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2nd century BC Greece Trigonometry Hipparchus (190–120 BC)

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Trigonometry is concerned with calculating sides of triangles from angles and early development was mainly used in astronomy.

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Trigonometry is taught throughout high schools. It is based on three functions: sine, cosine, and tangent.

The original trigonometric function was the chord function. Start with an isosceles triangle rather than a right-angled one. Let the equal sides each have length one unit. The chord function, crd(Ø), gives the third side of the triangle.


A definition of the chord function.

It is easy to convert between the chord and sine functions, with these formulae, which involve only doubling and halving: crd(Ø) = 2 sin(1/2 Ø) sin(Ø) = 1/2 crd(2Ø)

No trigonometrical work of Hipparchus survives but he is known to have compiled the first trigonometric table – a table of values of the crd function.

The oldest surviving table is in the Almagest of Ptolemy, a work of astronomy. The table is a feat of numerical complexity: starting with results like crd(60°) = 1 and crd(90°) = √2, and using formulae for crd(A + B) and crd(AB), the chords of angles are found for every 1/2°, to an accuracy of up to 6 decimal places.

The familiar functions of sine, cosine, and tangent, introduced by Indian and Arab mathematicians, are now used but the methods remain the same.

The Little Book of Mathematical Principles, Theories & Things

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