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A history of Greek mathematics - Wilbourhall.org

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258 TRIGONOMETRY<br />

in relation to one another ; they could not Calculate the actual<br />

times. As Hipparchus proved corresponding propositions by<br />

means <strong>of</strong> numbers, we can only conclude that he used propositions<br />

in spherical trigonometry, calculating arcs from others<br />

which are given, by means <strong>of</strong> tables. (3) In the only work<br />

<strong>of</strong> his which survives, the Commentary on the Phaenomena<br />

<strong>of</strong> Eudoxus and Aratus (an early work anterior to the<br />

discovery <strong>of</strong> the precession <strong>of</strong> the equinoxes), Hipparchus<br />

states that (presumably in the latitude <strong>of</strong> Rhodes) a star which<br />

lies 27^° north <strong>of</strong> the equator describes above the horizon an<br />

arc containing 3 minutes less than 15/24ths <strong>of</strong> the whole<br />

circle 1 ;<br />

then, after some more inferences, he says, ' For each<br />

<strong>of</strong> the aforesaid facts is proved by means <strong>of</strong> lines (8ia rS>v<br />

ypafificov) in the general treatises on these matters compiled<br />

by me '. In other places 2 <strong>of</strong> the Commentary he alludes to<br />

a work On simultaneous risings (ra irepl tcov o-vvavaroXcov),<br />

and in II. 4. 2 he says he will state summarily, about each <strong>of</strong><br />

the fixed stars, along with what sign <strong>of</strong> the zodiac it rises and<br />

sets and from which degree to which degree <strong>of</strong> each sign it<br />

rises or sets in the regions about Greece or wherever the<br />

longest day is<br />

14^ equinoctial hours, adding that he has given<br />

special pro<strong>of</strong>s in another work designed so that it is possible<br />

in practically every place in the inhabited earth to follow<br />

the differences between the concurrent risings and settings. 3<br />

Where Hipparchus speaks <strong>of</strong> pro<strong>of</strong>s ' by means <strong>of</strong> lines ', he<br />

does not mean a merely graphical method, by construction<br />

only, but theoretical determination by geometry, followed by<br />

calculation, just as Ptolemy uses the expression e/c tS>v ypa/i-<br />

/jlcov<br />

<strong>of</strong> his calculation <strong>of</strong> chords and the expressions cr(paipiKal<br />

SeigeLs and ypafifiLKal Seigeis <strong>of</strong> the fundamental proposition<br />

in spherical trigonometry (Menelaus's theorem applied to the<br />

sphere) and its various applications to particular cases. It<br />

is significant that in the Syntaxis VIII. 5, where Ptolemy<br />

applies the proposition to the very problem <strong>of</strong> finding the<br />

times <strong>of</strong> concurrent rising, culmination and setting <strong>of</strong> the<br />

fixed stars, he says that the times can be obtained ' by lines<br />

only ' (8ia ixovoav tcov ypafifi(£>v).<br />

A<br />

Hence we may be certain<br />

that, in the other books <strong>of</strong> his own to which Hipparchus refers<br />

1<br />

3<br />

2<br />

Ed. Manitius, pp. 148-50. lb., pp. 128. 5, 148. 20.<br />

4<br />

lb., pp. 182. 19-184. 5.<br />

Syntaxis, vol. ii, p. 193.

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