Trigonometry

See also the Wikipedia article:
***Trigonometry***

**Trigonometry** (literally "measurement of figures with three angles") is the area of mathematics that deals with relationships between the side lengths and angles of triangles.

Although one can consider triangles on curved surfaces (using spherical and hyperbolic trigonometry), the term *trigonometry* usually refers to **planar trigonometry** — that is, the study of triangles in a plane (two-dimensional Euclidean space).

After considering the measurement of angles in degrees and radians, one may define the following six basic trigonometric functions using any right triangle containing a specified acute angle

θ

{\displaystyle \theta}

:

⁡
(
θ
# )

opp
hyp

{\displaystyle \sin(\theta)=\frac{\text{opp}}{\text{hyp}}}
* cos
⁡
(
θ
# )

adj
hyp

{\displaystyle \cos(\theta)=\frac{\text{adj}}{\text{hyp}}}
* tan
⁡
(
θ
# )

opp
adj

{\displaystyle \tan(\theta)=\frac{\text{opp}}{\text{adj}}}
⁡
(
θ
# )

hyp
opp

{\displaystyle \csc(\theta)=\frac{\text{hyp}}{\text{opp}}}
* sec
⁡
(
θ
# )

hyp
adj

{\displaystyle \sec(\theta)=\frac{\text{hyp}}{\text{adj}}}
* cot
⁡
(
θ
# )

adj
opp

{\displaystyle \cot(\theta)=\frac{\text{adj}}{\text{opp}}}

Here "opp" and "adj" represent, respectively, the lengths of the sides opposite and adjacent to the angle

θ

{\displaystyle \theta}

, and "hyp" represents the length of the hypotenuse (the side opposite the right angle).

The names of the functions above are abbreviated forms of the words sine, cosine, tangent, cotangent, secant and cosecant.

The values of these six functions for non-acute angles (less than or equal to zero, or greater than a right angle) can be found by reference to the **unit circle**.

There are many properties of these functions that are true for any given angle. The most fundamental of these are:

* tan
⁡
(
θ
# )

sin
⁡
(
θ
)

cos
⁡
(
θ
)

{\displaystyle \tan(\theta)=\frac{\sin(\theta)}{\cos(\theta)}}

* cot
⁡
(
θ
# )

cos
⁡
(
θ
)

sin
⁡
(
θ
)

=

1

tan
⁡
(
θ
)

{\displaystyle \cot(\theta)=\frac{\cos(\theta)}{\sin(\theta)}=\frac{1}{\tan(\theta)}}

* sec
⁡
(
θ
# )

1

cos
⁡
(
θ
)

{\displaystyle \sec(\theta)=\frac{1}{\cos(\theta)}}

* csc
⁡
(
θ
# )

1

sin
⁡
(
θ
)

{\displaystyle \csc(\theta)=\frac{1}{\sin(\theta)}}

* sin
2

⁡
(
θ
)

cos
2

⁡
(
θ
# )
1

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

For other similar properties, see our list of trigonometric identities.

## History

Main article: History of trigonometry

Sumerian astronomers studied angle measure, using a division of circles into 360 degrees. They, and later the Babylonians, studied the ratios of the sides of similar triangles and discovered some properties of these ratios, but did not turn that into a systematic method for finding sides and angles of triangles. The ancient Nubians used a similar method.

The ancient Egyptians and Babylonians had known of theorems on the ratios of the sides of similar triangles for many centuries. But pre-Hellenic societies lacked the concept of an angle measure and consequently, the sides of triangles were studied instead, a field that would be better called "trilaterometry".

In the 3rd century BCE, classical Hellenistic mathematicians (such as Euclid and Archimedes) studied the properties of chords and inscribed angles in circles, and proved theorems that are equivalent to modern trigonometric formulae, although they presented them geometrically rather than algebraically. The Hellenized Egyptian mathematician Claudius Ptolemy expanded upon Hipparchus' *Chords in a Circle* in his *Almagest*.

The modern sine function was first defined in the *Surya Siddhanta*, and its properties were further documented by the 5th century (CE) Indian mathematician and astronomer Aryabhata. The *Siddhantas* and the *Aryabhatiya* contain the earliest surviving tables of sine values and versine (1 − cosine) values, in 3.75° intervals from 0° to 90°, to an accuracy of 4 decimal places.

The Indian works were translated and expanded by Islamic mathematicians. By the 10th century, in the work of Abū al-Wafā' al-Būzjānī, Islamic mathematicians were using all six trigonometric functions, had tabulated their values (Abu al-Wafa had sine tables in 0.25° increments, to 8 decimal places of accuracy, and accurate tables of tangent values), and were applying them to problems in spherical geometry. At about the same time, Chinese mathematicians also translated Indian works and developed their own field of trigonometry independently, although it was not a major field of study for them. Knowledge of trigonometric functions and methods reached Europe via Latin translations of the works of Persian and Arabic astronomers such as Al Battani and Nasir al-Din al-Tusi.

One of the earliest works on trigonometry by a European mathematician is *De Triangulis* by the 15th century German mathematician Regiomontanus. Trigonometry was still so little known in 16th-century Europe that Nicolaus Copernicus devoted two chapters of *De revolutionibus orbium coelestium* to explain its basic concepts.

## See also

Template:Colbegin

* Aryabhata's sine table
* Generalized trigonometry
* Lénárt sphere
* List of triangle topics
* List of trigonometric identities
* Rational trigonometry
* Skinny triangle
* Small-angle approximation
* Trigonometric functions
* Trigonometry in Galois fields
* Unit circle
* Uses of trigonometry

Template:Colend

### Bibliography

* Template:Cite book
* Template:Springer
* Christopher M. Linton (2004). From Eudoxus to Einstein: A History of Mathematical Astronomy . Cambridge University Press.
* Weisstein, Eric W. "Trigonometric Addition Formulas". Wolfram MathWorld. Weiner.

## External links

 Search Wikiversity | Learning resources from Wikiversity

Template:Library resources box

* Trigonometry Index at Math is Fun
* Khan Academy: Trigonometry, free online micro lectures
* Trigonometry by Alfred Monroe Kenyon and Louis Ingold, The Macmillan Company, 1914. In images, full text presented.
* Benjamin Banneker's Trigonometry Puzzle at Convergence
* Dave's Short Course in Trigonometry by David Joyce of Clark University
* Trigonometry, by Michael Corral, Covers elementary trigonometry, Distributed under GNU Free Documentation License

1. ↑ Aaboe, Asger. Episodes from the Early History of Astronomy. New York: Springer, 2001. ISBN 0-387-95136-9
2. ↑ Template:Cite book
3. ↑ Template:Cite book
4. ↑ Marlow Anderson, Victor J. Katz, Robin J. Wilson (2004). *Sherlock Holmes in Babylon: and other tales of mathematical history*. MAA. p. 36. ISBN 0-88385-546-1
5. ↑ Boyer p. 215
6. ↑ Boyer (1991), p. 215
7. ↑ 7.0 7.1 Boyer (1991) p. 238.
8. ↑ Boyer pp. 237, 274