Trigonometry/Print version

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Contents[edit]

Algebra

  • Geometry
  • Trigonometry
  • Introduction (page 1)
  • In simple terms
  • Radian and Degree Measure
  • The Unit Circle
  • Trigonometric Angular Functions
  • Right Angle Trigonometry
  • Graphs of Sine and Cosine Functions
  • Graphs of Other Trigonometric Functions
  • Inverse Trigonometric Functions
  • Applications and Models
  • Analytic Trigonometry
  • Using Fundamental Identities
  • Verifying Trigonometric Identities
  • Solving Trigonometric Equations
  • Sum and Difference Formulas
  • Multiple-Angle and Product-to-sum Formulas
  • Additional Topics in Trigonometry
  • Law of Sines
  • Law of Cosines
  • Vectors in the Plane
  • Vectors and Dot Products
  • Trigonometric Form of the Complex Number
  • Trigonometric Unit Circle and Graph Reference
  • Trigonometric Formula Reference
  • Trigonometric Identities Reference
  • Natural Trigonometric Functions of Primary Angles

Prerequisites And Basics[edit]

To be able to study Trigonometry successfully, it is recommended that students complete Geometry and Algebra prior to digging in to the course material. Students should also be familiar with the arithmetic of the real number system. It is helpful to have a graphing calculator and graph paper on hand to be able to follow along as well. If one is not available, software available on sites such as GraphCalc or GeoGebra may be helpful. Geometric constructions proposed in the text can be drawn using Geops, free software for performing geometric constructions in the manner of the Ancient Greeks.

Next Page: In simple terms

Home: Trigonometry

Introduction[edit]

Trigonometry is the study of the properties of triangles.

  • "Tri" is Ancient Greek word for three,
  • "gon" means side,
  • "metry" measurement

Together they make "measuring three sides".

If you know some facts about a triangle, such as the lengths of its sides, then using trigonometry you can find out other facts about it. If you know the lengths of sides then you can find what the angles are. If you know the length of one side and of two of the angles, then you can work out what the remaining angle is, and also what the lengths of the other two sides are.

As a consequence the Ancient Greeks were able to use trigonometry to calculate the distance from the Earth to the Moon.

Starting Learning Trigonometry[edit]

One of the first things we learn in trigonometry is how to calculate what the third angle in a triangle is when given the other two angles. For example, in a triangle if two of the angles are 60^{\circ}\, then the third angle must be 60^{\circ}\, too.

However, if we're instead told two lengths, say 7cm and 10cm, and if we're not told anything about the angles, then the third length has a range of possibilities. It could be 5cm. It could be 15cm.

To calculate lengths we start out by examining a right-angled triangle, i.e. one where one of the angles is 90^{\circ}\,.

A right-angle triangle

We'll be using right-angled triangles a lot.

In a right-angled triangle we can work out the length of the longest side if given the lengths of the two shorter sides. In a right-angled triangle the lengths of the sides have a particularly nice relationship to each other. The formula for this relationship is written:

a^2 + b^2 = c^2\!\,

How you use this formula to calculate the third side when you know two of the sides in a right-angled triangle is explained in the page on the 'Pythagoras' Theorem'

What if the triangle isn't a right-angled triangle, though? What if it doesn't have a right angle?

More complex triangles can be built by joining right-angled triangles together. What we learn about right-angled triangles enables us to work with other kinds of triangles too. Trigonometry and trigonometric functions can also be used with more complex shapes such as squares, hexagons, circles and ellipses. Ultimately the most important mathematical tools we have for measuring the universe are based on the study of the mathematics of triangles.

Trigonometry is a fundamental step in your mathematical education. From the seemingly simple shape, the right triangle, we gain tools and insight that help us in practical and theoretical endeavors. The subtle mathematical relationships between the right triangle, the circle, the sine wave, and the exponential curve can only be fully understood with a firm foundation in trigonometry.


Applications[edit]

Triangles used in architecture. This is part of a roof.
Triangles and trigonometry are important in engineering.

Trigonometry is a branch of mathematics concerned with the lengths of the sides and size of the angles of triangles. Because many physical questions can be framed in terms of triangles, trigonometry has found wide use in the physical sciences and engineering.

Trigonometry is needed in surveying and architecture since relationships between lengths and angles in triangles are used directly.

3 phase AC waveform. Trigonometry functions are used in Electrical Engineering

Trigonometry is also used in electrical engineering. The functions that relate angles and side lengths in right triangles turn out to also be useful in expressing how AC electric current varies with time.


In simple terms[edit]


Introduction to Angles[edit]

An angle between two lines in a 2-dimensional plane

An angle is formed when two lines intersect; the point of intersection is called the vertex. We can think of an angle as the wedge-shaped space between the lines where they meet. Note that if both lines are extended through the meeing point, there are in fact four angles.

The size of the angle is the degree of rotation between the lines. The more we must rotate one line to meet the other, the larger the angle is.

Suppose you wish to measure the angle between two lines exactly so that you can tell a remote friend about it: draw a circle with its center located at the meeting of the two lines, making sure that the circle is small enough to cross both lines, but large enough for you to measure the distance along the circle's edge, the circumference, between the two cross points. Obviously this distance depends on the size of the circle, but as long as you tell your friend both the radius of the circle used, and the length along the circumference, then your friend will be able to reconstruct the angle exactly.

Definition of an Angle[edit]

An angle is determined by rotating a ray about its endpoint. The starting position of the ray is called the initial side of the angle. The ending position of the ray is called the terminal side. The endpoint of the ray is called its vertex. Positive angles are generated by counter-clockwise rotation. Negative angles are generated by clockwise rotation.

Consequently an angle has four parts: its vertex, its initial side, its terminal side, and its rotation.

An angle is said to be in standard position when it is drawn in a cartesian coordinate system in such a way that its vertex is at the origin and its initial side is the positive x-axis.

an angle in standard position

Definition of a Triangle[edit]

A triangle is a planar (flat) shape with three straight sides. An angle is formed between each two sides of a triangle, and a triangle has three angles, hence the name tri-angle. So a triangle has three straight sides and three angles.

If you give me three lengths, I can only make a triangle from them if the greatest length is less than the sum of the other two. Three lengths that do not make the sides of a triangle are your height, the height of the nearest tree, the distance from the top of the tree to the center of the sun.

Triangle Ratios[edit]

Angles are not affected by the length of lines: an angle is invariant under transformations of scale, that is:

If you make the triangle bigger,
but keep the sides in the same ratio,
its angles won't change.

Right Angles[edit]

An angle of particular significance is the right angle: the angle at each corner of a square or a rectangle. A rectangle can always be divided into two triangles by drawing a line from one corner of the rectangle to the opposite corner.

It is also true that every right-angled triangle is half a rectangle.

Right Triangle

A rectangle has four sides; they are generally of two different lengths: two long sides and two short sides. (A rectangle with all sides equal is a square.) When we split the rectangle into two right-angled triangles, each triangle has a long side and a short side from the rectangle as well as a copy of the split line.

So the area of a right-angled triangle is half the area of the rectangle from which it was split. Looking at a right-angled triangle, we can tell what the long and short sides of that rectangle were; they are the sides, the lines, that meet at a right angle. The area of the complete rectangle is the long side times the short side. The area of a right-angled triangle is therefore half as much.

Right Triangles and Measurement[edit]

How to bisect an angle

It is possible to bisect any angle using only circles (which can be drawn with a compass) and straight lines by the following procedure:

  1. Call the vertex of the angle O. Draw a circle centered at O.
  2. Mark where the circle intersects each ray. Call these points A and B.
  3. Draw circles centered at A and B with equal radii, but make sure that these radii are large enough to make the circles intersect at two points. One sure way to do this is to draw line segment AB and make the radius of the circles equal to the length of that line segment. On the diagram, circles A and B are shown as near-half portions of a circle.
  4. Mark where these circles intersect, and connect these two points with a line. This line bisects the original angle.

A proof that the line bisects the angle is found in Proposition 9 of Book 1 of the Elements.

Given a right angle, we can use this process to split that right angle indefinitely to form any binary fraction (i.e., \frac{1}{2^n}, n \in \mathbb{Z}, e.g. \frac{1}{2}, \frac{1}{4}, \frac{1}{8}, \frac{1}{16}, \frac{1}{32}...) of it. Thus, we can measure any angle in terms of right angles. That is, a measurement system in which the size of the right angle is considered to be one.

Introduction to Radian Measure[edit]

En Radian cropped color.png
Of course, it is equally possible to start with a different sized angle and split it into two equal angles. We might consider the angle made by half a circle to be "one", or the angle made by a full circle to be "one".

Trigonometry is simplified if we choose the following strange angle as "one":

    1. Draw a circle with the radius marked.
    2. From the point where the radius meets the circumference of the circle, measure one radius length along the circumference of the circle moving counterclockwise and mark this point.
    3. Draw a line from this mark back to the center of the circle.
    4. The angle so formed is considered to be of size one in trigonometry; in order to tell your friends that this is the method you were using, you would say 'measuring in radians'.

Understanding the three sides of a Radian[edit]

To illustrate how the three sides of a radian relate to one another try the below thought experiment:

    1. Assume you have a piece of string that is exactly the length of the radius of a circle.
    2. Assume you have drawn a radian in the same circle. The radian has 3 points. One is the center of your circle and the other two are on the circumference of the circle where the sides of the radian intersect with the circle.
    3. Attach one end of the string at one of the points where the radian intersects with the circumference of the circle.
    4. Take the other end of the string and, starting at the point you chose in Step 2 above, trace the circumference of the circle towards the second point where the radian intersects with the circle until the string is pulled tight.
    5. You will see that the end of the string travels past the second point.
    6. This is because the string is now in a straight line. However, the radian has an arc for its third side, not a straight line. Even though a radian has three equal sides, the arc's curve causes the two points where the radian intersects with the circle to be closer together than they are to the third point of the triangle, which is at the center of our circle in this example.
    7. Now, with the string still pulled tight, find the half way point of the string, then pull it onto the circumference of the circle while allowing the end of the string to move along the circle's circumference. The end of the string is now closer to the second point because the path of the string is closer to the path of the circle's circumference.
    8. We can keep improving the fit of the string's path to the path of the circle's circumference by dividing each new section of the string in half and pulling it towards the circumference of the circle.

Is a radian affected by the size of its circle?[edit]

Does it matter what size circle is used to measure in radians? Perhaps using the radius of a large circle will produce a different angle than that produced by the radius of a small circle. The answer is no.

Two different size radian-arcs have the same angle-measure regardless of their radius.


Recall our radian and circle from the experiment in the subsection above. Draw another circle inside the first circle, with the same center, but with half the radius. You will see that you have created a new radian inside the smaller circle that shares the same angle as the radian in the larger circle. We know that the two sides of the radians emanating from the center of the circles are equal to the radius of their respective circle. We also know that the third side of the radian in the larger circle (the arc) is also equal to the larger circle's radius. But how do we know that the third side of the radian in the smaller circle (the arc that follows the circumference of the smaller circle) is equal to the radius of the smaller circle? To see why we do know that the third side of the smaller circle's radian is equal to its radius, we first connect the two points of each radian that intersect with the circle with each other. By doing so, you will have created two isosceles triangles (triangles with two equal sides and two equal angles).

An isosceles triangle has two equal angles and two equal sides. If you know one angle of any isosceles triangle and the length of two sides that make up that angle, then you can easily deduce the remaining characteristics of the isosceles triangle. For instance, if the two equidistant sides of an isosceles triangle intersect to form an angle that is equal to 40o, then you know the remaining angles must both equal 70º. Since we know that the equidistant sides of our two isosceles triangles make up our known angle, then we can deduce that both of our radians (when converted to isosceles triangles with straight lines) have identical second and third angles. We also know that triangles with identical angles, regardless of their size, will have the length of their sides in a constant ratio to each other. For instance, we can deduce that an isosceles triangle will have sides that measure 2 meters by 4 meters by 4 meters if we know that an isoscleses triangle with identical angles measures 1 meter by 2 meters by 2 meters. Therefore, in our example, our isosceles triangle formed by the second smaller circle will have a third side exaclty equal to half of the third side of the isosceles triangle created by the larger circle. The relationship between the size of the sides of two triangles that share identical angles is also found in the relationship between radius and circumference of two circles that share the same center point - they will share the exact same ratio. In our example then, since the radius of our second smaller circle is exactly half of the larger circle, the circumference between the two points where the radian of the smaller circle intersect (which we have shown is one half of the distance between the two similar points on the larger circle) will share the same exact ratio. And there you have it - the size of the circle does not matter.

Using Radians to Measure Angles[edit]

Once we have an angle of one radian, we can chop it up into binary fractions as we did with the right angle to get a vast range of known angles with which to measure unknown angles. A protractor is a device which uses this technique to measure angles approximately. To measure an angle with a protractor: place the marked center of the protractor on the corner of the angle to be measured, align the right hand zero radian line with one line of the angle, and read off where the other line of the angle crosses the edge of the protractor. A protractor is often transparent with angle lines drawn on it to help you measure angles made with short lines: this is allowed because angles do not depend on the length of the lines from which they are made.

If we agree to measure angles in radians, it would be useful to know the size of some easily defined angles. We could of course simply draw the angles and then measure them very accurately, though still approximately, with a protractor: however, we would then be doing physics, not mathematics.

The ratio of the length of the circumference of a circle to its radius is defined as 2π, where π is an invariant independent of the size of the circle by the argument above. Hence if we were to move 2π radii around the circumference of a circle from a given point on the circumference of that circle, we would arrive back at the starting point. We have to conclude that the size of the angle made by one circuit around the circumference of a circle is 2π radians. Likewise a half circuit around a circle would be π radians. Imagine folding a circle in half along an axis of symmetry: the resulting crease will be a diameter, a straight line through the center of the circle. Hence a straight line has an angle of size π radians.

Folding a half circle in half again produces a quarter circle which must therefore have an angle of size π/2 radians. Is a quarter circle a right angle? To see that it is: draw a square whose corner points lie on the circumference of a circle. Draw the diagonal lines that connect opposing corners of the square, by symmetry they will pass through the center of the circle, to produce 4 similar triangles. Each such triangle is isoceles, and has an angle of size 2π/4 = π/2 radians where the two equal length sides meet at the center of the circle. Thus the other two angles of the triangles must be equal and sum to π/2 radians, that is each angle must be of size π/4 radians. We know that such a triangle is right angled, we must conclude that an angle of size π/2 radians is indeed a right angle.

Summary and Extra Notes[edit]

In summary: it is possible to make deductions about the sizes of angles in certain special conditions using geometrical arguments. However, in general, geometry alone is not powerful enough to determine the size of unknown angles for any arbitrary triangle. To solve such problems we will need the help of trigonometric functions.

In principle, all angles and trigonometric functions are defined on the unit circle. The term unit in mathematics applies to a single measure of any length. We will later apply the principles gleaned from unit measures to larger (or smaller) scaled problems. All the functions we need can be derived from a triangle inscribed in the unit circle: it happens to be a right-angled triangle.

The hypotenuse rotate counter-clockwise

The center point of the unit circle will be set on a Cartesian plane, with the circle's centre at the origin of the plane — the point (0,0). Thus our circle will be divided into four sections, or quadrants.

