$

The angle $z = a + bi$ makes with the positive real axis. Pick the quadrant from the signs of $a$ and $b$ to get the principal argument.

Polar form

$z = r(\cos\theta + i\sin\theta)$

Writes $z$ using its modulus $r = \lvert z \rvert$ and argument $\theta$, so $a = r\cos\theta$ and $b = r\sin\theta$.

Euler's formula

$e^{i\theta} = \cos\theta + i\sin\theta$

Links the exponential function to sine and cosine for any real $\theta$.

Euler (exponential) form

$z = re^{i\theta}$

A short way to write the polar form. Makes multiplication, division and powers easy.

Euler's identity

$e^{i\pi} + 1 = 0$

Euler's formula with $\theta = \pi$. It connects $e$, $i$, $\pi$, 1 and 0.

Product in polar form

$z_{1}z_{2} = r_{1}r_{2}[\cos(\theta_{1} + \theta_{2}) + i\sin(\theta_{1} + \theta_{2})]$

Multiply the moduli and add the arguments. So $\arg(z_{1}z_{2}) = \arg z_{1} + \arg z_{2}$, up to a multiple of $2\pi$.

Quotient in polar form

$\frac{z_{1}}{z_{2}} = \frac{r_{1}}{r_{2}}[\cos(\theta_{1} - \theta_{2}) + i\sin(\theta_{1} - \theta_{2})]$

Divide the moduli and subtract the arguments, with $z_{2} \neq 0$.

De Moivre's theorem

$(\cos\theta + i\sin\theta)^{n} = \cos n\theta + i\sin n\theta$

Raises a complex number in polar form to an integer power $n$ by multiplying the angle by $n$.

nth roots of a complex number

$r^{\frac{1}{n}}\left[\cos\frac{\theta + 2k\pi}{n} + i\sin\frac{\theta + 2k\pi}{n}\right]$

Gives all $n$ distinct roots of $z = re^{i\theta}$ as $k$ runs through $0, 1, \ldots, n-1$.

Cube roots of unity

$1$, $\omega = \frac{-1 + i\sqrt{3}}{2}$, $\omega^{2} = \frac{-1 - i\sqrt{3}}{2}$

The three solutions of $z^{3} = 1$. The two complex ones are roots of $z^{2} + z + 1 = 0$ and are conjugates of each other.

Properties of omega

$1 + \omega + \omega^{2} = 0$ and $\omega^{3} = 1$

The key facts used to simplify any expression in $\omega$. Also $\lvert \omega \rvert = 1$ and $\bar{\omega} = \omega^{2}$.

nth roots of unity

$e^{\frac{2k\pi i}{n}}$ for $k = 0, 1, \ldots, n-1$

The $n$ solutions of $z^{n} = 1$, equally spaced on the unit circle. Their sum is 0 for $n \geq 2$ and their product is $(-1)^{n-1}$.

Example: $1 + i = \sqrt{2}\left(\cos\frac{\pi}{4} + i\sin\frac{\pi}{4}\right)$, so by De Moivre $(1 + i)^{8} = (\sqrt{2})^{8}(\cos 2\pi + i\sin 2\pi) = 16$.

Matrix Operations And Transpose

Formula

Expression

What it means

Order of a matrix

$m \times n$ matrix has $mn$ entries

A matrix with $m$ rows and $n$ columns. The entry in row $i$ and column $j$ is written $a_{ij}$.

Matrix addition

$(A + B){ij} = a{ij} + b_{ij}$

Add entries in the same position. Defined only when $A$ and $B$ have the same order.

Scalar multiplication

$(kA){ij} = k,a{ij}$

Multiply every entry of $A$ by the number $k$.

Multiplication of matrices

$(AB){ij} = \sum{k=1}^{n} a_{ik}b_{kj}$

Entry $(i, j)$ of the product is row $i$ of $A$ times column $j$ of $B$, added term by term.

Order of a product

$A_{m \times n}B_{n \times p} = C_{m \times p}$

$AB$ exists only when the number of columns of $A$ equals the number of rows of $B$.

Laws of matrix multiplication

$(AB)C = A(BC)$, $A(B + C) = AB + AC$, but $AB \neq BA$ in general

Matrix multiplication is associative and distributive but usually not commutative, so the order of factors matters.

Identity matrix

$AI = IA = A$

$I$ has 1 on the main diagonal and 0 elsewhere. It acts like the number 1 for square matrices of the same order.

Transpose of a matrix

$(A^{T}){ij} = a{ji}$

Rows become columns. An $m \times n$ matrix has an $n \times m$ transpose, also written $A'$.

Transpose rules

$(A^{T})^{T} = A$, $(A + B)^{T} = A^{T} + B^{T}$, $(kA)^{T} = kA^{T}$

Transposing twice returns the original, and transpose passes through sums and scalar multiples.

Reversal law for transpose

$(AB)^{T} = B^{T}A^{T}$

The transpose of a product is the product of the transposes in reverse order.

Symmetric matrix

$A^{T} = A$

A square matrix equal to its own transpose, so $a_{ij} = a_{ji}$ for all $i$ and $j$.

Skew symmetric matrix

$A^{T} = -A$

A square matrix with $a_{ij} = -a_{ji}$. All its diagonal entries are 0.

Symmetric plus skew symmetric split

$A = \frac{1}{2}(A + A^{T}) + \frac{1}{2}(A - A^{T})$

Every square matrix is the sum of a symmetric part and a skew symmetric part, and this split is unique.

Trace

$\text{tr}(A) = \sum_{i=1}^{n} a_{ii}$

Sum of the main diagonal entries of a square matrix. Also $\text{tr}(AB) = \text{tr}(BA)$.

Orthogonal matrix

$AA^{T} = A^{T}A = I$

A square matrix whose transpose is its inverse. Its determinant is $1$ or $-1$.

Example: If $A$ has rows $(1, 2)$ and $(3, 4)$ and $B$ has rows $(5, 6)$ and $(7, 8)$, then $(AB)_{11} = 1 \times 5 + 2 \times 7 = 19$ and $AB$ has rows $(19, 22)$ and $(43, 50)$.

Determinants

Every result in this table applies to square matrices only.

Formula

Expression

What it means

2 by 2 determinant

$\det A = ad - bc$

For the matrix with rows $(a, b)$ and $(c, d)$: the product of the main diagonal minus the product of the other diagonal.

3 by 3 determinant

$a_{11}(a_{22}a_{33} - a_{23}a_{32}) - a_{12}(a_{21}a_{33} - a_{23}a_{31}) + a_{13}(a_{21}a_{32} - a_{22}a_{31})$

Expansion along the first row. The signs alternate plus, minus, plus.

Minor and cofactor

$C_{ij} = (-1)^{i+j}M_{ij}$

$M_{ij}$ is the determinant left after deleting row $i$ and column $j$. The cofactor attaches the checkerboard sign.

Expansion along any row

$\det A = \sum_{j=1}^{n} a_{ij}C_{ij}$

Any row or column gives the same value, so expand along the one with the most zeros.

Determinant of a transpose

$\det(A^{T}) = \det A$

Swapping rows and columns does not change the determinant, so every row rule also holds for columns.

Product rule

$\det(AB) = \det A \cdot \det B$

The determinant of a product of two square matrices of the same order is the product of their determinants.

Scalar multiple

$\det(kA) = k^{n}\det A$

For an $n \times n$ matrix, multiplying the whole matrix by $k$ multiplies the determinant by $k^{n}$.

Row operation rules

Swap two rows gives $-\det A$, scale one row by $k$ gives $k\det A$

Adding a multiple of one row to another leaves the determinant unchanged. These rules speed up evaluation.

Zero determinant cases

$\det A = 0$

Always happens when two rows are equal or proportional, or a whole row is zero, though these are not the only cases. Such a matrix is called singular.

Triangular matrix

$\det A = a_{11}a_{22}\cdots a_{nn}$

For an upper or lower triangular or diagonal matrix, the determinant is the product of the diagonal entries.

Determinant of an inverse

$\det(A^{-1}) = \frac{1}{\det A}$

Holds for any invertible matrix, since $AA^{-1} = I$ and $\det I = 1$.

Area of triangle in determinant form

$\text{Area} = \frac{1}{2}\lvert x_{1}(y_{2} - y_{3}) + x_{2}(y_{3} - y_{1}) + x_{3}(y_{1} - y_{2}) \rvert$

Half the absolute value of the determinant with rows $(x_{1}, y_{1}, 1)$, $(x_{2}, y_{2}, 1)$, $(x_{3}, y_{3}, 1)$. It equals 0 when the points are collinear.

Example: For rows $(2, 1, 3)$, $(0, 4, 5)$ and $(1, 0, 6)$, $\det A = 2(24 - 0) - 1(0 - 5) + 3(0 - 4) = 48 + 5 - 12 = 41$.

Inverse Of A Matrix And Cramer's Rule

Formula

Expression

What it means

Adjoint of a matrix

$\text{adj},A = C^{T}$

The transpose of the cofactor matrix $C$. Also called the adjugate.

Adjoint identity

$A(\text{adj},A) = (\text{adj},A)A = (\det A)I$

Holds for every square matrix and leads straight to the inverse formula.

Inverse of a matrix

$A^{-1} = \frac{1}{\det A},\text{adj},A$

The matrix with $AA^{-1} = A^{-1}A = I$. It exists only when $\det A \neq 0$.

Inverse of a 2x2 matrix

$A^{-1} = \frac{1}{ad - bc}$ times the matrix with rows $(d, -b)$ and $(-c, a)$

For $A$ with rows $(a, b)$ and $(c, d)$: swap the diagonal entries, negate the other two and divide by $ad - bc \neq 0$.

Inverse of a product

$(AB)^{-1} = B^{-1}A^{-1}$

The inverse of a product is the product of the inverses in reverse order, when both are invertible.

Inverse of a transpose

$(A^{T})^{-1} = (A^{-1})^{T}$

Transposing and inverting can be done in either order.

Determinant of the adjoint

$\det(\text{adj},A) = (\det A)^{n-1}$

For an $n \times n$ matrix. For a 3 by 3 matrix this gives $(\det A)^{2}$.

Adjoint of the adjoint

$\text{adj}(\text{adj},A) = (\det A)^{n-2}A$

For an $n \times n$ matrix with $n \geq 2$. A frequent JEE result.

Matrix method for linear equations

$AX = B \Rightarrow X = A^{-1}B$

Solves a square system where $A$ holds the coefficients, $X$ the unknowns and $B$ the constants, when $\det A \neq 0$.

Cramer's rule

$x = \frac{D_{x}}{D}$, $y = \frac{D_{y}}{D}$, $z = \frac{D_{z}}{D}$

$D$ is the coefficient determinant and $D_{x}$ replaces the $x$ column with the constants, and so on. Needs $D \neq 0$.

Consistency test

$D \neq 0$ gives a unique solution

If $D = 0$ and some $D_{x}$, $D_{y}$ or $D_{z}$ is nonzero, there is no solution. If all are zero, there are infinitely many solutions or none.

Example: For $2x + 3y = 8$ and $x - y = -1$, $D = -2 - 3 = -5$, $D_{x} = -8 + 3 = -5$ and $D_{y} = -2 - 8 = -10$, so $x = 1$ and $y = 2$.

Set Operations And Venn Diagram Counts

Formula

Expression

What it means

A union B formula

$n(A \cup B) = n(A) + n(B) - n(A \cap B)$

Counts elements in at least one of two finite sets. The overlap is subtracted once because it was counted twice.

Disjoint sets

$n(A \cup B) = n(A) + n(B)$

When $A \cap B = \emptyset$ there is no overlap, so the counts simply add.

Union of three sets

$n(A \cup B \cup C) = n(A) + n(B) + n(C) - n(A \cap B) - n(B \cap C) - n(A \cap C) + n(A \cap B \cap C)$

Inclusion-exclusion for three sets. Add singles, subtract pairs, add back the triple overlap.

Only A

$n(A - B) = n(A) - n(A \cap B)$

Elements in $A$ but not in $B$, the difference of sets $A - B$.

Symmetric difference

$n(A \Delta B) = n(A) + n(B) - 2n(A \cap B)$

Elements in exactly one of $A$ and $B$, written $A \Delta B = (A - B) \cup (B - A)$.

Complement of a set

$n(A') = n(U) - n(A)$

Elements of the universal set $U$ that are not in $A$. Also written $A^{c}$.

Neither A nor B

$n(A' \cap B') = n(U) - n(A \cup B)$

Elements of the universal set that lie outside both sets.

De Morgan's laws for sets

$(A \cup B)' = A' \cap B'$ and $(A \cap B)' = A' \cup B'$

The complement of a union is the intersection of complements, and the complement of an intersection is the union of complements.

Distributive laws

$A \cup (B \cap C) = (A \cup B) \cap (A \cup C)$ and $A \cap (B \cup C) = (A \cap B) \cup (A \cap C)$

Union spreads over intersection and intersection spreads over union, like multiplication over addition.

Exactly one of three sets

$S_{1} - 2S_{2} + 3S_{3}$

$S_{1}$ is the sum of the three single counts, $S_{2}$ the sum of the three pair overlaps and $S_{3} = n(A \cap B \cap C)$.

Exactly two of three sets

$S_{2} - 3S_{3}$

Elements in exactly two of $A$, $B$, $C$, using the same $S_{2}$ and $S_{3}$ as the row above.

Example: In a class of 40, 25 play cricket, 18 play football and 8 play both, so $n(C \cup F) = 25 + 18 - 8 = 35$ and $40 - 35 = 5$ students play neither.

Subsets, Relations And Functions

Here $n(A) = m$ and $n(B) = n$, both finite, unless the row says otherwise.

Formula

Expression

What it means

Number of subsets

$2^{m}$

A set with $m$ elements has $2^{m}$ subsets, because each element is either in or out.

Proper subsets

$2^{m} - 1$

All subsets except the set itself. Nonempty proper subsets number $2^{m} - 2$ for $m \geq 1$.

Subsets of a fixed size

$^{m}C_{r}$

Number of subsets with exactly $r$ elements, for $0 \leq r \leq m$.

Power set

$n(P(A)) = 2^{m}$

$P(A)$ is the set of all subsets of $A$, including $\emptyset$ and $A$ itself.

Cartesian product

$n(A \times B) = mn$

Number of ordered pairs $(a, b)$ with $a$ in $A$ and $b$ in $B$.

Number of relations from A to B

$2^{mn}$

A relation is any subset of $A \times B$, so the count is the number of subsets of a set of size $mn$.

Relations on a set

$2^{m^{2}}$

Number of relations from a set with $m$ elements to itself.

Reflexive relations, symmetric relations

$2^{m^{2} - m}$ reflexive, $2^{\frac{m(m+1)}{2}}$ symmetric

Counts of relations on a set of $m$ elements that are reflexive, or separately that are symmetric.

Number of functions from A to B

$n^{m}$

Each of the $m$ elements of $A$ can be sent to any of the $n$ elements of $B$.

One-to-one functions

$^{n}P_{m} = \frac{n!}{(n-m)!}$

Number of injective functions from $A$ to $B$ when $m \leq n$. There are none if $m > n$.

Bijections

$n!$

Number of one-to-one and onto functions between two sets that both have $n$ elements.

Onto functions

$\sum_{k=0}^{n} (-1)^{k}\binom{n}{k}(n - k)^{m}$

Number of surjective functions from $A$ onto $B$, for $m \geq n$, found by inclusion-exclusion.

Binary operations on a set

$m^{m^{2}}$

Number of binary operations on a set with $m$ elements, since each of the $m^{2}$ ordered pairs gets one of $m$ outputs.

Example: For a set $A$ with 3 elements and a set $B$ with 2 elements, there are $2^{3} = 8$ functions, $2^{6} = 64$ relations and $2^{3} - 2 \times 1^{3} = 6$ onto functions from $A$ to $B$.

Mathematical Logic

Here $p$ and $q$ are statements that are either true (T) or false (F).

Formula

Expression

What it means

Negation

$\sim p$

True when $p$ is false and false when $p$ is true. Also written $\neg p$.

Conjunction (AND)

$p \wedge q$

True only when both $p$ and $q$ are true.

Disjunction (OR)

$p \vee q$

False only when both $p$ and $q$ are false. This is the inclusive or.

Implication (if p then q)

$p \Rightarrow q \equiv \sim p \vee q$

False only when $p$ is true and $q$ is false. A false $p$ makes the implication true.

Biconditional (if and only if)

$p \Leftrightarrow q \equiv (p \Rightarrow q) \wedge (q \Rightarrow p)$

True when $p$ and $q$ have the same truth value.

Converse

$q \Rightarrow p$

Swaps the two parts of $p \Rightarrow q$. It is not equivalent to the original.

Inverse

$\sim p \Rightarrow \sim q$

Negates both parts of $p \Rightarrow q$. It is equivalent to the converse, not to the original.

Contrapositive

$\sim q \Rightarrow \sim p$

Swaps and negates both parts. It always has the same truth value as $p \Rightarrow q$, so it is used in indirect proofs.

De Morgan's laws for statements

$\sim(p \wedge q) \equiv \sim p \vee \sim q$ and $\sim(p \vee q) \equiv \sim p \wedge \sim q$

To negate an AND statement, negate each part and use OR, and the reverse for an OR statement.

Negation of an implication

$\sim(p \Rightarrow q) \equiv p \wedge \sim q$

The only way an implication fails is when $p$ holds and $q$ does not.

Double negation

$\sim(\sim p) \equiv p$

Negating a statement twice gives back the original statement.

Tautology and contradiction

$p \vee \sim p$ is always T, $p \wedge \sim p$ is always F

A tautology is true in every row of its truth table and a contradiction is false in every row.

Negation of quantifiers

$\sim(\forall x,, P(x)) \equiv \exists x,, \sim P(x)$

The negation of "for all" is "there exists one that fails", and the negation of "there exists" is "for all, it fails".

Rows in a truth table

$2^{n}$

A compound statement built from $n$ simple statements needs $2^{n}$ rows to list every combination.

Example: For "if $x = 2$ then $x^{2} = 4$", the contrapositive is "if $x^{2} \neq 4$ then $x \neq 2$" (true), while the converse "if $x^{2} = 4$ then $x = 2$" is false since $x = -2$ also works.

Geometry Formulas: Area, Perimeter, Surface Area And Volume

This section covers plane and solid geometry, from angle facts and triangle areas to the surface area and volume of 3D solids. Students use it from Grade 6 mensuration through board exams, SAT, GCSE and the geometry parts of JEE.

Angles And Polygon Angles

Formula

Expression

What it means

Complementary angles

$A + B = 90^{\circ}$

Two angles are complementary when they add to $90^{\circ}$, so the complement of an angle $x$ is $90^{\circ} - x$.

Supplementary angles

$A + B = 180^{\circ}$

Two angles are supplementary when they add to $180^{\circ}$, so the supplement of an angle $x$ is $180^{\circ} - x$.

Linear pair of angles

$\angle 1 + \angle 2 = 180^{\circ}$

Two adjacent angles that sit on a straight line always add to $180^{\circ}$.

Vertical angles

$\angle 1 = \angle 3$

When two straight lines cross, each pair of vertically opposite angles is equal.

Angles at a point (complete angle)

$\angle 1 + \angle 2 + \dots + \angle k = 360^{\circ}$

All the angles around one point add to a full turn of $360^{\circ}$, whatever their number $k$.

Corresponding angles

$\angle a = \angle b$

When a transversal cuts two parallel lines, the angles in matching positions at each crossing are equal.

Alternate interior angles

$\angle a = \angle b$

With parallel lines and a transversal, angles on opposite sides of the transversal and between the lines are equal.

Co-interior angles (same-side interior angles)

$\angle a + \angle b = 180^{\circ}$

With parallel lines and a transversal, the two interior angles on the same side of the transversal are supplementary.

Sum of interior angles of a polygon

$S = (n - 2) \times 180^{\circ}$

For a polygon with $n$ sides, $n \geq 3$, because it splits into $n - 2$ triangles from one vertex.

Each interior angle of a regular polygon

$\frac{(n - 2) \times 180^{\circ}}{n}$

A regular polygon has $n$ equal angles, so divide the interior angle sum by $n$.

Sum of exterior angles of a polygon

$360^{\circ}$

Taking one exterior angle at each vertex of a convex polygon, the total is always $360^{\circ}$, for any $n$.

Each exterior angle of a regular polygon

$\frac{360^{\circ}}{n}$

$n$ is the number of sides. Also used in reverse to find it: $n = \frac{360^{\circ}}{\text{exterior angle}}$.

Interior and exterior angle at a vertex

$\text{interior} + \text{exterior} = 180^{\circ}$

At each vertex the interior angle and its exterior angle form a linear pair on the extended side.

Number of diagonals of a polygon

$\frac{n(n - 3)}{2}$

Each of the $n$ vertices joins $n - 3$ non-adjacent vertices, and every diagonal gets counted twice, hence the division by 2.

Example: A regular polygon with each exterior angle $24^{\circ}$ has $n = \frac{360}{24} = 15$ sides, each interior angle $180^{\circ} - 24^{\circ} = 156^{\circ}$ and $\frac{15 \times 12}{2} = 90$ diagonals.

Triangle Formulas

Formula

Expression

What it means

Area of a triangle

$A = \frac{1}{2} \times b \times h$

$b$ is any side taken as the base and $h$ is the perpendicular height to that side from the opposite vertex.

Heron's formula

$A = \sqrt{s(s - a)(s - b)(s - c)}$

Gives the area when all three sides $a$, $b$, $c$ are known, with $s$ the semi-perimeter. No height is needed.

Semi-perimeter

$s = \frac{a + b + c}{2}$

Half the perimeter of the triangle. It appears in Heron's formula and in the inradius formula.

Area from two sides and the included angle

$A = \frac{1}{2}ab\sin C$

$a$ and $b$ are two sides and $C$ is the angle between them. Works for every triangle, acute or obtuse.

Perimeter of a triangle

$P = a + b + c$

The perimeter is the total length of the boundary, found by adding the three side lengths.

Angle sum of a triangle (triangle sum theorem)

$A + B + C = 180^{\circ}$

The three interior angles of any triangle add to $180^{\circ}$, which is $\pi$ radians.

Exterior angle theorem

$\angle \text{exterior} = \angle A + \angle B$

An exterior angle of a triangle equals the sum of the two interior angles that are not next to it.

Triangle inequality theorem

$\lvert a - b \rvert < c < a + b$

Any two sides together must be longer than the third. Use it to test whether three lengths can form a triangle.

Area of an equilateral triangle

$A = \frac{\sqrt{3}}{4}a^{2}$

$a$ is the side length. All three sides are equal and each angle is $60^{\circ}$.

Height of an equilateral triangle

$h = \frac{\sqrt{3}}{2}a$

For side $a$, the altitude bisects the base, so Pythagoras on half the triangle gives $h^{2} = a^{2} - \frac{a^{2}}{4}$.

Perimeter of an equilateral triangle

$P = 3a$

Three equal sides of length $a$, so the perimeter is three times one side.

Area of an isosceles triangle (isosceles triangle formula)

$A = \frac{b}{4}\sqrt{4a^{2} - b^{2}}$

$a$ is each of the two equal sides and $b$ is the base, which must satisfy $b < 2a$.

Example: For sides $13$, $14$ and $15$, $s = 21$ and Heron's formula gives $A = \sqrt{21 \times 8 \times 7 \times 6} = \sqrt{7056} = 84$ square units.

Right Triangle Formulas

Formula

Expression

What it means

Pythagorean theorem (Pythagoras theorem)

$a^{2} + b^{2} = c^{2}$

In a right triangle, $a$ and $b$ are the legs and $c$ is the hypotenuse, the side opposite the right angle.

Hypotenuse and missing leg

$c = \sqrt{a^{2} + b^{2}}$, $a = \sqrt{c^{2} - b^{2}}$

Rearranged forms of Pythagoras for finding an unknown side once the other two are known.

Converse of Pythagoras theorem

$a^{2} + b^{2} = c^{2} \Rightarrow \angle C = 90^{\circ}$

If the squares of two sides add to the square of the third, the angle opposite that third side is a right angle.

Acute or obtuse test

$c^{2} < a^{2} + b^{2}$ (acute), $c^{2} > a^{2} + b^{2}$ (obtuse)

Here $c$ is the longest side. Compare $c^{2}$ with $a^{2} + b^{2}$ to classify the largest angle.

Area of a right triangle (right triangle formulas)

$A = \frac{1}{2}ab$

The two legs $a$ and $b$ are perpendicular, so one acts as the base and the other as the height.

45-45-90 triangle (isosceles right triangle)

$x : x : x\sqrt{2}$

Both legs equal $x$ and the hypotenuse is $x\sqrt{2}$. This is half of a square cut along its diagonal.

30-60-90 triangle

$x : x\sqrt{3} : 2x$

The side opposite $30^{\circ}$ is $x$, opposite $60^{\circ}$ is $x\sqrt{3}$, and the hypotenuse is $2x$.

Altitude to the hypotenuse

$h = \frac{ab}{c}$

The height from the right angle to the hypotenuse, found by writing the area two ways: $\frac{1}{2}ab = \frac{1}{2}ch$.

Hypotenuse segment relations

$h^{2} = pq$, $a^{2} = pc$, $b^{2} = qc$

The altitude splits the hypotenuse into $p$ (next to leg $a$) and $q$ (next to leg $b$), with $p + q = c$.

Circumradius of a right triangle

$R = \frac{c}{2}$

The hypotenuse is a diameter of the circumcircle, so the circumcentre is the midpoint of the hypotenuse.

Inradius of a right triangle

$r = \frac{a + b - c}{2}$

Radius of the circle touching all three sides, with legs $a$, $b$ and hypotenuse $c$.

Pythagorean triples

$(m^{2} - n^{2}, , 2mn, , m^{2} + n^{2})$

For whole numbers $m > n > 0$ this gives integer sides of a right triangle, such as $(3, 4, 5)$ from $m = 2$, $n = 1$.

Example: Legs $6$ and $8$ give $c = \sqrt{36 + 64} = 10$, and the altitude to the hypotenuse is $h = \frac{6 \times 8}{10} = 4.8$.

Triangle Centres, Medians And Radii

For the radius formulas below, $A$ is the area of the triangle and $s$ is its semi-perimeter.

Formula

Expression

What it means

Centroid of a triangle

$AG : GM = 2 : 1$

The three medians meet at the centroid $G$, which divides each median in the ratio $2 : 1$ measured from the vertex.

Length of a median

$m_{a} = \frac{1}{2}\sqrt{2b^{2} + 2c^{2} - a^{2}}$

The median from vertex $A$ to the midpoint of side $a$. This comes from Apollonius' theorem.

Altitude of a triangle

$h_{a} = \frac{2A}{a}$

The perpendicular height onto side $a$, found by rearranging $A = \frac{1}{2}ah_{a}$.

Circumradius (circumcentre)

$R = \frac{abc}{4A}$

Radius of the circle through all three vertices. Its centre is where the perpendicular bisectors of the sides meet.

Circumradius from the sine rule

$R = \frac{a}{2\sin A}$

Here $A$ is the angle opposite side $a$. Any side and its opposite angle give the same $R$.

Inradius (incentre)

$r = \frac{A}{s}$

Radius of the circle touching all three sides. Its centre is where the angle bisectors meet, and $A = rs$.

Circumradius and inradius of an equilateral triangle

$R = \frac{a}{\sqrt{3}}$, $r = \frac{a}{2\sqrt{3}}$

For side $a$ the centroid, circumcentre and incentre coincide, so $R = 2r$.

Euler's distance between centres

$OI^{2} = R^{2} - 2Rr$

$O$ is the circumcentre and $I$ the incentre. It shows $R \geq 2r$, with equality only for an equilateral triangle.

Example: For sides $13$, $14$, $15$ with $A = 84$ and $s = 21$, the inradius is $r = \frac{84}{21} = 4$ and the circumradius is $R = \frac{13 \times 14 \times 15}{4 \times 84} = \frac{2730}{336} = 8.125$.

Similarity And Scale Factor

These hold for two similar figures whose matching lengths are in the ratio $k$ (the scale factor).

Formula

Expression

What it means

Ratio of lengths

$\frac{a'}{a} = k$

Every pair of matching sides, heights, medians or radii in similar figures has the same ratio $k$.

Ratio of perimeters

$\frac{P'}{P} = k$

Perimeters are lengths, so they scale by the same factor $k$ as the sides.

Ratio of areas (area of similar triangles)

$\frac{A'}{A} = k^{2}$

Areas of similar figures scale by the square of the side ratio. Surface areas of similar solids also scale by $k^{2}$.

Ratio of volumes

$\frac{V'}{V} = k^{3}$

Volumes of similar solids scale by the cube of the length ratio, so doubling every length multiplies volume by 8.

Basic proportionality theorem (Thales)

$\frac{AD}{DB} = \frac{AE}{EC}$

If a line parallel to $BC$ cuts $AB$ at $D$ and $AC$ at $E$, it divides those two sides in the same ratio.

Midsegment of a triangle

$DE = \frac{1}{2}BC$

The segment joining the midpoints of two sides is parallel to the third side and half its length.

Angle bisector theorem

$\frac{BD}{DC} = \frac{AB}{AC}$

The bisector of angle $A$ meets $BC$ at $D$ and splits it in the ratio of the two sides next to angle $A$.

