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1 The Birth of Science - MSRI

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2.8 Trigonometry and Spherical Geometry 47<br />

for use in astronomy. <strong>The</strong> only difference between ancient and modern<br />

trigonometry is in the choice <strong>of</strong> the fundamental function, which was then page 78<br />

the chord, rather than the sine. <strong>The</strong> two choices are clearly equivalent, as<br />

one can pass from one function to the other using the obvious formula<br />

chord a = 2 sin a<br />

2 ,<br />

since the sine <strong>of</strong> an angle is simply half the chord subtended by twice the<br />

angle.<br />

It is not possible to compute the chord associated to an arc <strong>of</strong> a given<br />

length using the methods typical <strong>of</strong> geometric algebra; that is, one cannot<br />

compute the chord function using ruler and compass (this task being<br />

one <strong>of</strong> the possible formulations <strong>of</strong> the famous problem <strong>of</strong> squaring<br />

the circle). 63 That this impossibility had not blocked the development <strong>of</strong><br />

trigonometry, but had instead channeled it toward methods other than<br />

geometric algebra, such as numerical tables written in positional notation,<br />

shows that the use <strong>of</strong> ruler and compass was a matter <strong>of</strong> convenience<br />

rather than an intellectual prejudice.<br />

In the fourth century A.D., trigonometry was imported into India together<br />

with astronomy, to which it had become an indispensable technical<br />

adjunct. 64 Indeed, at various times during the century, Alexandrian astronomers<br />

and mathematicians decided to emigrate to India, pressed by<br />

their ever more precarious situation in Alexandria. 65 It seems, for example,<br />

that the Paulisa who authored the Indian astronomical work Paulisa page 79<br />

siddhanta was the astronomer Paulus, a refugee from Alexandria.<br />

Indian mathematicians, having to use half-chords <strong>of</strong>ten, decided to pick<br />

the half-chord as the main variable. (<strong>The</strong>y eventually even transferred to<br />

it the Sanskrit term for the chord or bowstring itself, jiva. <strong>The</strong> Arabs, instead<br />

<strong>of</strong> translating this term, transliterated it with consonants that could<br />

also be interpreted as jaib, meaning “bosom <strong>of</strong> dress, cavity”; this was subsequently<br />

translated into Latin as “sinus”, with the same meaning. 66 ) <strong>The</strong><br />

novelty consisted <strong>of</strong> a trivial change in variables, which eliminated factors<br />

<strong>of</strong> 2 in some formulas but did not alter in any way the theorems <strong>of</strong> Hellenistic<br />

trigonometry; the latter were recovered intact on the other side <strong>of</strong><br />

63 Obviously one can draw, with ruler alone, the chord corresponding to a given arc, but computing<br />

the chord function with ruler and compass would require constructing with these instruments<br />

the chord <strong>of</strong> an arc whose length is the same as that <strong>of</strong> a given segment. <strong>The</strong> construction <strong>of</strong> such<br />

an arc is effectively equivalent to the inverse operation <strong>of</strong> rectifying a circumference.<br />

64 It seems certain that the astronomical methods developed in the West were first introduced in<br />

India in the second century A.D., but these were Mesopotamian arithmetic methods used in Greek<br />

astrological texts; see [Neugebauer: HAMA], vol. 1, p. 6. <strong>The</strong> use in Indian astronomy <strong>of</strong> geometric<br />

methods, which required trigonometric functions, started in the fourth century.<br />

65 Hypatia’s end early in the next century (see page 9) shows that this was not at all a bad idea.<br />

66 [Rosenfeld], p. 11.<br />

Revision: 1.12 Date: 2003/01/10 06:11:21

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