Quadrants are always counted counter-clockwise, as is the default rotation of angular velocity \omega (omega). Now we inscribe a triangle in the first quadrant (that is, where the x- and y-axes are assigned positive values) and let one leg of the angle be on the x-axis and the other be parallel to the y-axis. (Just look at the illustration for clarification). Now we let the hypotenuse (which is always 1, the radius of our unit circle) rotate counter-clockwise. You will notice that a new triangle is formed as we move into a new quadrant, not only because the sum of a triangle's angles cannot be beyond 180°, but also because there is no way on a two-dimensional plane to imagine otherwise.

Radian and Degree Measure[edit]

Contents

There are 360o in
a complete circle


Units of Measure[edit]

We have been measuring angles in degrees, with 360o in a complete circle.

Choice of Units for Length and Weight[edit]

In measuring many quantities we have a choice of units. For example with distances we can use the metric system and measure in metres, kilometres, centimetres, millimetres. It is also possible to measure distances in miles, yards, feet and inches. With weights we can measure in kilogrammes and grammes. We can also measure in pounds and ounces.

Choice of Units for Measuring Time[edit]

In measuring time we choose to have sixty seconds in a minute and sixty minutes in an hour. We could devise a new more metric system for time and divide an hour into 100 units, each three fifths of our current minute, and then divide these shorter 'minutes' up into 100 units each of which would be about a third of a second.

Why 60? Why 360?[edit]

The choice of dividing into 60 is not entirely arbitrary. 60 can be divided evenly into 2,3,4,5 or 6 or 10 or 12 parts. 60 can't be divided evenly into 7 equal parts, each a whole number in size, but it's still pretty good. Using 360 degrees in a full circle gives us many ways to divide the circle evenly with a whole number of degrees. Nevertheless, we could divide the circle into other numbers of units.

Metric Degrees?[edit]

From the earlier talk of the metric system you might be anticipating that we are about to divide the circle up into 100 or 1000 'degrees'. There is actually a unit called the 'grade' or 'Gradian' (Grad on calculators which have it) in which angles are measured by dividing a right angle up into 100 equal parts, each of one Gradian in size. One Gradian is 0.9 of a degree - quite close to being one degree. The grade is in turn divided into 100 minutes and one minute into 100 seconds. This centesimal system (from the Latin centum, 100) was introduced as part of the metric system after the French Revolution. The Gradian unit is nothing like as widely used as either degrees or the units that interests us most on this page. The unit we introduce here is called the Radian.

Choice of Units for Radians[edit]

Radians are quite large compared to degrees (and to Gradians). There are about 6.28 Radians to a complete circle. There are about 57.3 degrees in one Radian.

Exercise: Check the Statements

Are the statements:

  • There are about 6.28 Radians to a complete circle.
  • There are about 57.3 degrees in one Radian.

Compatible? It is not hard to check.

Digression: In maths books it is well worth quickly checking statements that can be checked easily. It helps reinforce your understanding and confirm that you are understanding what is being said. Also, unfortunately, it isn't that unusual for maths books have tiny slips in them, where the person writing the book has written say, \displaystyle x_i instead of \displaystyle x_j or some other small slip. These tend to happen where the author knows the material very well and is seeing what he expects to see rather than what is actually written. They can be very confusing to someone new to the material. These kinds of mistakes can also happen in wikibooks, sometimes a visitor trying to improve the content can actually introduce errors. In wikibooks you may also see sudden changes in notation or notation that does not match a diagram, where material has been written by different people.


We said "there are about 6.28 Radians to a complete circle". The exact number is \displaystyle 2\pi, making the number of radians in a complete circle the same as the length of the circumference of a unit circle.

Remember that:

The circumference of a circle is
\displaystyle 2\pi \times R
where \displaystyle R is the radius.


Justifying Choice of Units for Radians[edit]

At this stage in explaining trigonometry it is rather difficult to justify the use of these strange units. There aren't even an exact whole number of radians in a complete circle. In more advanced work, particularly when we use calculus they become the most natural units to use for angles with functions like \displaystyle \cos \alpha and \displaystyle \sin \alpha. A flavour of that, but it is only a hint as to why it is a good unit to use, is that for very small angles.

\displaystyle \sin \alpha \approx \alpha

And the approximation is better the smaller the angle is. This only works if we choose Radians as our unit of measure and small angles.


Worked Example: Small angles in Radians and Degrees

We claim that for small angles measured in radians the angle measure and the sine of the angle are very similar.

Let us take one millionth of a circle. In degrees that is 0.00036 degrees. In Radians that is \displaystyle \frac{2\pi}{1,000,000} \approx 0.00000628 Radians. The angle of course is the same. It's one millionth of a circle, however we choose to measure it. It is just as with weights where a weight is the same whether we measure it in kilogrammes or pounds.

The sine of this angle, which is the same value whether we chose to measure the angle in degrees or in radians, it turns out, is about 0.00000628. If your calculator is set to use degrees then \displaystyle \sin 0.00036^\circ will give you this answer.


The Radian Measure[edit]

There are
\displaystyle 2\pi Radians
in a complete circle.


It is traditional to measure angles in degrees; there are 360 degrees in a full revolution. In mathematically more advanced work we use a different unit, the radian. This makes no fundamental difference, any more than the laws of physics change if you measure lengths in metres rather than inches. In advanced work, If no unit is given on an angle measure, the angle is assumed to be in radians.

\frac{3\pi}{2}^{c} \equiv \frac{3\pi}{2} \;\mathrm{rad.} \equiv \frac{3\pi}{2}

A notation used to make it really clear that an angle is being measured in radians is to write 'radians' or just 'rad' after the angle. Very very occasionally you might see a superscript c written above the angle in question.

What You need to Know[edit]

For book one of trigonometry you need to know how to convert from degrees to radians and from radians to degrees. You also need to become familiar with frequently seen angles which you know in terms of degrees, such as \displaystyle 90^\circ in terms of radians as well (it's \displaystyle \pi/2 Radians). Angles in Radians are nearly always written in terms of multiples of Pi.

You will also need to be familiar with switching your calculator between degrees and radians mode.

Everything that is said about angles in degrees, such as that the angles in a triangle add up to 180 degrees has an equivalent in Radians. The angles in a triangle add up to \displaystyle \pi Radians.

Defining a radian[edit]

A single radian is defined as the angle formed in the minor sector of a circle, where the minor arc length is the same as the radius of the circle.

Defining a radian with respect to the unit circle.


1 rad \approx 57.296^{\circ}

Measuring an angle in radians[edit]

The size of an angle, in radians, is the length of the circle arc s divided by the circle radius r.

\mbox{angle in radians} = \frac sr

Measuring an Angle in Radians

We know the circumference of a circle to be equal to 2 \pi r, and it follows that a central angle of one full counterclockwise revolution gives an arc length (or circumference) of s = 2 \pi r. Thus 2 π radians corresponds to 360°, that is, there are 2\pi radians in a circle.

Converting between Radians and Degrees[edit]

Because there are 2π radians in a circle:

To convert degrees to radians:
 \theta ^{c} = \theta^\circ \times \frac{\pi}{180}

To convert radians to degrees:
 \phi ^\circ= \phi^{c} \times \frac{180}{\pi}

Exercises[edit]

Conversion from degrees to radians
  • Convert
  • 180° into radian measure.


  • 90° into radian measure.


  • 45° into radian measure.


  • 137° into radian measure.



Conversion from radians to degrees
  • Convert:
  • \frac{\pi}{3} into degree measure.


  • \frac{\pi}{6} into degree measure.


  • \frac{7\pi}{3} into degree measure.


  • \frac{3\pi}{4} into degree measure.



The Unit Circle[edit]

The Unit Circle is a circle with its center at the origin (0,0) and a radius of one unit.

Unit Circle

Angles are always measured from the positive x-axis (also called the "right horizon"). Angles measured counterclockwise have positive values; angles measured clockwise have negative values.

Defining Sine and Cosine in terms of the unit circle[edit]

In the unit circle shown here, a unit-length radius has been drawn from the origin to a point (x,y) on the circle.

Defining sine and cosine

A line perpendicular to the x-axis, drawn through the point (x,y), intersects the x-axis at the point with the abscissa x. Similarly, a line perpendicular to the y-axis intersects the y-axis at the point with the ordinate y. The angle between the x-axis and the radius is \alpha.

We define the basic trigonometric functions of any angle \alpha as follows:


\begin{matrix}
\mathrm{Sine:} & \sin(\alpha) & = & y \\
\mathrm{Cosine:} & \cos(\alpha) & = & x \\
\end{matrix}

\tan\theta can be algebraically defined.

\tan\theta = \frac{\sin\theta}{\cos\theta} \qquad \cos\theta \ne 0

\tan\alpha = \frac{y}{x} \qquad x \ne 0

These three trigonometric functions can be used whether the angle is measured in degrees or radians as long as it specified which, when calculating trigonometric functions from angles or vice versa.

Alternative definitions[edit]

  • A previous chapter used Soh-Cah-Toa to define the trigonometric functions. The advantage of the unit circle is that θ can be extended outside the first quadrant [0,π/2], which allows us to define these functions on the interval [-∞,+-∞].
  • If trigonometry is applied to vectors, it is more convenient if the radius of the circle is not equal to unity. For example, if vector A has magnitude A=|A|:


\begin{matrix}
x   = r\cos\alpha & \rightarrow  & A_x  = A\cos\alpha \\
y    = r\sin\alpha & \rightarrow  & A_y  = A\sin\alpha \\
r^2  =  x^2+y^2     & \rightarrow  & A^2  =  A_x^2+A_y^2 \\
\end{matrix}

Video Links[edit]

More about this topic can be found at the 'Khan Academy:'

Some Values for Sine and Cosine[edit]

A unit circle with certain exact values marked on it is below:

Labeled Unit Circle

It is worth memorizing some of the values of sine and cosine on the unit circle (cosine is equal to x while sine is equal to y). You should at least become familiar with the values for \displaystyle 0^\circ, 30^\circ 45^\circ, 90^\circ and know where \displaystyle \pi/2, \pi, 3\pi/2, 2\pi are on the unit circle .

Unit circles form the basis of most analog clocks and animations on computers since the cos and sin correspond to the x and y positions of the end of the line segments representing the hands of the clock.

Clock Hands
  • What angle (a) in degrees and (b) in radians do the hour and minute hands of a clock move through in:
  • One hour
  • One minute
  • How far apart in degrees are the hour and minute hand at five minutes past five? (you should take into account that the hour hand is not exactly at the five, but has moved a little further)

Trigonometric Angular Functions[edit]

Geometrically defining tangent[edit]

In the previous section, we algebraically defined tangent as \displaystyle\tan\theta=\frac{\sin\theta}{\cos\theta}, and this is the definition that we will use most in the future. It can, however, be helpful to understand the tangent function from a geometric perspective.

Geometrically defining tangent

A line is drawn at a tangent to the unit circle: (i.e. x = 1). Another line is drawn from the point on the radius of the circle where the given angle falls, through the origin(O), to a point (Q) on the drawn tangent. The ordinate (QP) of this point is called the tangent of the angle.

The slope of the line OQ = \frac {KC}{OC} and as we mentioned before

KC = sin(θ) , OC = cos(θ)

Hence , the Slope of the line OQ = \frac {\sin(\theta)}{\cos(\theta)}

and also the slope of OQ = \frac {QP}{OP} = \frac {QP}{1} = \frac {\tan(\theta)}{1} = tan(θ)

Hence , we can deduce that tan(θ) = \frac {KC}{OC} = \frac {\sin(\theta)}{\cos(\theta)} = QP = the ordinate of the point Q = the slope of OQ

Domain and range of circular functions[edit]

Any size angle, positive or negative, can be the input to sine or cosine — the result will be as if the largest multiple of 2π (or 360°) were subtracted from or added to the angle. The output of the two functions is limited by the absolute value of the radius of the unit circle, |1|.


\begin{matrix}
 & \mathrm{domain}&\mathrm{range} \\
\mathrm{sine} & \mathbb{R} & [-1,1] \\
\mathrm{cosine} & \mathbb{R} & [-1,1] \\
\end{matrix}

R represents the set of all real numbers.

No such restrictions apply to the tangent, however, as can be seen in the diagram in the preceding section. The only restriction on the domain of tangent is that odd integer multiples of \frac{\pi}{2} are undefined, as a line parallel to the tangent will never intersect it.


\begin{matrix}
 & \mathrm{domain}&\mathrm{range} \\
\mathrm{tangent} & \mathbb{R} \setminus \left \{ \cdots,-\frac{\pi}{2},\frac{\pi}{2},\frac{3\pi}{2},\frac{5\pi}{2},\cdots \right \} & \mathbb{R} \\
\end{matrix}

for a deep understanding of trigonometric functions explore this Applet

Applying the trigonometric functions to a right-angled triangle[edit]

If you redefine the variables as follows to correspond to the sides of a right triangle:
• x = a (adjacent)
• y = o (opposite)
• a = h (hypotenuse)


Next Page: Right Angle Trigonometry
Previous Page: The unit circle

Home: Trigonometry

Right Angle Trigonometry[edit]

Construction of Right Triangles[edit]

Provided AC is a diameter, angle B is always a constant right angle

Right triangles are easily constructed. Recall that a diameter is a straight line which starts at one point on the circle and goes through the center to the other side. Using this property of a circle:

  1. Construct a diameter of a circle. Call the points where the diameter touches the circle a and c.
  2. Choose a distinct point b on the circle (any point that is neither a nor c).
  3. Construct line segments connecting points a, b and c.

Provided the above three directions are followed, the resulting triangle Δabc will be a right triangle. This result is known as Thales' theorem.

This right triangle can be further divided into two isosceles triangles by adding a line segment from b to the center of the circle.

To simplify the following discussion, we specify that the circle has diameter 1 and is oriented such that the diameter drawn above runs left to right. We shall denote the angle of the triangle at the right θ and that at the left φ. The sides of the right triangle will be labeled, starting on the right, a, b, c, so that a is the rightmost side, c the leftmost, and b the diameter. We know from earlier that side b is opposite the right angle and is called the hypotenuse. Side a is opposite angle φ, while side c is opposite angle θ. We reiterate that the diameter, now called b, shall be assumed to have length 1 except where otherwise noted.

By constructing a right angle to the diameter at one of the points where it crosses the circle and then using the method outlined earlier for producing binary fractions of the right angle, we can construct one of the angles, say θ, as an angle of known measure between 0 and π / 2. The measure of the other angle φ is then π - π/2 - θ = π/2 - θ, the complement of angle θ. Likewise, we can bisect the diameter of the circle to produce lengths which are binary fractions of the length of the diameter. Using a compass, a binary fractional length of the diameter can be used to construct side a (or c) having a known size (with regard to the diameter b) from which side c can be constructed.