Example: Two similar triangles have matching sides $4,\text{cm}$ and $6,\text{cm}$, so $k = 1.5$ and $k^{2} = 2.25$. If the smaller area is $20,\text{cm}^{2}$, the larger is $20 \times 2.25 = 45,\text{cm}^{2}$.

Square And Rectangle Formulas

Formula

Expression

What it means

Area of a square

$A = a^{2}$

$a$ is the side length. The side from a known area is $a = \sqrt{A}$.

Perimeter of a square

$P = 4a$

A square has four equal sides of length $a$, so the boundary is four times one side.

Diagonal of a square

$d = a\sqrt{2}$

Both diagonals are equal, bisect each other at right angles and follow from Pythagoras on two sides.

Area of a square from its diagonal

$A = \frac{d^{2}}{2}$

Useful when only the diagonal $d$ is given. It matches the rhombus rule $\frac{1}{2}d_{1}d_{2}$ with equal diagonals.

Area of a rectangle

$A = l \times w$

$l$ is the length and $w$ the width (breadth), measured in the same unit.

Perimeter of a rectangle

$P = 2(l + w)$

Two lengths plus two widths. Use it for fencing, borders and frame problems.

Diagonal of a rectangle

$d = \sqrt{l^{2} + w^{2}}$

The diagonal is the hypotenuse of a right triangle with legs $l$ and $w$. Both diagonals are equal.

Area of a path around a rectangle

$(l + 2x)(w + 2x) - lw$

Area of a uniform border of width $x$ outside an $l$ by $w$ rectangle: outer rectangle minus inner rectangle.

Example: A $12,\text{cm}$ by $5,\text{cm}$ rectangle has area $60,\text{cm}^{2}$, perimeter $2(12 + 5) = 34,\text{cm}$ and diagonal $\sqrt{144 + 25} = 13,\text{cm}$.

Parallelogram, Rhombus, Trapezium And Kite Formulas

Formula

Expression

What it means

Area of a parallelogram

$A = b \times h$

$b$ is a base and $h$ is the perpendicular distance between that base and the opposite side, not the slanted side.

Area of a parallelogram from sides and angle

$A = ab\sin\theta$

$a$ and $b$ are adjacent sides and $\theta$ is the angle between them.

Perimeter of a parallelogram

$P = 2(a + b)$

Opposite sides are equal, so add the two adjacent sides $a$ and $b$ and double.

Diagonals of a parallelogram

$d_{1}^{2} + d_{2}^{2} = 2(a^{2} + b^{2})$

The parallelogram law: the squares of the diagonals add to twice the sum of the squares of the adjacent sides.

Area of a rhombus (rhombus formula)

$A = \frac{1}{2}d_{1}d_{2}$

$d_{1}$ and $d_{2}$ are the diagonals. The rule works because a rhombus has perpendicular diagonals.

Perimeter of a rhombus

$P = 4a$

All four sides of a rhombus are equal to $a$.

Side of a rhombus from its diagonals (diagonal of rhombus)

$a = \frac{1}{2}\sqrt{d_{1}^{2} + d_{2}^{2}}$

The diagonals bisect each other at right angles, so each side is the hypotenuse of a right triangle with legs $\frac{d_{1}}{2}$ and $\frac{d_{2}}{2}$.

Area of a trapezium (trapezoid)

$A = \frac{1}{2}(a + b)h$

$a$ and $b$ are the two parallel sides and $h$ is the perpendicular distance between them.

Midsegment of a trapezium

$m = \frac{a + b}{2}$

The segment joining the midpoints of the non-parallel sides. It is the mean of the parallel sides, and $A = mh$.

Diagonal of an isosceles trapezoid

$d = \sqrt{c^{2} + ab}$

$a$ and $b$ are the parallel sides and $c$ is each equal leg. Both diagonals have this length.

Area of a kite (properties of a kite)

$A = \frac{1}{2}d_{1}d_{2}$

$d_{1}$ and $d_{2}$ are the diagonals, which meet at right angles in every kite.

Perimeter of a kite

$P = 2(a + b)$

A kite has two pairs of equal adjacent sides, $a$ and $b$.

Area of any quadrilateral from a diagonal

$A = \frac{1}{2}d(h_{1} + h_{2})$

$d$ is one diagonal and $h_{1}$, $h_{2}$ are the perpendiculars to it from the other two vertices.

Angle sum of a quadrilateral (angles of quadrilateral)

$A + B + C + D = 360^{\circ}$

Any quadrilateral splits into two triangles along a diagonal, giving $2 \times 180^{\circ}$.

Example: A rhombus with diagonals $16,\text{cm}$ and $12,\text{cm}$ has area $\frac{1}{2} \times 16 \times 12 = 96,\text{cm}^{2}$, side $\frac{1}{2}\sqrt{256 + 144} = 10,\text{cm}$ and perimeter $40,\text{cm}$.

Regular Polygon Formulas

A regular polygon has $n$ equal sides of length $s$ and $n$ equal angles.

Formula

Expression

What it means

Area of a regular polygon (area of polygons)

$A = \frac{1}{2} \times P \times a$

$P$ is the perimeter and $a$ is the apothem, the perpendicular distance from the centre to a side.

Area of a regular polygon from its side

$A = \frac{ns^{2}}{4\tan\left(\frac{180^{\circ}}{n}\right)}$

Use when only the side $s$ and the number of sides $n$ are known.

Apothem

$a = \frac{s}{2\tan\left(\frac{180^{\circ}}{n}\right)}$

Distance from the centre to the midpoint of a side. It is also the radius of the inscribed circle.

Circumradius of a regular polygon

$R = \frac{s}{2\sin\left(\frac{180^{\circ}}{n}\right)}$

Distance from the centre to a vertex, which is the radius of the circle through all vertices.

Perimeter of a regular polygon

$P = ns$

Multiply the number of sides by the side length.

Area of a regular hexagon

$A = \frac{3\sqrt{3}}{2}s^{2}$

A regular hexagon splits into six equilateral triangles of side $s$, and its circumradius equals $s$.

Diagonals of a regular hexagon

$d_{\text{long}} = 2s$, $d_{\text{short}} = s\sqrt{3}$

The long diagonals pass through the centre. The short diagonals skip one vertex.

Area of a regular pentagon

$A = \frac{1}{4}\sqrt{5(5 + 2\sqrt{5})},s^{2} \approx 1.7205s^{2}$

Exact area of a regular pentagon with side $s$. Each interior angle is $108^{\circ}$.

Perimeter of a pentagon

$P = 5s$

For a regular pentagon. For an irregular one, add the five side lengths.

Area of a regular octagon

$A = 2(1 + \sqrt{2})s^{2} \approx 4.8284s^{2}$

Exact area of a regular octagon with side $s$. Each interior angle is $135^{\circ}$.

Example: A regular hexagon with side $4,\text{cm}$ has area $\frac{3\sqrt{3}}{2} \times 16 = 24\sqrt{3} \approx 41.57,\text{cm}^{2}$ and perimeter $24,\text{cm}$.

Circle Formulas

Formula

Expression

What it means

Diameter (diameter formula)

$d = 2r$

The diameter is a chord through the centre and is twice the radius $r$.

Circumference of a circle

$C = 2\pi r = \pi d$

The perimeter of a circle. Use $\pi \approx 3.1416$ or $\frac{22}{7}$ when the question says so.

Area of a circle (circle area formulas)

$A = \pi r^{2} = \frac{\pi d^{2}}{4}$

Area enclosed by a circle of radius $r$ or diameter $d$.

Area from the circumference

$A = \frac{C^{2}}{4\pi}$

Finds the area directly from a known circumference $C$, without first finding $r$.

Radius from the area

$r = \sqrt{\frac{A}{\pi}}$

Rearranged area formula for when the area is given and the radius is unknown.

Area of a semicircle (semicircle formulas)

$A = \frac{1}{2}\pi r^{2}$

Half of a full circle of radius $r$, cut along a diameter.

Perimeter of a semicircle

$P = \pi r + 2r$

The curved half of the circumference plus the straight diameter. Using $\pi r$ alone gives only the arc.

Area of a quadrant

$A = \frac{1}{4}\pi r^{2}$

A quarter circle, which is a sector with a central angle of $90^{\circ}$.

Perimeter of a quadrant

$P = \frac{\pi r}{2} + 2r$

One quarter of the circumference plus the two bounding radii.

Area of an annulus (ring)

$A = \pi(R^{2} - r^{2}) = \pi(R + r)(R - r)$

Area between two concentric circles with outer radius $R$ and inner radius $r$, where $R > r$.

Distance covered by a wheel

$D = N \times 2\pi r$

A wheel of radius $r$ travels one circumference per revolution, so $N$ revolutions cover $D$.

Example: A circle of radius $7,\text{cm}$ with $\pi = \frac{22}{7}$ has circumference $2 \times \frac{22}{7} \times 7 = 44,\text{cm}$ and area $\frac{22}{7} \times 49 = 154,\text{cm}^{2}$.

Arc, Sector, Segment And Chord Formulas

Here $\theta$ is the central angle. Use the degree forms when $\theta$ is in degrees and the radian forms when it is in radians.

Formula

Expression

What it means

Arc length (degrees)

$L = \frac{\theta}{360^{\circ}} \times 2\pi r$

On a circle of radius $r$, the arc is the same fraction of the circumference as $\theta$ is of a full turn.

Arc length (radians)

$L = r\theta$

The simplest form, valid only when $\theta$ is measured in radians.

Area of a sector (degrees)

$A = \frac{\theta}{360^{\circ}} \times \pi r^{2}$

A sector is the slice between two radii, so its area is that fraction of the full circle.

Area of a sector (radians)

$A = \frac{1}{2}r^{2}\theta = \frac{1}{2}Lr$

With $\theta$ in radians, or with arc length $L$ known and no angle needed.

Perimeter of a sector

$P = 2r + L$

Two radii plus the arc length. Students often forget the two straight edges.

Area of a segment (radians)

$A = \frac{1}{2}r^{2}(\theta - \sin\theta)$

The region between a chord and its arc, equal to the sector minus the triangle, with $\theta$ in radians.

Area of a segment (degrees)

$A = \frac{\theta}{360^{\circ}}\pi r^{2} - \frac{1}{2}r^{2}\sin\theta$

Same idea in degrees: sector area minus the area of the triangle formed by the two radii.

Chord length from the central angle

$c = 2r\sin\left(\frac{\theta}{2}\right)$

Length of the chord cut off by a central angle $\theta$ in a circle of radius $r$.

Chord length from its distance to the centre

$c = 2\sqrt{r^{2} - d^{2}}$

$d$ is the perpendicular distance from the centre to the chord, with $0 \leq d \leq r$. That perpendicular bisects the chord.

Central angle from arc length

$\theta = \frac{L}{r}$

Gives $\theta$ in radians. Multiply by $\frac{180^{\circ}}{\pi}$ to convert to degrees.

Example: With $r = 6,\text{cm}$ and $\theta = 60^{\circ}$, the arc is $\frac{60}{360} \times 12\pi = 2\pi \approx 6.28,\text{cm}$, the sector is $6\pi \approx 18.85,\text{cm}^{2}$ and the chord is $2 \times 6 \times \sin 30^{\circ} = 6,\text{cm}$.

Circle Theorems

Formula

Expression

What it means

Inscribed angle theorem

$\angle ACB = \frac{1}{2}\angle AOB$

An angle at the circle is half the angle at the centre $O$ standing on the same arc $AB$.

Angle in a semicircle

$\angle ACB = 90^{\circ}$

If $AB$ is a diameter, the angle it makes at any other point $C$ on the circle is a right angle.

Angles in the same segment (arcs and subtended angles)

$\angle ACB = \angle ADB$

Angles at $C$ and $D$ on the same side of chord $AB$, standing on the same arc, are equal.

Cyclic quadrilateral

$\angle A + \angle C = 180^{\circ}$, $\angle B + \angle D = 180^{\circ}$

When all four vertices lie on a circle, each pair of opposite angles is supplementary.

Brahmagupta's formula

$A = \sqrt{(s - a)(s - b)(s - c)(s - d)}$

Area of a cyclic quadrilateral with sides $a$, $b$, $c$, $d$ and semi-perimeter $s = \frac{a + b + c + d}{2}$.

Ptolemy's theorem

$AC \cdot BD = AB \cdot CD + AD \cdot BC$

In a cyclic quadrilateral $ABCD$, the product of the diagonals equals the sum of products of opposite sides.

Tangent perpendicular to radius

$OT \perp PT$

The tangent line $PT$ touching the circle at $T$ meets the radius $OT$ from centre $O$ at a right angle.

Tangents from an external point

$PA = PB = \sqrt{d^{2} - r^{2}}$

From a point $P$ at distance $d > r$ from the centre, both tangents to the circle have equal length.

Intersecting chords theorem

$AE \times EB = CE \times ED$

When chords $AB$ and $CD$ cross at $E$ inside the circle, the products of their parts are equal.

Tangent-secant theorem

$PT^{2} = PA \times PB$

From external point $P$, tangent $PT$ and a secant meeting the circle at $A$ (near) and $B$ (far).

Secant-secant theorem

$PA \times PB = PC \times PD$

Two secants from external point $P$ cut the circle at $A$, $B$ and $C$, $D$. Use whole secant lengths $PB$ and $PD$.

Alternate segment theorem

$\angle TAB = \angle ACB$

The angle between tangent $TA$ and chord $AB$ equals the inscribed angle at $C$ in the opposite segment.

Example: From a point $P$, a secant meets a circle at $A$ and $B$ with $PA = 4$ and $PB = 9$, so the tangent length is $PT = \sqrt{4 \times 9} = 6$.

Ellipse Formulas

Here $a$ is the semi-major axis and $b$ is the semi-minor axis, with $a \geq b > 0$.

Formula

Expression

What it means

Area of an ellipse

$A = \pi ab$

Exact area of an ellipse. It stretches the circle formula along two axes.

Perimeter of an ellipse (Ramanujan)

$P \approx \pi\left[3(a + b) - \sqrt{(3a + b)(a + 3b)}\right]$

No simple exact formula exists. This approximation is accurate to a tiny fraction of a percent for most ellipses.

Rough perimeter of an ellipse

$P \approx 2\pi\sqrt{\frac{a^{2} + b^{2}}{2}}$

A quicker estimate that works well when $a$ and $b$ are close in size.

Area of a semi-ellipse

$A = \frac{1}{2}\pi ab$

Half of an ellipse cut along either axis.

Circle as a special case

$a = b = r \Rightarrow A = \pi r^{2}$

When both semi-axes are equal, the ellipse is a circle and the formulas reduce to the circle forms.

Area of an elliptical ring

$A = \pi(ab - cd)$

Region between an outer ellipse with semi-axes $a$, $b$ and an inner ellipse with semi-axes $c$, $d$.

Example: For $a = 5$ and $b = 3$, the area is $15\pi \approx 47.12$ and the Ramanujan perimeter is $\pi(24 - \sqrt{252}) \approx \pi \times 8.1255 \approx 25.53$.

Cube And Cuboid Formulas

Formula

Expression

What it means

Volume of a cube (cube formula)

$V = a^{3}$

$a$ is the edge length. Volume is measured in cubic units.

Lateral surface area of a cube

$\text{LSA} = 4a^{2}$

Area of the four side faces only, leaving out the top and bottom.

Total surface area of a cube

$\text{TSA} = 6a^{2}$

Area of all six square faces of the cube.

Face diagonal of a cube

$a\sqrt{2}$

Diagonal across one square face, found from Pythagoras on two edges.

Space diagonal of a cube

$d = a\sqrt{3}$

Line through the centre joining opposite corners of the cube.

Edge of a cube from its volume

$a = \sqrt[3]{V}$

Take the cube root of the volume to recover the edge.

Volume of a cuboid (rectangular prism)

$V = l \times w \times h$

$l$, $w$ and $h$ are the length, width (breadth) and height in the same unit.

Lateral surface area of a cuboid

$\text{LSA} = 2h(l + w)$

Area of the four walls, as used for painting the walls of a room.

Total surface area of a cuboid

$\text{TSA} = 2(lw + wh + hl)$

Area of all six rectangular faces, which come in three equal pairs.

Space diagonal of a cuboid

$d = \sqrt{l^{2} + w^{2} + h^{2}}$

Longest straight rod that fits inside the box, joining opposite corners.

Total edge length

$4(l + w + h)$ for a cuboid, $12a$ for a cube

A cuboid has 12 edges, four each of length $l$, $w$ and $h$.

Example: A cuboid $3 \times 4 \times 12$ has $V = 144$, $\text{TSA} = 2(12 + 48 + 36) = 192$ and space diagonal $\sqrt{9 + 16 + 144} = 13$.

Cylinder Formulas

Formula

Expression

What it means

Volume of a cylinder

$V = \pi r^{2}h$

Base area $\pi r^{2}$ times height $h$. It also holds for an oblique cylinder if $h$ is the perpendicular height.

Curved surface area of a right circular cylinder

$\text{CSA} = 2\pi rh$

Area of the side only. Unrolled, it is a rectangle of width $2\pi r$ and height $h$.

Total surface area of a cylinder

$\text{TSA} = 2\pi r(r + h)$

Curved surface plus the two circular ends, $2\pi rh + 2\pi r^{2}$.

Volume of a hollow cylinder

$V = \pi(R^{2} - r^{2})h$

Volume of material in a pipe with outer radius $R$, inner radius $r$ and length $h$.

Total surface area of a hollow cylinder

$2\pi(R + r)h + 2\pi(R^{2} - r^{2})$

Outer and inner curved surfaces plus the two ring-shaped ends.

Height of a cylinder from its volume

$h = \frac{V}{\pi r^{2}}$

Rearranged volume formula, used for tank and container filling questions.

Example: A cylinder with $r = 7,\text{cm}$, $h = 10,\text{cm}$ and $\pi = \frac{22}{7}$ has $V = \frac{22}{7} \times 49 \times 10 = 1540,\text{cm}^{3}$, $\text{CSA} = 440,\text{cm}^{2}$ and $\text{TSA} = 440 + 308 = 748,\text{cm}^{2}$.

Cone And Frustum Formulas

For a frustum, $R$ and $r$ are the radii of the two circular ends and $h$ is the perpendicular height.

Formula

Expression

What it means

Volume of a cone

$V = \frac{1}{3}\pi r^{2}h$

One third of a cylinder with the same base radius $r$ and height $h$.

Slant height of a right circular cone

$l = \sqrt{r^{2} + h^{2}}$

Distance from the apex to the edge of the base, found from the right triangle formed by $r$, $h$ and $l$.

Curved surface area of a cone

$\text{CSA} = \pi rl$

Area of the sloping surface only. It uses the slant height $l$, not the vertical height.

Total surface area of a cone

$\text{TSA} = \pi r(l + r)$

Curved surface plus the circular base, $\pi rl + \pi r^{2}$.

Cone made from a sector

$l = \text{sector radius}$, $r = \frac{\theta}{360^{\circ}} \times l$

Rolling a sector of angle $\theta$ into a cone turns the sector radius into $l$ and the arc into the base circumference.

Volume of a frustum of a cone

$V = \frac{1}{3}\pi h(R^{2} + Rr + r^{2})$

Volume of a cone with its top cut off parallel to the base, such as a bucket or lampshade.

Slant height of a frustum

$l = \sqrt{h^{2} + (R - r)^{2}}$

Found from a right triangle with legs $h$ and $R - r$.

Curved surface area of a frustum

$\text{CSA} = \pi l(R + r)$

Area of the sloping side of the frustum only.

Total surface area of a frustum

$\text{TSA} = \pi l(R + r) + \pi R^{2} + \pi r^{2}$

Curved surface plus both circular ends. Drop $\pi r^{2}$ for an open-topped bucket.

Example: A cone with $r = 3$ and $h = 4$ has $l = 5$, $V = \frac{1}{3}\pi \times 9 \times 4 = 12\pi \approx 37.70$, $\text{CSA} = 15\pi \approx 47.12$ and $\text{TSA} = 24\pi \approx 75.40$.

Sphere And Hemisphere Formulas

Formula

Expression

What it means

Volume of a sphere

$V = \frac{4}{3}\pi r^{3}$

$r$ is the radius. The volume grows with the cube of the radius.

Surface area of a sphere

$A = 4\pi r^{2}$

Equal to four times the area of a great circle of the same radius.

Volume of a hemisphere

$V = \frac{2}{3}\pi r^{3}$

Half the volume of a sphere of radius $r$.

Curved surface area of a hemisphere

$\text{CSA} = 2\pi r^{2}$

Area of the dome only, which is half the sphere's surface.

Total surface area of a hemisphere

$\text{TSA} = 3\pi r^{2}$

Curved dome $2\pi r^{2}$ plus the flat circular base $\pi r^{2}$.

Volume of a spherical shell

$V = \frac{4}{3}\pi(R^{3} - r^{3})$

Material in a hollow ball with outer radius $R$ and inner radius $r$.

Volume of a spherical cap

$V = \frac{1}{3}\pi h^{2}(3r - h)$

A cap of height $h$ cut from a sphere of radius $r$, with $0 < h \leq 2r$.

Curved surface area of a spherical cap

$A = 2\pi rh$

Area of the curved part of a cap of height $h$ on a sphere of radius $r$.

Volume of an ellipsoid

$V = \frac{4}{3}\pi abc$

$a$, $b$ and $c$ are the three semi-axes. It becomes the sphere formula when all three equal $r$.

Radius of a sphere from its volume

$r = \sqrt[3]{\frac{3V}{4\pi}}$

Rearranged volume formula for when the volume is known.

Example: A sphere of radius $3,\text{cm}$ has volume $\frac{4}{3}\pi \times 27 = 36\pi \approx 113.10,\text{cm}^{3}$ and surface area $4\pi \times 9 = 36\pi \approx 113.10,\text{cm}^{2}$.

Prism And Pyramid Formulas

In these rows, $B$ is the area of the base and $P$ is the perimeter of the base.

Formula

Expression

What it means

Volume of a prism

$V = B \times h$

Base area times the perpendicular height $h$ between the two identical end faces.

Lateral surface area of a prism (lateral area formula)

$\text{LSA} = P \times h$

For a right prism, the side faces are rectangles whose total area is the base perimeter times height.

Total surface area of a prism

$\text{TSA} = Ph + 2B$

Lateral area plus the two congruent end faces.

Volume of a triangular prism

$V = \frac{1}{2}bh_{t} \times l$

$b$ and $h_{t}$ are the base and height of the triangular face, and $l$ is the length of the prism.

Volume of a pyramid

$V = \frac{1}{3}Bh$

One third of the prism with the same base and height. $h$ is the perpendicular height to the apex.

Lateral surface area of a regular pyramid

$\text{LSA} = \frac{1}{2}Pl$

$l$ is the slant height of each triangular face, measured from the apex to the midpoint of a base edge.

Total surface area of a regular pyramid

$\text{TSA} = \frac{1}{2}Pl + B$

Area of all the triangular side faces plus the area $B$ of the base.

Square pyramid

$V = \frac{1}{3}a^{2}h$, $l = \sqrt{h^{2} + \frac{a^{2}}{4}}$

$a$ is the base edge, $h$ the height and $l$ the slant height of each face.

Total surface area of a square pyramid

$\text{TSA} = a^{2} + 2al$

Square base $a^{2}$ plus four triangles of area $\frac{1}{2}al$ each.

Volume of a frustum of a pyramid

$V = \frac{h}{3}\left(B_{1} + B_{2} + \sqrt{B_{1}B_{2}}\right)$

$B_{1}$ and $B_{2}$ are the areas of the two parallel faces and $h$ is the perpendicular height between them.

Regular tetrahedron (triangular pyramid)

$V = \frac{a^{3}}{6\sqrt{2}}$, $\text{TSA} = \sqrt{3}a^{2}$

A pyramid whose four faces are equilateral triangles with edge $a$.

Example: A square pyramid with base edge $10$ and height $12$ has slant height $l = \sqrt{144 + 25} = 13$, volume $\frac{1}{3} \times 100 \times 12 = 400$ and $\text{TSA} = 100 + 2 \times 10 \times 13 = 360$.

Euler's Formula For Polyhedra

The formula holds for every convex polyhedron, where $V$, $E$ and $F$ count its vertices, edges and faces.

Formula

Expression

What it means

Euler's formula for a polyhedron

$V - E + F = 2$

Vertices minus edges plus faces always equals 2 for a convex solid. Use it to find one count from the other two.

Edges from the faces

$E = \frac{1}{2} \sum (\text{sides of each face})$

Each edge is shared by exactly two faces, so adding the sides of all faces counts every edge twice.

Tetrahedron

$V = 4$, $E = 6$, $F = 4$

Four triangular faces. Check: $4 - 6 + 4 = 2$.

Cube (hexahedron)

$V = 8$, $E = 12$, $F = 6$

Six square faces. Check: $8 - 12 + 6 = 2$.

Octahedron

$V = 6$, $E = 12$, $F = 8$

Eight triangular faces, with four meeting at each vertex. Check: $6 - 12 + 8 = 2$.

Dodecahedron

$V = 20$, $E = 30$, $F = 12$

Twelve regular pentagon faces, with three meeting at each vertex.

Icosahedron

$V = 12$, $E = 30$, $F = 20$

Twenty triangular faces, with five meeting at each vertex.

Prism with an $n$-sided base

$V = 2n$, $E = 3n$, $F = n + 2$

Two $n$-gon ends plus $n$ rectangular sides. A triangular prism has 6 vertices, 9 edges and 5 faces.

Pyramid with an $n$-sided base

$V = n + 1$, $E = 2n$, $F = n + 1$

One $n$-gon base plus $n$ triangular faces meeting at the apex.

Example: A polyhedron with $12$ faces and $30$ edges has $V = 2 + E - F = 2 + 30 - 12 = 20$ vertices, which matches the dodecahedron.

Coordinate Geometry And Vector Formulas

Coordinate geometry turns points, lines and curves into equations, and vectors describe quantities that have both size and direction. This branch covers the coordinate geometry, conics, vectors and 3D geometry taught from Class 9 to Class 12, in precalculus, and for JEE and SAT.

Distance, Midpoint And Section Formulas

Formula

Expression

What it means

Distance formula in 2D

$d = \sqrt{(x_{2} - x_{1})^{2} + (y_{2} - y_{1})^{2}}$

Length of the segment joining $(x_{1}, y_{1})$ and $(x_{2}, y_{2})$, built from the Pythagorean theorem on the horizontal and vertical gaps.

Euclidean distance formula in 3D

$d = \sqrt{(x_{2} - x_{1})^{2} + (y_{2} - y_{1})^{2} + (z_{2} - z_{1})^{2}}$

Straight-line distance between two points in space. Add the squared gap along the $z$-axis to the 2D formula.

Midpoint formula

$M = \left(\frac{x_{1} + x_{2}}{2}, \frac{y_{1} + y_{2}}{2}\right)$

Point exactly halfway between two endpoints, found by averaging the $x$-coordinates and the $y$-coordinates separately.

Midpoint in 3D

$M = \left(\frac{x_{1} + x_{2}}{2}, \frac{y_{1} + y_{2}}{2}, \frac{z_{1} + z_{2}}{2}\right)$

The same averaging rule applied to all three coordinates of two endpoints in space.

Section formula (internal division)

$P = \left(\frac{mx_{2} + nx_{1}}{m + n}, \frac{my_{2} + ny_{1}}{m + n}\right)$

Point $P$ between $A(x_{1}, y_{1})$ and $B(x_{2}, y_{2})$ with $AP : PB = m : n$. Note that $m$ multiplies the coordinates of $B$.

Section formula (external division)

$P = \left(\frac{mx_{2} - nx_{1}}{m - n}, \frac{my_{2} - ny_{1}}{m - n}\right)$

Point on line $AB$ extended, outside the segment, with $AP : PB = m : n$. It needs $m \neq n$.

Section formula in 3D

$P = \left(\frac{mx_{2} + nx_{1}}{m + n}, \frac{my_{2} + ny_{1}}{m + n}, \frac{mz_{2} + nz_{1}}{m + n}\right)$

Internal division of a segment in space in the ratio $m : n$, with the same weights applied to the $z$-coordinates.

Ratio in which a line divides a segment

$\frac{m}{n} = -\frac{ax_{1} + by_{1} + c}{ax_{2} + by_{2} + c}$

Ratio in which the line $ax + by + c = 0$ cuts the segment from $(x_{1}, y_{1})$ to $(x_{2}, y_{2})$. A positive value means internal division.

Example: The point dividing $A(1, 2)$ and $B(7, 8)$ internally in the ratio $1 : 2$ is $\left(\frac{1 \cdot 7 + 2 \cdot 1}{3}, \frac{1 \cdot 8 + 2 \cdot 2}{3}\right) = (3, 4)$, and $AB = \sqrt{6^{2} + 6^{2}} = 6\sqrt{2} \approx 8.49$.

Triangle Centres And Area From Coordinates

In this table the vertices are $A(x_{1}, y_{1})$, $B(x_{2}, y_{2})$, $C(x_{3}, y_{3})$, and the side lengths are $a = BC$, $b = CA$, $c = AB$.

Formula

Expression

What it means

Centroid of a triangle

$G = \left(\frac{x_{1} + x_{2} + x_{3}}{3}, \frac{y_{1} + y_{2} + y_{3}}{3}\right)$

Meeting point of the three medians, found by averaging the vertices. It divides each median in the ratio $2 : 1$ from the vertex.

Incentre (incenter) of a triangle

$I = \left(\frac{ax_{1} + bx_{2} + cx_{3}}{a + b + c}, \frac{ay_{1} + by_{2} + cy_{3}}{a + b + c}\right)$

Centre of the inscribed circle, where the angle bisectors meet. Each vertex is weighted by the length of the side opposite it.

Excentre opposite $A$

$I_{1} = \left(\frac{-ax_{1} + bx_{2} + cx_{3}}{-a + b + c}, \frac{-ay_{1} + by_{2} + cy_{3}}{-a + b + c}\right)$

Centre of the circle touching side $BC$ and the extensions of $AB$ and $AC$. Flip the sign of the weight on $A$.

Circumcentre (circumcenter)

$(x - x_{1})^{2} + (y - y_{1})^{2} = (x - x_{2})^{2} + (y - y_{2})^{2} = (x - x_{3})^{2} + (y - y_{3})^{2}$

The point $(x, y)$ equidistant from all three vertices. Expand to get two linear equations. In a right triangle it is the midpoint of the hypotenuse.

Euler line relation

$G = \frac{H + 2O}{3}$

Orthocentre $H$, centroid $G$ and circumcentre $O$ are collinear, and $G$ divides $HO$ in the ratio $2 : 1$. Apply it coordinate by coordinate.

Area of a triangle from coordinates

$\text{Area} = \frac{1}{2}\lvert x_{1}(y_{2} - y_{3}) + x_{2}(y_{3} - y_{1}) + x_{3}(y_{1} - y_{2}) \rvert$

Area straight from the three vertices. The absolute value keeps the answer positive whatever order the vertices are listed in.

Shoelace formula for a polygon

$\text{Area} = \frac{1}{2}\left\lvert \sum_{k=1}^{n} (x_{k}y_{k+1} - x_{k+1}y_{k}) \right\rvert$

Area of a simple polygon with $n$ vertices listed in order around the boundary, taking $(x_{n+1}, y_{n+1}) = (x_{1}, y_{1})$.

Collinearity condition

$x_{1}(y_{2} - y_{3}) + x_{2}(y_{3} - y_{1}) + x_{3}(y_{1} - y_{2}) = 0$

Three points lie on one straight line exactly when the triangle they form has zero area. Equal slopes of $AB$ and $BC$ give the same test.

Example: For $A(1, 2)$, $B(4, 6)$, $C(7, 2)$, the area is $\frac{1}{2}\lvert 1(6 - 2) + 4(2 - 2) + 7(2 - 6) \rvert = \frac{1}{2}\lvert -24 \rvert = 12$ square units, and the centroid is $\left(4, \frac{10}{3}\right)$.

Slope And Angle Between Lines

Formula

Expression

What it means

Slope from two points

$m = \frac{y_{2} - y_{1}}{x_{2} - x_{1}}$

Rise over run between $(x_{1}, y_{1})$ and $(x_{2}, y_{2})$. It needs $x_{1} \neq x_{2}$, because a vertical line has undefined slope.

Slope from the angle of inclination

$m = \tan\theta$

$\theta$ is the angle the line makes with the positive $x$-axis, measured anticlockwise, with $0^{\circ} \leq \theta < 180^{\circ}$ and $\theta \neq 90^{\circ}$.

Slope from the general equation

$m = -\frac{a}{b}$

Slope of the line $ax + by + c = 0$ when $b \neq 0$. If $b = 0$ the line is vertical.

Angle between two lines

$\tan\theta = \left\lvert \frac{m_{1} - m_{2}}{1 + m_{1}m_{2}} \right\rvert$

Acute angle $\theta$ between lines with slopes $m_{1}$ and $m_{2}$. If $m_{1}m_{2} = -1$ the lines are perpendicular and $\theta = 90^{\circ}$.

Angle between lines in general form

$\cos\theta = \frac{\lvert a_{1}a_{2} + b_{1}b_{2} \rvert}{\sqrt{a_{1}^{2} + b_{1}^{2}}\sqrt{a_{2}^{2} + b_{2}^{2}}}$

Acute angle between $a_{1}x + b_{1}y + c_{1} = 0$ and $a_{2}x + b_{2}y + c_{2} = 0$. It works even when a line is vertical.

Parallel lines (slope test)

$m_{1} = m_{2}$

Two non-vertical lines are parallel exactly when their slopes are equal.

Perpendicular lines (slope test)

$m_{1}m_{2} = -1$

Two lines, neither of them vertical, meet at a right angle exactly when the product of their slopes is $-1$.

Parallel lines in general form

$a_{1}b_{2} = a_{2}b_{1}$

Condition for $a_{1}x + b_{1}y + c_{1} = 0$ and $a_{2}x + b_{2}y + c_{2} = 0$ to be parallel. If the constants share that ratio, the lines coincide.

Perpendicular lines in general form

$a_{1}a_{2} + b_{1}b_{2} = 0$

Condition for the two lines above to be perpendicular, read from their normal vectors $(a_{1}, b_{1})$ and $(a_{2}, b_{2})$.

Example: For slopes $m_{1} = 2$ and $m_{2} = \frac{1}{3}$, $\tan\theta = \left\lvert \frac{2 - \frac{1}{3}}{1 + \frac{2}{3}} \right\rvert = \frac{5/3}{5/3} = 1$, so the acute angle between the lines is $45^{\circ}$.

Straight Line Forms And Conditions

Formula

Expression

What it means

Normal (perpendicular) form

$x\cos\alpha + y\sin\alpha = p$

$p \geq 0$ is the perpendicular distance from the origin to the line, and $\alpha$ is the angle that perpendicular makes with the positive $x$-axis.

Parametric (distance) form

$\frac{x - x_{1}}{\cos\theta} = \frac{y - y_{1}}{\sin\theta} = r$

The point $(x_{1} + r\cos\theta, y_{1} + r\sin\theta)$ lies at signed distance $r$ from $(x_{1}, y_{1})$ along a line inclined at $\theta$.

Line parallel to a given line

$ax + by + k = 0$

Every line parallel to $ax + by + c = 0$ keeps $a$ and $b$ and changes only the constant. Find $k$ from one point on it.

Line perpendicular to a given line

$bx - ay + k = 0$

Every line perpendicular to $ax + by + c = 0$. Swap the coefficients of $x$ and $y$ and change one sign, then find $k$.

Point of intersection of two lines

$\left(\frac{b_{1}c_{2} - b_{2}c_{1}}{a_{1}b_{2} - a_{2}b_{1}}, \frac{c_{1}a_{2} - c_{2}a_{1}}{a_{1}b_{2} - a_{2}b_{1}}\right)$

Where $a_{1}x + b_{1}y + c_{1} = 0$ meets $a_{2}x + b_{2}y + c_{2} = 0$, valid when $a_{1}b_{2} \neq a_{2}b_{1}$, that is, the lines are not parallel.

Family of lines through an intersection

$(a_{1}x + b_{1}y + c_{1}) + \lambda(a_{2}x + b_{2}y + c_{2}) = 0$

Any line through the meeting point of the two given lines, except the second line itself. One more condition fixes the value of $\lambda$.

Concurrency of three lines

$a_{1}(b_{2}c_{3} - b_{3}c_{2}) - b_{1}(a_{2}c_{3} - a_{3}c_{2}) + c_{1}(a_{2}b_{3} - a_{3}b_{2}) = 0$

Three lines $a_{i}x + b_{i}y + c_{i} = 0$, no two of them parallel, pass through one point exactly when this coefficient determinant equals zero.

Side of a line on which a point lies

$\text{sign of } ax_{1} + by_{1} + c$

Two points are on the same side of $ax + by + c = 0$ when substituting them gives values of the same sign, and on opposite sides otherwise.

Angle bisectors of two lines

$\frac{a_{1}x + b_{1}y + c_{1}}{\sqrt{a_{1}^{2} + b_{1}^{2}}} = \pm \frac{a_{2}x + b_{2}y + c_{2}}{\sqrt{a_{2}^{2} + b_{2}^{2}}}$

The two lines that bisect the angles between the given lines. Every point on them is equidistant from both lines.

Pair of straight lines through the origin

$ax^{2} + 2hxy + by^{2} = 0$

Represents two lines through the origin when $h^{2} \geq ab$. The acute angle between them satisfies $\tan\theta = \frac{2\sqrt{h^{2} - ab}}{\lvert a + b \rvert}$.

Example: The line through $(2, 3)$ parallel to $3x - 4y + 5 = 0$ is $3x - 4y + k = 0$ with $6 - 12 + k = 0$, so $k = 6$ and the line is $3x - 4y + 6 = 0$.

Distance From A Line, Foot Of Perpendicular And Reflection

Formula

Expression

What it means

Distance of a point from a line

$d = \frac{\lvert ax_{1} + by_{1} + c \rvert}{\sqrt{a^{2} + b^{2}}}$

Shortest (perpendicular) distance from the point $(x_{1}, y_{1})$ to the line $ax + by + c = 0$.

Distance between parallel lines

$d = \frac{\lvert c_{1} - c_{2} \rvert}{\sqrt{a^{2} + b^{2}}}$

Gap between $ax + by + c_{1} = 0$ and $ax + by + c_{2} = 0$. Scale one equation first so the $x$ and $y$ coefficients match.

Distance between parallel lines in slope form

$d = \frac{\lvert c_{1} - c_{2} \rvert}{\sqrt{1 + m^{2}}}$

Gap between the parallel lines $y = mx + c_{1}$ and $y = mx + c_{2}$.

Foot of the perpendicular

$\frac{h - x_{1}}{a} = \frac{k - y_{1}}{b} = -\frac{ax_{1} + by_{1} + c}{a^{2} + b^{2}}$

$(h, k)$ is the point on $ax + by + c = 0$ nearest to $(x_{1}, y_{1})$. If $a$ or $b$ is $0$, that coordinate stays unchanged.

Image (reflection) of a point in a line

$\frac{h - x_{1}}{a} = \frac{k - y_{1}}{b} = -\frac{2(ax_{1} + by_{1} + c)}{a^{2} + b^{2}}$

Mirror image $(h, k)$ of $(x_{1}, y_{1})$ in $ax + by + c = 0$. The foot of the perpendicular is the midpoint of the point and its image.

Reflection in the axes and in $y = x$

$(x, y) \to (x, -y), (-x, y), (y, x)$

Images of the point $(x, y)$ in the $x$-axis, the $y$-axis and the line $y = x$, in that order.

Area cut off by a line and the axes

$\text{Area} = \frac{c^{2}}{2\lvert ab \rvert}$

Area of the triangle formed by $ax + by + c = 0$ and the two coordinate axes, with $a \neq 0$ and $b \neq 0$.

Example: The distance from $(3, 4)$ to $3x + 4y - 10 = 0$ is $\frac{\lvert 9 + 16 - 10 \rvert}{\sqrt{9 + 16}} = \frac{15}{5} = 3$ units.

Equation Of A Circle

Formula

Expression

What it means

Equation of a circle (centre-radius form)

$(x - h)^{2} + (y - k)^{2} = r^{2}$

Circle with centre $(h, k)$ and radius $r > 0$. Every point on it is at distance $r$ from the centre.

General form of a circle

$x^{2} + y^{2} + 2gx + 2fy + c = 0$

Expanded form. The coefficients of $x^{2}$ and $y^{2}$ are equal and there is no $xy$ term.

Centre of a circle and radius from the general form

$(-g, -f)$ and $r = \sqrt{g^{2} + f^{2} - c}$

Read these off the general form. The circle is real only if $g^{2} + f^{2} - c > 0$, and shrinks to a point if it equals $0$.

Diameter form

$(x - x_{1})(x - x_{2}) + (y - y_{1})(y - y_{2}) = 0$

Circle that has the segment from $(x_{1}, y_{1})$ to $(x_{2}, y_{2})$ as a diameter.

Parametric form

$x = h + r\cos\theta$, $y = k + r\sin\theta$

Gives every point of the circle as $\theta$ runs over $0 \leq \theta < 2\pi$. Useful when a point moves around the circle.

Position of a point

$S_{1} = x_{1}^{2} + y_{1}^{2} + 2gx_{1} + 2fy_{1} + c$

Substitute the point into the general form. $S_{1} < 0$ means inside, $S_{1} = 0$ on the circle and $S_{1} > 0$ outside.

Tangent at a point on the circle

$xx_{1} + yy_{1} = r^{2}$

Tangent to $x^{2} + y^{2} = r^{2}$ at $(x_{1}, y_{1})$. For the general form use $xx_{1} + yy_{1} + g(x + x_{1}) + f(y + y_{1}) + c = 0$.

Condition of tangency

$c^{2} = r^{2}(1 + m^{2})$

The line $y = mx + c$ touches $x^{2} + y^{2} = r^{2}$ exactly when this holds, which gives the tangents $y = mx \pm r\sqrt{1 + m^{2}}$.

Length of the tangent from an external point

$L = \sqrt{S_{1}}$

Tangent length from an outside point $(x_{1}, y_{1})$ to the point of contact. Equivalently $\sqrt{d^{2} - r^{2}}$, with $d$ the distance to the centre.

Chord of contact

$xx_{1} + yy_{1} = r^{2}$

For an external point $(x_{1}, y_{1})$, this is the chord joining the two points where its tangents touch $x^{2} + y^{2} = r^{2}$.

Orthogonal circles

$2g_{1}g_{2} + 2f_{1}f_{2} = c_{1} + c_{2}$

Two circles in general form cut each other at right angles exactly when this holds, equivalently $d^{2} = r_{1}^{2} + r_{2}^{2}$ for centre distance $d$.

Example: For $x^{2} + y^{2} - 6x + 4y - 12 = 0$, $g = -3$ and $f = 2$, so the centre is $(3, -2)$ and $r = \sqrt{9 + 4 + 12} = 5$.

Parabola

Unless a row says otherwise, the parabola is $y^{2} = 4ax$ with $a > 0$, which opens to the right.

Formula

Expression

What it means

Parabola in standard form

$y^{2} = 4ax$

Vertex at the origin and axis along the $x$-axis. It is the set of points equally far from the focus and the directrix.

Focus of parabola

$(a, 0)$

Fixed point inside the curve on its axis, at distance $a$ from the vertex.

Directrix of parabola

$x = -a$

Fixed line perpendicular to the axis, at distance $a$ from the vertex on the side away from the focus.

Latus rectum of parabola

$\text{length} = 4a$

Focal chord perpendicular to the axis, with endpoints $(a, 2a)$ and $(a, -2a)$.

Other standard orientations

$y^{2} = -4ax$, $x^{2} = 4ay$, $x^{2} = -4ay$

Parabolas opening left with focus $(-a, 0)$, up with focus $(0, a)$ and down with focus $(0, -a)$. The directrix is always opposite the focus.

Parabola with vertex $(h, k)$

$(y - k)^{2} = 4a(x - h)$

Right-opening parabola shifted so the vertex is $(h, k)$, with focus $(h + a, k)$ and directrix $x = h - a$.

Parametric form

$x = at^{2}$, $y = 2at$

The point with parameter $t$ on $y^{2} = 4ax$. Each real value of $t$ gives exactly one point of the curve.

Focal distance of a point

$PS = x_{1} + a$

Distance from a point $P(x_{1}, y_{1})$ on the parabola to the focus $S$, which equals its distance from the directrix.

Tangent at a point

$yy_{1} = 2a(x + x_{1})$

Tangent to $y^{2} = 4ax$ at the point $(x_{1}, y_{1})$ on the curve.

Tangent in slope form

$y = mx + \frac{a}{m}$

Tangent to $y^{2} = 4ax$ with slope $m \neq 0$. It touches the curve at $\left(\frac{a}{m^{2}}, \frac{2a}{m}\right)$.

Normal in slope form

$y = mx - 2am - am^{3}$

Normal to $y^{2} = 4ax$ with slope $m$, meeting the curve at $(am^{2}, -2am)$.

Eccentricity of parabola

$e = 1$

Every point is exactly as far from the focus as from the directrix, so the ratio of the two distances is $1$.

Example: For $y^{2} = 12x$, $4a = 12$ gives $a = 3$, so the focus is $(3, 0)$, the directrix is $x = -3$ and the latus rectum has length $12$.

Ellipse

Formula

Expression

What it means

Ellipse in standard form

$\frac{x^{2}}{a^{2}} + \frac{y^{2}}{b^{2}} = 1$

Centre at the origin with $a > b > 0$. The major axis lies along the $x$-axis, $a$ is the semi-major axis and $b$ the semi-minor axis.

Focus distance relation

$c^{2} = a^{2} - b^{2}$

$c$ is the distance from the centre to each focus. Since $a > b$, the foci lie inside the ellipse with $c < a$.

Foci of ellipse

$(\pm c, 0)$

Two fixed points on the major axis, one on each side of the centre.

Eccentricity of ellipse

$e = \frac{c}{a} = \sqrt{1 - \frac{b^{2}}{a^{2}}}$

Measures how stretched the ellipse is, with $0 < e < 1$. Values near $0$ look almost like a circle.

Vertex of ellipse (vertices)

$(\pm a, 0)$

Ends of the major axis, of length $2a$. The ends of the minor axis, of length $2b$, are $(0, \pm b)$.

Directrices

$x = \pm \frac{a}{e}$

Two lines perpendicular to the major axis, outside the ellipse, one paired with each focus.

Latus rectum of ellipse

$\text{length} = \frac{2b^{2}}{a}$

Length of the focal chord through either focus, perpendicular to the major axis.

Sum of focal distances

$PF_{1} + PF_{2} = 2a$

Defining property of every point $P$ on the ellipse. For $P$ with abscissa $x_{1}$, the distances are $a - ex_{1}$ and $a + ex_{1}$.

Vertical ellipse

$\frac{x^{2}}{b^{2}} + \frac{y^{2}}{a^{2}} = 1$

With $a > b$, the major axis lies along the $y$-axis and the foci are $(0, \pm c)$, still with $c^{2} = a^{2} - b^{2}$.

Ellipse with centre $(h, k)$

$\frac{(x - h)^{2}}{a^{2}} + \frac{(y - k)^{2}}{b^{2}} = 1$

The standard ellipse shifted so its centre is $(h, k)$. The foci move to $(h \pm c, k)$.

Parametric form

$x = a\cos\theta$, $y = b\sin\theta$

The point with eccentric angle $\theta$ on the ellipse, for $0 \leq \theta < 2\pi$.

Tangent at a point

$\frac{xx_{1}}{a^{2}} + \frac{yy_{1}}{b^{2}} = 1$

Tangent at $(x_{1}, y_{1})$ on the ellipse. In slope form the tangents are $y = mx \pm \sqrt{a^{2}m^{2} + b^{2}}$.

Example: For $\frac{x^{2}}{25} + \frac{y^{2}}{9} = 1$, $a = 5$, $b = 3$ and $c = \sqrt{25 - 9} = 4$, so the foci are $(\pm 4, 0)$, $e = \frac{4}{5} = 0.8$ and the latus rectum is $\frac{2 \times 9}{5} = 3.6$.

Hyperbola

Compared with the ellipse, the equation has a minus sign and the focus relation has a plus sign.

Formula

Expression

What it means

Hyperbola in standard form

$\frac{x^{2}}{a^{2}} - \frac{y^{2}}{b^{2}} = 1$

Centre at the origin, $a > 0$, $b > 0$, transverse axis along the $x$-axis, with two branches opening left and right.

Focus distance relation

$c^{2} = a^{2} + b^{2}$

$c$ is the distance from the centre to each focus, so $c > a$ and the foci lie beyond the vertices.

Foci of hyperbola

$(\pm c, 0)$

Two fixed points on the transverse axis, each inside one branch.

Eccentricity of hyperbola

$e = \frac{c}{a} = \sqrt{1 + \frac{b^{2}}{a^{2}}}$

Always $e > 1$. A larger $e$ means the branches open more widely.

Vertex of hyperbola (vertices)

$(\pm a, 0)$

Where the branches cross the transverse axis. The transverse axis has length $2a$ and the conjugate axis has length $2b$.

Asymptotes

$y = \pm \frac{b}{a}x$

Lines that the branches approach but never touch as $x$ grows. Setting the right side of the equation to $0$ gives them.

Directrices

$x = \pm \frac{a}{e}$

Two lines perpendicular to the transverse axis, between the centre and the vertices, one for each focus.

Latus rectum

$\text{length} = \frac{2b^{2}}{a}$

Length of the focal chord through either focus, perpendicular to the transverse axis.

Difference of focal distances

$\lvert PF_{1} - PF_{2} \rvert = 2a$

Defining property of every point $P$ on the hyperbola, in contrast to the constant sum for an ellipse.

Vertical hyperbola

$\frac{y^{2}}{a^{2}} - \frac{x^{2}}{b^{2}} = 1$

Opens up and down, with foci $(0, \pm c)$ and asymptotes $y = \pm \frac{a}{b}x$.

Conjugate hyperbola

$\frac{x^{2}}{a^{2}} - \frac{y^{2}}{b^{2}} = -1$

Shares its asymptotes with the standard hyperbola. The two eccentricities satisfy $\frac{1}{e_{1}^{2}} + \frac{1}{e_{2}^{2}} = 1$.

Rectangular hyperbola

$x^{2} - y^{2} = a^{2}$

The case $a = b$, with perpendicular asymptotes and $e = \sqrt{2}$. Turning the axes clockwise through $45^{\circ}$ turns it into $xy = \frac{a^{2}}{2}$.

Tangent at a point

$\frac{xx_{1}}{a^{2}} - \frac{yy_{1}}{b^{2}} = 1$

Tangent at $(x_{1}, y_{1})$ on the hyperbola. In slope form, $y = mx \pm \sqrt{a^{2}m^{2} - b^{2}}$ with $a^{2}m^{2} > b^{2}$.

Example: For $\frac{x^{2}}{16} - \frac{y^{2}}{9} = 1$, $c = \sqrt{16 + 9} = 5$, so the foci are $(\pm 5, 0)$, $e = \frac{5}{4} = 1.25$ and the asymptotes are $y = \pm \frac{3}{4}x$.

Conic Sections And Transformation Of Axes

Formula

Expression

What it means

Eccentricity (focus-directrix definition)

$PS = e \cdot PM$

A conic is the path of a point $P$ whose distance $PS$ to a fixed focus is $e$ times its distance $PM$ to a fixed directrix.

Type of conic from eccentricity

$e = 0$, $0 < e < 1$, $e = 1$, $e > 1$

These give a circle, an ellipse, a parabola and a hyperbola, in that order.

General second-degree equation

$Ax^{2} + Bxy + Cy^{2} + Dx + Ey + F = 0$

Every conic in the plane, including shifted and rotated ones, has this form. The $xy$ term appears only when the axes of the conic are tilted.

Conic section type test

$B^{2} - 4AC$

For a non-degenerate conic, a negative value means an ellipse (a circle if $A = C$ and $B = 0$), zero means a parabola and positive means a hyperbola.

Rotation angle that removes the $xy$ term

$\cot 2\theta = \frac{A - C}{B}$

Turning the axes through this $\theta$, with $B \neq 0$, removes the $xy$ term so the conic can be written in standard form.

Shift of origin

$x = X + h$, $y = Y + k$

Moving the origin to $(h, k)$ without turning the axes. $(x, y)$ are old coordinates and $(X, Y)$ are new ones.

Rotation of axes

$x = X\cos\theta - Y\sin\theta$, $y = X\sin\theta + Y\cos\theta$

Old coordinates in terms of new ones when the axes are turned anticlockwise through $\theta$ about the origin.

Example: For $4x^{2} + 9y^{2} - 36 = 0$, $A = 4$, $B = 0$, $C = 9$ and $B^{2} - 4AC = -144 < 0$, so it is an ellipse, which is $\frac{x^{2}}{9} + \frac{y^{2}}{4} = 1$ in standard form.

Polar, Cylindrical And Spherical Coordinates

Formula

Expression

What it means

Polar to rectangular

$x = r\cos\theta$, $y = r\sin\theta$

Converts polar $(r, \theta)$ to Cartesian $(x, y)$, where $r$ is the distance from the pole and $\theta$ the angle from the positive $x$-axis.

Polar coordinates from rectangular

$r = \sqrt{x^{2} + y^{2}}$, $\tan\theta = \frac{y}{x}$

Converts $(x, y)$ to $(r, \theta)$. Pick $\theta$ in the quadrant of the point, because $\tan^{-1}$ alone gives only angles in $\left(-\frac{\pi}{2}, \frac{\pi}{2}\right)$.

Distance between two polar points

$d = \sqrt{r_{1}^{2} + r_{2}^{2} - 2r_{1}r_{2}\cos(\theta_{1} - \theta_{2})}$

The law of cosines on the triangle formed by the pole and the points $(r_{1}, \theta_{1})$ and $(r_{2}, \theta_{2})$.

Polar equation of a line

$r\cos(\theta - \alpha) = p$

Line at perpendicular distance $p$ from the pole, with that perpendicular at angle $\alpha$. It is the normal form written in polar terms.

Polar equations of circles

$r = a$, $r = 2a\cos\theta$

The first is a circle of radius $a$ centred at the pole. The second has radius $a$, centre $(a, 0)$ and passes through the pole.

Polar equation of a conic

$r = \frac{l}{1 + e\cos\theta}$

Conic with one focus at the pole, eccentricity $e$ and semi-latus rectum $l$. It is the standard form for orbit problems.

Cylindrical coordinates

$x = r\cos\theta$, $y = r\sin\theta$, $z = z$

A 3D system that uses polar coordinates in the $xy$-plane and keeps the height $z$. Suited to cylinders and shapes with an axis.

Spherical coordinates

$x = \rho\sin\phi\cos\theta$, $y = \rho\sin\phi\sin\theta$, $z = \rho\cos\phi$

$\rho$ is distance from the origin, $\phi$ the angle from the positive $z$-axis with $0 \leq \phi \leq \pi$, and $\theta$ the angle in the $xy$-plane.

Example: The polar point $\left(4, \frac{\pi}{3}\right)$ has $x = 4\cos\frac{\pi}{3} = 2$ and $y = 4\sin\frac{\pi}{3} = 2\sqrt{3} \approx 3.46$.

Vector Basics

Formula

Expression

What it means

Components of a vector

$\vec{a} = a_{1}\hat{i} + a_{2}\hat{j} + a_{3}\hat{k}$

$a_{1}$, $a_{2}$, $a_{3}$ are the parts of the vector along the $x$, $y$ and $z$ axes, and $\hat{i}$, $\hat{j}$, $\hat{k}$ are unit vectors along them.

Magnitude of a vector

$\lvert \vec{a} \rvert = \sqrt{a_{1}^{2} + a_{2}^{2} + a_{3}^{2}}$

Length of the vector, also written $\lVert \vec{a} \rVert$. In 2D, leave out $a_{3}$.

Unit vector

$\hat{a} = \frac{\vec{a}}{\lvert \vec{a} \rvert}$

Vector of length $1$ pointing the same way as $\vec{a}$, defined only for $\vec{a} \neq \vec{0}$.

Position vector of $B$ relative to $A$

$\overrightarrow{AB} = \vec{b} - \vec{a} = (x_{2} - x_{1})\hat{i} + (y_{2} - y_{1})\hat{j} + (z_{2} - z_{1})\hat{k}$

Vector from $A$ to $B$, where $\vec{a}$ and $\vec{b}$ are the position vectors of the two points. Always head minus tail.

Vector addition

$\vec{a} + \vec{b} = (a_{1} + b_{1})\hat{i} + (a_{2} + b_{2})\hat{j} + (a_{3} + b_{3})\hat{k}$

Add matching components. Geometrically this is the triangle law or the parallelogram law of addition.

Scalar multiple

$\lambda\vec{a} = \lambda a_{1}\hat{i} + \lambda a_{2}\hat{j} + \lambda a_{3}\hat{k}$

Multiplies the length by $\lvert \lambda \rvert$. The direction reverses when $\lambda < 0$.

Collinear vectors

$\vec{a} = \lambda\vec{b}$

Non-zero vectors are parallel exactly when one is a scalar multiple of the other, so $\frac{a_{1}}{b_{1}} = \frac{a_{2}}{b_{2}} = \frac{a_{3}}{b_{3}}$ when no $b_{i}$ is zero.

Section formula for vectors (internal)

$\vec{r} = \frac{m\vec{b} + n\vec{a}}{m + n}$

Position vector of the point dividing $AB$ internally in the ratio $m : n$.

Section formula for vectors (external)

$\vec{r} = \frac{m\vec{b} - n\vec{a}}{m - n}$

Position vector of the point dividing $AB$ externally in the ratio $m : n$, with $m \neq n$.

Midpoint and centroid in vector form

$\frac{\vec{a} + \vec{b}}{2}$, $\frac{\vec{a} + \vec{b} + \vec{c}}{3}$

Position vectors of the midpoint of $AB$ and of the centroid of triangle $ABC$.

Example: For $\vec{a} = 3\hat{i} - 4\hat{j} + 12\hat{k}$, $\lvert \vec{a} \rvert = \sqrt{9 + 16 + 144} = 13$, so $\hat{a} = \frac{3}{13}\hat{i} - \frac{4}{13}\hat{j} + \frac{12}{13}\hat{k}$.