Using Right Triangles to find Unknown Sides[edit]

Finding unknown sides from two other sides[edit]

From the Pythagorean Theorem, we know that:

a^2 + b^2 = c^2. \,

Recall that c (the diameter/hypotenuse in the above example) has been defined as having a length of one, therefore:

b^2 = 1 - a^2. \,

permits us to calculate the length of b squared. It may happen that b squared is a fraction such as 1/4 for which a rational square root can be found, in this case as 1/2, alternatively, we could use Newton's Method to find an approximate value for b.

Finding unknown sides from one side and one (non-right) angle[edit]

As any triangle could be compared to our basic triangle (formed from a circle with a diameter of one), a table enumerating the relationships between angles and side lengths would be very useful to understanding the properties of any triangle. However, such a table would be unwieldy in practice and it is often not necessary to know the exact value.

Of course, given an angle \theta, we could construct a right angled triangle using ruler and compass that had \theta\, as one of its angles, we could then measure the length of the side that corresponds to a to evaluate the \cos function. Such measurements would necessarily be inexact; it would be a problem in physics to see how accurately such measurements can be made; using trigonometry we can make precise predictions with which the results of these physical measurements can be compared.

The most common way of communicating the idea that relationships exist without providing exact details takes the form of a 'function'. A function is like a machine that takes some simple input and produces some simple output. Usually a function defines some kind of rule ([Function]) and provides us a handy notation useful in trigonometry. That way, we know that we're using a certain relationship without needing to know the exact numerical values. Basic trigonometric functions are simply stand-ins for the relationship between angles and sides of a triangle.

One such function, which allows us to know the relationship between any value of \theta\, and the corresponding value of a\, is called the cosine or \cos\,. This universal relationship is represented as: \frac{a}{c} = \cos\theta which would save us the work of constructing angles and lengths and making difficult deductions from them.

This means that if you know the cosine of an angle, you also know the relationship between the lengths of the sides. The actual size of the triangle can be bigger or smaller, but the mathematical relationship represented by the cosine does not change so long as the size of the angle remains constant.

Cosine example[edit]

Some explicit values for the cos function are known. For \theta\, = 0, sides a\, and c\, coincide: a = c = \frac{a}{c} = 1, so \cos\left(0\right) = 1. For \theta = \frac{\pi}{2}, sides b\, and c\, coincide and are of length 1, and side a\, is of zero length, consequently a\, = 0, c\, = 1. \frac{a}{c} = 0 and \cos\frac{\pi}{2} = 0.


The simplest right angle triangle we can draw is the isosceles right angled triangle, it has a pair of angles of size \frac{\pi}{4} radians, and if its hypotenuse is considered to be of length one, then the sides a\, and b are of length \sqrt{\frac{1}{2}} as can be verified by the theorem of Pythagoras. If the side a\, is chosen to be the same length as the radius of the circle containing the right angled triangle, then the right hand isosceles triangle obtained by splitting the right angled triangle from the circumference of the circle to its center is an equilateral triangle, so \theta must be \frac{\pi}{3}, and \phi must be \frac{\pi}{6} and b\,^2 must be 1 - \frac{1}{2}\cdot\frac{1}{2} = \frac{3}{4}.

Properties of the cosine and sine functions[edit]

Period[edit]

A full revolution is an angle of 2π radians, so increasing an angle by this amount gets you exactly back to your starting point. Therefore, a perfect circle is maintained, along with the relationships formed by triangles within, by adding 2π to any angle θ. This is called the period, --the size of the angle or the time period over which the relationships begin to repeat (correlating the two is complex, and allows us to talk about wave theory).

Using functions, we can represent this fact in terms of the cosine function by stating that : \cos\theta = \cos\left(\theta + 2\pi n \right),\,

Knowing the period of the sine and cosine functions (and by derivation, that of other functions) is useful because it means that we can substitute one angle for another when we know that the period is the same. This helps in calculations, such as when there is the need to add or subtract angles.

Half Angle and Double Angle Formulas[edit]

We can derive a formula for cos(θ/2) in terms of cos(θ) which allows us to find the value of the cos() function for many more angles. To derive the formula, draw an isoceles triangle, draw a circle through its corners, connect the center of the circle with radii to each corner of the isoceles triangle, extend the radius through the apex of the isoceles triangle into a diameter of the circle and connect the point where the diameter crosses the other side of the circle with lines to the other corners of the isoceles triangle.

Therefore:

\cos (\theta /2) = \sqrt{\frac {1 + \cos \theta}{2}}

which gives a method of calculating the cos() of half an angle in terms of the cos() of the original angle. For this reason * is called the "Cosine Half Angle Formula".

The half angle formula can be applied to split the newly discovered angle which in turn can be split again ad infinitum. Of course, each new split involves finding the square root of a term with a square root, so this cannot be recommended as an effective procedure for computing values of the cos() function.

Equation * can be inverted to find cos(θ) in terms of cos(θ)/2:

\begin{matrix}&\cos (\theta /2)  =  \sqrt{\frac{1 + \cos (\theta)}{2}}\\
  \Rightarrow  &  \cos^2(\theta/2)  =  \frac{1 + \cos(\theta)}{2} \\
  \Rightarrow  &  \cos^2(\theta/2) - \frac{1}{2}  =  \frac{\cos (\theta)}{2}  \\
  \Rightarrow  & 2\cos^2(\theta/2) - 1   =  \cos(\theta) \\
 \end{matrix}

substituting \delta\ = \frac{\theta}{2} gives:

2\cos^2(\delta) - 1     = \cos(2\delta) \,

that is a formula for the cos() of double an angle in terms of the cos() of the original angle, and is called the "cosine double angle sum formula".


Next Page: Trigonometric identities
Previous Page: Trigonometric Angular Functions

Home: Trigonometry

Graphs of Sine and Cosine Functions[edit]

The graph of the sine function looks like this:

Graph of the sine function

Careful analysis of this graph will show that the graph corresponds to the unit circle. X is essentially the degree measure (in radians), while Y is the value of the sine function.

The graph of the cosine function looks like this:

Graph of the cosine function

As with the sine function, analysis of the cosine function will show that the graph corresponds to the unit circle. One of the most important differences between the sine and cosine functions is that sine is an odd function (i.e. sin(-θ) = -sin θ) while cosine is an even function (i.e. cos(-θ) = cos θ).

Sine and cosine are periodic functions; that is, the above is repeated for preceding and following intervals with length 2π.

Sine and cosine on same graph


Exercises[edit]

When does Sine = Cosine?

For what value of \displaystyle\theta does \displaystyle \sin \theta=\cos\theta? (Choose a value between 0 and 90o or equivalently in radians between 0 and \displaystyle \frac{\pi}{2}).

  • Convince yourself you are right by drawing the triangle and using SOH-CAH-TOA.



Graphs of Other Trigonometric Functions[edit]

A graph of \tan(x). \tan(x) is defined as \frac{\sin(x)}{\cos(x)}.

Graph of tan(x)

A graph of \csc(x). \csc(x) is defined as \frac{1}{\sin(x)}.

Graph of csc(x)

A graph of \sec(x). \sec(x) is defined as \frac{1}{\cos(x)}.

Graph of sec(x)

A graph of \cot(x). \cot(x) is defined as \frac{1}{\tan(x)} or \frac{\cos(x)}{\sin(x)}.

Graph of cot(x)

Note that \tan(x), \sec(x), and \csc(x) are unbounded, positive or negative. While \tan(x) (and \cot(x)) can take any value, \sec(x) and \csc(x) can never lie between -1 and 1.

Inverse Trigonometric Functions[edit]

The Basic Idea[edit]

In the equation

\displaystyle y = \sin x

if we are given \displaystyle x we can work out \displaystyle y .

If we are given \displaystyle y , can we work out \displaystyle x?

Look at the graph of \displaystyle \sin x and you will see that for \displaystyle y > 1 or \displaystyle y < -1 there aren't any answers at all, whilst for other values of \displaystyle y there are infinitely many answers.


If

\displaystyle y = \sin x

we write the inverse of \displaystyle \sin as follows

\displaystyle x = \sin^{-1}y

Notice the strange notation. It's just a convention, and does not really fit in well with the convention of \displaystyle \sin^2 x meaning \displaystyle (\sin x)^2. However, we are stuck with this notation. It is so widely used and so familiar in mathematical work that in practice it does not cause confusion. On many calculators the alternative notation \displaystyle \arcsin is used.

A calculator will only give one answer (or error) for \displaystyle \sin^{-1}y. You can get some of the other answers by adding or subtracting multiples of 360o. In a later section we spell out the conventions as to which answer is given by \displaystyle \sin^{-1}y.

arcsin[edit]

A common notation used for the inverse functions is the "arcfunction" notation, prefixing the function name by "arc" or sometimes just "a".

\displaystyle \mbox{Sin}^{-1}x=\arcsin x=\mbox{asin} \,x,
\displaystyle \mbox{Cos}^{-1}x=\arccos x=\mbox{acos} \,x, and
\displaystyle \mbox{Tan}^{-1}x=\arctan x=\mbox{atan} \,x.

The arcfunctions might perhaps be so named because of the relationship between radian measure of angles and arclength--the arcfunctions yield arc lengths on a unit circle.


The Inverse Functions, Domain and Range[edit]

The inverse of sine or cosine for some values has multiple answers and some values does not exist at all. We'd like it if the inverse were a function, but according to the mathematical definition of a function it is not:

  • A function is something that given one value always gives back a unique value as its 'answer'.

\displaystyle \sin x is a function because given any x it gives back some value. There is not really a function that is an inverse for \displaystyle \sin x because, for example, \displaystyle \sin 20^\circ and \displaystyle \sin 160^\circ have the same value. The inverse 'function' does not know whether to go back to 20o or 160o.

To deal with this we need some more mathematical language. We have mathematical terminology for what a function operates on and where its values end up. A function like \displaystyle \sqrt{x} needs to be accompanied by some agreement as to what values it can operate on and where they end up. By convention \displaystyle \sqrt{25}=5, though \displaystyle x=-5 is also a valid solution to \displaystyle x^2=25. So how do we describe this kind of thing?

  • The domain of a function is the set of values which it is defined on.
Example: Reciprocal function

The function \displaystyle \frac{1}{x} is defined on all values of x except for 0. Its domain is the real numbers excluding zero.

Example: Factorial function

The factorial function, operates on the positive whole numbers. As a function f - \displaystyle f(1) = 1, f(2)=2, f(3)=6, f(4)=24 \cdots. The factorial function is usually written by writing an exclamation point after a number. So, 3 factorial is usually written as 3! and it is \displaystyle 3 \times 2 \times 1 = 6. 4 factorial is written as 4! and it is \displaystyle 4 \times 3 \times 2 \times 1 = 24.

The domain of the factorial function is the positive whole numbers.


  • The range of a function is the set of values which it can take. The range will depend on the domain too.
Range of x2

Consider the function

\displaystyle f(x)=x^2

If we use ordinary numbers for x like 37.2 or -1001.56 we always find \displaystyle f(x) is a positive number (or zero). The range of \displaystyle f(x) is the numbers greater than or equal to zero.

Range of 2x

Consider the function

\displaystyle f(x)=2x

If we choose the domain of \displaystyle f(x) to be the numbers greater than or equal to 1, then the range of \displaystyle f(x) is the numbers greater than or equal to two.

More Notation[edit]

  • The integers are whole numbers like 1,2,3,4 and also include 0, -1, -2,-3... A symbol we use to indicate the integers is \mathbb{Z}. The statement x \in \mathbb{Z} means exactly the same thing as x is an integer.


  • The reals include all the integers, and also fractions, and also other numbers like pi, and square root of 2. The reals 'fill in the gaps' between the integers. You'll get a better definition of the reals in a later book. A symbol we use to indicate the reals is \mathbb{R}. The statement x \in \mathbb{R} means exactly the same thing as x is a real number.


  • A range of numbers in the reals can often be written using interval notation. Here is an example for numbers greater than or equal to zero and less than one: [0,1). The square and round brackets have special meaning. The square bracket means the number is included. A round bracket means the number is excluded.
Interval Notation
  • The notation (1.3,100.7] means all numbers between 1.3 and 100.7, including 100.7 but excluding 1.3.
  • The notation [-59.1,12.5] means all numbers between -59.1 and 12.5, including -59.1 and including 12.5.
  • The notation (0,71.2) means all numbers between 0 and 71.2, excluding 0 and excluding 71.2.


  • Function composition is applying one function after another. If we have two functions f and g, we write the composite function, applied to x as: f \circ g(x). This means first apply g to x, then apply f to that result. We can regard f \circ g as a new function in its own right.


  • An inverse to a function \displaystyle f is written \displaystyle f^{-1}. If \displaystyle f is the function that adds 12 to a number, then \displaystyle f^{-1} is the function that subtracts 12 from a number.


Inverses to Trig functions[edit]

Some textbooks 'solve' the problem of inverses for trig functions by defining new functions \displaystyle \mbox{Sin}\, x, \displaystyle \mbox{Cos}\, x, and \displaystyle  \mbox{Tan}\, x (all with initial capitals) to equal the original functions but with restricted domain.

With suitably restricted domain the functions \displaystyle \mbox{Sin}\, x, \displaystyle \mbox{Cos}\, x, and \displaystyle \mbox{Tan}\, x (all with initial capitals) do have inverses which are functions too.

The restrictions to allow the inverses to be functions are standard. Here (and for the rest of this page) we are using radians to measure angles rather than degrees:

\displaystyle \mbox{Sin}\, x has domain \left[-\begin{matrix} \frac{\pi}{2} \end{matrix},\begin{matrix} \frac{\pi}{2} \end{matrix}\right];
\displaystyle \mbox{Cos}\, x has domain \left[0,\pi\right]; and
\displaystyle \mbox{Tan}\, x has domain \left(-\begin{matrix} \frac{\pi}{2} \end{matrix},\begin{matrix} \frac{\pi}{2} \end{matrix}\right)

For each function, the restricted domain includes first-quadrant angles as well as an adjacent quadrant.

Inverses, Really?[edit]

It is important to note that because of these restricted domains, the inverse trigonometric functions do not necessarily behave as one might expect an inverse function to behave. While

\displaystyle \mbox{Sin}^{-1}\left(\sin\left(\begin{matrix} \frac{\pi}{6} \end{matrix}\right)\right)=\mbox{Sin}^{-1}\left(\begin{matrix} \frac{1}{2} \end{matrix}\right)=\begin{matrix} \frac{\pi}{6} \end{matrix} (following the expected \displaystyle  \mbox{Sin}^{-1}\left(\sin x\right)=x),
\displaystyle \mbox{Sin}^{-1}\left(\sin\left(\begin{matrix} \frac{5\pi}{6} \end{matrix}\right)\right)=\mbox{Sin}^{-1}\left(\begin{matrix} \frac{1}{2} \end{matrix}\right)=\begin{matrix} \frac{\pi}{6} \end{matrix}.

For the inverse trigonometric functions, \displaystyle f^{-1}\circ f(x)=x only when \displaystyle x is in the range of the inverse function.

The other direction, however: \displaystyle f\circ f^{-1}(x)=x for all \displaystyle x to which we can apply the inverse function.