Dot Product And Projection

Formula

Expression

What it means

Dot product (scalar product)

$\vec{a} \cdot \vec{b} = \lvert \vec{a} \rvert \lvert \vec{b} \rvert \cos\theta$

$\theta$ is the angle between the vectors, with $0 \leq \theta \leq \pi$. The result is a number, not a vector.

Dot product in components

$\vec{a} \cdot \vec{b} = a_{1}b_{1} + a_{2}b_{2} + a_{3}b_{3}$

Multiply matching components and add. This is how the dot product is worked out in practice.

Angle between two vectors

$\cos\theta = \frac{\vec{a} \cdot \vec{b}}{\lvert \vec{a} \rvert \lvert \vec{b} \rvert}$

Angle between two non-zero vectors. A negative dot product means the angle is obtuse.

Perpendicular vectors

$\vec{a} \cdot \vec{b} = 0$

Two non-zero vectors are perpendicular (orthogonal) exactly when their dot product is zero.

Dot products of unit vectors

$\hat{i} \cdot \hat{i} = \hat{j} \cdot \hat{j} = \hat{k} \cdot \hat{k} = 1$, $\hat{i} \cdot \hat{j} = \hat{j} \cdot \hat{k} = \hat{k} \cdot \hat{i} = 0$

The axis unit vectors have length $1$ and are mutually perpendicular, which is why the component formula works.

Dot product of a vector with itself

$\vec{a} \cdot \vec{a} = \lvert \vec{a} \rvert^{2}$

Gives the squared length. The dot product is also commutative, so $\vec{a} \cdot \vec{b} = \vec{b} \cdot \vec{a}$.

Square of a sum of vectors

$\lvert \vec{a} + \vec{b} \rvert^{2} = \lvert \vec{a} \rvert^{2} + \lvert \vec{b} \rvert^{2} + 2\vec{a} \cdot \vec{b}$

Finds the length of a resultant. For $\lvert \vec{a} - \vec{b} \rvert^{2}$, change the last sign to minus.

Scalar projection of $\vec{a}$ on $\vec{b}$

$\frac{\vec{a} \cdot \vec{b}}{\lvert \vec{b} \rvert}$

Signed length of the shadow of $\vec{a}$ along the direction of $\vec{b}$, for $\vec{b} \neq \vec{0}$.

Projection vector of $\vec{a}$ on $\vec{b}$

$\left(\frac{\vec{a} \cdot \vec{b}}{\lvert \vec{b} \rvert^{2}}\right)\vec{b}$

The part of $\vec{a}$ that points along $\vec{b}$, written as a vector.

Cauchy-Schwarz inequality

$\lvert \vec{a} \cdot \vec{b} \rvert \leq \lvert \vec{a} \rvert \lvert \vec{b} \rvert$

Follows from $\lvert \cos\theta \rvert \leq 1$. Equality holds only when the vectors are parallel or one of them is zero.

Work done by a constant force

$W = \vec{F} \cdot \vec{d}$

Work when force $\vec{F}$ moves an object through displacement $\vec{d}$, equal to $\lvert \vec{F} \rvert \lvert \vec{d} \rvert \cos\theta$.

Example: For $\vec{a} = 2\hat{i} + 2\hat{j} - \hat{k}$ and $\vec{b} = \hat{i} + 2\hat{j} + 2\hat{k}$, $\vec{a} \cdot \vec{b} = 2 + 4 - 2 = 4$ and both lengths are $3$, so $\cos\theta = \frac{4}{9}$ and $\theta \approx 63.61^{\circ}$.

Cross Product

Formula

Expression

What it means

Cross product of two vectors

$\vec{a} \times \vec{b} = \lvert \vec{a} \rvert \lvert \vec{b} \rvert \sin\theta,\hat{n}$

$\hat{n}$ is the unit vector perpendicular to both vectors, set by the right-hand rule, and $0 \leq \theta \leq \pi$ is the angle between them.

Magnitude of the cross product

$\lvert \vec{a} \times \vec{b} \rvert = \lvert \vec{a} \rvert \lvert \vec{b} \rvert \sin\theta$

Never negative. It equals the area of the parallelogram spanned by the two vectors.

Cross product in components

$\vec{a} \times \vec{b} = (a_{2}b_{3} - a_{3}b_{2})\hat{i} - (a_{1}b_{3} - a_{3}b_{1})\hat{j} + (a_{1}b_{2} - a_{2}b_{1})\hat{k}$

Expansion of the determinant with rows $\hat{i}, \hat{j}, \hat{k}$, then $a_{1}, a_{2}, a_{3}$, then $b_{1}, b_{2}, b_{3}$. Watch the minus sign on $\hat{j}$.

Anticommutative law

$\vec{a} \times \vec{b} = -(\vec{b} \times \vec{a})$

Swapping the order reverses the direction, so the cross product is not commutative.

Cross products of unit vectors

$\hat{i} \times \hat{j} = \hat{k}$, $\hat{j} \times \hat{k} = \hat{i}$, $\hat{k} \times \hat{i} = \hat{j}$

Cyclic order gives the third vector, reverse order gives its negative, and $\hat{i} \times \hat{i} = \hat{j} \times \hat{j} = \hat{k} \times \hat{k} = \vec{0}$.

Parallel vectors test

$\vec{a} \times \vec{b} = \vec{0}$

Two non-zero vectors are parallel exactly when their cross product is the zero vector.

Unit vector perpendicular to two vectors

$\hat{n} = \pm \frac{\vec{a} \times \vec{b}}{\lvert \vec{a} \times \vec{b} \rvert}$

The two unit vectors perpendicular to both $\vec{a}$ and $\vec{b}$, when $\vec{a}$ and $\vec{b}$ are not parallel.

Area of a parallelogram

$\text{Area} = \lvert \vec{a} \times \vec{b} \rvert$

Parallelogram with adjacent sides $\vec{a}$ and $\vec{b}$. With diagonals $\vec{d}{1}$ and $\vec{d}{2}$ it is $\frac{1}{2}\lvert \vec{d}{1} \times \vec{d}{2} \rvert$.

Area of a triangle in vector form

$\text{Area} = \frac{1}{2}\lvert \overrightarrow{AB} \times \overrightarrow{AC} \rvert$

Half the parallelogram on two sides of triangle $ABC$. It works for triangles in space too.

Lagrange's identity

$\lvert \vec{a} \times \vec{b} \rvert^{2} + (\vec{a} \cdot \vec{b})^{2} = \lvert \vec{a} \rvert^{2} \lvert \vec{b} \rvert^{2}$

Links the two products, because $\sin^{2}\theta + \cos^{2}\theta = 1$. Handy for finding one product from the other.

Example: For $\vec{a} = \hat{i} + 2\hat{j} + 3\hat{k}$ and $\vec{b} = 4\hat{i} + 5\hat{j} + 6\hat{k}$, $\vec{a} \times \vec{b} = (12 - 15)\hat{i} - (6 - 12)\hat{j} + (5 - 8)\hat{k} = -3\hat{i} + 6\hat{j} - 3\hat{k}$, so the parallelogram area is $\sqrt{54} \approx 7.35$.

Scalar And Vector Triple Products

Formula

Expression

What it means

Scalar triple product

$[\vec{a},\vec{b},\vec{c}] = \vec{a} \cdot (\vec{b} \times \vec{c})$

A number built from three vectors. It is positive when $\vec{a}$, $\vec{b}$, $\vec{c}$ form a right-handed set.

Scalar triple product in components

$a_{1}(b_{2}c_{3} - b_{3}c_{2}) - a_{2}(b_{1}c_{3} - b_{3}c_{1}) + a_{3}(b_{1}c_{2} - b_{2}c_{1})$

Value of the $3 \times 3$ determinant whose rows are the components of $\vec{a}$, $\vec{b}$ and $\vec{c}$.

Cyclic property

$\vec{a} \cdot (\vec{b} \times \vec{c}) = \vec{b} \cdot (\vec{c} \times \vec{a}) = \vec{c} \cdot (\vec{a} \times \vec{b})$

Rotating the order keeps the value, while swapping any two vectors changes its sign. The dot and cross can also be interchanged.

Volume of a parallelepiped

$V = \lvert [\vec{a},\vec{b},\vec{c}] \rvert$

Volume of the box whose three edges from one corner are $\vec{a}$, $\vec{b}$ and $\vec{c}$.

Volume of a tetrahedron

$V = \frac{1}{6}\lvert [\vec{a},\vec{b},\vec{c}] \rvert$

Tetrahedron with three edges $\vec{a}$, $\vec{b}$, $\vec{c}$ from one vertex, one sixth of the parallelepiped on the same edges.

Coplanarity condition

$[\vec{a},\vec{b},\vec{c}] = 0$

Three vectors lie in one plane exactly when the box they span has zero volume. For points $A, B, C, D$, test $\overrightarrow{AB}$, $\overrightarrow{AC}$, $\overrightarrow{AD}$.

Vector triple product

$\vec{a} \times (\vec{b} \times \vec{c}) = (\vec{a} \cdot \vec{c})\vec{b} - (\vec{a} \cdot \vec{b})\vec{c}$

The result lies in the plane of $\vec{b}$ and $\vec{c}$. Often remembered as "BAC minus CAB".

Vector triple product (other bracketing)

$(\vec{a} \times \vec{b}) \times \vec{c} = (\vec{a} \cdot \vec{c})\vec{b} - (\vec{b} \cdot \vec{c})\vec{a}$

Differs from the row above, so the cross product is not associative and the brackets matter.

Example: For $\vec{a} = \hat{i} + \hat{j}$, $\vec{b} = \hat{j} + \hat{k}$, $\vec{c} = \hat{i} + \hat{k}$, $[\vec{a},\vec{b},\vec{c}] = 1(1 - 0) - 1(0 - 1) + 0 = 2$, so the parallelepiped has volume $2$ cubic units.

Direction Cosines And Direction Ratios

Formula

Expression

What it means

Direction cosines

$l = \cos\alpha$, $m = \cos\beta$, $n = \cos\gamma$

$\alpha$, $\beta$, $\gamma$ are the angles a line or vector makes with the positive $x$, $y$ and $z$ axes.

Sum of squares of direction cosines

$l^{2} + m^{2} + n^{2} = 1$

True for every line, so two direction cosines fix the third up to its sign.

Direction cosines from direction ratios

$l = \frac{a}{\sqrt{a^{2} + b^{2} + c^{2}}}$, $m = \frac{b}{\sqrt{a^{2} + b^{2} + c^{2}}}$, $n = \frac{c}{\sqrt{a^{2} + b^{2} + c^{2}}}$

Direction ratios $a, b, c$ are any numbers proportional to $l, m, n$. Changing all three signs gives the opposite direction.

Direction ratios of a line through two points

$x_{2} - x_{1}, y_{2} - y_{1}, z_{2} - z_{1}$

For the line through $(x_{1}, y_{1}, z_{1})$ and $(x_{2}, y_{2}, z_{2})$. Divide by the distance between the points to get direction cosines.

Angle between two lines (direction cosines)

$\cos\theta = \lvert l_{1}l_{2} + m_{1}m_{2} + n_{1}n_{2} \rvert$

Acute angle between two lines with direction cosines $l_{1}, m_{1}, n_{1}$ and $l_{2}, m_{2}, n_{2}$.

Angle between two lines (direction ratios)

$\cos\theta = \frac{\lvert a_{1}a_{2} + b_{1}b_{2} + c_{1}c_{2} \rvert}{\sqrt{a_{1}^{2} + b_{1}^{2} + c_{1}^{2}}\sqrt{a_{2}^{2} + b_{2}^{2} + c_{2}^{2}}}$

The same acute angle when only direction ratios $a_{1}, b_{1}, c_{1}$ and $a_{2}, b_{2}, c_{2}$ are known.

Perpendicular and parallel lines in 3D

$a_{1}a_{2} + b_{1}b_{2} + c_{1}c_{2} = 0$, $\frac{a_{1}}{a_{2}} = \frac{b_{1}}{b_{2}} = \frac{c_{1}}{c_{2}}$

The first condition makes two lines perpendicular and the second makes them parallel.

Projection of a segment on a line

$\lvert (x_{2} - x_{1})l + (y_{2} - y_{1})m + (z_{2} - z_{1})n \rvert$

Length of the projection of the segment from $(x_{1}, y_{1}, z_{1})$ to $(x_{2}, y_{2}, z_{2})$ onto a line with direction cosines $l, m, n$.

Example: A line with direction ratios $2, -1, 2$ has $\sqrt{4 + 1 + 4} = 3$, so its direction cosines are $\frac{2}{3}, -\frac{1}{3}, \frac{2}{3}$, and $\frac{4}{9} + \frac{1}{9} + \frac{4}{9} = 1$.

Lines In 3D

Formula

Expression

What it means

Vector equation of a line

$\vec{r} = \vec{a} + \lambda\vec{b}$

Line through the point with position vector $\vec{a}$, parallel to $\vec{b}$. Each real $\lambda$ gives one point on it.

Cartesian (symmetric) form

$\frac{x - x_{1}}{a} = \frac{y - y_{1}}{b} = \frac{z - z_{1}}{c}$

Line through $(x_{1}, y_{1}, z_{1})$ with direction ratios $a, b, c$. A zero denominator means that coordinate stays fixed.

Parametric form

$x = x_{1} + a\lambda$, $y = y_{1} + b\lambda$, $z = z_{1} + c\lambda$

Every point of the line for real $\lambda$. Substitute these into a plane equation to find where a line meets a plane.

Line through two points (vector form)

$\vec{r} = \vec{a} + \lambda(\vec{b} - \vec{a})$

Line through the points with position vectors $\vec{a}$ and $\vec{b}$.

Line through two points (Cartesian form)

$\frac{x - x_{1}}{x_{2} - x_{1}} = \frac{y - y_{1}}{y_{2} - y_{1}} = \frac{z - z_{1}}{z_{2} - z_{1}}$

The same line in coordinates, using the coordinate differences as direction ratios.

Angle between two lines (vector form)

$\cos\theta = \frac{\lvert \vec{b}{1} \cdot \vec{b}{2} \rvert}{\lvert \vec{b}{1} \rvert \lvert \vec{b}{2} \rvert}$

Acute angle between $\vec{r} = \vec{a}{1} + \lambda\vec{b}{1}$ and $\vec{r} = \vec{a}{2} + \mu\vec{b}{2}$, from their direction vectors.

Shortest distance between skew lines

$d = \frac{\lvert (\vec{a}{2} - \vec{a}{1}) \cdot (\vec{b}{1} \times \vec{b}{2}) \rvert}{\lvert \vec{b}{1} \times \vec{b}{2} \rvert}$

Length of the common perpendicular between two lines that are neither parallel nor intersecting.

Distance between parallel lines in 3D

$d = \frac{\lvert \vec{b} \times (\vec{a}{2} - \vec{a}{1}) \rvert}{\lvert \vec{b} \rvert}$

Gap between the parallel lines $\vec{r} = \vec{a}{1} + \lambda\vec{b}$ and $\vec{r} = \vec{a}{2} + \mu\vec{b}$.

Condition for two lines to intersect

$(\vec{a}{2} - \vec{a}{1}) \cdot (\vec{b}{1} \times \vec{b}{2}) = 0$

Two non-parallel lines meet exactly when they are coplanar, which makes the shortest distance between them zero.

Distance from a point to a line in 3D

$d = \frac{\lvert (\vec{p} - \vec{a}) \times \vec{b} \rvert}{\lvert \vec{b} \rvert}$

Perpendicular distance from the point with position vector $\vec{p}$ to the line $\vec{r} = \vec{a} + \lambda\vec{b}$.

Example: For $\vec{r} = \hat{i} + \lambda(\hat{i} + \hat{j})$ and $\vec{r} = \hat{j} + 3\hat{k} + \mu(\hat{j} + \hat{k})$, $\vec{b}{1} \times \vec{b}{2} = \hat{i} - \hat{j} + \hat{k}$ and $\vec{a}{2} - \vec{a}{1} = -\hat{i} + \hat{j} + 3\hat{k}$, so $d = \frac{\lvert -1 - 1 + 3 \rvert}{\sqrt{3}} = \frac{1}{\sqrt{3}} \approx 0.58$.

Planes In 3D

Formula

Expression

What it means

Equation of a plane in normal form

$\vec{r} \cdot \hat{n} = d$

Plane at perpendicular distance $d \geq 0$ from the origin, where $\hat{n}$ is the unit normal pointing from the origin toward the plane.

Normal form in Cartesian coordinates

$lx + my + nz = d$

The same plane written with the direction cosines $l, m, n$ of its normal.

General form

$ax + by + cz + d = 0$

Any plane, with normal vector $a\hat{i} + b\hat{j} + c\hat{k}$, where $a$, $b$, $c$ are not all zero.

Point-normal form

$a(x - x_{1}) + b(y - y_{1}) + c(z - z_{1}) = 0$

Plane through $(x_{1}, y_{1}, z_{1})$ with normal direction ratios $a, b, c$. In vector form it reads $(\vec{r} - \vec{a}) \cdot \vec{n} = 0$.

Intercept form

$\frac{x}{a} + \frac{y}{b} + \frac{z}{c} = 1$

Plane cutting the axes at $(a, 0, 0)$, $(0, b, 0)$ and $(0, 0, c)$, with $a$, $b$, $c$ all non-zero.

Plane through three points

$(\vec{r} - \vec{a}) \cdot [(\vec{b} - \vec{a}) \times (\vec{c} - \vec{a})] = 0$

Plane through three non-collinear points with position vectors $\vec{a}$, $\vec{b}$, $\vec{c}$. The cross product supplies the normal.

Plane through the line of intersection of two planes

$(a_{1}x + b_{1}y + c_{1}z + d_{1}) + \lambda(a_{2}x + b_{2}y + c_{2}z + d_{2}) = 0$

Any plane containing the line where the two given planes meet. One more condition fixes $\lambda$.

Angle between two planes

$\cos\theta = \frac{\lvert a_{1}a_{2} + b_{1}b_{2} + c_{1}c_{2} \rvert}{\sqrt{a_{1}^{2} + b_{1}^{2} + c_{1}^{2}}\sqrt{a_{2}^{2} + b_{2}^{2} + c_{2}^{2}}}$

Acute angle between two planes, which is the angle between their normal vectors.

Parallel and perpendicular planes

$\frac{a_{1}}{a_{2}} = \frac{b_{1}}{b_{2}} = \frac{c_{1}}{c_{2}}$, $a_{1}a_{2} + b_{1}b_{2} + c_{1}c_{2} = 0$

The first condition makes the two planes parallel and the second makes them perpendicular.

Angle between a line and a plane

$\sin\phi = \frac{\lvert \vec{b} \cdot \vec{n} \rvert}{\lvert \vec{b} \rvert \lvert \vec{n} \rvert}$

Angle $\phi$ between a line with direction $\vec{b}$ and a plane with normal $\vec{n}$. Sine appears because $\phi$ is the complement of the angle with the normal.

Distance from a point to a plane

$D = \frac{\lvert ax_{1} + by_{1} + cz_{1} + d \rvert}{\sqrt{a^{2} + b^{2} + c^{2}}}$

Perpendicular distance from the point $(x_{1}, y_{1}, z_{1})$ to the plane $ax + by + cz + d = 0$.

Distance between two planes

$D = \frac{\lvert d_{1} - d_{2} \rvert}{\sqrt{a^{2} + b^{2} + c^{2}}}$

Gap between the parallel planes $ax + by + cz + d_{1} = 0$ and $ax + by + cz + d_{2} = 0$, with $a$, $b$, $c$ matched first.

Example: The distance from $(2, 3, -5)$ to the plane $x + 2y - 2z - 9 = 0$ is $\frac{\lvert 2 + 6 + 10 - 9 \rvert}{\sqrt{1 + 4 + 4}} = \frac{9}{3} = 3$ units.

Trigonometry Formulas

Trigonometry links angles to side lengths, first in right triangles and then for any angle on the unit circle. These formulas cover Grade 9 and 10 basics through the identities, triangle rules, inverse functions and equations tested in Grade 11 and 12, JEE, SAT and A level papers.

Basic Trigonometric Ratios (SOH CAH TOA)

Formula

Expression

What it means

Sin cos tan memory aid (SOH CAH TOA)

$\text{S} = \frac{\text{O}}{\text{H}}$, $\text{C} = \frac{\text{A}}{\text{H}}$, $\text{T} = \frac{\text{O}}{\text{A}}$

Sine is Opposite over Hypotenuse, Cosine is Adjacent over Hypotenuse, Tangent is Opposite over Adjacent, all measured from the chosen acute angle.

Sine

$\sin\theta = \frac{\text{opposite}}{\text{hypotenuse}}$

In a right triangle, the side facing angle $\theta$ divided by the hypotenuse, the side facing the right angle.

Cosine

$\cos\theta = \frac{\text{adjacent}}{\text{hypotenuse}}$

The side next to angle $\theta$ (not the hypotenuse) divided by the hypotenuse. Its value lies between 0 and 1 for acute angles.

Tangent

$\tan\theta = \frac{\text{opposite}}{\text{adjacent}}$

The side facing $\theta$ divided by the side next to it. Used for slopes, heights and gradients.

Cosecant (cosec or csc)

$\csc\theta = \frac{\text{hypotenuse}}{\text{opposite}}$

The sine ratio turned upside down. Indian textbooks write it as cosec, US and UK books often write csc.

Secant

$\sec\theta = \frac{\text{hypotenuse}}{\text{adjacent}}$

The cosine ratio turned upside down, defined only when the adjacent side is not zero.

Cotangent

$\cot\theta = \frac{\text{adjacent}}{\text{opposite}}$

The tangent ratio turned upside down, defined only when the opposite side is not zero.

Unit circle definition

$(x, y) = (\cos\theta, \sin\theta)$

The point at angle $\theta$ on a circle of radius 1 centred at the origin. This extends sine and cosine to every angle, not only acute ones.

Ratios for any point

$\sin\theta = \frac{y}{r}$, $\cos\theta = \frac{x}{r}$, $\tan\theta = \frac{y}{x}$

For a point $(x, y)$ on the terminal side of $\theta$, with $r = \sqrt{x^{2} + y^{2}}$ and $x \neq 0$ for tangent.

Example: In a right triangle with sides 3, 4 and hypotenuse 5, the angle opposite side 3 has $\sin\theta = \frac{3}{5} = 0.6$, $\cos\theta = \frac{4}{5} = 0.8$ and $\tan\theta = \frac{3}{4} = 0.75$.

Reciprocal And Quotient Identities

Each reciprocal ratio exists only where the ratio it inverts is not zero.

Formula

Expression

What it means

Cosecant as a reciprocal

$\csc\theta = \frac{1}{\sin\theta}$

Valid when $\sin\theta \neq 0$, so it is undefined at $0^{\circ}$, $180^{\circ}$ and $360^{\circ}$.

Secant as a reciprocal

$\sec\theta = \frac{1}{\cos\theta}$

Valid when $\cos\theta \neq 0$, so it is undefined at $90^{\circ}$ and $270^{\circ}$.

Cotangent as a reciprocal

$\cot\theta = \frac{1}{\tan\theta}$

Valid when $\tan\theta$ is defined and not zero. At $90^{\circ}$ use the quotient form instead, which gives $\cot 90^{\circ} = 0$.

Reciprocal identities in product form

$\sin\theta\csc\theta = 1$, $\cos\theta\sec\theta = 1$, $\tan\theta\cot\theta = 1$

Each ratio times its reciprocal equals 1. Handy for cancelling terms when simplifying an expression.

Tangent quotient identity

$\tan\theta = \frac{\sin\theta}{\cos\theta}$

Tangent is sine divided by cosine, valid whenever $\cos\theta \neq 0$. Used to rewrite everything in sine and cosine.

Cotangent quotient identity

$\cot\theta = \frac{\cos\theta}{\sin\theta}$

Cotangent is cosine divided by sine, valid whenever $\sin\theta \neq 0$.

Example: If $\sin\theta = 0.6$ and $\cos\theta = 0.8$, then $\csc\theta = \frac{1}{0.6} \approx 1.6667$, $\tan\theta = \frac{0.6}{0.8} = 0.75$ and $\cot\theta = \frac{0.8}{0.6} \approx 1.3333$.

Pythagorean Identities

Formula

Expression

What it means

Pythagorean identities (sine and cosine)

$\sin^{2}\theta + \cos^{2}\theta = 1$

True for every angle $\theta$. It is the Pythagorean theorem applied to the point $(\cos\theta, \sin\theta)$ on the unit circle.

Secant and tangent identity

$1 + \tan^{2}\theta = \sec^{2}\theta$

The first identity divided by $\cos^{2}\theta$, so it holds wherever $\cos\theta \neq 0$.

Cosecant and cotangent identity

$1 + \cot^{2}\theta = \csc^{2}\theta$

The first identity divided by $\sin^{2}\theta$, so it holds wherever $\sin\theta \neq 0$.

Sine from cosine

$\sin\theta = \pm\sqrt{1 - \cos^{2}\theta}$

Finds sine when cosine is known. Pick the sign from the quadrant of $\theta$.

Cosine from sine

$\cos\theta = \pm\sqrt{1 - \sin^{2}\theta}$

Finds cosine when sine is known. The sign is positive in quadrants I and IV.

Secant and tangent factor form

$(\sec\theta - \tan\theta)(\sec\theta + \tan\theta) = 1$

So $\sec\theta + \tan\theta$ and $\sec\theta - \tan\theta$ are reciprocals. A common step in board-exam proofs.

Cosecant and cotangent factor form

$(\csc\theta - \cot\theta)(\csc\theta + \cot\theta) = 1$

So $\csc\theta + \cot\theta$ and $\csc\theta - \cot\theta$ are reciprocals of each other.

Fourth powers

$\sin^{4}\theta + \cos^{4}\theta = 1 - 2\sin^{2}\theta\cos^{2}\theta$

Comes from squaring $\sin^{2}\theta + \cos^{2}\theta = 1$. Used when an expression has fourth powers of sine and cosine.

Example: If $\cos\theta = \frac{5}{13}$ with $\theta$ acute, then $\sin\theta = \sqrt{1 - \frac{25}{169}} = \sqrt{\frac{144}{169}} = \frac{12}{13}$ and $\tan\theta = \frac{12}{5} = 2.4$.

Trigonometric Values Of Standard Angles

Formula

Expression

What it means

Angle $0^{\circ}$ (0 rad)

$\sin 0^{\circ} = 0$, $\cos 0^{\circ} = 1$, $\tan 0^{\circ} = 0$

At zero angle the opposite side shrinks to nothing and the adjacent side equals the hypotenuse.

Angle $30^{\circ}$ ($\frac{\pi}{6}$)

$\sin 30^{\circ} = \frac{1}{2}$, $\cos 30^{\circ} = \frac{\sqrt{3}}{2}$, $\tan 30^{\circ} = \frac{1}{\sqrt{3}}$

From half of an equilateral triangle. As decimals, $\cos 30^{\circ} \approx 0.8660$ and $\tan 30^{\circ} \approx 0.5774$.

Angle $45^{\circ}$ ($\frac{\pi}{4}$)

$\sin 45^{\circ} = \frac{1}{\sqrt{2}}$, $\cos 45^{\circ} = \frac{1}{\sqrt{2}}$, $\tan 45^{\circ} = 1$

From an isosceles right triangle with legs 1 and hypotenuse $\sqrt{2}$. Here $\frac{1}{\sqrt{2}} = \frac{\sqrt{2}}{2} \approx 0.7071$.

Angle $60^{\circ}$ ($\frac{\pi}{3}$)

$\sin 60^{\circ} = \frac{\sqrt{3}}{2}$, $\cos 60^{\circ} = \frac{1}{2}$, $\tan 60^{\circ} = \sqrt{3}$

The values of $30^{\circ}$ with sine and cosine swapped. $\tan 60^{\circ} \approx 1.7321$.

Angle $90^{\circ}$ ($\frac{\pi}{2}$)

$\sin 90^{\circ} = 1$, $\cos 90^{\circ} = 0$

$\tan 90^{\circ}$ is undefined because it would need division by $\cos 90^{\circ} = 0$.

Angle $180^{\circ}$ ($\pi$)

$\sin 180^{\circ} = 0$, $\cos 180^{\circ} = -1$, $\tan 180^{\circ} = 0$

The point on the unit circle is $(-1, 0)$, on the negative x-axis.

Angle $270^{\circ}$ ($\frac{3\pi}{2}$)

$\sin 270^{\circ} = -1$, $\cos 270^{\circ} = 0$

The point on the unit circle is $(0, -1)$, so $\tan 270^{\circ}$ is undefined.

Angle $15^{\circ}$

$\sin 15^{\circ} = \frac{\sqrt{6} - \sqrt{2}}{4}$, $\cos 15^{\circ} = \frac{\sqrt{6} + \sqrt{2}}{4}$, $\tan 15^{\circ} = 2 - \sqrt{3}$

Found from $45^{\circ} - 30^{\circ}$. Swap sine and cosine to get the values for $75^{\circ}$, and $\tan 75^{\circ} = 2 + \sqrt{3}$.

Angles $18^{\circ}$ and $36^{\circ}$

$\sin 18^{\circ} = \frac{\sqrt{5} - 1}{4}$, $\cos 36^{\circ} = \frac{\sqrt{5} + 1}{4}$

Exact values linked to the regular pentagon, often asked in JEE. Also $\cos 72^{\circ} = \sin 18^{\circ}$.

Trigonometric table memory pattern

$\sin\theta = \frac{\sqrt{n}}{2}$ for $n = 0, 1, 2, 3, 4$

Gives sine at $0^{\circ}$, $30^{\circ}$, $45^{\circ}$, $60^{\circ}$, $90^{\circ}$ in that order. Cosine uses the same values in reverse order.

Example: $\sin^{2}45^{\circ} + \cos^{2}60^{\circ} = \frac{1}{2} + \frac{1}{4} = \frac{3}{4} = 0.75$.

Signs In The Four Quadrants (ASTC)

Angles are measured anticlockwise from the positive x-axis.

Formula

Expression

What it means

ASTC rule (All Students Take Calculus)

$\text{I: All}$, $\text{II: Sine}$, $\text{III: Tangent}$, $\text{IV: Cosine}$

In each quadrant the named ratio and its reciprocal are positive and the rest are negative. In quadrant I all six are positive.

Quadrant I

$0^{\circ} < \theta < 90^{\circ}$

Both $x$ and $y$ are positive, so all six ratios are positive.

Quadrant II

$90^{\circ} < \theta < 180^{\circ}$

Here $x < 0$ and $y > 0$, so only sine and cosecant are positive.

Quadrant III

$180^{\circ} < \theta < 270^{\circ}$

Here $x < 0$ and $y < 0$, so only tangent and cotangent are positive.

Quadrant IV

$270^{\circ} < \theta < 360^{\circ}$

Here $x > 0$ and $y < 0$, so only cosine and secant are positive.

Reference angle

$180^{\circ} - \theta$ (II), $\theta - 180^{\circ}$ (III), $360^{\circ} - \theta$ (IV)

The acute angle between the terminal side and the x-axis. A ratio of $\theta$ equals the same ratio of the reference angle, with the ASTC sign.

Coterminal angles

$\theta + 360^{\circ} n$ or $\theta + 2\pi n$

For any integer $n$ these angles share one terminal side, so all six ratios are equal.

Example: For $\cos 120^{\circ}$, the reference angle is $60^{\circ}$ and cosine is negative in quadrant II, so $\cos 120^{\circ} = -\cos 60^{\circ} = -\frac{1}{2}$.

Cofunction And Allied Angle Identities

Formula

Expression

What it means

Cofunction identities (sine and cosine)

$\sin(90^{\circ} - \theta) = \cos\theta$, $\cos(90^{\circ} - \theta) = \sin\theta$

The two acute angles of a right triangle add to $90^{\circ}$, so the sine of one is the cosine of the other.

Tangent and cotangent cofunctions

$\tan(90^{\circ} - \theta) = \cot\theta$, $\cot(90^{\circ} - \theta) = \tan\theta$

Tangent of an angle equals cotangent of its complement.

Secant and cosecant cofunctions

$\sec(90^{\circ} - \theta) = \csc\theta$, $\csc(90^{\circ} - \theta) = \sec\theta$

Secant of an angle equals cosecant of its complement.

Angle $90^{\circ} + \theta$

$\sin(90^{\circ} + \theta) = \cos\theta$, $\cos(90^{\circ} + \theta) = -\sin\theta$, $\tan(90^{\circ} + \theta) = -\cot\theta$

For acute $\theta$ the angle lies in quadrant II, so only sine stays positive.

Angle $180^{\circ} - \theta$

$\sin(180^{\circ} - \theta) = \sin\theta$, $\cos(180^{\circ} - \theta) = -\cos\theta$, $\tan(180^{\circ} - \theta) = -\tan\theta$

Supplementary angles have equal sines and opposite cosines. Used for obtuse angles in triangles.

Angle $180^{\circ} + \theta$

$\sin(180^{\circ} + \theta) = -\sin\theta$, $\cos(180^{\circ} + \theta) = -\cos\theta$, $\tan(180^{\circ} + \theta) = \tan\theta$

The angle lies in quadrant III, where only tangent and cotangent are positive.

Angle $270^{\circ} \pm \theta$

$\sin(270^{\circ} \pm \theta) = -\cos\theta$, $\cos(270^{\circ} - \theta) = -\sin\theta$, $\cos(270^{\circ} + \theta) = \sin\theta$

An odd multiple of $90^{\circ}$ switches sine to cosine. Signs follow quadrant III for the minus case and quadrant IV for the plus case.

Angle $360^{\circ} - \theta$

$\sin(360^{\circ} - \theta) = -\sin\theta$, $\cos(360^{\circ} - \theta) = \cos\theta$, $\tan(360^{\circ} - \theta) = -\tan\theta$

The angle lies in quadrant IV and gives the same values as $-\theta$.

Negative angle (even and odd)

$\sin(-\theta) = -\sin\theta$, $\cos(-\theta) = \cos\theta$, $\tan(-\theta) = -\tan\theta$

Cosine and secant are even functions. Sine, tangent, cosecant and cotangent are odd functions.

Allied angle rule

$n \times 90^{\circ} \pm \theta$

For odd $n$, switch sine and cosine, tangent and cotangent, secant and cosecant. For even $n$, keep the function. Take the sign from ASTC.

Example: $\sin 150^{\circ} = \sin(180^{\circ} - 30^{\circ}) = \sin 30^{\circ} = \frac{1}{2}$.

Degree And Radian Conversion

Formula

Expression

What it means

Basic relation

$\pi,\text{rad} = 180^{\circ}$

Half a turn is $\pi$ radians. Every conversion between the two units comes from this one fact.

Full turn

$360^{\circ} = 2\pi,\text{rad}$

One complete revolution. So a right angle is $\frac{\pi}{2}$ radians.

Degrees to radians

$\theta_{\text{rad}} = \theta_{\text{deg}} \times \frac{\pi}{180}$

Multiply a degree measure by $\frac{\pi}{180}$ to get radians. Calculus formulas need radians.

Radians to degrees

$\theta_{\text{deg}} = \theta_{\text{rad}} \times \frac{180}{\pi}$

Multiply a radian measure by $\frac{180}{\pi}$ to get degrees.

1 radian to degrees

$1,\text{rad} = \frac{180^{\circ}}{\pi} \approx 57.2958^{\circ}$

One radian is a little under $57.3^{\circ}$.

One degree in radians

$1^{\circ} = \frac{\pi}{180},\text{rad} \approx 0.01745,\text{rad}$

A small angle, useful when converting minutes and seconds of arc.

Radian measure of an angle

$\theta = \frac{s}{r}$

The angle at the centre of a circle of radius $r$ cut off by an arc of length $s$. It is 1 radian when $s = r$.

Minutes and seconds

$1^{\circ} = 60'$, $1' = 60''$

A degree splits into 60 minutes and a minute into 60 seconds, so $1^{\circ} = 3600''$.

Example: $135^{\circ} = 135 \times \frac{\pi}{180} = \frac{3\pi}{4} \approx 2.3562,\text{rad}$.

Arc Length And Sector Area In Radians

These forms need $\theta$ in radians. For an angle in degrees, replace $\theta$ with $\frac{\pi\theta}{180}$ first.

Formula

Expression

What it means

Arc length

$s = r\theta$

Length of the arc cut off by a central angle $\theta$ in a circle of radius $r$.

Sector area

$A = \frac{1}{2}r^{2}\theta$

Area of the slice of the circle bounded by two radii and the arc, with $\theta$ in radians.

Sector area from arc length

$A = \frac{1}{2}rs$

Same area written with the arc length $s$, useful when the angle is not given.

Perimeter of a sector

$P = 2r + r\theta$

Two radii plus the arc length.

Area of a minor segment

$A = \frac{1}{2}r^{2}(\theta - \sin\theta)$

Region between a chord and its arc: sector area minus triangle area, with $\theta$ in radians.

Chord length

$c = 2r\sin\frac{\theta}{2}$

Length of the straight chord joining the ends of an arc with central angle $\theta$.

Linear and angular speed

$v = r\omega$

A point at distance $r$ from the centre, turning at $\omega$ radians per second, moves at speed $v$.

Example: For $r = 10,\text{cm}$ and $\theta = 1.2,\text{rad}$, the arc is $s = 10 \times 1.2 = 12,\text{cm}$ and the sector area is $\frac{1}{2} \times 100 \times 1.2 = 60,\text{cm}^{2}$.

Sum And Difference Formulas

Formula

Expression

What it means

Sin (A + B)

$\sin(A + B) = \sin A\cos B + \cos A\sin B$

Sine of a sum of two angles. Use it to find exact values such as $\sin 75^{\circ}$.

Sin (a - b)

$\sin(A - B) = \sin A\cos B - \cos A\sin B$

Sine of a difference. Same pattern as the sum with the middle sign changed.

Cos (A + B)

$\cos(A + B) = \cos A\cos B - \sin A\sin B$

Cosine of a sum. Note the sign in the middle is the opposite of the sign between the angles.

Cos(A - B) formula

$\cos(A - B) = \cos A\cos B + \sin A\sin B$

Cosine of a difference. Setting $A = B$ gives $\cos 0 = \cos^{2}A + \sin^{2}A = 1$.

Tan (A + B)

$\tan(A + B) = \frac{\tan A + \tan B}{1 - \tan A\tan B}$

Valid when $\tan A$, $\tan B$ exist and $\tan A\tan B \neq 1$.

Tan (A - B)

$\tan(A - B) = \frac{\tan A - \tan B}{1 + \tan A\tan B}$

Valid when $\tan A$, $\tan B$ exist and $\tan A\tan B \neq -1$. Used for the angle between two lines.

Cot (A + B)

$\cot(A + B) = \frac{\cot A\cot B - 1}{\cot A + \cot B}$

Cotangent of a sum, valid when $\cot A + \cot B \neq 0$.

Product of sum and difference sines

$\sin(A + B)\sin(A - B) = \sin^{2}A - \sin^{2}B$

Also equals $\cos^{2}B - \cos^{2}A$. Saves expanding both brackets.

Product of sum and difference cosines

$\cos(A + B)\cos(A - B) = \cos^{2}A - \sin^{2}B$

Also equals $\cos^{2}B - \sin^{2}A$.

Tan of three angles

$\tan(A + B + C) = \frac{\tan A + \tan B + \tan C - \tan A\tan B\tan C}{1 - \tan A\tan B - \tan B\tan C - \tan C\tan A}$

Extends the two-angle formula. When $A + B + C = \pi$ the numerator must be zero.

Example: $\sin 75^{\circ} = \sin(45^{\circ} + 30^{\circ}) = \frac{\sqrt{2}}{2} \cdot \frac{\sqrt{3}}{2} + \frac{\sqrt{2}}{2} \cdot \frac{1}{2} = \frac{\sqrt{6} + \sqrt{2}}{4} \approx 0.9659$.

Double Angle Formulas

Formula

Expression

What it means

Sin 2x formula

$\sin 2A = 2\sin A\cos A$

Sine of double an angle, from $\sin(A + A)$. Used to simplify products of sine and cosine.

Sin 2A in terms of tan A

$\sin 2A = \frac{2\tan A}{1 + \tan^{2}A}$

Writes $\sin 2A$ using only $\tan A$, valid wherever $\tan A$ is defined.

Cos2x (basic form)

$\cos 2A = \cos^{2}A - \sin^{2}A$

Cosine of double an angle, from $\cos(A + A)$. The other forms follow from it.

Cos 2A in cosine only

$\cos 2A = 2\cos^{2}A - 1$

Use when only $\cos A$ is known or when an expression has $\cos^{2}A$.

Cos 2A in sine only

$\cos 2A = 1 - 2\sin^{2}A$

Use when only $\sin A$ is known or to remove $\sin^{2}A$.

Cos 2A in terms of tan A

$\cos 2A = \frac{1 - \tan^{2}A}{1 + \tan^{2}A}$

Writes $\cos 2A$ using only $\tan A$, valid wherever $\tan A$ is defined.

Tan2x formula

$\tan 2A = \frac{2\tan A}{1 - \tan^{2}A}$

Tangent of double an angle, valid when $\tan^{2}A \neq 1$, that is $A$ is not an odd multiple of $45^{\circ}$.

Power reduction for cosine

$\cos^{2}A = \frac{1 + \cos 2A}{2}$

Turns a square into a first power. Also written $1 + \cos 2A = 2\cos^{2}A$.

Power reduction for sine

$\sin^{2}A = \frac{1 - \cos 2A}{2}$

Turns a square into a first power, often needed before integrating $\sin^{2}x$.

Example: If $\sin A = \frac{3}{5}$ with $A$ acute, then $\cos A = \frac{4}{5}$, $\sin 2A = 2 \times \frac{3}{5} \times \frac{4}{5} = \frac{24}{25} = 0.96$ and $\cos 2A = 1 - 2 \times \frac{9}{25} = \frac{7}{25} = 0.28$.

Triple Angle Formulas

Formula

Expression

What it means

Sin 3A

$\sin 3A = 3\sin A - 4\sin^{3}A$

Sine of three times an angle, written in powers of $\sin A$.

Cos 3A

$\cos 3A = 4\cos^{3}A - 3\cos A$

Cosine of three times an angle, written in powers of $\cos A$. The order of terms is reversed compared with $\sin 3A$.

Tan3x

$\tan 3A = \frac{3\tan A - \tan^{3}A}{1 - 3\tan^{2}A}$

Tangent of three times an angle, valid when $\tan^{2}A \neq \frac{1}{3}$.

Cube of sine

$\sin^{3}A = \frac{3\sin A - \sin 3A}{4}$

The $\sin 3A$ formula rearranged. Used to remove cubes before integrating.

Cube of cosine

$\cos^{3}A = \frac{3\cos A + \cos 3A}{4}$

The $\cos 3A$ formula rearranged. Note the plus sign, unlike the sine version.

Sine product with $60^{\circ}$

$\sin A\sin(60^{\circ} - A)\sin(60^{\circ} + A) = \frac{1}{4}\sin 3A$

A JEE shortcut for products like $\sin 20^{\circ}\sin 40^{\circ}\sin 80^{\circ}$.

Cosine product with $60^{\circ}$

$\cos A\cos(60^{\circ} - A)\cos(60^{\circ} + A) = \frac{1}{4}\cos 3A$

The cosine version of the same shortcut.

Tangent product with $60^{\circ}$

$\tan A\tan(60^{\circ} - A)\tan(60^{\circ} + A) = \tan 3A$

The tangent version, with no factor of $\frac{1}{4}$.

Example: With $A = 30^{\circ}$, $\sin 90^{\circ} = 3 \times \frac{1}{2} - 4 \times \frac{1}{8} = 1.5 - 0.5 = 1$, which matches the known value.

Half Angle Formulas

The $\pm$ sign is set by the quadrant in which $\frac{A}{2}$ lies.

Formula

Expression

What it means

Half angle formula for sine

$\sin\frac{A}{2} = \pm\sqrt{\frac{1 - \cos A}{2}}$

Finds sine of half an angle from the cosine of the full angle.

Cosine half angle

$\cos\frac{A}{2} = \pm\sqrt{\frac{1 + \cos A}{2}}$

Finds cosine of half an angle from the cosine of the full angle.

Tangent half angle, root form

$\tan\frac{A}{2} = \pm\sqrt{\frac{1 - \cos A}{1 + \cos A}}$

Valid when $\cos A \neq -1$. The sign again depends on the quadrant of $\frac{A}{2}$.

Tangent half angle, no root

$\tan\frac{A}{2} = \frac{\sin A}{1 + \cos A} = \frac{1 - \cos A}{\sin A}$

Gives the correct sign automatically. The second form needs $\sin A \neq 0$.

Sine from $t = \tan\frac{A}{2}$

$\sin A = \frac{2t}{1 + t^{2}}$

Writes $\sin A$ as a rational function of $t$. Used in the t-substitution for integrals and equations.

Cosine from $t = \tan\frac{A}{2}$

$\cos A = \frac{1 - t^{2}}{1 + t^{2}}$

Writes $\cos A$ as a rational function of $t = \tan\frac{A}{2}$.

Tangent from $t = \tan\frac{A}{2}$

$\tan A = \frac{2t}{1 - t^{2}}$

Writes $\tan A$ using $t$, valid when $t^{2} \neq 1$.

Example: $\cos 22.5^{\circ} = \sqrt{\frac{1 + \cos 45^{\circ}}{2}} = \sqrt{\frac{1 + 0.7071}{2}} = \sqrt{0.85355} \approx 0.9239$.

Product To Sum Formulas

Formula

Expression

What it means

2 sin A cos B

$2\sin A\cos B = \sin(A + B) + \sin(A - B)$

Turns a product of sine and cosine into a sum of sines.

2 cos A sin B

$2\cos A\sin B = \sin(A + B) - \sin(A - B)$

Same idea with the sine on the second angle, which gives a difference.

2 cos A cos B

$2\cos A\cos B = \cos(A + B) + \cos(A - B)$

Turns a product of two cosines into a sum of cosines.

2 sin A sin B

$2\sin A\sin B = \cos(A - B) - \cos(A + B)$

Turns a product of two sines into a difference of cosines. Watch the order of the terms.

Sin A cos B

$\sin A\cos B = \frac{1}{2}[\sin(A + B) + \sin(A - B)]$

The first formula divided by 2, the form usually needed when integrating a product.

Sin A sin B

$\sin A\sin B = \frac{1}{2}[\cos(A - B) - \cos(A + B)]$

The sine product formula divided by 2.

Cos A cos B

$\cos A\cos B = \frac{1}{2}[\cos(A + B) + \cos(A - B)]$

The cosine product formula divided by 2.

Example: $2\sin 75^{\circ}\cos 15^{\circ} = \sin 90^{\circ} + \sin 60^{\circ} = 1 + 0.8660 = 1.8660$.

Sum To Product Formulas

Formula

Expression

What it means

Sin A + Sin B formula

$\sin A + \sin B = 2\sin\frac{A + B}{2}\cos\frac{A - B}{2}$

Turns a sum of two sines into a product, useful for factorising and solving equations.

Sin A minus sin B

$\sin A - \sin B = 2\cos\frac{A + B}{2}\sin\frac{A - B}{2}$

Difference of two sines as a product. Cosine takes the half sum, sine takes the half difference.

Cos A plus cos B

$\cos A + \cos B = 2\cos\frac{A + B}{2}\cos\frac{A - B}{2}$

Sum of two cosines as a product of two cosines.

Cos A minus cos B

$\cos A - \cos B = -2\sin\frac{A + B}{2}\sin\frac{A - B}{2}$

Difference of two cosines. Keep the minus sign in front, or write it as $2\sin\frac{A + B}{2}\sin\frac{B - A}{2}$.

Tan A plus or minus tan B

$\tan A \pm \tan B = \frac{\sin(A \pm B)}{\cos A\cos B}$

Sum or difference of tangents, valid when $\cos A$ and $\cos B$ are both non-zero.

Cot A plus or minus cot B

$\cot A \pm \cot B = \frac{\sin(B \pm A)}{\sin A\sin B}$

Sum or difference of cotangents, valid when $\sin A$ and $\sin B$ are both non-zero.

Example: $\sin 75^{\circ} + \sin 15^{\circ} = 2\sin 45^{\circ}\cos 30^{\circ} = 2 \times 0.7071 \times 0.8660 \approx 1.2247$.

Law Of Sines, Law Of Cosines And Law Of Tangents

In triangle ABC, sides $a$, $b$, $c$ lie opposite angles $A$, $B$, $C$, and $R$ is the circumradius.

Formula

Expression

What it means

Angle sum of a triangle

$A + B + C = 180^{\circ}$

The three angles add to $180^{\circ}$, or $\pi$ radians. Gives the third angle when two are known.

Law of sines (sine rule)

$\frac{a}{\sin A} = \frac{b}{\sin B} = \frac{c}{\sin C} = 2R$

Each side over the sine of its opposite angle is the same. Use with two angles and a side, or two sides and a non-included angle.

Law of cosines (cosine rule)

$a^{2} = b^{2} + c^{2} - 2bc\cos A$

Finds the third side from two sides and the included angle. When $A = 90^{\circ}$ it becomes the Pythagorean theorem.

Law of cosines for sides b and c

$b^{2} = c^{2} + a^{2} - 2ca\cos B$, $c^{2} = a^{2} + b^{2} - 2ab\cos C$

The same rule written for the other two sides.

Angle from three sides

$\cos A = \frac{b^{2} + c^{2} - a^{2}}{2bc}$

Finds an angle when all three sides are known. A negative value means $A$ is obtuse.

Law of tangents

$\frac{a - b}{a + b} = \frac{\tan\frac{A - B}{2}}{\tan\frac{A + B}{2}}$

Links two sides to the half difference and half sum of their opposite angles. Useful when two sides and the included angle are known.

Napier's analogy

$\tan\frac{B - C}{2} = \frac{b - c}{b + c}\cot\frac{A}{2}$

Another form of the law of tangents that gives $B - C$ directly when $b$, $c$ and $A$ are known.

Projection formula

$a = b\cos C + c\cos B$

Side $a$ equals the sum of the projections of the other two sides onto it. Similar forms hold for $b$ and $c$.

Tangent sum in a triangle

$\tan A + \tan B + \tan C = \tan A\tan B\tan C$

Holds when $A + B + C = \pi$ and no angle is $90^{\circ}$. A frequent JEE identity.

Example: With $b = 5$, $c = 7$ and $A = 60^{\circ}$, $a^{2} = 25 + 49 - 2 \times 5 \times 7 \times 0.5 = 39$, so $a = \sqrt{39} \approx 6.2450$.

Area Of A Triangle Using Sine

Formula

Expression

What it means

Two sides and included angle

$\Delta = \frac{1}{2}bc\sin A = \frac{1}{2}ca\sin B = \frac{1}{2}ab\sin C$

Half the product of two sides times the sine of the angle between them. No height is needed.

Heron's formula

$\Delta = \sqrt{s(s - a)(s - b)(s - c)}$

Area from the three sides alone, where $s = \frac{a + b + c}{2}$ is the semi-perimeter.

Area and circumradius

$\Delta = \frac{abc}{4R}$

Links the area, the three sides and the radius $R$ of the circle through all three vertices.

Circumradius

$R = \frac{a}{2\sin A}$

Radius of the circumcircle, from any side and its opposite angle. Comes from the law of sines.

Area and inradius

$\Delta = rs$

Area equals the inradius $r$ (radius of the inscribed circle) times the semi-perimeter $s$.

Area from R and the angles

$\Delta = 2R^{2}\sin A\sin B\sin C$

Area when the circumradius and all three angles are known.

Area from one side and the angles

$\Delta = \frac{a^{2}\sin B\sin C}{2\sin A}$

Area when one side and all three angles are known, found by combining the sine rule with $\frac{1}{2}ab\sin C$.

Example: With $a = 8$, $b = 10$ and $C = 30^{\circ}$, the area is $\frac{1}{2} \times 8 \times 10 \times \sin 30^{\circ} = 40 \times 0.5 = 20$ square units.

Semi-Perimeter And Half Angle Formulas In A Triangle

Formula

Expression

What it means

Semi-perimeter

$s = \frac{a + b + c}{2}$

Half the perimeter of the triangle. Every formula below uses it.

Sine of a half angle

$\sin\frac{A}{2} = \sqrt{\frac{(s - b)(s - c)}{bc}}$

Sine of half of angle $A$ from the sides. Always positive because $\frac{A}{2}$ is acute.

Cosine of a half angle

$\cos\frac{A}{2} = \sqrt{\frac{s(s - a)}{bc}}$

Cosine of half of angle $A$ from the sides. Similar forms hold for $B$ and $C$.

Tangent of a half angle

$\tan\frac{A}{2} = \sqrt{\frac{(s - b)(s - c)}{s(s - a)}} = \frac{\Delta}{s(s - a)}$

Tangent of half of angle $A$, where $\Delta$ is the area of the triangle.

Inradius

$r = \frac{\Delta}{s}$

Radius of the circle that touches all three sides from inside.

Inradius from a half angle

$r = (s - a)\tan\frac{A}{2}$

Uses the tangent length $s - a$ from vertex A to the incircle.

Inradius and circumradius

$r = 4R\sin\frac{A}{2}\sin\frac{B}{2}\sin\frac{C}{2}$

Links the inradius $r$ with the circumradius $R$ through the half angles.

Exradius

$r_{1} = \frac{\Delta}{s - a}$

Radius of the excircle opposite vertex A, which touches side $a$ and the extensions of the other two sides.

Example: For sides $a = 3$, $b = 4$, $c = 5$, $s = 6$, $\Delta = \sqrt{6 \times 3 \times 2 \times 1} = 6$, $r = \frac{6}{6} = 1$ and $\tan\frac{A}{2} = \frac{6}{6 \times 3} = \frac{1}{3}$.

Principal Values Of Inverse Trigonometric Functions

Each inverse function returns one angle, called the principal value, from the range shown.

Formula

Expression

What it means

Arcsin (inverse sine)

$\sin^{-1}x \in \left[-\frac{\pi}{2}, \frac{\pi}{2}\right]$

Defined for $-1 \leq x \leq 1$. Returns the angle in that range whose sine is $x$.

Arccosine (inverse cosine)

$\cos^{-1}x \in [0, \pi]$

Defined for $-1 \leq x \leq 1$. Returns the angle between 0 and $\pi$ whose cosine is $x$.

Arctan (inverse tangent)

$\tan^{-1}x \in \left(-\frac{\pi}{2}, \frac{\pi}{2}\right)$

Defined for every real $x$. The end points are excluded because tangent is undefined there.

Inverse cosecant

$\csc^{-1}x \in \left[-\frac{\pi}{2}, \frac{\pi}{2}\right] \setminus \lbrace 0 \rbrace$

Defined for $\lvert x \rvert \geq 1$. Zero is excluded because $\csc 0$ is undefined, as $\sin 0 = 0$.

Inverse secant

$\sec^{-1}x \in [0, \pi] \setminus \left\lbrace \frac{\pi}{2} \right\rbrace$

Defined for $\lvert x \rvert \geq 1$. The angle $\frac{\pi}{2}$ is excluded because secant is undefined there.

Inverse cotangent

$\cot^{-1}x \in (0, \pi)$

Defined for every real $x$. Both end points are excluded.

Inverse trigonometric functions notation

$\sin^{-1}x = \arcsin x \neq \frac{1}{\sin x}$

The $-1$ marks an inverse function, not a reciprocal. Both notations mean the same thing.

Function after its inverse

$\sin(\sin^{-1}x) = x$

True for every $x$ with $-1 \leq x \leq 1$. Likewise $\tan(\tan^{-1}x) = x$ for every real $x$.

Inverse after the function

$\sin^{-1}(\sin x) = x$

True only for $-\frac{\pi}{2} \leq x \leq \frac{\pi}{2}$. Likewise $\cos^{-1}(\cos x) = x$ only for $0 \leq x \leq \pi$.

Example: $\sin^{-1}\left(-\frac{1}{2}\right) = -\frac{\pi}{6}$, not $\frac{7\pi}{6}$, because the answer must lie in $\left[-\frac{\pi}{2}, \frac{\pi}{2}\right]$, while $\cos^{-1}\left(-\frac{1}{2}\right) = \frac{2\pi}{3}$.

Inverse Trigonometric Identities

Formula

Expression

What it means

Inverse sine plus inverse cosine

$\sin^{-1}x + \cos^{-1}x = \frac{\pi}{2}$

Holds for $-1 \leq x \leq 1$. Lets you replace one inverse function with the other.

Inverse tangent plus inverse cotangent

$\tan^{-1}x + \cot^{-1}x = \frac{\pi}{2}$

Holds for every real $x$.

Inverse secant plus inverse cosecant

$\sec^{-1}x + \csc^{-1}x = \frac{\pi}{2}$

Holds for $\lvert x \rvert \geq 1$.

Negative argument, odd functions

$\sin^{-1}(-x) = -\sin^{-1}x$, $\tan^{-1}(-x) = -\tan^{-1}x$, $\csc^{-1}(-x) = -\csc^{-1}x$

The minus sign comes straight out, because these ranges are symmetric about zero.

Negative argument, pi minus form

$\cos^{-1}(-x) = \pi - \cos^{-1}x$, $\sec^{-1}(-x) = \pi - \sec^{-1}x$, $\cot^{-1}(-x) = \pi - \cot^{-1}x$

These ranges start at 0, so a negative input gives $\pi$ minus the positive answer.

Reciprocal argument

$\sin^{-1}\frac{1}{x} = \csc^{-1}x$, $\cos^{-1}\frac{1}{x} = \sec^{-1}x$

Both hold for $\lvert x \rvert \geq 1$. Converts between an inverse function and its reciprocal partner.

Inverse tangent of a reciprocal

$\tan^{-1}\frac{1}{x} = \cot^{-1}x$

Holds for $x > 0$. For $x < 0$ it becomes $\tan^{-1}\frac{1}{x} = \cot^{-1}x - \pi$.

Sum of inverse tangents

$\tan^{-1}x + \tan^{-1}y = \tan^{-1}\frac{x + y}{1 - xy}$

Holds when $xy < 1$. If $x > 0$, $y > 0$ and $xy > 1$, add $\pi$ to the right side.