The Inverse Relations[edit]

'For completeness', here are definitions of the inverse trigonometric relations based on the inverse trigonometric functions. This section is really mostly about using mathematical notation to express how adding multiples of 360o to an angle gives us another solution for the inverse. Because we are working in radians we're adding multiples of two pi. Some more notation being used here:

  • Curly braces like so {} mean the 'set of', i.e. the set of whatever is inside them.
  • The symbol \displaystyle \cup is read as union. The union of two sets is everything that is in either of them.


  • \sin^{-1} x = \left\{ \mbox{Sin}^{-1} x + 2\pi n, n \in \mathbb{Z} \right\} \cup \left\{ \pi - \mbox{Sin}^{-1} x + 2\pi n, n \in \mathbb{Z} \right\} (the sine function has period 2\pi, but within any given period may have two solutions and \sin x=\sin\left(\pi-x\right))
  • \cos^{-1} x = \left\{ \pm \mbox{Cos}^{-1} x + 2\pi n, n \in \mathbb{Z} \right\} (the cosine function has period 2\pi, but within any given period may have two solutions and cosine is even--\cos x=\cos\left(-x\right))
  • \tan^{-1} x = \left\{ \mbox{Tan}^{-1} x + \pi n, n \in \mathbb{Z} \right\} (the tangent function has period \pi and is one-to-one within any given period)


Applications and Models[edit]

Simple harmonic motion[edit]

Simple harmonic motion. Notice that the position of the dot matches that of the sine wave.

Simple harmonic motion (SHM) is the motion of an object which can be modeled by the following function:

x = A \sin \left(\omega t + \phi\right)

or

x = c_{1} \cos\left(\omega t\right) + c_{2} \sin\left(\omega t\right)
where c1 = A sin φ and c2 = A cos φ.

In the above functions, A is the amplitude of the motion, ω is the angular velocity, and φ is the phase.

The velocity of an object in SHM is

v = A \omega \cos \left(\omega t + \phi\right)

The acceleration is

a = -A \omega^2 \sin \left(\omega t + \phi\right) = -\omega^2 x

An alternative definition of harmonic motion is motion such that

\displaystyle a =  -\omega^2 x

Springs and Hooke's Law[edit]

An application of this is the motion of a weight hanging on a spring. The motion of a spring can be modeled approximately by Hooke's law:

F = -kx

where F is the force the spring exerts, x is the extension in meters of the spring, and k is a constant characterizing the spring's 'stiffness' hence the name 'stiffness constant'.

Calculus-based derivation[edit]

From Newton's laws we know that F = ma where m is the mass of the weight, and a is its acceleration. Substituting this into Hooke's Law, we get

ma = -kx

Dividing through by m:

a = -\frac{k}{m}x

The calculus definition of acceleration gives us

x'' = -\frac{k}{m}x
x'' + \frac{k}{m}x = 0

Thus we have a second-order differential equation. Solving it gives us

x = c_{1} \cos\left(\sqrt{\frac{k}{m}}t\right) + c_{2} \sin\left(\sqrt{\frac{k}{m}}t\right) (2)

with an independent variable t for time.


We can change this equation into a simpler form. By lettting c1 and c2 be the legs of a right triangle, with angle φ adjacent to c2, we get

\sin \phi = \frac{c_{1}}{\sqrt{c_{1}^{2} + c_{2}^{2}}}
\cos \phi = \frac{c_{2}}{\sqrt{c_{1}^{2} + c_{2}^{2}}}

and

c_{1} = \sqrt{c_{1}^{2} + c_{2}^{2}} \sin \phi
c_{2} = \sqrt{c_{1}^{2} + c_{2}^{2}} \cos \phi

Substituting into (2), we get

x = \sqrt{c_{1}^{2} + c_{2}^{2}} \sin \phi \cos\left(\sqrt{\frac{k}{m}}t\right) + \sqrt{c_{1}^{2} + c_{2}^{2}} \cos \phi \sin\left(\sqrt{\frac{k}{m}}t\right)

Using a trigonometric identity, we get:

x = \sqrt{c_{1}^{2} + c_{2}^{2}} \left[\sin \left(\phi + \sqrt{\frac{k}{m}}t\right) + \sin \left(\phi - \sqrt{\frac{k}{m}}t\right)\right] + \sqrt{c_{1}^{2} + c_{2}^{2}} \left[\sin \left(\sqrt{\frac{k}{m}}t + \phi\right) + \sin \left(\sqrt{\frac{k}{m}}t - \phi\right)\right]
x = \sqrt{c_{1}^{2} + c_{2}^{2}} \sin \left(\sqrt{\frac{k}{m}}t + \phi\right) (3)

Let A = \sqrt{c_{1}^{2} + c_{2}^{2}} and \omega^{2} = \frac{k}{m}. Substituting this into (3) gives

x = A \sin \left(\omega t + \phi\right)


Next Page: Using Fundamental Identities
Previous Page: Inverse Trigonometric Functions

Home: Trigonometry

Analytic Trigonometry[edit]

Using Fundamental Identities[edit]

Remembering Formulas[edit]

This page is about how to remember trig formulas - so it is more than just a summary of trig formulas.

You will need to have read most of the rest of the book for this page to be useful to you.

The Blue-Box Formulae[edit]

In any triangle the angles
always sum to 180^{\circ}\,



In a right angled triangle
The square of the hypotenuse
is equal to
the sum of the squares of the other two sides.




Soh-Cah-Toa\,



\displaystyle{
\begin{array}{ccc}
\sin A &=& \displaystyle\frac{\text{opposite side}}{\text{hypotenuse}}\\
\\
\cos A &=& \displaystyle\frac{\text{adjacent side}}{\text{hypotenuse}}\\
\\
\tan A &=& \displaystyle\frac{\text{opposite side}}{\text{adjacent side}}
\end{array}
}

Tips on checking and remembering Formulae[edit]

This page contains some trigonometric identities. It does not contain all trigonometric identities. It couldn't possibly. As well as the trigonometric identities for 'double angles' such as:

 \displaystyle\cos(2t) = \cos^2t - \sin^2t

there exist trigonometrical identities for treble angles, quadruple angles and so on. We could not list them all. Also the same formula can be presented in different disguises as we'll see below.

It's useful to learn some of the trig identities and to know how to quickly and easily derive one trigonometric identities from another.

Checking Formulas[edit]

It is also very important to be able to check that the formulas you come up with make sense. We know that \cos(0^\circ)=1\,. If your formula for \cos(2t)\, does not give the answer 1 when t=0\, then it is wrong! Don't stop there though. You can work out where you went wrong and save yourself making the same mistake again. How do you do that?

If you worked out the formula for \cos(2t)\,from the formula for \cos(A+B)\, you need to check through the steps you took. If the mistake isn't obvious, try putting A=0 and B=0. It is very very easy to get a sign wrong, a plus for a minus, when working with equations quickly. It is only through practice that you will become both fast at it and accurate.

Identities Based on the Pythagorean Theorem[edit]

Some of the most fundamental trigonometric identities are those derived from the Pythagorean Theorem. These are defined using a right triangle:

right triangle

At this stage in the course the Pythagorean Theorem should be second nature to you. If you have not yet learned it, learn it now.

a^2+b^2=c^2\,

a\, and b\, of course are the legs or the adjacent and opposite edges, and c\, is the hypotenuse, the longest side, the side that does not include the right angle. This formula only works for a right angle triangle. If the angle shown as a right angle in the diagram were obtuse, larger than a right angle, then c^2\, would be larger than the Pythagorean sum. If the angle shown as a right angle were smaller than a right angle, then c^2\, would be smaller than a^2+b^2\,


Pythagorean Theorem in Terms of sine and cosine[edit]

The Pythagorean Theorem is the same thing as

\sin^2 A + \cos^2 A =1\,

We know this from the earlier in the book where we introduced sine\, and cosine\,.

  • The cosine\, is the adjacent side when the hypotenuse is one.
  • The sine\, is the opposite side when the hypotenuse is one.

The \sin^2 A + \cos^2 A =1\, identity should be second nature to you too, but you should also be able to derive it from the Pythagorean relation.

We can see it's true from a right triangle that has a hypotenuse that is 'c' rather than one. Dividing the Pythagorean relation through by c2 gives us

\bigg(\frac{a}{c}\bigg)^2+\bigg(\frac{b}{c}\bigg)^2=\bigg(\frac{c}{c}\bigg)^2=1

And we have already seen from soh-cah-toa that the sine of A is \bigg(\frac{a}{c}\bigg) and the cosine of A is \bigg(\frac{b}{c}\bigg).


Identities based on Addition Formula[edit]

We saw the addition formula earlier.

Letters are Arbitrary[edit]

The letters in these equations A\, and B\, are arbitrary. We could equally use \omega\, and \theta\,. We're pointing this out because we happen to have a diagram on this page that has angles A\,, B\, and C\, in it, and we want to make it clear that that was for Pythagoras and we're not talking about that diagram any more. In these equations you can also always substitute actual values, e.g. replace A\, by \pi\, and they'd still be true. Or you could replace A\, by 2t\, or \pi - t\,and they'd still be true.

Addition Formula[edit]

The addition formula for cosine is:

 \displaystyle\cos(A + B) = \cos(A)\cos(B) - \sin(A)\sin(B)

and is worth learning. But don't learn the next one:

'Subtraction' Formula[edit]

 \displaystyle\cos(A - B) = \cos(A)\cos(B) + \sin(A)\sin(B)

Learning the second formula is extra effort that does not really gain you anything. You can get it instantly by replacing B\, by -B\, in the first equation. The only things on the right hand side that will change are the terms that had B in them. The \cos B\, is unchanged because \cos(-B) = \cos B\,. The minus sign before the second term changes because \sin(-B) = -\sin B\,.

Checking the 'subtraction' formula[edit]

Now do a quick check. If A=B\, then cos(A-B)\, is \cos( 0 )\, which is one, right? And on the right hand side we have \cos^2 A + \sin^2 A\,, which is also one. Looks good.

It is much better to remember it this way, because you are doing less rote learning and you're also becoming more fluent with the algebra.


Double Angle Formula[edit]

You can immediately get to the next formula by putting B equal to A in the addition formula. This is a double angle formula.

 \displaystyle\cos(2A) = \cos^2 A - \sin^2 A


Half Angle Formula[edit]

Replace A by A/2 in the previous result and you get the half angle formula.

 \displaystyle\cos(A) = \cos^2A/2 - \sin^2A/2


Sum of two shifted Cosines[edit]

For the next formula, you could just plough through the algebra...

 \displaystyle\cos(x + \theta) + \cos(x - \theta)= ...\,


Waves in and out of phase[edit]

Before we do, notice that we are adding two cosine waves, the first shifted left and the second shifted right. We've seen this before when we looked at waves in and out of phase. We're going to get another sinusoidal wave. The expression is fairly symmetric, and actually we can quickly show that the expression gives an even function, that is that the value for -x is the same as for x:

 \displaystyle\cos(-x + \theta) + \cos(-x - \theta)= \, using cos(x) = cos(-x) we get to:
 \displaystyle\cos(x - \theta) + \cos(x + \theta)= \, and now swapping the two terms:
 \displaystyle\cos(x + \theta) + \cos(x - \theta) \, which is the original expression.

with practice you'll be able to see those steps and that the expression is an even function immediately.

A sinusoidal wave that is an even function - well it is something based on cosine. We're expecting the formula will simplify to give us something like:

 \displaystyle A\cos(x) \,

Where A will depend on \theta.

Values to Check With[edit]

When \theta=0^\circ (try it in the original formula) we expect A to be 2. When \theta=90^\circ we expect A to be 0, as the two cosine waves are 180^\circ out of phase. So now to plough through the algebra:

 \displaystyle\cos(x + \theta) + \cos(x - \theta)= \,
 \displaystyle \cos x\cos\theta - \sin x\sin\theta + \cos x\cos(-\theta) - \sin x\sin(-\theta)=
 \displaystyle \cos x\cos\theta - \sin x\sin\theta + \cos x\cos\theta + \sin x\sin\theta=
 \displaystyle \cos x\cos\theta + \cos x\cos\theta =
 \displaystyle 2\cos\theta\cos x

And to check we try with \theta=0^\circ and get  \displaystyle 2\cos x, and we check with \theta=90^\circ and get  \displaystyle 0 \times \cos x, as we hoped.

Knowing roughly what we expected made it easier to get the algebraic steps right. We knew where we were going. We knew we weren't going to end up with four separate terms, some would have to cancel or combine in some other way.

Identities based on Sine and Cosine rules[edit]

{a \over \sin A} = {b \over \sin B} = {c \over \sin C}.

This is easy to remember because it is so symmetrical. You do not even need to remember which way up the ratios are as this is also true:

{\sin A \over a} = {\sin B \over b} = {\sin C \over c}.

What you do need to remember is how the triangle is labelled for it to be true.


With the cosine law formula:

a^2+b^2-2ab\cos{\theta}=c^2, \,

It is best to think of it as a more general version of Pythagoras' theorem. The a and b have to be on equal footing, so ab as a multiplier is reasonable.

If you are familiar with 'units' in physics, then use the fact that units must match up. The quantities a,b,c are measurements of length. It is no good adding \displaystyle a^2 to \displaystyle -2(a+b)\cos{\theta}. One might have units Km2 the other units of Km. Adding \displaystyle a^2 to \displaystyle -2ab\cos{\theta} the units, e.g: Km2, do match.

In some more detail, it has got to be minus for \displaystyle -2ab\cos{\theta}. That's because for \displaystyle\theta<90^\circ we need \displaystyle c^2 to be less than for Pythagoras' theorem.

How can you remember and be sure the 2 is right? Think of an equilateral triangle with each side of length 1. The angle \displaystyle \theta=60^\circ and \displaystyle \cos(60^\circ)=0.5. We need the 2 to get the right answer 1 + 1 + 2x1x1x0.5 = 1.


Ratio identities[edit]

\tan A =\frac{\sin A}{\cos A}\,

This is one definition of tan, and is something you should just learn.

Identities based on symmetry[edit]

These symmetry identities are best remembered by remembering the graphs for these functions. Have a look at the graphs again if you don't remember them.

0, \pi/2, \pi, 3\pi/2, 2\pi\, are landmarks on the graphs of sine and cosine, and you should know what happens for both those functions at those landmarks. When you have that knowledge the following symmetry identities are easy to write down, because you can see them visually.

Shifting Left[edit]

\cos(\pi+A)= -\cos A \quad \sin(\pi+A)=-\sin A \quad \tan(\pi+A)=\tan A

The identities above are visualised as shifting the graph left by \pi. It's a half cycle, and both cosine and sine change signs - and hence tan does not change sign, because when it is expressed as a ratio of sine over cosine both the top and bottom change signs.


Reflecting in x=π/2[edit]

\cos(\pi-A)=-\cos A \quad \sin(\pi-A)=\sin A \quad \tan(\pi-A)=-\tan A

In the above we are reflecting the graph about the vertical line \displaystyle x=\pi/2. Spend enough time looking at this on the graph to see that that is true. It is important to do that to remember this trick for remembering what happens.