Difference of inverse tangents

$\tan^{-1}x - \tan^{-1}y = \tan^{-1}\frac{x - y}{1 + xy}$

Holds when $xy > -1$.

Twice the inverse tangent

$2\tan^{-1}x = \tan^{-1}\frac{2x}{1 - x^{2}} = \sin^{-1}\frac{2x}{1 + x^{2}}$

The tangent form holds for $\lvert x \rvert < 1$ and the sine form for $\lvert x \rvert \leq 1$.

Example: $\tan^{-1}\frac{1}{2} + \tan^{-1}\frac{1}{3} = \tan^{-1}\frac{\frac{5}{6}}{1 - \frac{1}{6}} = \tan^{-1}1 = \frac{\pi}{4}$, which is allowed because $xy = \frac{1}{6} < 1$.

General Solutions Of Trigonometric Equations

Here $n$ is any integer, $\alpha$ is the principal value, and all angles are in radians.

Formula

Expression

What it means

Sine equal to zero

$\sin\theta = 0 \Rightarrow \theta = n\pi$

Sine is zero at every integer multiple of $\pi$.

Cosine equal to zero

$\cos\theta = 0 \Rightarrow \theta = (2n + 1)\frac{\pi}{2}$

Cosine is zero at every odd multiple of $\frac{\pi}{2}$.

Tangent equal to zero

$\tan\theta = 0 \Rightarrow \theta = n\pi$

Tangent is zero exactly where sine is zero.

Sine equal to sine

$\sin\theta = \sin\alpha \Rightarrow \theta = n\pi + (-1)^{n}\alpha$

Covers both angles in each turn with the same sine, with $\alpha$ in $\left[-\frac{\pi}{2}, \frac{\pi}{2}\right]$.

Cosine equal to cosine

$\cos\theta = \cos\alpha \Rightarrow \theta = 2n\pi \pm \alpha$

Covers both angles in each turn with the same cosine, with $\alpha$ in $[0, \pi]$.

Tangent equal to tangent

$\tan\theta = \tan\alpha \Rightarrow \theta = n\pi + \alpha$

Tangent repeats every $\pi$, with $\alpha$ in $\left(-\frac{\pi}{2}, \frac{\pi}{2}\right)$.

Squared equations

$\sin^{2}\theta = \sin^{2}\alpha \Rightarrow \theta = n\pi \pm \alpha$

The same solution holds for $\cos^{2}\theta = \cos^{2}\alpha$ and $\tan^{2}\theta = \tan^{2}\alpha$.

Sine equal to 1 or minus 1

$\sin\theta = 1 \Rightarrow \theta = 2n\pi + \frac{\pi}{2}$

Similarly $\sin\theta = -1$ gives $\theta = 2n\pi - \frac{\pi}{2}$.

Cosine equal to 1 or minus 1

$\cos\theta = 1 \Rightarrow \theta = 2n\pi$

Similarly $\cos\theta = -1$ gives $\theta = (2n + 1)\pi$.

Example: For $\sin\theta = \frac{1}{2}$, $\alpha = \frac{\pi}{6}$, so $\theta = n\pi + (-1)^{n}\frac{\pi}{6}$, which gives $\frac{\pi}{6}$ for $n = 0$ and $\frac{5\pi}{6}$ for $n = 1$.

Periods, Ranges And Maximum Values

Formula

Expression

What it means

Range of sine and cosine

$-1 \leq \sin\theta \leq 1$, $-1 \leq \cos\theta \leq 1$

Sine and cosine never go above 1 or below $-1$ for any real angle.

Range of secant and cosecant

$\lvert \sec\theta \rvert \geq 1$, $\lvert \csc\theta \rvert \geq 1$

These reciprocals never take values strictly between $-1$ and 1.

Range of tangent and cotangent

$\tan\theta \in (-\infty, \infty)$

Tangent and cotangent can take every real value.

Period of sine and cosine

$\sin(\theta + 2\pi) = \sin\theta$, $\cos(\theta + 2\pi) = \cos\theta$

Values repeat every $2\pi$ radians, or $360^{\circ}$. The same holds for cosecant and secant.

Period of tangent

$\tan(\theta + \pi) = \tan\theta$

Tangent and cotangent repeat every $\pi$ radians, or $180^{\circ}$.

Period with a coefficient

$T = \frac{2\pi}{\lvert k \rvert}$

Period of $\sin kx$ and $\cos kx$ for $k \neq 0$. For $\tan kx$ the period is $\frac{\pi}{\lvert k \rvert}$.

Harmonic form

$a\sin\theta + b\cos\theta = \sqrt{a^{2} + b^{2}},\sin(\theta + \phi)$

Combines two waves into one, where $\cos\phi = \frac{a}{\sqrt{a^{2} + b^{2}}}$ and $\sin\phi = \frac{b}{\sqrt{a^{2} + b^{2}}}$.

Maximum and minimum of a combination

$-\sqrt{a^{2} + b^{2}} \leq a\sin\theta + b\cos\theta \leq \sqrt{a^{2} + b^{2}}$

Gives the greatest and least values. The equation $a\sin\theta + b\cos\theta = c$ has solutions only if $\lvert c \rvert \leq \sqrt{a^{2} + b^{2}}$.

Example: $3\sin\theta + 4\cos\theta$ has maximum $\sqrt{9 + 16} = 5$ and minimum $-5$.

Heights And Distances

The angle of elevation is measured upward from the horizontal, and the angle of depression downward from it.

Formula

Expression

What it means

Angle of elevation

$\tan\theta = \frac{h}{d}$

Looking up at an object of height $h$ above eye level from a horizontal distance $d$.

Angle of depression

$\tan\theta = \frac{h}{d}$

Looking down from height $h$ to a point at horizontal distance $d$. It equals the angle of elevation from that point, as alternate angles.

Height from distance

$h = d\tan\theta$

Finds the height of a tower, tree or building when the distance and angle are known.

Distance from height

$d = \frac{h}{\tan\theta} = h\cot\theta$

Finds how far away an object is when its height and the angle are known.

Length of the line of sight

$l = \frac{h}{\sin\theta}$

The straight-line distance from the eye to the top of the object, which is the hypotenuse.

Heights and distances with two observation points

$h = \frac{x\tan\alpha\tan\beta}{\tan\alpha - \tan\beta}$

The observer walks a distance $x$ toward the object and the elevation rises from $\beta$ to $\alpha$, with $\alpha > \beta$.

Example: From $50,\text{m}$ away the top of a tower is seen at $30^{\circ}$, so $h = 50 \times \tan 30^{\circ} = 50 \times 0.5774 \approx 28.87,\text{m}$.

Calculus Formulas

Calculus studies how quantities change (derivatives) and how they add up (integrals). These formulas cover limits, differentiation, integration, differential equations and series for Grade 11 and 12 students preparing for board exams, JEE, AP Calculus or A-level.

Limit Laws

Each law below assumes $\lim_{x \to a} f(x) = L$ and $\lim_{x \to a} g(x) = M$ both exist as finite numbers.

Formula

Expression

What it means

Limit of a constant

$\lim_{x \to a} c = c$

A constant function keeps the same value $c$ however close $x$ gets to $a$.

Limit of the identity

$\lim_{x \to a} x = a$

As $x$ approaches $a$, the function $f(x) = x$ approaches $a$ itself.

Sum and difference law

$\lim_{x \to a} [f(x) \pm g(x)] = L \pm M$

The limit of a sum or difference is the sum or difference of the separate limits.

Constant multiple law

$\lim_{x \to a} k f(x) = kL$

A constant factor $k$ can be taken outside the limit.

Product law

$\lim_{x \to a} [f(x) \cdot g(x)] = L \cdot M$

The limit of a product equals the product of the two limits.

Quotient law

$\lim_{x \to a} \frac{f(x)}{g(x)} = \frac{L}{M}$

The limit of a quotient is the quotient of the limits, valid only when $M \neq 0$.

Power and root law

$\lim_{x \to a} [f(x)]^{n} = L^{n}$, $\lim_{x \to a} \sqrt[n]{f(x)} = \sqrt[n]{L}$

Holds for a positive integer $n$, and for the root with even $n$ you also need $L > 0$.

Existence of a limit

$\lim_{x \to a^{-}} f(x) = \lim_{x \to a^{+}} f(x) = L$

The two-sided limit equals $L$ only when the left-hand and right-hand limits are both equal to $L$.

Continuity at a point

$\lim_{x \to a} f(x) = f(a)$

A function is continuous at $a$ when $f(a)$ is defined and equals the limit there.

Squeeze (sandwich) theorem

$g(x) \leq f(x) \leq h(x)$ and $\lim_{x \to a} g(x) = \lim_{x \to a} h(x) = L$

If $f$ is trapped between two functions with the same limit $L$ near $a$, then $\lim_{x \to a} f(x) = L$ too.

Example: $\lim_{x \to 2} (3x^{2} + 5) = 3(2)^{2} + 5 = 12 + 5 = 17$, using the sum, constant multiple and power laws.

Standard Limits

All trigonometric limits here assume $x$ is measured in radians.

Formula

Expression

What it means

Sine limit

$\lim_{x \to 0} \frac{\sin x}{x} = 1$

Near zero, $\sin x$ and $x$ are almost equal, so their ratio tends to 1.

Tangent limit

$\lim_{x \to 0} \frac{\tan x}{x} = 1$

Near zero, $\tan x$ behaves like $x$, so the ratio tends to 1.

Cosine limit

$\lim_{x \to 0} \frac{1 - \cos x}{x} = 0$

The gap $1 - \cos x$ shrinks faster than $x$, so the ratio tends to 0.

Cosine limit over $x^{2}$

$\lim_{x \to 0} \frac{1 - \cos x}{x^{2}} = \frac{1}{2}$

Dividing by $x^{2}$ instead of $x$ gives the finite value one half.

Exponential limit

$\lim_{x \to 0} \frac{e^{x} - 1}{x} = 1$

The graph of $e^{x}$ has slope 1 at $x = 0$, which is what this limit states.

General exponential limit

$\lim_{x \to 0} \frac{a^{x} - 1}{x} = \ln a$

For any base $a > 0$, the ratio tends to the natural log of the base.

Logarithmic limit

$\lim_{x \to 0} \frac{\ln(1 + x)}{x} = 1$

Near zero, $\ln(1 + x)$ is close to $x$, so the ratio tends to 1.

Definition of $e$

$\lim_{n \to \infty} \left(1 + \frac{1}{n}\right)^{n} = e$

As $n$ grows without bound, this expression approaches $e \approx 2.71828$.

Alternative form of $e$

$\lim_{x \to 0} (1 + x)^{\frac{1}{x}} = e$

The same number $e$ written as a limit with $x$ approaching zero. Used for $1^{\infty}$ forms.

Power difference limit

$\lim_{x \to a} \frac{x^{n} - a^{n}}{x - a} = n a^{n-1}$

Holds for any rational $n$ with $a > 0$, and for every real $a$ when $n$ is a positive integer.

Reciprocal power at infinity

$\lim_{x \to \infty} \frac{1}{x^{p}} = 0$

For any $p > 0$, the reciprocal power shrinks to zero as $x$ grows. Used for limits of rational functions.

L'Hôpital's rule

$\lim_{x \to a} \frac{f(x)}{g(x)} = \lim_{x \to a} \frac{f'(x)}{g'(x)}$

Use only for $\frac{0}{0}$ or $\frac{\infty}{\infty}$ forms, when $g'(x) \neq 0$ near $a$ and the right-hand limit exists.

Example: $\lim_{x \to 0} \frac{\sin 5x}{x} = 5 \cdot \lim_{x \to 0} \frac{\sin 5x}{5x} = 5 \times 1 = 5$.

Definition Of The Derivative And Derivative Rules

Formula

Expression

What it means

Derivative formula (first principles)

$f'(x) = \lim_{h \to 0} \frac{f(x + h) - f(x)}{h}$

The derivative is the limit of the average rate of change over a shrinking interval $h$, when this limit exists.

Derivative at a point

$f'(a) = \lim_{x \to a} \frac{f(x) - f(a)}{x - a}$

Gives the slope of the tangent to $y = f(x)$ at the single point $x = a$.

Constant rule

$\frac{d}{dx}(c) = 0$

A constant never changes, so its rate of change is zero.

Power rule

$\frac{d}{dx}(x^{n}) = n x^{n-1}$

Bring the power down and reduce it by one. Works for any real $n$ when $x > 0$, and for every $x$ when $n$ is a positive integer.

Constant multiple rule

$\frac{d}{dx}[c f(x)] = c f'(x)$

A constant factor $c$ stays in front while you differentiate the function.

Sum and difference rule

$\frac{d}{dx}[f(x) \pm g(x)] = f'(x) \pm g'(x)$

Differentiate each term separately and keep the plus or minus signs.

Product rule (uv differentiation formula)

$\frac{d}{dx}(uv) = u\frac{dv}{dx} + v\frac{du}{dx}$

For a product of two functions $u$ and $v$ of $x$: first times derivative of second, plus second times derivative of first.

Quotient rule

$\frac{d}{dx}\left(\frac{u}{v}\right) = \frac{v\frac{du}{dx} - u\frac{dv}{dx}}{v^{2}}$

For a ratio of two functions with $v \neq 0$. The order in the numerator matters because of the minus sign.

Chain rule (Leibniz form)

$\frac{dy}{dx} = \frac{dy}{du} \cdot \frac{du}{dx}$

When $y$ depends on $u$ and $u$ depends on $x$, multiply the two rates of change.

Chain rule (function form)

$\frac{d}{dx} f(g(x)) = f'(g(x)) \cdot g'(x)$

Differentiate the outer function at the inner one, then multiply by the derivative of the inner function.

Parametric derivative

$\frac{dy}{dx} = \frac{\frac{dy}{dt}}{\frac{dx}{dt}}$

When $x$ and $y$ are both given in terms of a parameter $t$, valid wherever $\frac{dx}{dt} \neq 0$.

Second derivative

$\frac{d^{2}y}{dx^{2}} = \frac{d}{dx}\left(\frac{dy}{dx}\right)$

The derivative of the derivative. It measures how fast the slope changes and gives concavity.

Derivative of an inverse function

$\frac{dx}{dy} = \frac{1}{\frac{dy}{dx}}$

The rate of $x$ with respect to $y$ is the reciprocal of the rate of $y$ with respect to $x$, when $\frac{dy}{dx} \neq 0$.

Logarithmic differentiation

$y = u^{v} \Rightarrow \frac{dy}{dx} = u^{v}\left(\frac{v}{u}\frac{du}{dx} + \ln u \cdot \frac{dv}{dx}\right)$

For a variable base $u > 0$ raised to a variable power $v$. Take $\ln$ of both sides, then differentiate.

Example: For $y = (3x + 1)^{4}$, the chain rule gives $\frac{dy}{dx} = 4(3x + 1)^{3} \cdot 3 = 12(3x + 1)^{3}$, which equals $12$ at $x = 0$.

Derivatives Of Algebraic, Exponential And Logarithmic Functions

Formula

Expression

What it means

Derivative of $\sqrt{x}$

$\frac{d}{dx}(\sqrt{x}) = \frac{1}{2\sqrt{x}}$

A special case of the power rule with $n = \frac{1}{2}$, valid for $x > 0$.

Derivative of $\frac{1}{x}$

$\frac{d}{dx}\left(\frac{1}{x}\right) = -\frac{1}{x^{2}}$

The power rule with $n = -1$, valid for $x \neq 0$.

Derivative of $e^{x}$

$\frac{d}{dx}(e^{x}) = e^{x}$

The natural exponential function is its own derivative.

Derivative of $e^{kx}$

$\frac{d}{dx}(e^{kx}) = k e^{kx}$

The constant $k$ in the exponent comes down as a factor, by the chain rule.

Derivative of $e^{f(x)}$

$\frac{d}{dx}\left(e^{f(x)}\right) = f'(x) e^{f(x)}$

The exponential stays the same and is multiplied by the derivative of its exponent.

Derivative of $a^{x}$

$\frac{d}{dx}(a^{x}) = a^{x} \ln a$

For a constant base $a > 0$, $a \neq 1$. When $a = e$ this reduces to $e^{x}$.

Derivative of $\ln x$

$\frac{d}{dx}(\ln x) = \frac{1}{x}$

The natural log has derivative $\frac{1}{x}$ on its domain $x > 0$.

Derivative of $\ln \lvert x \rvert$

$\frac{d}{dx}(\ln \lvert x \rvert) = \frac{1}{x}$

Extends the previous rule to negative $x$. Valid for every $x \neq 0$.

Derivative of $\log_{a} x$

$\frac{d}{dx}(\log_{a} x) = \frac{1}{x \ln a}$

For base $a > 0$, $a \neq 1$ and $x > 0$. Follows from the change of base rule.

Derivative of $\ln f(x)$

$\frac{d}{dx}[\ln f(x)] = \frac{f'(x)}{f(x)}$

The derivative of the inside divided by the inside, where $f(x) > 0$.

Derivative of $x^{x}$

$\frac{d}{dx}(x^{x}) = x^{x}(1 + \ln x)$

Found by taking $\ln$ of both sides and differentiating, valid for $x > 0$. The power rule does not apply here.

Example: $\frac{d}{dx}(\log_{2} x)$ at $x = 4$ is $\frac{1}{4 \ln 2} = \frac{1}{2.7726} \approx 0.3607$.

Derivatives Of Trigonometric Functions

Formula

Expression

What it means

Derivative of $\sin x$

$\frac{d}{dx}(\sin x) = \cos x$

The rate of change of sine is cosine, with $x$ in radians.

Derivative of $\cos x$

$\frac{d}{dx}(\cos x) = -\sin x$

The derivative of cosine is negative sine, with $x$ in radians.

Derivative of $\tan x$

$\frac{d}{dx}(\tan x) = \sec^{2} x$

Valid wherever $\cos x \neq 0$, that is $x \neq \frac{\pi}{2} + n\pi$ for any integer $n$.

Derivative of $\cot x$

$\frac{d}{dx}(\cot x) = -\csc^{2} x$

Valid wherever $\sin x \neq 0$, that is $x \neq n\pi$. Here $\csc$ is cosec.

Derivative of $\sec x$

$\frac{d}{dx}(\sec x) = \sec x \tan x$

Valid wherever $\cos x \neq 0$. The function itself stays as a factor in its derivative.

Derivative of cosec x (csc x)

$\frac{d}{dx}(\csc x) = -\csc x \cot x$

Valid wherever $\sin x \neq 0$. Note the minus sign, shared by all the co-functions.

Derivative of $\sin(ax + b)$

$\frac{d}{dx}\sin(ax + b) = a\cos(ax + b)$

The chain rule brings out the coefficient $a$ of $x$ inside the angle.

Derivative of $\cos(ax + b)$

$\frac{d}{dx}\cos(ax + b) = -a\sin(ax + b)$

Same idea for cosine, with the minus sign kept.

Example: At $x = \frac{\pi}{4}$, $\frac{d}{dx}(\tan x) = \sec^{2}\frac{\pi}{4} = (\sqrt{2})^{2} = 2$.

Derivatives Of Inverse Trigonometric Functions

Formula

Expression

What it means

Derivative of $\sin^{-1} x$

$\frac{d}{dx}(\sin^{-1} x) = \frac{1}{\sqrt{1 - x^{2}}}$

Valid for $-1 < x < 1$. Also written as the derivative of $\arcsin x$.

Derivative of arccos

$\frac{d}{dx}(\cos^{-1} x) = -\frac{1}{\sqrt{1 - x^{2}}}$

Valid for $-1 < x < 1$. It is the negative of the derivative of $\sin^{-1} x$.

Derivative of $\tan^{-1} x$

$\frac{d}{dx}(\tan^{-1} x) = \frac{1}{1 + x^{2}}$

Valid for every real $x$. Also written as the derivative of $\arctan x$.

Derivative of $\cot^{-1} x$

$\frac{d}{dx}(\cot^{-1} x) = -\frac{1}{1 + x^{2}}$

Valid for every real $x$. It is the negative of the derivative of $\tan^{-1} x$.

Derivative of $\sec^{-1} x$

$\frac{d}{dx}(\sec^{-1} x) = \frac{1}{\lvert x \rvert \sqrt{x^{2} - 1}}$

Valid for $\lvert x \rvert > 1$, using the principal range $[0, \pi]$ without $\frac{\pi}{2}$.

Derivative of $\csc^{-1} x$

$\frac{d}{dx}(\csc^{-1} x) = -\frac{1}{\lvert x \rvert \sqrt{x^{2} - 1}}$

Valid for $\lvert x \rvert > 1$. It is the negative of the derivative of $\sec^{-1} x$.

Chain rule with inverse trig

$\frac{d}{dx}\tan^{-1}(u) = \frac{1}{1 + u^{2}} \cdot \frac{du}{dx}$

When the argument is a function $u$ of $x$, multiply by $\frac{du}{dx}$. The same pattern holds for all six.

Example: At $x = 0.6$, $\frac{d}{dx}(\sin^{-1} x) = \frac{1}{\sqrt{1 - 0.36}} = \frac{1}{0.8} = 1.25$.

Tangents, Normals And Rates Of Change

Formula

Expression

What it means

Slope of the tangent

$m = f'(x_{1})$

The slope of the curve $y = f(x)$ at the point $(x_{1}, y_{1})$ is the derivative there.

Equation of the tangent

$y - y_{1} = f'(x_{1})(x - x_{1})$

The straight line touching the curve at $(x_{1}, y_{1})$, written in point-slope form.

Slope of the normal

$m_{n} = -\frac{1}{f'(x_{1})}$

The normal is perpendicular to the tangent, so its slope is the negative reciprocal, when $f'(x_{1}) \neq 0$.

Equation of the normal

$y - y_{1} = -\frac{1}{f'(x_{1})}(x - x_{1})$

The line through $(x_{1}, y_{1})$ perpendicular to the tangent. If $f'(x_{1}) = 0$, the normal is $x = x_{1}$.

Horizontal and vertical tangents

$\frac{dy}{dx} = 0$ or $\frac{dx}{dy} = 0$

$\frac{dy}{dx} = 0$ gives a horizontal tangent $y = y_{1}$, and $\frac{dx}{dy} = 0$ gives a vertical tangent $x = x_{1}$.

Angle between two curves

$\tan\theta = \left\lvert \frac{m_{1} - m_{2}}{1 + m_{1}m_{2}} \right\rvert$

$m_{1}$ and $m_{2}$ are the tangent slopes at the point where the curves meet, with $m_{1}m_{2} \neq -1$.

Average rate of change

$\frac{f(b) - f(a)}{b - a}$

The slope of the secant line joining $x = a$ and $x = b$ on the graph.

Related rates

$\frac{dy}{dt} = \frac{dy}{dx} \cdot \frac{dx}{dt}$

Links how fast $y$ changes in time to how fast $x$ changes, when $y$ depends on $x$.

Velocity and acceleration

$v = \frac{ds}{dt}$, $a = \frac{dv}{dt} = \frac{d^{2}s}{dt^{2}}$

For position $s(t)$, velocity is the first derivative and acceleration is the second.

Linear approximation (differentials)

$f(x + \Delta x) \approx f(x) + f'(x),\Delta x$

Estimates a nearby function value using the tangent line, accurate when $\Delta x$ is small.

Marginal cost and revenue

$MC = \frac{dC}{dx}$, $MR = \frac{dR}{dx}$

The rate at which total cost $C$ or revenue $R$ changes with the number of units $x$.

Example: For $y = x^{2}$ at $(3, 9)$, the slope is $2 \times 3 = 6$, so the tangent is $y - 9 = 6(x - 3)$, that is $y = 6x - 9$.

Maxima, Minima And Mean Value Theorems

Formula

Expression

What it means

Increasing test

$f'(x) > 0$ on $(a, b)$

If the derivative is positive throughout an interval, $f$ is strictly increasing there.

Decreasing test

$f'(x) < 0$ on $(a, b)$

If the derivative is negative throughout an interval, $f$ is strictly decreasing there.

Critical point

$f'(c) = 0$ or $f'(c)$ undefined

A point $c$ in the domain where a local maximum or minimum can occur.

First derivative test

$f'$ changes from $+$ to $-$ at $c$

Sign change $+$ to $-$ gives a local maximum, $-$ to $+$ gives a local minimum, and no change gives neither.

Second derivative test

$f'(c) = 0$ and $f''(c) < 0$ or $f''(c) > 0$

$f''(c) < 0$ means local maximum, $f''(c) > 0$ means local minimum, and $f''(c) = 0$ means the test is inconclusive.

Concavity

$f''(x) > 0$ or $f''(x) < 0$

$f'' > 0$ means concave up (convex), $f'' < 0$ means concave down, on that interval.

Point of inflection

$f''(c) = 0$ or undefined, with a sign change

The curve switches concavity at $c$. The sign of $f''$ must actually change, and $f$ must be continuous at $c$.

Absolute extrema on $[a, b]$

compare $f(a)$, $f(b)$ and $f(c)$ for each critical $c$

For a continuous $f$ on a closed interval, the largest and smallest of these values are the absolute maximum and minimum.

Rolle's theorem

$f(a) = f(b) \Rightarrow f'(c) = 0$ for some $c \in (a, b)$

Requires $f$ continuous on $[a, b]$ and differentiable on $(a, b)$. Some point then has a horizontal tangent.

Mean value theorem (Lagrange)

$f'(c) = \frac{f(b) - f(a)}{b - a}$ for some $c \in (a, b)$

Same continuity and differentiability conditions. Some tangent is parallel to the chord joining the endpoints.

Example: For $f(x) = x^{3} - 3x$, $f'(x) = 3x^{2} - 3 = 0$ gives $x = \pm 1$, and $f''(x) = 6x$ shows a local minimum $f(1) = -2$ and a local maximum $f(-1) = 2$.

Basic Integrals

Every indefinite integral carries an arbitrary constant $C$.

Formula

Expression

What it means

Integration formula for powers

$\int x^{n},dx = \frac{x^{n+1}}{n+1} + C$

Raise the power by one and divide by the new power. Valid for every real $n \neq -1$.

Integral of a constant

$\int k,dx = kx + C$

The antiderivative of a constant $k$ is a straight line with slope $k$.

Integral of $\frac{1}{x}$

$\int \frac{1}{x},dx = \ln\lvert x \rvert + C$

Covers the $n = -1$ case the power rule misses. Valid for $x \neq 0$.

Integral of $e^{x}$

$\int e^{x},dx = e^{x} + C$

The natural exponential function $e^{x}$ is its own antiderivative, just as it is its own derivative.

Integral of $e^{kx}$

$\int e^{kx},dx = \frac{1}{k}e^{kx} + C$

Divide by the coefficient $k$ of $x$, where $k \neq 0$.

Integral of $a^{x}$

$\int a^{x},dx = \frac{a^{x}}{\ln a} + C$

For a constant base $a > 0$, $a \neq 1$. Divide by $\ln a$, the reverse of the derivative rule.

Integral of $\sin x$

$\int \sin x,dx = -\cos x + C$

The minus sign appears because the derivative of $\cos x$ is $-\sin x$.

Integral of $\cos x$

$\int \cos x,dx = \sin x + C$

Reverses the rule that the derivative of $\sin x$ is $\cos x$.

Integral of $\sec^{2} x$

$\int \sec^{2} x,dx = \tan x + C$

Reverses the rule that the derivative of $\tan x$ is $\sec^{2} x$.

Integral of $\csc^{2} x$

$\int \csc^{2} x,dx = -\cot x + C$

Reverses the derivative of $\cot x$. Here $\csc$ is cosec.

Integral of $\sec x \tan x$

$\int \sec x \tan x,dx = \sec x + C$

Reverses the rule that the derivative of $\sec x$ is $\sec x \tan x$.

Integral of $\csc x \cot x$

$\int \csc x \cot x,dx = -\csc x + C$

Reverses the rule that the derivative of $\csc x$ is $-\csc x \cot x$.

Integral of $\tan x$

$\int \tan x,dx = \ln\lvert \sec x \rvert + C$

Found by substituting $u = \cos x$. Equivalent to $-\ln\lvert \cos x \rvert + C$ and valid where $\cos x \neq 0$.

Integral of $\cot x$

$\int \cot x,dx = \ln\lvert \sin x \rvert + C$

Found by substituting $u = \sin x$, since $\cot x = \frac{\cos x}{\sin x}$. Valid where $\sin x \neq 0$.

Integral of $\sec x$

$\int \sec x,dx = \ln\lvert \sec x + \tan x \rvert + C$

Valid wherever $\cos x \neq 0$. An equivalent form often used in answers is $\ln\left\lvert \tan\left(\frac{\pi}{4} + \frac{x}{2}\right) \right\rvert + C$.

Integral of cosec x (csc x)

$\int \csc x,dx = \ln\lvert \csc x - \cot x \rvert + C$

Valid wherever $\sin x \neq 0$. An equivalent form often used in answers is $\ln\left\lvert \tan\frac{x}{2} \right\rvert + C$.

Example: $\int (6x^{2} + 2x),dx = \frac{6x^{3}}{3} + \frac{2x^{2}}{2} + C = 2x^{3} + x^{2} + C$.

Standard Integral Forms

Formula

Expression

What it means

Integral of $\frac{1}{a^{2} + x^{2}}$

$\int \frac{dx}{a^{2} + x^{2}} = \frac{1}{a}\tan^{-1}\frac{x}{a} + C$

For a constant $a > 0$. Used whenever the denominator is a sum of two squares.

Integral of $\frac{1}{\sqrt{a^{2} - x^{2}}}$

$\int \frac{dx}{\sqrt{a^{2} - x^{2}}} = \sin^{-1}\frac{x}{a} + C$

For a constant $a > 0$ and $\lvert x \rvert < a$. The inverse sine appears when a square root of a difference sits in the denominator.

Integral of $\frac{1}{x^{2} - a^{2}}$

$\int \frac{dx}{x^{2} - a^{2}} = \frac{1}{2a}\ln\left\lvert \frac{x - a}{x + a} \right\rvert + C$

For $a > 0$ and $x \neq \pm a$. Comes from splitting into partial fractions.

Integral of $\frac{1}{a^{2} - x^{2}}$

$\int \frac{dx}{a^{2} - x^{2}} = \frac{1}{2a}\ln\left\lvert \frac{a + x}{a - x} \right\rvert + C$

For $a > 0$ and $x \neq \pm a$. Note the order of $a$ and $x$ is swapped from the previous row.

Integral of $\frac{1}{\sqrt{x^{2} + a^{2}}}$

$\int \frac{dx}{\sqrt{x^{2} + a^{2}}} = \ln\left\lvert x + \sqrt{x^{2} + a^{2}} \right\rvert + C$

For a constant $a > 0$, valid for every real $x$.

Integral of $\frac{1}{\sqrt{x^{2} - a^{2}}}$

$\int \frac{dx}{\sqrt{x^{2} - a^{2}}} = \ln\left\lvert x + \sqrt{x^{2} - a^{2}} \right\rvert + C$

For a constant $a > 0$, valid only where $\lvert x \rvert > a$ so that the square root is real.

Integral of $\frac{1}{x\sqrt{x^{2} - a^{2}}}$

$\int \frac{dx}{x\sqrt{x^{2} - a^{2}}} = \frac{1}{a}\sec^{-1}\frac{x}{a} + C$

For $x > a > 0$. The extra factor $x$ outside the root turns the answer into an inverse secant.

Integral of $\sqrt{a^{2} - x^{2}}$

$\int \sqrt{a^{2} - x^{2}},dx = \frac{x}{2}\sqrt{a^{2} - x^{2}} + \frac{a^{2}}{2}\sin^{-1}\frac{x}{a} + C$

For $a > 0$ and $\lvert x \rvert \leq a$. Gives areas of circular regions.

Integral of $\sqrt{x^{2} + a^{2}}$

$\int \sqrt{x^{2} + a^{2}},dx = \frac{x}{2}\sqrt{x^{2} + a^{2}} + \frac{a^{2}}{2}\ln\left\lvert x + \sqrt{x^{2} + a^{2}} \right\rvert + C$

For a constant $a > 0$, valid for every real $x$.

Integral of $\sqrt{x^{2} - a^{2}}$

$\int \sqrt{x^{2} - a^{2}},dx = \frac{x}{2}\sqrt{x^{2} - a^{2}} - \frac{a^{2}}{2}\ln\left\lvert x + \sqrt{x^{2} - a^{2}} \right\rvert + C$

For $a > 0$ and $\lvert x \rvert \geq a$. The log term is subtracted here.

Integral of $\frac{f'(x)}{f(x)}$

$\int \frac{f'(x)}{f(x)},dx = \ln\lvert f(x) \rvert + C$

When the numerator is the derivative of the denominator, the answer is a log. Needs $f(x) \neq 0$.

Integral of $e^{x}[f(x) + f'(x)]$

$\int e^{x}[f(x) + f'(x)],dx = e^{x} f(x) + C$

Spot a function plus its own derivative multiplied by $e^{x}$, and the answer is immediate.

Example: $\int_{0}^{3} \frac{dx}{9 + x^{2}} = \frac{1}{3}\tan^{-1}(1) - \frac{1}{3}\tan^{-1}(0) = \frac{\pi}{12} \approx 0.2618$.

Integration Techniques

Formula

Expression

What it means

Substitution (u-substitution)

$\int f(g(x)),g'(x),dx = \int f(u),du$

Set $u = g(x)$ so that $du = g'(x),dx$, integrate in $u$, then substitute back.

Linear substitution

$\int f(ax + b),dx = \frac{1}{a}F(ax + b) + C$

$F$ is an antiderivative of $f$ and $a \neq 0$. Divide by the coefficient of $x$.

Integration by parts (integration of uv formula)

$\int u,dv = uv - \int v,du$

Used for products of functions. Choose $u$ so that $du$ is simpler than $u$.

Integration by parts (product form)

$\int uv,dx = u\int v,dx - \int \left(\frac{du}{dx}\int v,dx\right)dx$

The same rule written for a product $uv$, where $u$ is differentiated and $v$ is integrated.

ILATE rule for choosing $u$

$\text{I} \to \text{L} \to \text{A} \to \text{T} \to \text{E}$

Inverse trig, Logarithmic, Algebraic, Trigonometric, Exponential. Pick $u$ as the type that comes first (LIATE in US books).

Partial fractions: distinct linear factors

$\frac{px + q}{(x - a)(x - b)} = \frac{A}{x - a} + \frac{B}{x - b}$

For $a \neq b$. Find the constants $A$ and $B$, then integrate each term to a log.

Partial fractions: repeated linear factor

$\frac{px^{2} + qx + r}{(x - a)^{2}(x - b)} = \frac{A}{x - a} + \frac{B}{(x - a)^{2}} + \frac{C}{x - b}$

A squared factor needs one term for each power, up to the square. $A$, $B$, $C$ are constants to find.

Partial fractions: irreducible quadratic factor

$\frac{px^{2} + qx + r}{(x - a)(x^{2} + bx + c)} = \frac{A}{x - a} + \frac{Bx + C}{x^{2} + bx + c}$

Used when $b^{2} - 4c < 0$, so the quadratic has no real factors. It gets a linear numerator.

Improper rational function

$\frac{P(x)}{Q(x)} = S(x) + \frac{R(x)}{Q(x)}$

If the degree of $P$ is at least that of $Q$, divide first. $S$ is the quotient, $R$ the remainder.

Trigonometric substitution

$x = a\sin\theta$, $x = a\tan\theta$, $x = a\sec\theta$

Use these for $\sqrt{a^{2} - x^{2}}$, $\sqrt{a^{2} + x^{2}}$ and $\sqrt{x^{2} - a^{2}}$ respectively, with $a > 0$.

Completing the square in a quadratic

$ax^{2} + bx + c = a\left[\left(x + \frac{b}{2a}\right)^{2} + \frac{4ac - b^{2}}{4a^{2}}\right]$

Rewrites a quadratic denominator into a standard form above, for $a \neq 0$.

Integral of $e^{ax}\sin bx$

$\int e^{ax}\sin bx,dx = \frac{e^{ax}}{a^{2} + b^{2}}(a\sin bx - b\cos bx) + C$

Found by using integration by parts twice. Needs $a^{2} + b^{2} \neq 0$.

Integral of $e^{ax}\cos bx$

$\int e^{ax}\cos bx,dx = \frac{e^{ax}}{a^{2} + b^{2}}(a\cos bx + b\sin bx) + C$

The cosine version of the previous row. Note the plus sign inside the bracket.

Example: For $\int x e^{x},dx$, take $u = x$ and $dv = e^{x},dx$, so $\int x e^{x},dx = xe^{x} - \int e^{x},dx = xe^{x} - e^{x} + C$.

Definite Integrals And Their Properties

Formula

Expression

What it means

Fundamental theorem of calculus, part 1

$\frac{d}{dx}\int_{a}^{x} f(t),dt = f(x)$

For a continuous $f$, differentiating an integral with a variable upper limit gives back the integrand.

Fundamental theorem of calculus, part 2

$\int_{a}^{b} f(x),dx = F(b) - F(a)$

$F$ is any antiderivative of $f$ on $[a, b]$, with $f$ continuous. The constant $C$ cancels.

Leibniz rule

$\frac{d}{dx}\int_{g(x)}^{h(x)} f(t),dt = f(h(x)),h'(x) - f(g(x)),g'(x)$

Differentiates an integral whose limits are both functions of $x$, for continuous $f$.

Reversing the limits

$\int_{a}^{b} f(x),dx = -\int_{b}^{a} f(x),dx$

Swapping the upper and lower limits changes the sign of the integral.

Equal limits

$\int_{a}^{a} f(x),dx = 0$

An interval of zero width has zero area.

Splitting the interval

$\int_{a}^{b} f(x),dx = \int_{a}^{c} f(x),dx + \int_{c}^{b} f(x),dx$

Break the integral at any point $c$. Useful for piecewise and absolute value functions.

Change of dummy variable

$\int_{a}^{b} f(x),dx = \int_{a}^{b} f(t),dt$

The letter used for the variable of integration does not affect the value.

King property

$\int_{a}^{b} f(x),dx = \int_{a}^{b} f(a + b - x),dx$

Replacing $x$ by $a + b - x$ leaves the value unchanged. Often adds to the original to simplify.

Property for $\int_{0}^{a}$

$\int_{0}^{a} f(x),dx = \int_{0}^{a} f(a - x),dx$

The special case of the king property with lower limit 0.

Even function rule

$\int_{-a}^{a} f(x),dx = 2\int_{0}^{a} f(x),dx$

Holds when $f(-x) = f(x)$, because the two halves of the area are mirror images.

Odd function rule

$\int_{-a}^{a} f(x),dx = 0$

Holds when $f(-x) = -f(x)$, because the areas on the two sides cancel.

Property for $\int_{0}^{2a}$

$\int_{0}^{2a} f(x),dx = 2\int_{0}^{a} f(x),dx$

Holds when $f(2a - x) = f(x)$. If instead $f(2a - x) = -f(x)$, the integral is 0.

Periodic function rule

$\int_{0}^{nT} f(x),dx = n\int_{0}^{T} f(x),dx$

For $f$ with period $T$ and a positive integer $n$, the integral over $n$ periods is $n$ times one period.

Example: $\int_{1}^{3} 3x^{2},dx = \left[x^{3}\right]_{1}^{3} = 27 - 1 = 26$.

Numerical Integration

Here $h = \frac{b - a}{n}$ is the strip width, $x_{k} = a + kh$ and $y_{k} = f(x_{k})$.

Formula

Expression

What it means

Definite integral as a limit of sums

$\int_{a}^{b} f(x),dx = \lim_{n \to \infty} \sum_{k=1}^{n} f(x_{k}),h$

The exact integral is the limit of Riemann sums as the number of strips $n$ grows without bound.

Left Riemann sum

$L_{n} = h\sum_{k=0}^{n-1} f(x_{k})$

Adds rectangles whose heights come from the left end of each strip.

Right Riemann sum

$R_{n} = h\sum_{k=1}^{n} f(x_{k})$

Adds rectangles whose heights come from the right end of each strip.

Midpoint rule

$M_{n} = h\sum_{k=1}^{n} f\left(\frac{x_{k-1} + x_{k}}{2}\right)$

Uses the height at the centre of each strip, usually more accurate than left or right sums.

Trapezoidal rule

$T_{n} = \frac{h}{2}[y_{0} + 2(y_{1} + y_{2} + \cdots + y_{n-1}) + y_{n}]$

Replaces the curve on each strip with a straight line, so each strip becomes a trapezium (trapezoid).

Simpson's rule (one-third rule)

$S_{n} = \frac{h}{3}[y_{0} + 4(y_{1} + y_{3} + \cdots + y_{n-1}) + 2(y_{2} + y_{4} + \cdots + y_{n-2}) + y_{n}]$

Fits parabolas through pairs of strips, so $n$ must be even. Odd-index ordinates get weight 4, even inner ones weight 2.

Simpson's three-eighths rule

$\frac{3h}{8}[y_{0} + 3y_{1} + 3y_{2} + y_{3}]$

Fits a cubic across three strips. Repeat it for any $n$ that is a multiple of 3.

Example: For $\int_{0}^{2} x^{2},dx$ with $n = 2$ and $h = 1$, the trapezoidal rule gives $\frac{1}{2}[0 + 2(1) + 4] = 3$, while Simpson's rule gives $\frac{1}{3}[0 + 4(1) + 4] = \frac{8}{3} \approx 2.6667$, the exact value.

Applications Of Integrals

Formula

Expression

What it means

Area under a curve

$A = \int_{a}^{b} f(x),dx$

Area between $y = f(x)$ and the x-axis from $x = a$ to $x = b$, when $f(x) \geq 0$ there.

Area when the curve crosses the axis

$A = \int_{a}^{b} \lvert f(x) \rvert,dx$

Parts below the axis count as positive area. Split the integral at each root of $f$.

Area with respect to the y-axis

$A = \int_{c}^{d} g(y),dy$

Area between the curve $x = g(y) \geq 0$ and the y-axis from $y = c$ to $y = d$.

Area between two curves

$A = \int_{a}^{b} [f(x) - g(x)],dx$

Area between the upper curve $f$ and lower curve $g$, where $f(x) \geq g(x)$ on $[a, b]$.

Volume by the disk method

$V = \pi\int_{a}^{b} [f(x)]^{2},dx$

Volume when the region under $y = f(x)$ is rotated about the x-axis, built from circular slices.

Volume by the washer method

$V = \pi\int_{a}^{b} \left([R(x)]^{2} - [r(x)]^{2}\right)dx$

For a region between an outer radius $R(x)$ and inner radius $r(x)$ rotated about the x-axis.

Volume by the shell method

$V = 2\pi\int_{a}^{b} x f(x),dx$

Volume when the region under $y = f(x)$, with $0 \leq a < b$, is rotated about the y-axis, using cylindrical shells.

Arc length of a curve

$L = \int_{a}^{b} \sqrt{1 + [f'(x)]^{2}},dx$

Length of the curve $y = f(x)$ from $x = a$ to $x = b$, for $f'$ continuous.

Arc length of a parametric curve

$L = \int_{\alpha}^{\beta} \sqrt{\left(\frac{dx}{dt}\right)^{2} + \left(\frac{dy}{dt}\right)^{2}},dt$

Length of a curve given by $x(t)$ and $y(t)$ as $t$ runs from $\alpha$ to $\beta$.

Surface area of revolution

$S = 2\pi\int_{a}^{b} f(x)\sqrt{1 + [f'(x)]^{2}},dx$

Curved surface area when $y = f(x) \geq 0$ is rotated about the x-axis.

Average value of a function

$f_{\text{avg}} = \frac{1}{b - a}\int_{a}^{b} f(x),dx$

The constant height giving the same area as $f$ over $[a, b]$, for $a < b$.

Displacement and distance from velocity

$s = \int_{t_{1}}^{t_{2}} v(t),dt$, $d = \int_{t_{1}}^{t_{2}} \lvert v(t) \rvert,dt$

Integrating velocity gives net displacement, and integrating speed gives total distance travelled.

Example: The area between $y = x$ and $y = x^{2}$ from $x = 0$ to $x = 1$ is $\int_{0}^{1} (x - x^{2}),dx = \frac{1}{2} - \frac{1}{3} = \frac{1}{6} \approx 0.1667$.

Differential Equations

Formula

Expression

What it means

Order and degree

$\left(\frac{d^{2}y}{dx^{2}}\right)^{3} + \frac{dy}{dx} = x$ has order 2, degree 3

Order is the highest derivative present. Degree is its power, once the equation is a polynomial in the derivatives.

Separable equation

$\frac{dy}{dx} = g(x),h(y) \Rightarrow \int \frac{dy}{h(y)} = \int g(x),dx + C$

Move all $y$ terms to one side and all $x$ terms to the other, then integrate, where $h(y) \neq 0$.

Linear first-order equation

$\frac{dy}{dx} + P(x),y = Q(x)$

Standard form of a linear equation in $y$, where $P$ and $Q$ are functions of $x$ only.

Integrating factor

$\text{IF} = e^{\int P(x),dx}$

Multiplying the linear equation by this factor turns its left side into the derivative of $y \cdot \text{IF}$.

Solution of a linear equation

$y \cdot \text{IF} = \int Q(x) \cdot \text{IF},dx + C$

Integrate the right side, then divide by the integrating factor to get $y$.

Linear equation in $x$

$\frac{dx}{dy} + P(y),x = Q(y)$, $\text{IF} = e^{\int P(y),dy}$

Same method with the roles of $x$ and $y$ swapped, giving $x \cdot \text{IF} = \int Q(y) \cdot \text{IF},dy + C$.

Homogeneous equation

$\frac{dy}{dx} = F\left(\frac{y}{x}\right)$, $y = vx$, $\frac{dy}{dx} = v + x\frac{dv}{dx}$

Substituting $y = vx$ turns the equation into a separable one in $v$ and $x$.

Exponential growth and decay

$\frac{dy}{dt} = ky \Rightarrow y = y_{0}e^{kt}$

$y_{0}$ is the value at $t = 0$. The quantity grows when $k > 0$ and decays when $k < 0$.

Half-life from the decay constant

$t_{\frac{1}{2}} = \frac{\ln 2}{\lvert k \rvert}$

Time for a decaying quantity with $k < 0$ to halve. Doubling time for growth uses the same form with $k > 0$.

Newton's law of cooling

$\frac{dT}{dt} = -k(T - T_{s}) \Rightarrow T = T_{s} + (T_{0} - T_{s})e^{-kt}$

$T_{s}$ is the surrounding temperature, $T_{0}$ the starting temperature and $k > 0$ a cooling constant.

Logistic growth

$\frac{dP}{dt} = kP\left(1 - \frac{P}{K}\right) \Rightarrow P = \frac{K}{1 + Ae^{-kt}}$

Growth that levels off at the carrying capacity $K$, with $A = \frac{K - P_{0}}{P_{0}}$ and $P_{0}$ the starting value.

Example: If $\frac{dy}{dt} = 0.05y$ and $y(0) = 200$, then $y(10) = 200e^{0.5} \approx 200 \times 1.6487 = 329.74$.

Taylor And Maclaurin Series

Each series equals its function only on the interval stated.

Formula

Expression

What it means

Taylor series about $x = a$

$f(x) = \sum_{n=0}^{\infty} \frac{f^{(n)}(a)}{n!}(x - a)^{n}$

Writes $f$ as a power series in $(x - a)$ using its derivatives at $a$, where the series converges to $f$.

Maclaurin series

$f(x) = f(0) + f'(0)x + \frac{f''(0)}{2!}x^{2} + \frac{f'''(0)}{3!}x^{3} + \cdots$

The Taylor series centred at $a = 0$, used for approximating functions near zero.

Lagrange remainder

$R_{n}(x) = \frac{f^{(n+1)}(c)}{(n+1)!}(x - a)^{n+1}$

The error after the degree $n$ term, for some $c$ between $a$ and $x$. Used to bound approximation error.

Series for $e^{x}$

$e^{x} = 1 + x + \frac{x^{2}}{2!} + \frac{x^{3}}{3!} + \cdots$

Valid for every real $x$. Each term is $\frac{x^{n}}{n!}$ with $n$ starting from 0.

Series for $\sin x$

$\sin x = x - \frac{x^{3}}{3!} + \frac{x^{5}}{5!} - \cdots$

Valid for every real $x$ in radians. Only odd powers appear because sine is an odd function.

Series for $\cos x$

$\cos x = 1 - \frac{x^{2}}{2!} + \frac{x^{4}}{4!} - \cdots$

Valid for every real $x$ in radians. Only even powers appear because cosine is an even function.

Series for $\ln(1 + x)$

$\ln(1 + x) = x - \frac{x^{2}}{2} + \frac{x^{3}}{3} - \cdots$

Valid for $-1 < x \leq 1$. At $x = 1$ it gives $\ln 2$.

Geometric series for $\frac{1}{1 - x}$

$\frac{1}{1 - x} = 1 + x + x^{2} + x^{3} + \cdots$

Valid only for $\lvert x \rvert < 1$. The base series from which many others are built.

Series for $\frac{1}{1 + x}$

$\frac{1}{1 + x} = 1 - x + x^{2} - x^{3} + \cdots$

Replace $x$ by $-x$ in the geometric series. Valid for $\lvert x \rvert < 1$.

Series for $\tan^{-1} x$

$\tan^{-1} x = x - \frac{x^{3}}{3} + \frac{x^{5}}{5} - \cdots$

Valid for $-1 \leq x \leq 1$. At $x = 1$ it gives $\frac{\pi}{4}$.

Binomial series

$(1 + x)^{k} = 1 + kx + \frac{k(k-1)}{2!}x^{2} + \frac{k(k-1)(k-2)}{3!}x^{3} + \cdots$

For any real $k$, valid for $\lvert x \rvert < 1$. It ends after finitely many terms when $k$ is a whole number.

Example: Four terms of the $e^{x}$ series give $e^{0.1} \approx 1 + 0.1 + 0.005 + 0.000167 = 1.105167$, against the true value $1.105171$.

Statistics And Probability Formulas

These formulas summarise a data set, measure its spread, describe how two variables move together and work out the chance of events. They run from Grade 6 data handling up to Class 11 and 12 statistics, AP Statistics, GCSE, SAT and JEE probability.

Mean Of Ungrouped And Grouped Data

Formula

Expression

What it means

Average (arithmetic mean)

$\bar{x} = \frac{\sum x_{i}}{n}$

Add all $n$ values $x_{i}$ and divide by how many there are. Use it for a plain list of raw (ungrouped) data.

Population mean

$\mu = \frac{\sum x_{i}}{N}$

The same calculation over every member of a population of size $N$. Textbooks write $\mu$ for a population and $\bar{x}$ for a sample.

Mean of a frequency table (direct method)

$\bar{x} = \frac{\sum f_{i}x_{i}}{\sum f_{i}}$

Multiply each value $x_{i}$ by its frequency $f_{i}$, add, then divide by the total frequency. For grouped classes, $x_{i}$ is the class mark.

Class mark

$x_{i} = \frac{\text{lower limit} + \text{upper limit}}{2}$

The midpoint of a class interval. It stands in for every value in that class in all grouped-data formulas.

Assumed mean method

$\bar{x} = a + \frac{\sum f_{i}d_{i}}{\sum f_{i}}$ with $d_{i} = x_{i} - a$

Pick a convenient value $a$, usually a central class mark, and work with the smaller deviations $d_{i}$ instead of large class marks.

Step-deviation method

$\bar{x} = a + h \cdot \frac{\sum f_{i}u_{i}}{\sum f_{i}}$ with $u_{i} = \frac{x_{i} - a}{h}$

Here $h$ is the common class width. Dividing deviations by $h$ gives small whole numbers $u_{i}$, and multiplying by $h$ restores the scale.

Weighted mean

$\bar{x}{w} = \frac{\sum w{i}x_{i}}{\sum w_{i}}$

Each value $x_{i}$ counts in proportion to its weight $w_{i}$, as in a grade point average weighted by credit hours.

Combined mean of two groups

$\bar{x} = \frac{n_{1}\bar{x}{1} + n{2}\bar{x}{2}}{n{1} + n_{2}}$

Merges two groups of sizes $n_{1}$ and $n_{2}$ with means $\bar{x}{1}$ and $\bar{x}{2}$ into one overall mean.

Sum of deviations from the mean

$\sum (x_{i} - \bar{x}) = 0$

Deviations above and below the mean always cancel. A quick way to check that a calculated mean is correct.

Mean after a linear change

$\text{mean of } (ax_{i} + b) = a\bar{x} + b$

Multiplying every value by $a$ and then adding $b$ changes the mean in exactly the same way. Useful for coded data and unit changes.

Example: For classes 0 to 10, 10 to 20 and 20 to 30 with frequencies 3, 5 and 2, the class marks are 5, 15 and 25, so $\bar{x} = \frac{3(5) + 5(15) + 2(25)}{10} = \frac{140}{10} = 14$.

Median

Arrange the data in ascending order before using any median formula.

Formula

Expression

What it means

Median (n odd)

$\text{Median} = \left(\frac{n+1}{2}\right)^{\text{th}}$ value

With an odd number $n$ of ordered values, the median is the single middle value of the list.

Median (n even)

$\text{Median} = \frac{1}{2}\left[\left(\frac{n}{2}\right)^{\text{th}} + \left(\frac{n}{2} + 1\right)^{\text{th}}\right]$ values

With an even number $n$ of ordered values, the median is the average of the two middle values.

Median of a discrete frequency table

position $\frac{N+1}{2}$ in the cumulative frequency column

$N = \sum f_{i}$. Find the first value whose cumulative frequency reaches this position. For even $N$, average the two middle observations.

Median class

first class with $cf \geq \frac{N}{2}$

In grouped data, the class where the cumulative frequency first reaches half the total frequency $N$ holds the median.

Median of grouped data

$\text{Median} = l + \left(\frac{\frac{N}{2} - cf}{f}\right) \times h$

$l$ is the lower boundary of the median class, $cf$ the cumulative frequency before it, $f$ its frequency, $h$ the class width.

Median from an ogive

$x$ where $cf = \frac{N}{2}$ on the less-than ogive

Read across from half the total frequency. The same point is where the less-than and more-than ogives intersect.

Median as a quartile and percentile

$\text{Median} = Q_{2} = P_{50}$

The median is the second quartile and the 50th percentile, so half the data lies on each side of it.

Example: Classes 10 to 20, 20 to 30, 30 to 40 and 40 to 50 have frequencies 4, 6, 10 and 5, so $N = 25$, the median class is 30 to 40, and $\text{Median} = 30 + \frac{12.5 - 10}{10} \times 10 = 32.5$.

Mode And The Empirical Relation

Formula

Expression

What it means

Mode (ungrouped data)

$\text{Mode} =$ the most frequent value

A data set can have one mode, several modes (bimodal or multimodal) or no mode when every value occurs equally often.

Mode of grouped data

$\text{Mode} = l + \left(\frac{f_{1} - f_{0}}{2f_{1} - f_{0} - f_{2}}\right) \times h$

$l$ is the lower boundary of the modal class (highest frequency), $f_{1}$ its frequency, $f_{0}$ and $f_{2}$ the frequencies of the classes before and after, $h$ the width.

Mean, median and mode relation

$\text{Mode} = 3,\text{Median} - 2,\text{Mean}$

The empirical relation. It holds approximately for moderately skewed, single-peaked data and lets you estimate one measure from the other two.

Median from mean and mode

$\text{Median} = \frac{\text{Mode} + 2,\text{Mean}}{3}$

The empirical relation rearranged. The median lies between the mean and mode, one third of the way from the mean.

Mean from median and mode

$\text{Mean} = \frac{3,\text{Median} - \text{Mode}}{2}$

The empirical relation rearranged to find the mean when the median and mode of a moderately skewed distribution are known.

Symmetric distribution

$\text{Mean} = \text{Median} = \text{Mode}$

In a perfectly symmetric, single-peaked distribution such as the normal curve, all three averages coincide at the centre.

Positive (right) skew

$\text{Mean} > \text{Median} > \text{Mode}$

A long tail of large values pulls the mean to the right. Typical of incomes and house prices. Negative skew reverses the order.

Karl Pearson's coefficient of skewness

$Sk = \frac{\text{Mean} - \text{Mode}}{\sigma}$ or $Sk = \frac{3(\text{Mean} - \text{Median})}{\sigma}$

$\sigma$ is the standard deviation. Positive values mean right skew, negative values mean left skew, zero means symmetric.

Example: Classes 0 to 10, 10 to 20, 20 to 30 and 30 to 40 have frequencies 5, 8, 12 and 7, so the modal class is 20 to 30 and $\text{Mode} = 20 + \frac{12 - 8}{24 - 8 - 7} \times 10 = 20 + \frac{40}{9} \approx 24.44$.

Range, Quartiles And Percentiles

Formula

Expression

What it means

Range

$\text{Range} = x_{\text{max}} - x_{\text{min}}$

The largest value minus the smallest value. Quick to find but strongly affected by a single extreme value.

Coefficient of range

$\frac{L - S}{L + S}$

$L$ is the largest value and $S$ the smallest. A unit-free version of the range for comparing data sets.

First quartile position

$Q_{1} = \left(\frac{n+1}{4}\right)^{\text{th}}$ value

Position of the lower quartile in ordered data. Interpolate if it is not whole. Some courses use the median of the lower half instead.

Third quartile position

$Q_{3} = \left(\frac{3(n+1)}{4}\right)^{\text{th}}$ value

Position of the upper quartile in ordered data. Three quarters of the values lie at or below $Q_{3}$.

Interquartile range

$\text{IQR} = Q_{3} - Q_{1}$

The spread of the middle 50 percent of the data. It ignores extreme values, so outliers barely affect it.

Quartile deviation (semi-interquartile range)

$\text{QD} = \frac{Q_{3} - Q_{1}}{2}$

Half the interquartile range. Used as a measure of spread alongside the median.

Coefficient of quartile deviation

$\frac{Q_{3} - Q_{1}}{Q_{3} + Q_{1}}$

A unit-free measure of spread based on quartiles, used to compare the variability of different data sets.

Outlier fences

$Q_{1} - 1.5 \times \text{IQR}$ and $Q_{3} + 1.5 \times \text{IQR}$

Values below the lower fence or above the upper fence are flagged as outliers, as on a box plot.