Now sine has a maximum at \displaystyle x=\pi/2 (it has the value one) and it is symmetric about that x value, so \sin(\pi-A)=\sin A\,. Cosine is zero at \displaystyle x=\pi/2. Reflecting cosine in the line \displaystyle x=\pi/2 reverses the sign. \cos(\pi-A)=-\cos A \,

Co-function identities[edit]

\cos A =\sin\left(\frac{\pi}{2}-A\right)\quad \,
\sin A =\cos\left(\frac{\pi}{2}-A\right)\quad \,

The above two formulas are most easily seen from the right-triangle definition of cosine and sine. The two acute angles in such a triangle add up to \displaystyle\pi/2, and we are just giving the ratios of sides lengths in terms of a different angle's trig function.

\cos A = \sin\left(\frac{\pi}{2}+A\right)\quad \,
\sin A = -\cos\left(\frac{\pi}{2}+A\right) \quad \,

These two formulas are 'the same' as the previous formulas. We get there in two steps. First subtracted pi from the angle on the right hand side, which inverts the sign, and inverted the sign to compensate. Next invert the sign of the angle on the right hand side. For cosine on the right we are done. For sine on the right we have to invert its sign since inverting the angle's sign changed the sign of the result.

Yes - keeping track of signs is tricky, and always needs care.

Verifying Trigonometric Identities[edit]

To verify an identity means to prove that the equation is true by showing that both sides equal one another.

There is no set method that can be applied to verifying identities; there are, however, a few different ways to start based on the identity which is to be verified.

Trigonometric identities are used in both course texts and in real life applications to abbreviate trigonometric expressions. It is important to remember that merely verifying an identity or altering an expression is not an end in itself, but rather that identities are used to simplify expressions according to the task at hand. Trigonometric expressions can always be reduced to sines and cosines, which can be more manageable than other functions.

To verify an identity[edit]

  1. Always try to reduce the larger side first.
  2. Sometimes getting all trigonometric functions on one side can help.
  3. Remember to use and manipulate already existing identities. The Pythagorean identities are usually the most useful in simplifying.
  4. Remember to factor if needed.
  5. Whenever there is a squared trigonometric function such as sin2(t), always use the Pythagorean identities, which deal with squared functions.
  6. Sometimes doing the reverse of the normal steps helps. For example, adding 1 in unique forms (such as \cos(t)/\cos(t) can help simplify expressions by matching denominators and simplifying numerators.

Easy example 1/\cot(t)=\sin(t)/\cos(t)

1/cot(t)= tan(t), so \tan(t)=\sin(t)/\cos(t)

tan(t) is the same as sin(t)/cos(t)

and therefore the example can be rewritten as \sin(t)/\cos(t)=\sin(t)/\cos(t)

Identity verified

Solving Trigonometric Equations[edit]

Trigonometric equations are equations including trigonometric functions. If they have only such functions and constants, then the solution involves finding an unknown which is an argument to a trigonometric function.

Basic trigonometric equations[edit]

sin x = n[edit]

Sin unit circle.svg
n\,\! \sin x=n\,\!
\left|n\right|<1 \begin{matrix}x=\alpha + 2 k \pi \\
x=\pi - \alpha + 2 k \pi \\
\alpha \in \left[-\frac{\pi}{2};\frac{\pi}{2}\right]\end{matrix}
n=-1\,\! x=-\begin{matrix}\frac{\pi}{2}\end{matrix}+2k\pi
n=0\,\! x=k\pi\,\!
n=1\,\! x=\begin{matrix}\frac{\pi}{2}\end{matrix}+2k\pi
\left|n\right|>1 x\in\varnothing

The equation \sin x=n has solutions only when n is within the interval [-1; 1]. If n is within this interval, then we first find an \alpha such that:

\alpha=\sin^{-1} n\,\!

The solutions are then:

x=\alpha + 2 k \pi\,\!
x=\pi - \alpha + 2 k \pi\,\!

Where k is an integer.

In the cases when n equals 1, 0 or -1 these solutions have simpler forms which are summarized in the table on the right.

For example, to solve:

\sin \frac{x}{2}=\frac{\sqrt{3}}{2}

First find \alpha:

\alpha=\sin^{-1}{\frac{\sqrt{3}}{2}}=\frac{\pi}{3}

Then substitute in the formulae above:

\frac{x}{2}=\frac{\pi}{3} + 2 k \pi
\frac{x}{2}=\pi - \frac{\pi}{3} + 2 k \pi

Solving these linear equations for x gives the final answer:

x=\frac{2\pi}{3}\left(1+6k\right)
x=\frac{4\pi}{3}\left(1+3k\right)

Where k is an integer.

cos x = n[edit]

Cos unit circle.svg
n\,\! \cos x=n\,\!
\left|n\right|<1 \begin{matrix}x=\pm\alpha + 2 k \pi \\
\alpha \in \left[0;\pi\right]\end{matrix}
n=-1\,\! x=\pi+2k\pi\,\!
n=0\,\! x=\begin{matrix}\frac{\pi}{2}\end{matrix}+k\pi\,\!
n=1\,\! x=2k\pi\,\!
\left|n\right|>1 x\in\varnothing

Like the sine equation, an equation of the form \cos x=n only has solutions when n is in the interval [-1; 1]. To solve such an equation we first find one angle \alpha such that:

\alpha=\cos^{-1}n\,\!

Then the solutions for x are:

x=\pm\alpha+2k\pi \, \!

Where k is an integer.

Simpler cases with n equal to 1, 0 or -1 are summarized in the table on the right.

tan x = n[edit]

Tan unit circle.svg
n\,\! \tan x=n\,\!
General
case
\begin{matrix}x=\alpha + k\pi \\
\alpha \in \left[-\frac{\pi}{2};\frac{\pi}{2}\right]\end{matrix}
n=-1\,\! x=-\begin{matrix}\frac{\pi}{4}\end{matrix}+k\pi\,\!
n=0\,\! x=k\pi\,\!
n=1\,\! x=\begin{matrix}\frac{\pi}{4}\end{matrix}+k\pi\,\!

An equation of the form \tan x=n has solutions for any real n. To find them we must first find an angle \alpha such that:

\alpha=\tan^{-1}n\,\!

After finding \alpha, the solutions for x are:

x=\alpha+k\pi\,\!

When n equals 1, 0 or -1 the solutions have simpler forms which are shown in the table on the right.

cot x = n[edit]

Cot unit circle.svg
n\,\! \cot x=n\,\!
General
case
\begin{matrix}x=\alpha + k\pi \\
\alpha \in \left[0;\pi\right]\end{matrix}
n=-1\,\! x=-\begin{matrix}\frac{3\pi}{4}\end{matrix}+k\pi\,\!
n=0\,\! x=\begin{matrix}\frac{\pi}{2}\end{matrix}+k\pi\,\!
n=1\,\! x=\begin{matrix}\frac{\pi}{4}\end{matrix}+k\pi\,\!

The equation \cot x=n has solutions for any real n. To find them we must first find an angle \alpha such that:

\alpha=\cot^{-1}n\,\!

After finding \alpha, the solutions for x are:

x=\alpha+k\pi\,\!

When n equals 1, 0 or -1 the solutions have simpler forms which are shown in the table on the right.

csc x = n and sec x = n[edit]

The trigonometric equations csc x = n and sec x = n can be solved by transforming them to other basic equations:

\csc x=n\Leftrightarrow\frac{1}{\sin x}=n\Leftrightarrow\sin x=\frac{1}{n}
\sec x=n\Leftrightarrow\frac{1}{\cos x}=n\Leftrightarrow\cos x=\frac{1}{n}

Further examples[edit]

Generally, to solve trigonometric equations we must first transform them to a basic trigonometric equation using the trigonometric identities. This sections lists some common examples.

a sin x + b cos x = c[edit]

To solve this equation we will use the identity:

a \sin x + b \cos x = \sqrt{a^2 + b^2} \sin \left(x + \alpha\right)
\alpha = \begin{cases} \tan^{-1} \left(b / a\right), & \mbox{if } a > 0 \\ \pi + \tan^{-1} \left(b / a\right), & \mbox{if } a < 0 \end{cases}

The equation becomes:

\sqrt{a^2 + b^2} \sin \left(x + \alpha\right) = c
\sin{\left(x + \alpha\right)} = \frac{c}{\sqrt{a^2 + b^2}}

This equation is of the form \sin x = n and can be solved with the formulae given above.

For example we will solve:

\sin 3 x - \sqrt{3}\cos 3 x = -\sqrt{3}

In this case we have:

a = 1, b = -\sqrt{3}
\sqrt{a^2+b^2} = \sqrt{1^2 + \left(-\sqrt{3}\right)^2} = 2
\alpha = \tan^{-1} \left(-\sqrt{3}\right) = -\frac{\pi}{3}

Apply the identity:

2 \sin \left(3x - \frac{\pi}{3}\right) = -\sqrt{3}
\sin \left(3x - \frac{\pi}{3}\right) = -\frac{\sqrt{3}}{2}

So using the formulae for \sin x = n the solutions to the equation are:

3x - \frac{\pi}{3} = -\frac{\pi}{3} + 2 k \pi \Leftrightarrow x = \frac{2 k \pi}{3}
3x - \frac{\pi}{3} = \pi + \frac{\pi}{3} + 2 k \pi \Leftrightarrow x = \frac{\pi}{9}\left(6k + 5\right)

Where k is an integer.

Sum and Difference Formulas[edit]

Sine Formulas[edit]

The addition formula for sines is as follows:

\displaystyle\sin(\alpha + \beta) = \sin \alpha \cos \beta + \cos \alpha \sin \beta

This is an important tool that allows us to relate the sines and cosines of angles of different sizes.

There is a related formula for cosines, discussed in the next section:

\displaystyle\cos (\alpha + \beta) = \cos \alpha \cos \beta - \sin \alpha \sin \beta


Worked Example: Sine of \displaystyle 75^\circ
  • You are told that:
\displaystyle\sin(45^\circ)\approx 0.7071
\displaystyle\cos(45^\circ)\approx 0.7071
\displaystyle\sin(30^\circ)= 0.5
\displaystyle\cos(30^\circ)\approx 0.866
  • Use the sine addition formula to calculate \displaystyle\sin(75^\circ)

Answer: Using the first formula:

\displaystyle\sin(45^\circ+30^\circ) = \sin 45^\circ \cos 30^\circ + \cos 45^\circ \sin 30^\circ
\displaystyle\sin(45^\circ+30^\circ) \approx 0.7071\times 0.866 + 0.7071\times 0.5
\displaystyle\sin(75^\circ) \approx 0.6123 + 0.3536 \approx 0.966


Exercise: Check the worked example
  • Check the answer in the worked example agrees with the correct value by using a calculator.
Exercise: Sines and Cosines of \displaystyle 20^\circ, 30^\circ, 40^\circ
  • You are told that
\displaystyle\sin(10^\circ)\approx 0.1736 and
\displaystyle\cos(10^\circ)\approx 0.9848
  • Use the formulas to calculate the sine and cosine of \displaystyle 20^\circ, 30^\circ, 40^\circ
  • Check that your answers agree with the values for sine and cosine given by using your calculator to calculate them directly.


The addition formulas are very useful.

Here is a geometric proof of the sine addition formula. The proof also shows how someone could have discovered it.

Proof[edit]

We want to prove:

\displaystyle\sin(\alpha + \beta) = \sin \alpha \cos \beta + \cos \alpha \sin \beta


About the Diagram[edit]

First, a word about the diagram used in the proof. How on earth would you come up with a diagram like that?

Well,

  • We need a diagram with right triangles and we need to show an angle of \displaystyle(\alpha+\beta), so having \displaystyle \triangle ABC is a must.
  • We want to express the lengths in this triangle in terms of lengths of two right triangles, one with angle \displaystyle\alpha and one with angle \displaystyle\beta, so adding points like \displaystyle E and \displaystyle F is essential.
  • Having got that far we could start trying to solve the problem, and we'd find we ran into a problem when calculating the distance \displaystyle \overline{BC}. That's why we split \displaystyle \overline{BC} into \displaystyle \overline{BD} and \displaystyle \overline{DC}. We can calculate the distance \displaystyle \overline{DC}. It is the same length as \displaystyle \overline{EF}. Also \displaystyle \overline{BD} is a length we can calculate using Soh-Cah-Toa.


Be aware that there is nothing really special about the diagram we chose. It's possible, for example, to calculate \displaystyle\sin(\alpha + \beta) using a diagram where the right triangle \displaystyle \triangle ABE has its right angle at \displaystyle B rather than at \displaystyle E. You might like to try that.


We've chosen this digram and this lettering because it is exactly the same as used in the Khan Academy video on proving addition formula for sine so if you have trouble with the proof presented here, you can follow it on video instead.

Video Link[edit]

There is a video of the proof which may be easier to follow at the Khan Academy.

The Proof[edit]

Trig-addition-laws.svg

First check that the \displaystyle \angle DBE really is the same as \displaystyle \angle FAE. That's going to be important to the proof. We're just using that angles in a triangle add up to 180 to make that check, noting that we know the 90 degree angles.

Now an expression for \displaystyle\sin(\alpha + \beta). Here we're using Soh-Cah-Toa. We're going to be using Soh-Cah-Toa a lot.

\displaystyle\sin(\alpha + \beta) = \frac{\overline{BC}}{\overline{AB}}

Looking at the diagram we can replace \displaystyle\overline{BC} by \displaystyle\overline{BD} + \overline{DC} and we also have \displaystyle\overline{DC}=\overline{EF} so:


\displaystyle\sin(\alpha + \beta) = \frac{\overline{BD}+\overline{DC}}{\overline{AB}}=\frac{\overline{BD}+\overline{EF}}{\overline{AB}}= \frac{\overline{BD}}{\overline{AB}} + \frac{\overline{EF}}{\overline{AB}}

Let's work out another way to express \displaystyle \overline{BD} and another way to express \displaystyle \overline{EF}. You'll need to look at the diagram to see which triangles we are using.


An expression for \displaystyle \overline{BD}

\displaystyle \overline{BD}=\overline{BE}\cos\alpha

and

\displaystyle \overline{BE}=\overline{AB}\sin\beta

so

\displaystyle \overline{BD}=\overline{AB}\sin\beta\cos\alpha

An expression for \displaystyle \overline{EF}

\displaystyle \overline{EF}=\overline{AE}\sin\alpha

and

\displaystyle \overline{AE}=\overline{AB}\cos\beta

so

\displaystyle \overline{EF}=\overline{AB}\cos\beta\sin\alpha


Putting it all Together[edit]

\displaystyle\sin(\alpha + \beta) = \frac{\overline{BD}}{\overline{AB}} + \frac{\overline{EF}}{\overline{AB}} = \frac{\overline{AB}\sin\beta\cos\alpha}{\overline{AB}} + \frac{\overline{AB}\cos\beta\sin\alpha}{\overline{AB}}


The \overline{AB}'s cancel.


\displaystyle\sin(\alpha + \beta) = \sin\beta\cos\alpha + \cos\beta\sin\alpha = \sin \alpha \cos \beta + \cos \alpha \sin \beta

We're done!

Exercises[edit]

Exercise: Make one of the sides 'one'

When we drew the diagram we said nothing about its size. That means we could still choose to make one of the sides be of whatever length we like. We can do this for just one edge. Once we've done that all the other sides lengths are determined. Fixing one length to be a nice value can shorten the proof.

So, let us decide that \displaystyle AB is 1 km. Actually we'll not worry about the units whether km, m or cm and just write '1'.

\displaystyle \triangle ABE is a right triangle and:

\displaystyle \overline{AE} = \overline{AB} \cos\beta = \cos\beta

Your task is to simplify the entire proof of the addition formula by replacing the lengths like \displaystyle \overline{AE} with the actual values assuming that we've set \displaystyle AB=1. You're effectively removing \displaystyle AB and multiplication and division by \displaystyle AB from the proof. It should become a lot shorter and clearer. You should also mark up the lengths on the diagram, assuming \displaystyle AB=1.

Exercise: Use a different diagram

Read the description About the Diagram of how the diagram was constructed again. Make your own diagram that is different to the one shown, with right angles in different places to the diagram shown, and do the proof using it instead.

  • Tip: If you find yourself adding lots of lines and lots of extra points then you are probably making the proof a lot harder than you need to. You want to add only enough lines to be able to 'chase' lengths from one place to another. Once you've got the three basic triangles, one extra line should be enough.


Multiple-Angle and Product-to-sum Formulas

Double angle formulae for cos and sine:

 \displaystyle\cos(2a) = 2\cos^2(a) - 1
\displaystyle\sin(2a) = 2\cos(a)\sin(a)


What Are the Double-Angle Formulas?[edit]

The Double-Angle formulas express the cosine and sine of twice an angle in terms of the cosine and sine of the original angle. We are going to derive them from the addition formulas for sine and cosine. The formulas are:

 \displaystyle\cos(2a) = 2\cos^2(a) - 1

and

\displaystyle\sin(2a) = 2\cos(a)\sin(a)

It is well worth practising the derivation so that you can do it quickly and easily. Then you will not need to remember the formulas, since you can get them quickly from the addition formulas for sine and cosine. It is also good to practice the derivation because being more fluent with the algebra will make you better at other algebra used with trigonometry.

Exercise: Check these Make Sense

Did we make a typo in these formulas? Check they at least make sense.

  • We know that \displaystyle \sin 0 = 0 and \displaystyle \cos 0 = 1. Try those values out. Do the formulas work?
  • \displaystyle -1 \leq cos \theta \leq 1 and \displaystyle -1 \leq sin \theta \leq 1. Are the formulas consistent with that?
  • Make up your own additional 'spot check' to check the formulas
Example: Half Angle formula for Cosine

If we put \displaystyle \alpha = 2a we immediately get

 \displaystyle\cos(\alpha) = 2\cos^2(\frac{\alpha}{2}) - 1

Check it. Do you agree? Or rearranging:

\displaystyle  \cos(\frac{\alpha}{2}) = \sqrt\frac{\cos(\alpha)+1}{2}

So, if we know the cosine of \displaystyle 90^\circ (we do, it is zero), we can compute the cosine of \displaystyle 45^\circ and \displaystyle 22.5^\circ and \displaystyle 11.25^\circ and so on.

\displaystyle  \cos(45^\circ) = \sqrt\frac{\cos(90^\circ)+1}{2} = \sqrt\frac{1}{2}
\displaystyle  \cos(22.5^\circ) = \sqrt\frac{\cos(45^\circ)+1}{2} = \sqrt\frac{\sqrt\frac{1}{2}+1}{2}
\displaystyle  \cos(11.25^\circ) = \sqrt\frac{\cos(22.5^\circ)+1}{2} = \sqrt\frac{\sqrt\frac{\sqrt\frac{1}{2}+1}{2}+1}{2}


Proofs for Double Angle Formulas[edit]

We'll prove the double angle formulas from the addition formulas. Recall that:

 \displaystyle\cos(a + b) = \cos(a)\cos(b) - \sin(a)\sin(b)

Putting b = a in the above formula yields:

 \displaystyle\cos(2a) = \cos(a + a)
 \displaystyle=\cos(a)\cos(a) - \sin(a)\sin(a)
 \displaystyle=\cos^2(a) - \sin^2(a)

So:

 \displaystyle\cos(2a) = \cos^2(a) - \sin^2(a)

Compare this with the "Pythagorean Theorem" expressed in terms of sine and cosine. Notice the double angle formula above has a minus not a plus, otherwise it would be saying  \displaystyle\cos(2a) = 1, which would mean cos was 1 for all values of t, which we know is not true.


In terms of just cosine or just sine[edit]

The formula

 \displaystyle\cos(2a) = \cos^2(a) - \sin^2(a)

isn't yet quite where we want it. We want to get rid of the sine term and express it all in terms of cosine. To do that we use the disguised "Pythagorean Theorem".

 \displaystyle \cos^2(a) + \sin^2(a) = 1

which is the same as:

 \displaystyle -\sin^2(a) = \cos^2(a) -1

so

 \displaystyle\cos(2a) = \cos^2(a) - \sin^2(a) = \cos^2(a) + \cos^2(a) -1 = 2\cos^2(a) -1

so

 \displaystyle\cos(2a) = 2\cos^2(a) -1

which is what we wanted.

We could, if we had preferred, have used the disguised Pythagorean theorem to replace the  \displaystyle \cos^2(a) in terms of  \displaystyle \sin^2(a)


Exercise: Double angle cosine formula in terms of sine.

Do that now, in other words express:

 \displaystyle\cos(2a)

in terms of  \displaystyle\sin(a)

  • Check your answer, particularly to make sure that you have all the minus signs right.


Double angle formula for sine[edit]

Now we will get the double angle formula for sine, this time using the addition formula for sine.

\displaystyle\sin(a + b) = \sin(a)\cos(b) + \sin(b)\cos(a)

Check that we've quoted the addition formula correctly, and then put b=a in the above

\displaystyle\sin(2a) = \sin(a + a)
\displaystyle=\sin(a)\cos(a) + \sin(a)\cos(a)
\displaystyle=2\cos(a)\sin(a)

So:

\displaystyle\sin(2a) = 2\sin(a)\cos(a)

Unlike the formula for cosine the substitutions to get \displaystyle \sin(2a) just in terms of \displaystyle \sin(a) would involve square roots, so we're not going to do that. The above formula is usually the nicest form to work with.

Treble and Higher Angles[edit]

Using the above procedures twice, and the Pythagorean theorem where appropriate, we find

\displaystyle \sin(3a) = 3\sin a - 4 \sin^3 a
\displaystyle \cos(3a) = 4 \cos^3 a - 3\cos a

By repeating the procedure, we can find formulae for \displaystyle \sin(na) and \displaystyle \cos(na) for any integer n. The formulas do however get rather long.

It is not really worthwhile remembering these formulas. They are not used often, and can either be looked up in tables of formulas or calculated when you need them. It is quite good for practising algebra to derive them yourself, so....


Exercise: Treble angle formulas for sine and cosine

Derive the formulas for \displaystyle \sin(3\alpha) and \displaystyle \cos(3\alpha) yourself.


Double and Treble Angles for Tangents[edit]

By using \tan a = \frac {\sin a}{\cos a}, it can be worked out that:


\tan(2a) = \frac {2\tan a}{1-\tan^2 a}


\tan(3a) = \frac {3\tan a - \tan^3 a}{1-3\tan^2 a}


Like the formulas for \displaystyle \sin(3\alpha) and \displaystyle \cos(3\alpha), these formulas aren't often useful, but again it is good to be able to work them out yourself.


Exercise: Multiple angle formulas for tan

Derive the formulas for \displaystyle \tan(2x) and \displaystyle \tan(3x) yourself.

  • If you don't get 'the right answer', don't panic. It takes time and practice to become fluent at algebraic manipulations. Here, where you know the right answer, you can work through your steps and try and find for yourself where you went wrong. Very often it is a sign error somewhere, adding a value instead of subtracting, and then everything from that point on is wrong. You can use the trick of putting in actual values for x (and calculating with a calculator) to check for the place where the first error creeps in.


Additional Topics in Trigonometry[edit]

Law of Sines[edit]

Law-of-sines1.svg

For any triangle with vertices A, B, and C, corresponding angles A, B, and C, and corresponding opposite side lengths a, b, and c, the Law of Sines states that

{a \over \sin A} = {b \over \sin B} = {c \over \sin C}.


Each of these expressions is also equal to the diameter of the triangle's circumcircle (the circle that passes through the points A, B, and C). The law can also be written in terms of the reciprocals:

{\sin A \over a} = {\sin B \over b} = {\sin C \over c}.

Proof[edit]

Law-of-sines2.svg

Dropping a perpendicular OC from vertex C to intersect AB (or AB extended) at O splits this triangle into two right-angled triangles AOC and BOC. We can calculate the length h of the altitude OC in two different ways:

  • Using the triangle AOC gives
\displaystyle h=b \sin A ;
  • and using the triangle BOC gives
\displaystyle h=a \sin B .
  • Eliminate h from these two equations:
\displaystyle a \sin B =b \sin A .
  • Rearrange to obtain
\displaystyle {a \over \sin A} = {b \over \sin B}.

By using the other two perpendiculars the full law of sines can be proved. QED.

Application[edit]

This formula can be used to find the other two sides of a triangle when one side and the three angles are known. (If two angles are known, the third is easily found since the sum of the angles is 180º.) See Solving Triangles Given ASA. It can also be used to find an angle when two sides and the angle opposite one side are known.

Area of a triangle[edit]

The area of a triangle may be found in various ways. If all three sides are known, use Heron's theorem.

If two sides and the included angle are known, consider the second diagram above. Let the sides b and c, and the angle between them α be known. From triangle ACO, the altitude h = CO is bsin(α) so the area is 12cbsin(α).

If two angles and the included side are known, again consider the second diagram above. Let the side c and the angles α and γ be known. Let AO =x. Then

\displaystyle \frac{x}{h} = \cot(\alpha) \text {; } \frac{c-x}{h} = \cot(\gamma) \text {; adding these, } \frac{c}{h} = \cot(\alpha) + \cot(\gamma)

Thus

\displaystyle h = \frac{c}{\cot(\alpha) + \cot(\gamma)} \text { so  area } = \frac{c^2}{2(\cot(\alpha) + \cot(\gamma))}.

Law of Cosines[edit]

Law of Cosines[edit]

Law-of-cosines1.svg

The Pythagorean theorem is a special case of the more general theorem relating the lengths of sides in any triangle, the law of cosines:[1]

a^2+b^2-2ab\cos{\theta}=c^2, \,

where θ is the angle between sides a and b.

Does the formula make sense?[edit]

This formula had better agree with the Pythagorean Theorem when \displaystyle \theta=90^\circ.

So try it...

When \displaystyle \theta=90^\circ, \displaystyle \cos\theta=\cos 90^\circ=0

The \displaystyle -2ab\cos\theta=0 and the formula reduces to the usual Pythagorean theorem.

Permutations[edit]

For any triangle with angles A, B, and C and corresponding opposite side lengths a, b, and c, the Law of Cosines states that

a^2=b^2 + c^2 - 2bc \cdot\cos A,
b^2=a^2 + c^2 - 2ac \cdot\cos B,
c^2=a^2 + b^2 - 2ab \cdot\cos C.

Proof[edit]

Law-of-cosines2.svg

Dropping a perpendicular OC from vertex C to intersect AB (or AB extended) at O splits this triangle into two right-angled triangles AOC and BOC, with altitude h from side c.

First we will find the lengths of the other two sides of triangle AOC in terms of known quantities, using triangle BOC.

h=a sin B

Side c is split into two segments, with total length c.

OB has length a cos B
AO has length c - a cos B

Now we can use the Pythagorean Theorem to find b, since b2 = AO2 + h2.

\begin{matrix}b^2 & = & (c-a\cos B)^2+a^2\sin^2 B \\
\ &=& c^2-2ac\cos B +a^2\cos^2 B+a^2\sin^2 B\\
\ &=& a^2+c^2-2ac\cos B\end{matrix}

The corresponding expressions for a and c can be proved similarly.

The formula can be rearranged:

cos(C) = \frac{a^2+b^2-c^2}{2ab}

and similarly for cos(A) and cos(B).

Applications[edit]

This formula can be used to find the third side of a triangle if the other two sides and the angle between them are known. The rearranged formula can be used to find the angles of a triangle if all three sides are known. See Solving Triangles Given SAS.

Notes[edit]

  1. Lawrence S. Leff (2005-05-01). cited work. Barron's Educational Series. p. 326. ISBN 0764128922. http://books.google.com/?id=y_7yrqrHTb4C&pg=PA326. 

Solving Triangles[edit]

One of the most common applications of trigonometry is solving triangles—finding missing sides and/or angles given some information about a triangle. The area of the triangle may also be required.

We can reconstruct the triangle given:

  • ASA Angle-Side-Angle (see illustration below).
  • AAS Angle-Angle-Side (see later on this page).
  • SAS Side-Angle-Side (see next page).
  • SSA Side-Side-Angle (later in this book). In the SSA case we may have one, two or no possible solutions.


Given ASA (Side and angles at each end of that side)[edit]

Solve-asa.svg

  • Given two angles, we can find the third angle (since the sum of the measures of the three angles in a triangle is \displaystyle 180^\circ.

The missing angle, \displaystyle \theta is given by:

\theta=180^\circ-(\alpha+\beta)
  • Knowing all three angles and one side, we can use the Law of Sines to find the missing sides.

In the illustration if the side we are given is the base and has length c, then the side opposite the angle \displaystyle \alpha has length \displaystyle a given by:

\displaystyle a= c \frac{\sin\alpha}{\sin\theta}
Check This
  • Check that this follows from the law of sines.

Now is also a good time to check that you can derive the law of sines for yourself. If given a problem triangle like this one in an exam, you might be asked both to find its missing sides and to derive the law of sines.

  • The area may then be found from Heron's Formula, or more easily by the formulae given in Law of Sines.

Given AAS (one side and two other angles)[edit]

Again we can work out the missing angle, since they sum to 180o. From there on we have the same information as after the first step in the ASA case.


Exercises[edit]

Exercise 1: Easy angles I

A triangle \displaystyle \Delta ABC has:


Side \displaystyle \overline{BC} of 30m
\displaystyle \angle ABC=30^\circ and
\displaystyle \angle BCA=45^\circ.


Draw a rough diagram.

  • What are the lengths of the remaining sides, and what is the missing angle?
Exercise 2: Easy angles II

A triangle \displaystyle \Delta ABC has:


Side \displaystyle \overline{BC} of 30m
\displaystyle \angle BCA=30^\circ and
\displaystyle \angle CAB=45^\circ.


Draw a rough diagram.

  • What are the lengths of the remaining sides, and what is the missing angle?
Exercise 3: Similar/Congruent?

Are these two triangles in Exercise 1 and Exercise 2:

  • Similar to each other?
  • Congruent to each other?


Vectors in the Plane[edit]

In practice, one of the most useful applications of trigonometry is in calculations related to vectors, which are frequently used in Physics. A vector is a quantity which has both magnitude (such as three or eight) and direction (such as north or 30 degrees south of east). It is represented in diagrams by an arrow, often pointing from the origin to a specific point.