Five-number summary

$x_{\text{min}},\ Q_{1},\ Q_{2},\ Q_{3},\ x_{\text{max}}$

The minimum, lower quartile, median, upper quartile and maximum. These five values are what a box-and-whisker plot draws.

Percentile formula

$\text{Position of } P_{k} = \frac{k(n+1)}{100}$

Gives where the $k$th percentile sits in ordered data of $n$ values, for $0 < k < 100$. Interpolate between neighbours if needed.

Percentile rank

$\text{PR} = \frac{\text{number of values below } x}{n} \times 100$

The percentage of values in the data set that are below the score $x$. A rank of 80 beats 80 percent of scores.

Quartile of grouped data

$Q_{k} = l + \left(\frac{\frac{kN}{4} - cf}{f}\right) \times h$

For $k = 1, 2, 3$. Same symbols as the grouped median, using the class where cumulative frequency first reaches $\frac{kN}{4}$.

Percentile of grouped data

$P_{k} = l + \left(\frac{\frac{kN}{100} - cf}{f}\right) \times h$

Same pattern for the $k$th percentile, using the class where cumulative frequency first reaches $\frac{kN}{100}$.

Example: For 3, 5, 7, 8, 9, 11, 13 ($n = 7$), $Q_{1}$ is the $\frac{8}{4} = 2$nd value, 5, and $Q_{3}$ is the $\frac{24}{4} = 6$th value, 11, so $\text{IQR} = 11 - 5 = 6$.

Mean Deviation

Formula

Expression

What it means

Mean deviation about the mean

$\text{MD}(\bar{x}) = \frac{\sum \lvert x_{i} - \bar{x} \rvert}{n}$

The average distance of the $n$ values from their mean, ignoring signs. Also called the mean absolute deviation (MAD).

Mean deviation about the median

$\text{MD}(M) = \frac{\sum \lvert x_{i} - M \rvert}{n}$

$M$ is the median. Mean deviation is smallest when it is measured about the median.

Mean deviation about any point

$\text{MD}(A) = \frac{\sum \lvert x_{i} - A \rvert}{n}$

The general form, where $A$ is the mean, median or any chosen central value.

Mean deviation for a frequency distribution (about the mean)

$\text{MD}(\bar{x}) = \frac{\sum f_{i}\lvert x_{i} - \bar{x} \rvert}{N}$

$f_{i}$ is the frequency of $x_{i}$ (or of the class mark) and $N = \sum f_{i}$ is the total frequency.

Mean deviation for a frequency distribution (about the median)

$\text{MD}(M) = \frac{\sum f_{i}\lvert x_{i} - M \rvert}{N}$

The same weighted average of absolute deviations, taken from the median $M$ of the distribution.

Coefficient of mean deviation

$\frac{\text{MD}(A)}{A}$

Mean deviation divided by the average $A$ it was measured from. A unit-free figure for comparing spreads.

Example: For 2, 4, 6, 8, 10 the mean is 6, the absolute deviations are 4, 2, 0, 2, 4, and $\text{MD}(\bar{x}) = \frac{12}{5} = 2.4$.

Variance And Standard Deviation

Use the population formulas (divide by $N$) when the data is the whole group, and the sample formulas (divide by $n - 1$) when the data is a sample used to estimate a population.

Formula

Expression

What it means

Population variance

$\sigma^{2} = \frac{\sum (x_{i} - \mu)^{2}}{N}$

The mean of the squared deviations from the population mean $\mu$, over all $N$ members of the population.

Population standard deviation

$\sigma = \sqrt{\frac{\sum (x_{i} - \mu)^{2}}{N}}$

The square root of the population variance. It measures typical distance from the mean in the original units.

Sample variance

$s^{2} = \frac{\sum (x_{i} - \bar{x})^{2}}{n - 1}$

Dividing by $n - 1$ (Bessel's correction) makes $s^{2}$ an unbiased estimate of the population variance from a sample of $n$ values.

Sample standard deviation

$s = \sqrt{\frac{\sum (x_{i} - \bar{x})^{2}}{n - 1}}$

The square root of the sample variance. This is the value most calculators label $s$ or $\sigma_{n-1}$.

Shortcut formula for variance

$\sigma^{2} = \frac{\sum x_{i}^{2}}{N} - \mu^{2}$

The mean of the squares minus the square of the mean. It avoids working out every deviation separately.

Sample shortcut formula

$s^{2} = \frac{\sum x_{i}^{2} - n\bar{x}^{2}}{n - 1}$

The computational form of the sample variance, using the sum of squares and the sample mean $\bar{x}$.

Variance of a frequency distribution

$\sigma^{2} = \frac{\sum f_{i}(x_{i} - \bar{x})^{2}}{N}$

Each squared deviation is weighted by its frequency $f_{i}$, and $N = \sum f_{i}$. For grouped data, $x_{i}$ is the class mark.

Frequency shortcut formula

$\sigma^{2} = \frac{\sum f_{i}x_{i}^{2}}{N} - \left(\frac{\sum f_{i}x_{i}}{N}\right)^{2}$

The mean of the squares minus the square of the mean, written for a frequency table.

Step-deviation method

$\sigma^{2} = h^{2}\left[\frac{\sum f_{i}u_{i}^{2}}{N} - \left(\frac{\sum f_{i}u_{i}}{N}\right)^{2}\right]$ with $u_{i} = \frac{x_{i} - a}{h}$

$a$ is an assumed mean and $h$ the class width. Work with small numbers $u_{i}$, then multiply by $h^{2}$.

Effect of a linear change on variance

$\text{Var}(ax_{i} + b) = a^{2},\text{Var}(x_{i})$

Adding a constant $b$ does not change spread. Multiplying every value by $a$ multiplies the variance by $a^{2}$.

Effect of a linear change on standard deviation

$\sigma_{ax + b} = \lvert a \rvert,\sigma_{x}$

The standard deviation scales by the absolute value of $a$ and ignores the added constant $b$.

Combined variance of two groups

$\sigma^{2} = \frac{n_{1}(\sigma_{1}^{2} + d_{1}^{2}) + n_{2}(\sigma_{2}^{2} + d_{2}^{2})}{n_{1} + n_{2}}$

$d_{1} = \bar{x}{1} - \bar{x}$ and $d{2} = \bar{x}_{2} - \bar{x}$, where $\bar{x}$ is the combined mean of both groups.

Example: For 2, 4, 4, 4, 5, 5, 7, 9, the mean is 5 and $\sum (x_{i} - \bar{x})^{2} = 32$, so $\sigma = \sqrt{\frac{32}{8}} = 2$ as a population and $s = \sqrt{\frac{32}{7}} \approx 2.14$ as a sample.

Coefficient Of Variation And Z-Score

Formula

Expression

What it means

Coefficient of variation

$\text{CV} = \frac{\sigma}{\bar{x}} \times 100%$

Standard deviation as a percentage of the mean (mean must be positive). The data set with the lower CV is more consistent.

Coefficient of standard deviation

$\frac{\sigma}{\bar{x}}$

A unit-free ratio of spread to average. The coefficient of variation is this value multiplied by 100.

Z-score (population)

$z = \frac{x - \mu}{\sigma}$

How many standard deviations the value $x$ lies above (positive) or below (negative) the population mean $\mu$.

Z-score (sample)

$z = \frac{x - \bar{x}}{s}$

The same idea using the sample mean $\bar{x}$ and sample standard deviation $s$. Used to compare scores from different tests.

Raw score from a z-score

$x = \mu + z\sigma$

Converts a z-score back to the original scale, for example to find the mark that sits 1.5 standard deviations above average.

Mean and spread of z-scores

$\bar{z} = 0$ and $\sigma_{z} = 1$

Converting every value in a data set to z-scores always gives a mean of 0 and a standard deviation of 1.

Example: A test has mean 70 and standard deviation 8, so a score of 82 has $z = \frac{82 - 70}{8} = 1.5$, meaning it is 1.5 standard deviations above the mean.

Correlation And Regression

Formula

Expression

What it means

Covariance

$\text{Cov}(x, y) = \frac{\sum (x_{i} - \bar{x})(y_{i} - \bar{y})}{n}$

Positive when $x$ and $y$ tend to rise together, negative when one rises as the other falls. Sample covariance divides by $n - 1$.

Pearson correlation coefficient

$r = \frac{\sum (x_{i} - \bar{x})(y_{i} - \bar{y})}{\sqrt{\sum (x_{i} - \bar{x})^{2} \sum (y_{i} - \bar{y})^{2}}}$

Measures the strength and direction of a straight-line relationship between paired data $x$ and $y$. It has no units.

Pearson r (computational form)

$r = \frac{n\sum xy - \sum x \sum y}{\sqrt{[n\sum x^{2} - (\sum x)^{2}][n\sum y^{2} - (\sum y)^{2}]}}$

The same coefficient written with raw sums, which is faster when working from a table of $n$ pairs.

Range of r

$-1 \leq r \leq 1$

$r = 1$ is a perfect positive line, $r = -1$ a perfect negative line, and $r = 0$ means no linear relationship.

Coefficient of determination

$r^{2}$

The fraction of the variation in $y$ that the regression line on $x$ explains. $r = 0.8$ gives $r^{2} = 0.64$, or 64 percent.

Spearman's rank correlation

$r_{s} = 1 - \frac{6\sum d_{i}^{2}}{n(n^{2} - 1)}$

$d_{i}$ is the difference between the two ranks of each item and $n$ the number of pairs. Exact when there are no tied ranks.

Regression line of y on x

$\hat{y} = a + bx$

The least-squares line used to predict $y$ from $x$. Some textbooks write it as $\hat{y} = b_{0} + b_{1}x$.

Slope of the regression line

$b = \frac{n\sum xy - \sum x \sum y}{n\sum x^{2} - (\sum x)^{2}}$

The predicted change in $y$ for each one-unit increase in $x$, computed from $n$ data pairs.

Slope in terms of r

$b_{yx} = r,\frac{s_{y}}{s_{x}}$

$s_{x}$ and $s_{y}$ are the standard deviations of $x$ and $y$. The slope always has the same sign as $r$.

Intercept of the regression line

$a = \bar{y} - b\bar{x}$

Chosen so the regression line always passes through the point of means $(\bar{x}, \bar{y})$.

Regression line of x on y

$x - \bar{x} = b_{xy}(y - \bar{y})$ with $b_{xy} = r,\frac{s_{x}}{s_{y}}$

Used to predict $x$ from $y$. It is a different line from $y$ on $x$ unless $r = \pm 1$.

Product of regression coefficients

$b_{yx} \cdot b_{xy} = r^{2}$

Both coefficients share the sign of $r$, so $r$ is the square root of their product with that common sign.

Residual

$e_{i} = y_{i} - \hat{y}_{i}$

The observed value minus the value predicted by the line. Least squares makes $\sum e_{i}^{2}$ as small as possible.

Example: For the pairs $(1, 2), (2, 4), (3, 5), (4, 4), (5, 5)$, $b = \frac{5(66) - 15(20)}{5(55) - 15^{2}} = \frac{30}{50} = 0.6$ and $a = 4 - 0.6(3) = 2.2$, so $\hat{y} = 2.2 + 0.6x$.

Probability Basics

Formula

Expression

What it means

Classical probability

$P(E) = \frac{n(E)}{n(S)}$

Favourable outcomes $n(E)$ divided by all outcomes $n(S)$ in the sample space. Valid only when every outcome is equally likely.

Range of a probability

$0 \leq P(E) \leq 1$

A probability of 0 means the event is impossible and 1 means it is certain. Any answer outside this range is wrong.

Empirical (experimental) probability

$P(E) = \frac{\text{number of times } E \text{ occurs}}{\text{total number of trials}}$

The relative frequency of an event in real trials. It approaches the theoretical probability as the number of trials grows.

Complement rule

$P(A') = 1 - P(A)$

$A'$ (also written $A^{c}$ or $\bar{A}$) means "A does not happen". Handy for "at least one" questions.

Addition rule

$P(A \cup B) = P(A) + P(B) - P(A \cap B)$

Probability that $A$ or $B$ (or both) happens. Subtract the overlap so it is not counted twice.

Mutually exclusive events

$P(A \cup B) = P(A) + P(B)$

When $A$ and $B$ cannot happen together, $A \cap B = \emptyset$, so the overlap term is zero.

Addition rule for three events

$P(A \cup B \cup C) = P(A) + P(B) + P(C) - P(A \cap B) - P(B \cap C) - P(A \cap C) + P(A \cap B \cap C)$

Add the single events, subtract the three pairwise overlaps, then add back the triple overlap (inclusion and exclusion).

Exactly A but not B

$P(A \cap B') = P(A) - P(A \cap B)$

The probability that $A$ happens and $B$ does not. Read it from the part of $A$ outside $B$ in a Venn diagram.

Exhaustive, mutually exclusive events

$P(E_{1}) + P(E_{2}) + \cdots + P(E_{n}) = 1$

When events cover the whole sample space and never overlap, their probabilities add to exactly 1.

Sample space for coins and dice

$n(S) = 2^{n}$ for $n$ coins and $n(S) = 6^{n}$ for $n$ dice

Each coin has 2 outcomes and each die has 6, so multiply. Two dice give 36 equally likely ordered outcomes.

Odds in favour

$\text{odds in favour} = \frac{P(E)}{1 - P(E)} = a : b$

$a$ is the number of favourable outcomes and $b$ the number of unfavourable ones, among equally likely outcomes.

Odds against

$\text{odds against} = b : a$

The ratio of unfavourable to favourable outcomes, the reverse of the odds in favour.

Probability from odds

$P(E) = \frac{a}{a + b}$

If the odds in favour of $E$ are $a : b$, the probability of $E$ is $a$ out of $a + b$.

Example: Drawing one card from a standard deck, $P(\text{king or heart}) = \frac{4}{52} + \frac{13}{52} - \frac{1}{52} = \frac{16}{52} = \frac{4}{13}$.

Conditional Probability, Independence And Bayes' Theorem

Formula

Expression

What it means

Conditional probability

$P(A \mid B) = \frac{P(A \cap B)}{P(B)}$

The probability of $A$ given that $B$ has happened, for $P(B) > 0$. The sample space shrinks to $B$.

Multiplication rule

$P(A \cap B) = P(A) \cdot P(B \mid A)$

Probability that both events happen. Works for dependent events, such as drawing two cards without replacement.

Independent events

$P(A \cap B) = P(A) \cdot P(B)$

$A$ and $B$ are independent when one happening does not change the chance of the other, as with separate coin tosses.

Test for independence

$P(A \mid B) = P(A)$

If knowing $B$ happened leaves the probability of $A$ unchanged, the events are independent (for $P(B) > 0$).

Several independent events

$P(A_{1} \cap A_{2} \cap \cdots \cap A_{n}) = P(A_{1})P(A_{2}) \cdots P(A_{n})$

For mutually independent events, the probability that all of them happen is the product of their probabilities.

At least one success

$P(\text{at least one}) = 1 - (1 - p)^{n}$

For $n$ independent trials each with success probability $p$. It is 1 minus the probability of no successes at all.

Complement of a conditional

$P(A' \mid B) = 1 - P(A \mid B)$

Given $B$, either $A$ happens or it does not, so the two conditional probabilities add to 1.

Law of total probability

$P(A) = \sum_{i=1}^{n} P(E_{i}) , P(A \mid E_{i})$

$E_{1}, \ldots, E_{n}$ are mutually exclusive and exhaustive. Add the chance of $A$ along every branch of the tree.

Bayes' theorem

$P(E_{i} \mid A) = \frac{P(E_{i}) , P(A \mid E_{i})}{\sum_{j=1}^{n} P(E_{j}) , P(A \mid E_{j})}$

Reverses a conditional probability. Given that $A$ happened, it gives the probability that it came from cause $E_{i}$.

Bayes' theorem (two events)

$P(A \mid B) = \frac{P(B \mid A) , P(A)}{P(B)}$

The short form, for $P(B) > 0$. Used when $P(B \mid A)$ is known but $P(A \mid B)$ is wanted.

Example: Machine A makes 60 percent of items with 2 percent defective and machine B makes the rest with 5 percent defective, so $P(D) = 0.6(0.02) + 0.4(0.05) = 0.032$ and $P(A \mid D) = \frac{0.012}{0.032} = 0.375$.

Discrete Random Variables And Expected Value

Formula

Expression

What it means

Probability distribution rule

$\sum p_{i} = 1$ with $0 \leq p_{i} \leq 1$

For a discrete random variable $X$ taking values $x_{i}$ with probabilities $p_{i}$, the probabilities must be valid and total 1.

Expected value (mean)

$E(X) = \mu = \sum x_{i}p_{i}$

The long-run average value of $X$ over many repetitions. It need not be a value $X$ can actually take.

Expected value of a function

$E[g(X)] = \sum g(x_{i}) , p_{i}$

Apply $g$ to each value, weight by its probability and add. With $g(x) = x^{2}$ this gives $E(X^{2})$.

Variance of a random variable

$\text{Var}(X) = \sum (x_{i} - \mu)^{2} p_{i}$

The probability-weighted average of squared distances from the mean $\mu = E(X)$.

Variance shortcut

$\text{Var}(X) = E(X^{2}) - [E(X)]^{2}$

The mean of the squares minus the square of the mean. Usually the quickest way to find variance.

Standard deviation of a random variable

$\sigma = \sqrt{\text{Var}(X)}$

The square root of the variance, giving the typical spread of $X$ in its own units.

Linear change of mean

$E(aX + b) = aE(X) + b$

Scaling by $a$ and shifting by $b$ changes the expected value in the same way, for constants $a$ and $b$.

Linear change of variance

$\text{Var}(aX + b) = a^{2},\text{Var}(X)$

The shift $b$ has no effect on spread. The scale factor $a$ enters squared.

Mean of a sum

$E(X + Y) = E(X) + E(Y)$

Expected values always add, whether or not $X$ and $Y$ are independent.

Variance of a sum or difference

$\text{Var}(X \pm Y) = \text{Var}(X) + \text{Var}(Y)$

Holds when $X$ and $Y$ are independent (being uncorrelated is enough). Variances add even for a difference.

Fair game

$E(\text{net gain}) = 0$

A game is fair when the expected net gain for a player is zero. A negative value means the player loses on average.

Example: For one fair die, $E(X) = \frac{21}{6} = 3.5$ and $E(X^{2}) = \frac{91}{6}$, so $\text{Var}(X) = \frac{91}{6} - 3.5^{2} = \frac{35}{12} \approx 2.92$.

Binomial Distribution

Use it when there are $n$ independent trials, each with only two outcomes and the same success probability $p$.

Formula

Expression

What it means

Binomial probability

$P(X = r) = \binom{n}{r} p^{r} q^{n-r}$

Probability of exactly $r$ successes in $n$ trials, for $r = 0, 1, \ldots, n$. $\binom{n}{r}$ is also written $^{n}C_{r}$.

Probability of failure

$q = 1 - p$

Each trial ends in success with probability $p$ or failure with probability $q$, so $p + q = 1$.

Mean of a binomial distribution

$\mu = np$

The expected number of successes in $n$ trials with success probability $p$ in each trial.

Variance of a binomial distribution

$\sigma^{2} = npq$

The spread of the number of successes. Variance is always less than the mean because $q < 1$ when $p > 0$.

Standard deviation of a binomial distribution

$\sigma = \sqrt{npq}$

The square root of $npq$, giving the typical distance of the success count from $np$.

At least one success

$P(X \geq 1) = 1 - q^{n}$

One minus the probability that all $n$ trials fail.

Cumulative binomial probability

$P(X \leq k) = \sum_{r=0}^{k} \binom{n}{r} p^{r} q^{n-r}$

Adds the probabilities of 0 up to $k$ successes. Used for "at most" questions and in binomial tables.

Recurrence between terms

$P(X = r + 1) = \frac{n - r}{r + 1} \cdot \frac{p}{q} \cdot P(X = r)$

Builds each probability from the one before it, which saves recomputing $\binom{n}{r}$ every time.

Most likely number of successes (mode)

$\lfloor (n + 1)p \rfloor$

The greatest integer not exceeding $(n + 1)p$. If $(n + 1)p$ is a whole number, both it and one less are modes.

Sum of all binomial probabilities

$\sum_{r=0}^{n} \binom{n}{r} p^{r} q^{n-r} = (q + p)^{n} = 1$

The binomial theorem shows the probabilities of all possible success counts add to 1.

Example: The probability of exactly 3 heads in 5 tosses of a fair coin is $\binom{5}{3}(0.5)^{3}(0.5)^{2} = \frac{10}{32} = 0.3125$.

Poisson Distribution

Formula

Expression

What it means

Poisson probability

$P(X = r) = \frac{e^{-\lambda}\lambda^{r}}{r!}$

Probability of exactly $r$ events in a fixed interval, for $r = 0, 1, 2, \ldots$, where $\lambda > 0$ is the average number of events.

Mean of a Poisson distribution

$E(X) = \lambda$

The average number of events per interval, such as calls per hour or typing errors per page.

Variance of a Poisson distribution

$\text{Var}(X) = \lambda$

Mean and variance are equal, which is a quick check that Poisson is a sensible model for count data.

Standard deviation of a Poisson distribution

$\sigma = \sqrt{\lambda}$

The square root of the mean rate $\lambda$.

Probability of no events

$P(X = 0) = e^{-\lambda}$

The chance that nothing happens in the interval. One minus this gives the chance of at least one event.

Recurrence between terms

$P(X = r + 1) = \frac{\lambda}{r + 1} , P(X = r)$

Builds each Poisson probability from the previous one, starting from $e^{-\lambda}$.

Poisson approximation to the binomial

$\lambda = np$

Replaces a binomial with a Poisson when $n$ is large and $p$ is small, a common guide being $n \geq 20$ and $p \leq 0.05$.

Sum of independent Poisson variables

$X + Y \sim \text{Poisson}(\lambda_{1} + \lambda_{2})$

If $X$ and $Y$ are independent Poisson counts with rates $\lambda_{1}$ and $\lambda_{2}$, their total is Poisson with the rates added.

Example: With an average of $\lambda = 3$ calls per minute, $P(X = 2) = \frac{e^{-3} \cdot 3^{2}}{2!} = 4.5e^{-3} \approx 0.2240$.

Normal Distribution

Formula

Expression

What it means

Normal probability density

$f(x) = \frac{1}{\sigma\sqrt{2\pi}},e^{-\frac{(x - \mu)^{2}}{2\sigma^{2}}}$

The bell-shaped curve with mean $\mu$ and standard deviation $\sigma > 0$. Probabilities are areas under this curve.

Normal notation

$X \sim N(\mu, \sigma^{2})$

$X$ is normally distributed with mean $\mu$ and variance $\sigma^{2}$. Check whether a textbook puts the variance or the standard deviation second.

Standardising

$Z = \frac{X - \mu}{\sigma}$

Converts any normal variable to the standard normal $Z \sim N(0, 1)$ so that one table or calculator function covers all cases.

Probability between two values

$P(a < X < b) = P\left(\frac{a - \mu}{\sigma} < Z < \frac{b - \mu}{\sigma}\right)$

Standardise both limits, then subtract the two cumulative areas read from the $Z$ table.

Symmetry of the standard normal

$P(Z < -z) = P(Z > z) = 1 - P(Z < z)$

The curve is symmetric about 0, so a left-tail area equals the matching right-tail area.

68 percent rule

$P(\mu - \sigma < X < \mu + \sigma) \approx 0.68$

About 68 percent (more precisely 0.6827) of normal data lies within one standard deviation of the mean.

95 percent rule

$P(\mu - 2\sigma < X < \mu + 2\sigma) \approx 0.95$

About 95 percent (more precisely 0.9545) of normal data lies within two standard deviations of the mean.

99.7 percent rule

$P(\mu - 3\sigma < X < \mu + 3\sigma) \approx 0.997$

About 99.7 percent (more precisely 0.9973) of normal data lies within three standard deviations of the mean.

Standard error of the mean

$\sigma_{\bar{x}} = \frac{\sigma}{\sqrt{n}}$

The standard deviation of sample means for samples of size $n$. Use $s$ in place of $\sigma$ when $\sigma$ is unknown.

Z-score of a sample mean

$z = \frac{\bar{x} - \mu}{\sigma / \sqrt{n}}$

By the central limit theorem, $\bar{x}$ is roughly normal for large samples, usually taken as $n \geq 30$.

Normal approximation to the binomial

$\mu = np$ and $\sigma = \sqrt{npq}$

Use when $np \geq 5$ and $nq \geq 5$ (some courses require 10), with a continuity correction of 0.5 on each boundary.

Continuity correction

$P(X \leq k) \approx P(Y < k + 0.5)$

$X$ is the discrete binomial count and $Y$ the approximating normal variable. Widen each whole-number boundary by 0.5.

Example: Heights have $\mu = 160,\text{cm}$ and $\sigma = 5,\text{cm}$, so 150 cm and 170 cm give $z = -2$ and $z = 2$, and about 95 percent of heights lie between them.

Geometric Probability

Geometric probability assumes the random point is equally likely to land anywhere in the region.

Formula

Expression

What it means

Length model

$P = \frac{\text{favourable length}}{\text{total length}}$

For a point chosen at random on a line segment, the chance it lands in a sub-segment is the ratio of lengths.

Area model

$P = \frac{\text{favourable area}}{\text{total area}}$

For a point chosen at random in a region, such as a dart hitting a board, compare the target area to the whole area.

Volume model

$P = \frac{\text{favourable volume}}{\text{total volume}}$

The three-dimensional version, for a point chosen at random inside a solid.

Spinner or sector model

$P = \frac{\theta}{360^{\circ}}$

$\theta$ is the central angle of the sector in degrees. Use $\frac{\theta}{2\pi}$ if the angle is in radians.

Circle inside a square

$P = \frac{\pi r^{2}}{(2r)^{2}} = \frac{\pi}{4}$

Chance that a random point in a square lands inside the circle inscribed in it, about 0.785, whatever the size.

Waiting time

$P = \frac{w}{T}$

If a bus comes every $T$ minutes and you arrive at a random time, the chance of waiting at most $w$ minutes, for $0 \leq w \leq T$.

Meeting problem

$P = 1 - \left(1 - \frac{t}{T}\right)^{2}$

Two people arrive at random within $T$ minutes and each waits $t$ minutes. This is the chance they meet, for $0 \leq t \leq T$.

Example: A circle of radius 5 cm is drawn on a square board of side 20 cm, so a random dart on the board lands in the circle with probability $\frac{25\pi}{400} \approx 0.1963$.

The Short Version

  • A math formula is a rule in symbols that calculates one quantity from others, and it only works when its conditions hold.

  • This page groups math formulas into nine branches, from basic arithmetic to statistics, with the meaning of every letter and a worked example for each subtopic.

  • The costliest mistakes are small ones: a missing bracket in the slope formula, a dropped $2ab$, the $n$ versus $n - 1$ in standard deviation.

  • Formulas stick when you derive them once and then use them, not when you reread a list.

  • To work through these formulas with a teacher, try a high school math tutor or live math classes online.

Read More

Pick one branch, cover the Expression column, and rewrite five formulas from memory. Check them against the tables, then work the Example under each one. Want a live Bhanzu trainer to go through the formulas your class is using? Book a free demo class.

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Frequently Asked Questions

What are math formulas?
Math formulas are rules written in symbols that show how one quantity is calculated from others, such as $A = \pi r^{2}$ for the area of a circle. Each one holds under stated conditions, which the tables above list next to every formula.
What are the basic math formulas every student should know?
Area and perimeter of the common shapes, the Pythagorean theorem, percent change, simple and compound interest, the laws of exponents, $(a + b)^{2}$, and the quadratic formula. Almost every later topic leans on these.
How many math formulas are there?
There is no fixed number, because every new result can be written as a formula. This page collects about 1,460 of the formulas used from Grade 6 to Grade 12, grouped into nine branches.
What is the difference between a formula and an equation?
We covered this near the top: a formula is a rule for calculating one quantity from others, while an equation is any statement that two expressions are equal. Most formulas are written as equations, but most equations, such as $2x + 3 = 11$, are not formulas.
How can I remember math formulas quickly?
Derive each formula once, learn formulas in families, and rewrite a chapter's formulas from memory before checking them. Using a formula on five or six real problems fixes it far better than rereading a list.
Do you get a formula sheet in the SAT or GCSE maths exams?
Yes for both, at present. The SAT shows a reference sheet of common formulas on every test with math questions, and GCSE maths students in England get a formulae sheet for the 2025, 2026 and 2027 exams.
What is the most important formula in math?
No single one. The Pythagorean theorem and the quadratic formula are probably the most used in school, and Euler's identity, $e^{i\pi} + 1 = 0$, is often called the most elegant.
✍️ Written By
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Bhanzu Team
Content Creator and Editor
Bhanzu’s editorial team, known as Team Bhanzu, is made up of experienced educators, curriculum experts, content strategists, and fact-checkers dedicated to making math simple and engaging for learners worldwide. Every article and resource is carefully researched, thoughtfully structured, and rigorously reviewed to ensure accuracy, clarity, and real-world relevance. We understand that building strong math foundations can raise questions for students and parents alike. That’s why Team Bhanzu focuses on delivering practical insights, concept-driven explanations, and trustworthy guidance-empowering learners to develop confidence, speed, and a lifelong love for mathematics.
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