A plane vector \vec{A} can be expressed in two ways -- as the sum of a horizontal vector of magnitude A_x and a vertical vector of magnitude A_y, or in terms of its angle \theta and magnitude \left|\vec{A}\right| (or simply A). These two methods are called "rectangular" and "polar" respectively.

Rectangular to Polar conversion[edit]

For simplicity, assume \vec{A} is in the first quadrant and has x-component A_x and y-component A_y (which will necessarily be positive). Given these components, we want to find the angle \theta and the magnitude A.

If we draw all three of these vectors, they form a right triangle. It is easy to see that \tan \theta = \frac{A_y}{A_x}, or \theta = \arctan \frac{A_y}{A_x} (A vector with an angle of zero is defined to be pointing directly to the right.) Furthermore, by the Pythagorean Theorem, A_x\,^2 + A_y\,^2=A^2, or A=\sqrt{A_x\,^2 + A_y\,^2}.

Polar to Rectangular conversion[edit]

This is essentially the same problem as above, but in reverse. Here, \theta and A are known and we want to calculate the values of A_x and A_y.

Using the same triangle as above, we can see that \cos \theta = \frac{A_x}{A}, or A_x=A \cos \theta. Also, \sin \theta = \frac{A_y}{A}, or A_y=A \sin \theta.

Review of conversions[edit]

  • \theta = \arctan \frac{A_y}{A_x}
  • \left|\vec{A}\right|=A=\sqrt{A_x\,^2 + A_y\,^2}
  • A_x=A \cos \theta
  • A_y=A \sin \theta

Next Page: Vectors and Dot Products | Previous Page: Solving Triangles

Home: Trigonometry

Vectors and Dot Products[edit]

Consider the vectors U and V (with respective magnitudes |U| and |V|). If those vectors enclose an angle θ then the dot product of those vectors can be written as:


\mathbf{U}\cdot\mathbf{V} = |\mathbf{U}||\mathbf{V}| \cos(\theta)

If the vectors can be written as:

\mathbf{U} = (U_x, U_y, U_z)
\mathbf{V} = (V_x, V_y, V_z)

then the dot product is given by:

\mathbf{U}\cdot\mathbf{V} = U_x V_x + U_y V_y + U_z V_z

For example,

(1, 2, 3) \cdot (2, 2, 2) = 1 (2) + 2 (2) + 3 (2) = 12.

and

(0, 5, 0) \cdot (4, 0, 0) = 0.

We can interpret the last case by noting that the product is zero because the angle between the two vectors is 90 degrees.

Since

|\mathbf{U}| = \sqrt{U_x^2+U_y^2+U_z^2}

and

|\mathbf{V}| = \sqrt{V_x^2+V_y^2+V_z^2}

this means that

\cos(\theta) = \frac{U_x V_x + U_y V_y + U_z V_z}{{\sqrt{U_x^2+U_y^2+U_z^2}}{\sqrt{V_x^2+V_y^2+V_z^2}}}

Trigonometric Form of the Complex Number[edit]

z=a+bi= r \left ( \cos \phi \ + i\sin \phi \right )

where

  • i is the imaginary number \left (i\ = \sqrt{-1}\right )
  • the modulus r=\operatorname{mod}(z)=|z|=\sqrt{a^2+b^2}
  • the argument \phi=\arg(z) is the angle formed by the complex number on a polar graph with one real axis and one imaginary axis. This can be found using the right angle trigonometry for the trigonometric functions.

This is sometimes abbreviated as r\left ( \cos \phi \ + i\sin \phi \right )=r\operatorname{cis}\phi and it is also the case that r\operatorname{cis}\phi=re^{i\phi} (provided that \phi is in radians). The latter identity is called Euler's formula.

Euler's formula can be used to prove DeMoivre's formula: ( \cos \phi \ + i\sin \phi )^n=\cos(n\phi)+i\sin(n\phi). This formula is valid for all values of n, real or complex.


Trigonometry References[edit]

Trigonometric Unit Circle and Graph Reference[edit]

The Unit Circle Unit circle angles.svg

The unit circle is a commonly used tool in trigonometry because it helps the user to remember the special angles and their trigonometric functions. The unit circle is a circle drawn with its center at the origin of a graph(0,0), and with a radius of 1. All angles are measured starting from the x-axis in quadrant one and may go around the unit circle any number of degrees. Points on the outside of the circle that are in line with the terminal (ending) sides of the angles are very useful to know, as they give the trigonometric function of the angle through their coordinants. The format is (cos, sin).

Note that in trigonometry, an angle can be of any size, positive or negative. An angle larger than 360º means that you have gone round the circle more than once.

Trigonometric Formula Reference[edit]

Exercise: Remembering Formulas

Cover the right hand side of each formula, and use the information about remembering formulas from the previous page to get the right hand side.

Principal Trig Relationships[edit]

The following identities give relationships between the trigonometric functions.

  1. \sin x =\cos\left(\frac{\pi}{2}-x\right)\quad \,
  2. \cos x =\sin\left(\frac{\pi}{2}-x\right)\quad \,
  3. \displaystyle\tan x =\frac{\sin x}{\cos x}
  4. \displaystyle\csc x = \frac{1}{\sin x}
  5. \displaystyle\sec x = \frac{1}{\cos x}

Pythagoras related[edit]

  1. \displaystyle\sin^2{\theta}+\cos^2{\theta}=1
  2. \displaystyle\tan^2{\theta}+1=\sec^2{\theta}


Worked Example: The cot formula is missing

One formula is missing.

By dividing the \displaystyle\sin^2{\theta}+\cos^2{\theta}=1 by

\displaystyle\sin^2{\theta}

or by

\displaystyle\cos^2{\theta}

we can get two other formulas.

The missing formula is obtained by dividing through by \displaystyle\sin^2{\theta}

\displaystyle\frac{\sin^2{\theta}}{\sin^2{\theta}}+\frac{\cos^2{\theta}}{\sin^2{\theta}}=\frac{1}{\sin^2{\theta}}

The missing formula is:

\displaystyle 1+\cot^2{\theta}=\csc^2{\theta}


Periodicity[edit]

Four trigonometric functions are \displaystyle2\pi periodic:

  1. \displaystyle\sin{\theta}=\sin{(\theta+2\pi)}
  2. \displaystyle\cos{\theta}=\cos{(\theta+2\pi)}
  3. \displaystyle\csc{\theta}=\csc{(\theta+2\pi)}
  4. \displaystyle\sec{\theta}=\sec{(\theta+2\pi)}

Two trigonometric functions are \displaystyle\pi periodic:

  1. \displaystyle\tan{\theta}=\tan{(\theta+\pi)}
  2. \displaystyle\cot{\theta}=\cot{(\theta+\pi)}

Angle Sums[edit]

Formulas involving sums of angles are as follows:

  1. \displaystyle\sin{(\alpha+\beta)}=\sin{\alpha}\cos{\beta}+\cos{\alpha}\sin{\beta}
  2. \displaystyle\cos{(\alpha+\beta)}=\cos{\alpha}\cos{\beta}-\sin{\alpha}\sin{\beta}
  3. \displaystyle\sin{(\alpha-\beta)}=\sin{\alpha}\cos{\beta}-\cos{\alpha}\sin{\beta}
  4. \displaystyle\cos{(\alpha-\beta)}=\cos{\alpha}\cos{\beta}+\sin{\alpha}\sin{\beta}

Multiple Angle Formulas[edit]

Substituting \displaystyle\beta=\alpha gives the double angle formulae

  1. \displaystyle\sin{(2\alpha)}=2\sin({\alpha})\cos({\alpha})
  2. \displaystyle\cos{(2\alpha)}=\cos^2{\alpha}-\sin^2{\alpha}

Substituting \displaystyle\sin^2{\alpha}+\cos^2{\alpha}=1 gives

  1. \displaystyle\cos{(2\alpha)}=2\cos^2{\alpha}-1
  2. \displaystyle\cos{(2\alpha)}=1-2\sin^2{\alpha}

These can be obtained by putting \displaystyle\beta=2\theta, \alpha=\theta in the addition formula.

  1. \displaystyle\sin{(3\theta)}=3\sin{\theta}-4\sin^3{\theta}
  2. \displaystyle\cos{(3\theta)}=4\cos^3{\theta}-3\cos{\theta}
  3. \displaystyle\tan{(3\theta)}=\frac{3\tan{\theta}-\tan^3{\theta}}{1-3\tan^2{\theta}}

This can also be obtained from the angle sums formula.

  1. \displaystyle2\sin{(A)}\cos{(B)}=\sin(A+B)+\sin(A-B)

Trigonometric functions of some closely related angles[edit]

This list may duplicate some of the periodicity formulas above, but all the formulas are given for the sake of completeness. Angles are expressed in degrees rather than radians. Similar relations for cot, sec and cosec follow immediately from the definitions of these functions; just replace sin by cosec, cos by sec and tan by cot (and vice versa).

sin(x)[edit]

  1. \displaystyle\sin(-x) = -\sin(x)
  2. \displaystyle\sin(90^\circ-x) = \cos(x)
  3. \displaystyle\sin(90^\circ+x) = \cos(x)
  4. \displaystyle\sin(180^\circ-x) = \sin(x)
  5. \displaystyle\sin(180^\circ+x) = -\sin(x)
  6. \displaystyle\sin(270^\circ-x) = -\cos(x)
  7. \displaystyle\sin(270^\circ+x) = -\cos(x)
  8. \displaystyle\sin(360^\circ-x) = -\sin(x)
  9. \displaystyle\sin(360^\circ+x) = \sin(x)

cos(x)[edit]

  1. \displaystyle\cos(-x) = \cos(x)
  2. \displaystyle\cos(90^\circ-x) = \sin(x)
  3. \displaystyle\cos(90^\circ+x) = -\sin(x)
  4. \displaystyle\cos(180^\circ-x) = -\cos(x)
  5. \displaystyle\cos(180^\circ+x) = -\cos(x)
  6. \displaystyle\cos(270^\circ-x) = -\sin(x)
  7. \displaystyle\cos(270^\circ+x) = \sin(x)
  8. \displaystyle\cos(360^\circ-x) = \cos(x)
  9. \displaystyle\cos(360^\circ+x) = \cos(x)

tan(x)[edit]

  1. \displaystyle\tan(-x) = -\tan(x)
  2. \displaystyle\tan(90^\circ-x) = \cot(x)
  3. \displaystyle\tan(90^\circ+x) = -\cot(x)
  4. \displaystyle\tan(180^\circ-x) = -\tan(x)
  5. \displaystyle\tan(180^\circ+x) = \tan(x)
  6. \displaystyle\tan(270^\circ-x) = \cot(x)
  7. \displaystyle\tan(270^\circ+x) = -\cot(x)
  8. \displaystyle\tan(360^\circ-x) = -\tan(x)
  9. \displaystyle\tan(360^\circ+x) = \tan(x)


Exercise: Radians

Rewrite the above formulas using radians.


Trigonometric Identities Reference[edit]

Triangle Identities[edit]

In addition to the Law of Sines, the Law of Cosines, and the Law of Tangents, there are numerous other identities that apply to the three angles A, B, and C of any triangle (where A+B+C=180° and each of A, B, and C is greater than zero). Some of the most notable ones follow:

  1. \displaystyle \cos^2A+\cos^2B+\cos^2C+2\cos A \cos B \cos C=1
  2. \sin A + \sin B + \sin C = 4\cos\frac{A}{2}\cos\frac{B}{2}\cos\frac{C}{2}
  3. \displaystyle \tan A + \tan B + \tan C = \tan A \tan B \tan C
  4. \tan \frac{A}{2}\tan\frac{B}{2} + \tan\frac{B}{2}\tan\frac{C}{2} + \tan\frac{C}{2}\tan\frac{A}{2} = 1
  5. \displaystyle \cot A \cot B + \cot B \cot C + \cot C \cot A = 1
  6. \cot\frac{A}{2}\cot\frac{B}{2}\cot\frac{C}{2} = \cot\frac{A}{2} + \cot\frac{B}{2} + \cot\frac{C}{2}
  7. \sin A \sin B \sin C = \frac{1}{(\cot A + \cot B)(\cot B + \cot C)(\cot C + \cot A)}
  8. \frac{\sin A + \sin B - \sin C}{\sin A + \sin B + \sin C} = \tan \frac{A}{2}\tan \frac{B}{2}

Pythagoras[edit]

  1. \displaystyle \sin^2(x)+\cos^2(x)=1
  2. \displaystyle 1+\tan^2(x)=\sec^2(x)
  3. \displaystyle 1+\cot^2(x)=\csc^2(x)

These are all direct consequences of Pythagoras's theorem.

Sum/Difference of angles[edit]

  1. \cos(x\pm y)=\cos(x)\cos(y) \mp \sin(x)\sin(y)
  2. \sin(x\pm y)=\sin(x)\cos(y) \pm \sin(y)\cos(x)
  3. \tan(x\pm y)=\frac{\tan(x) \pm \tan(y)}{1 \mp \tan(x) \tan(y)}

Product to Sum[edit]

  1. \displaystyle 2 \sin(x) \sin(y) = \cos(x-y)-\cos(x+y)
  2. \displaystyle 2 \cos(x) \cos(y) = \cos(x-y)+\cos(x+y)
  3. \displaystyle 2 \sin(x) \cos(y) = \sin(x-y)+\sin(x+y)

Sum and difference to product[edit]

  1. \displaystyle A \sin(x)+B\cos(x)= C \sin(x+y), where C=\sqrt{A^2+B^2} and y=\pm\arctan(B/A)
  2. \sin\alpha+\sin\beta=2\sin\frac{\alpha+\beta}{2}\cos\frac{\alpha-\beta}{2}
  3. \sin\alpha-\sin\beta=2\cos\frac{\alpha+\beta}{2}\sin\frac{\alpha-\beta}{2}
  4. \cos\alpha+\cos\beta=2\cos\frac{\alpha+\beta}{2}\cos\frac{\alpha-\beta}{2}
  5. \cos\alpha-\cos\beta=-2\sin\frac{\alpha+\beta}{2}\sin\frac{\alpha-\beta}{2}

Multiple angle[edit]

  1. \cos(2x)=\cos^2(x)- \sin^2(x)=2\cos^2(x)-1=1-2\sin^2(x)
  2. \sin(2x)=2\sin(x)\cos(x)
  3. \tan(2x)=\frac{2\tan(x)}{1- \tan^2(x)}
  4. \cot(2x)=\frac{1}{2}[\cot(x)-\tan(x)]
  5. \csc(2x)=\frac{1}{2}[\cot(x)+\tan(x)]
  6. \cos(3x)=4\cos^{3}(x)-3\cos(x)
  7. \sin(3x)=-4\sin^{3}(x)+3\sin(x)
  8. \tan(3x)=\frac{3\tan(x)-\tan^{3}(x)}{1-3\tan^{2}(x)}
  9. \cos(4x)=8\cos^{4}(x)-8\cos^{2}(x)+1
  10. \sin(4x)=4\sin(x)\cos^{3}(x)-4\sin^{3}(x)\cos(x)
  11. \sin^{2}(4x)=16[\sin^{2}(x)-5\sin^{4}(x)+8\sin^{6}(x)-4\sin^{8}(x)]
  12. \tan(4x)=\frac{4\tan(x)-4\tan^{3}(x)}{1-6\tan^{2}(x)+\tan^{4}(x)}
  13. \cos(5x)=16\cos^{5}(x)-20\cos^{3}(x)+5\cos(x)
  14. \sin(5x)=16\sin^{5}(x)-20\sin^{3}(x)+5\sin(x)
  15. \tan(5x)=\frac{5\tan(x)-10\tan^{3}(x)+\tan^{5}(x)}{1-10\tan^{2}(x)+5\tan^{4}(x)}
  16. \cos(6x)=32\cos^{6}(x)-48\cos^{4}(x)+18\cos^{2}(x)-1
  17. \cos(7x)=64\cos^{7}(x)-112\cos^{5}(x)+56\cos^{3}(x)-7\cos(x)
  18. \sin(7x)=-64\sin^{7}(x)+112\sin^{5}(x)-56\sin^{3}(x)+7\sin(x)
  19. \cos(8x)=128\cos^{8}(x)-256\cos^{6}(x)+160\cos^{4}(x)-32\cos^{2}(x)+1
  20. \cos(nx)=2\cos(x)\cos[(n-1)x]-\cos[(n-2)x]
  21. \sin(nx)=2\cos(x)\sin[(n-1)x]-\sin[(n-2)x]

These are all direct consequences of the sum/difference formulae

Half angle[edit]

  1. \cos(\frac{x}{2})=\pm\sqrt{\frac{1+\cos(x)}{2}}
  2. \sin(\frac{x}{2})=\pm\sqrt{\frac{1-\cos(x)}{2}}
  3. \tan(\frac{x}{2})=\frac{1-\cos(x)}{\sin(x)}=\frac{\sin(x)}{1+\cos(x)}=\pm\sqrt{\frac{1-\cos(x)}{1+\cos(x)}}
  4. \cos^{2}(\frac{3}{2}x)=2\cos^{3}(x)-\frac{3}{2}\cos(x)+\frac{1}{2}

In cases with \pm, the sign of the result must be determined from the value of \frac{x}{2}. These derive from the \cos(2x) formulae.

Power Reduction[edit]

  1. \sin^2\theta=\frac{1-\cos2\theta}{2}
  2. \cos^2\theta=\frac{1+\cos2\theta}{2}
  3. \tan^2\theta=\frac{1-\cos2\theta}{1+\cos2\theta}

Even/Odd[edit]

  1. \sin(-\theta)=-\sin(\theta)
  2. \cos(-\theta)=\cos(\theta)
  3. \tan(-\theta)=-\tan(\theta)
  4. \csc(-\theta)=-\csc(\theta)
  5. \sec(-\theta)=\sec(\theta)
  6. \cot(-\theta)=-\cot(\theta)

Calculus[edit]

  1. \frac{d}{dx}[\sin x] = \cos x
  2. \frac{d}{dx}[\cos x] = -\sin x
  3. \frac{d}{dx}[\tan x] = \sec^{2} x
  4. \frac{d}{dx}[\sec x] = \sec x \tan x
  5. \frac{d}{dx}[\csc x] = -\csc x \cot x
  6. \frac{d}{dx}[\cot x] = -\csc^{2} x

Natural Trigonometric Functions of Primary Angles[edit]

Note: Some values in the table are given in forms that include a radical in the denominator — this is done both to simplify recognition of reciprocal pairs and because the form given in the table is simpler in some sense. Note also that all absolute values of trigonometric functions for remarkable points that are listed in this table are contained in the first quadrant (from 0 to 90° or \pi/2 radians, inclusive); all others are deduced by simple symmetries with the horizontal or vertical axis, or by swapping axes (on the trigonometric circle) so that one trigonometric function is also swapped with its co-function.

\theta\, (positive) \sin\theta\, \cos\theta\, \tan\theta\, \cot\theta\, \sec\theta\, \csc\theta\, \theta\, (negative)
(degrees) (radians) (degrees) (radians)
0\, 0\, 1\, 0\, not
defined
1\, not
defined
−360° -2\pi\,
15° \frac{\pi}{12}\, \frac{\sqrt{6}-\sqrt{2}}{4}\, \frac{\sqrt{6}+\sqrt{2}}{4}\, 2-\sqrt{3}\, 2+\sqrt{3}\, \frac{4}{\sqrt{6}+\sqrt{2}}\, \frac{4}{\sqrt{6}-\sqrt{2}}\, −345° -\frac{13\pi}{12}\,
22.5° \frac{\pi}{8}\, \frac{\sqrt{2-\sqrt{2}}}{2}\, \frac{\sqrt{2+\sqrt{2}}}{2}\, \sqrt{2}-1\, \sqrt{2}+1\, \frac{2}{\sqrt{2+\sqrt{2}}}\, \frac{2}{\sqrt{2-\sqrt{2}}}\, −337.5° -\frac{15\pi}{8}\,
30° \frac{\pi}{6}\, \frac{1}{2}\, \frac{\sqrt{3}}{2}\, \frac{1}{\sqrt{3}}\, \sqrt{3}\, \frac{2}{\sqrt{3}}\, 2\, −330° -\frac{11\pi}{6}\,
45° \frac{\pi}{4}\, \frac{1}{\sqrt{2}}\, \frac{1}{\sqrt{2}}\, 1\, 1\, \sqrt{2}\, \sqrt{2}\, −315° -\frac{7\pi}{4}\,
60° \frac{\pi}{3}\, \frac{\sqrt{3}}{2}\, \frac{1}{2}\, \sqrt{3}\, \frac{1}{\sqrt{3}}\, 2\, \frac{2}{\sqrt{3}}\, −300° -\frac{5\pi}{3}\,
67.5° \frac{3\pi}{8}\, \frac{\sqrt{2+\sqrt{2}}}{2}\, \frac{\sqrt{2-\sqrt{2}}}{2}\, \sqrt{2}+1\, \sqrt{2}-1\, \frac{2}{\sqrt{2-\sqrt{2}}}\, \frac{2}{\sqrt{2+\sqrt{2}}}\, −292.5° -\frac{11\pi}{8}\,
75° \frac{5\pi}{12}\, \frac{\sqrt{6}+\sqrt{2}}{4}\, \frac{\sqrt{6}-\sqrt{2}}{4}\, 2+\sqrt{3}\, 2-\sqrt{3}\, \frac{4}{\sqrt{6}-\sqrt{2}}\, \frac{4}{\sqrt{6}+\sqrt{2}}\, −285° -\frac{19\pi}{12}\,
90° \frac{\pi}{2}\, 1\, 0\, not
defined
0\, not
defined
1\, −270° -\frac{3\pi}{2}\,
105° \frac{7\pi}{12}\, \frac{\sqrt{6}+\sqrt{2}}{4}\, -\frac{\sqrt{6}-\sqrt{2}}{4}\, -2-\sqrt{3}\, -2+\sqrt{3}\, -\frac{4}{\sqrt{6}-\sqrt{2}}\, \frac{4}{\sqrt{6}+\sqrt{2}}\, −255° -\frac{17\pi}{12}\,
112.5° \frac{5\pi}{8}\, \frac{\sqrt{2+\sqrt{2}}}{2}\, -\frac{\sqrt{2-\sqrt{2}}}{2}\, -\sqrt{2}-1\, -\sqrt{2}+1\, -\frac{2}{\sqrt{2-\sqrt{2}}}\, \frac{2}{\sqrt{2+\sqrt{2}}}\, −247.5° -\frac{11\pi}{8}\,
120° \frac{2\pi}{3}\, \frac{\sqrt{3}}{2}\, -\frac{1}{2}\, -\sqrt{3}\, -\frac{1}{\sqrt{3}}\, -2\, \frac{2}{\sqrt{3}}\, −240° -\frac{4\pi}{3}\,
135° \frac{3\pi}{4}\, \frac{1}{\sqrt{2}}\, -\frac{1}{\sqrt{2}}\, -1\, -1\, -\sqrt{2}\, \sqrt{2}\, −225° -\frac{5\pi}{4}\,
150° \frac{5\pi}{6}\, \frac{1}{2}\, -\frac{\sqrt{3}}{2}\, -\frac{1}{\sqrt{3}}\, -\sqrt{3}\, -\frac{2}{\sqrt{3}}\, 2\, −210° -\frac{7\pi}{6}\,
157.5° \frac{7\pi}{8}\, \frac{\sqrt{2-\sqrt{2}}}{2}\, -\frac{\sqrt{2+\sqrt{2}}}{2}\, -\sqrt{2}+1\, -\sqrt{2}-1\, -\frac{2}{\sqrt{2+\sqrt{2}}}\, \frac{2}{\sqrt{2-\sqrt{2}}}\, −202.5° -\frac{9\pi}{8}\,
165° \frac{11\pi}{12}\, \frac{\sqrt{6}-\sqrt{2}}{4}\, -\frac{\sqrt{6}+\sqrt{2}}{4}\, -2+\sqrt{3}\, -2-\sqrt{3}\, -\frac{4}{\sqrt{6}+\sqrt{2}}\, \frac{4}{\sqrt{6}-\sqrt{2}}\, −195° -\frac{13\pi}{12}\,
180° \pi\, 0\, -1\, 0\, not
defined
-1\, not
defined
−180° -\pi\,
195° \frac{13\pi}{12}\, -\frac{\sqrt{6}-\sqrt{2}}{4}\, -\frac{\sqrt{6}+\sqrt{2}}{4}\, 2-\sqrt{3}\, 2+\sqrt{3}\, -\frac{4}{\sqrt{6}+\sqrt{2}}\, -\frac{4}{\sqrt{6}-\sqrt{2}}\, −165° -\frac{11\pi}{12}\,
202.5° \frac{9\pi}{8}\, -\frac{\sqrt{2-\sqrt{2}}}{2}\, -\frac{\sqrt{2+\sqrt{2}}}{2}\, \sqrt{2}-1\, \sqrt{2}+1\, -\frac{2}{\sqrt{2+\sqrt{2}}}\, -\frac{2}{\sqrt{2-\sqrt{2}}}\, −157.5° -\frac{7\pi}{8}\,
210° \frac{7\pi}{6}\, -\frac{1}{2}\, -\frac{\sqrt{3}}{2}\, \frac{1}{\sqrt{3}}\, \sqrt{3}\, -\frac{2}{\sqrt{3}}\, -2\, −150° -\frac{5\pi}{6}\,
225° \frac{5\pi}{4}\, -\frac{1}{\sqrt{2}}\, -\frac{1}{\sqrt{2}}\, 1\, 1\, -\sqrt{2}\, -\sqrt{2}\, −135° -\frac{3\pi}{4}\,
240° \frac{4\pi}{3}\, -\frac{\sqrt{3}}{2}\, -\frac{1}{2}\, \sqrt{3}\, \frac{1}{\sqrt{3}}\, -2\, -\frac{2}{\sqrt{3}}\, −120° -\frac{2\pi}{3}\,
247.5° \frac{11\pi}{8}\, -\frac{\sqrt{2+\sqrt{2}}}{2}\, -\frac{\sqrt{2-\sqrt{2}}}{2}\, \sqrt{2}+1\, \sqrt{2}-1\, -\frac{2}{\sqrt{2-\sqrt{2}}}\, -\frac{2}{\sqrt{2+\sqrt{2}}}\, −112.5° -\frac{5\pi}{8}\,
255° \frac{17\pi}{12}\, -\frac{\sqrt{6}+\sqrt{2}}{4}\, -\frac{\sqrt{6}-\sqrt{2}}{4}\, 2+\sqrt{3}\, 2-\sqrt{3}\, -\frac{4}{\sqrt{6}-\sqrt{2}}\, -\frac{4}{\sqrt{6}+\sqrt{2}}\, −105° -\frac{7\pi}{12}\,
270° \frac{3\pi}{2}\, -1\, 0\, not
defined
0\, not
defined
-1\, −90° -\frac{\pi}{2}\,
285° \frac{19\pi}{12}\, -\frac{\sqrt{6}+\sqrt{2}}{4}\, \frac{\sqrt{6}-\sqrt{2}}{4}\, -2-\sqrt{3}\, -2+\sqrt{3}\, \frac{4}{\sqrt{6}-\sqrt{2}}\, -\frac{4}{\sqrt{6}+\sqrt{2}}\, −75° -\frac{5\pi}{12}\,
292.5° \frac{11\pi}{8}\, -\frac{\sqrt{2+\sqrt{2}}}{2}\, \frac{\sqrt{2-\sqrt{2}}}{2}\, -\sqrt{2}-1\, -\sqrt{2}+1\, \frac{2}{\sqrt{2-\sqrt{2}}}\, -\frac{2}{\sqrt{2+\sqrt{2}}}\, −67.5° -\frac{3\pi}{8}\,
300° \frac{5\pi}{3}\, -\frac{\sqrt{3}}{2}\, \frac{1}{2}\, -\sqrt{3}\, -\frac{1}{\sqrt{3}}\, 2\, -\frac{2}{\sqrt{3}}\, −60° -\frac{\pi}{3}\,
315° \frac{7\pi}{4}\, -\frac{1}{\sqrt{2}}\, \frac{1}{\sqrt{2}}\, -1\, -1\, \sqrt{2}\, -\sqrt{2}\, −45° -\frac{\pi}{4}\,
330° \frac{11\pi}{6}\, -\frac{1}{2}\, \frac{\sqrt{3}}{2}\, -\frac{1}{\sqrt{3}}\, -\sqrt{3}\, \frac{2}{\sqrt{3}}\, -2\, −30° -\frac{\pi}{6}\,
337.5° \frac{15\pi}{8}\, -\frac{\sqrt{2-\sqrt{2}}}{2}\, \frac{\sqrt{2+\sqrt{2}}}{2}\, -\sqrt{2}+1\, -\sqrt{2}-1\, \frac{2}{\sqrt{2+\sqrt{2}}}\, -\frac{2}{\sqrt{2-\sqrt{2}}}\, −22.5° -\frac{\pi}{8}\,
345° \frac{13\pi}{12}\, -\frac{\sqrt{6}-\sqrt{2}}{4}\, \frac{\sqrt{6}+\sqrt{2}}{4}\, -2+\sqrt{3}\, -2-\sqrt{3}\, \frac{4}{\sqrt{6}+\sqrt{2}}\, -\frac{4}{\sqrt{6}-\sqrt{2}}\, −15° -\frac{\pi}{12}\,
360° 2\pi\, 0\, 1\, 0\, not
defined
1\, not
defined
0\,

Notice that for certain values of x\,, the tangent, cotangent, secant, and cosecant functions are undefined. This is because these functions are defined as \frac{\sin x}{\cos x}\,, \frac{\cos x}{\sin x}\,, \frac1{\cos x}\,, and \frac1{\sin x}\,, respectively. Since an expression is undefined if it contains division by zero, the functions are therefore undefined at angle measures where the denominator (the sine or cosine of x\,, depending on the trigonometric function) is equal to zero. For example, the tangent function for 90º (\pi/2\, radians) is equivalent to \frac{\sin(\pi/2)}{\cos(\pi/2)}\,, or \frac10\,, which is an undefined value.