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A history of Greek mathematics - Wilbourhall.org

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;<br />

108 ERATOSTHENES<br />

out <strong>of</strong> 83 contained in the whole meridian circle'. 1 The<br />

mean <strong>of</strong> Ptolemy's estimates, 4 7° 42' 30", is <strong>of</strong> course nearly<br />

ll/83rds <strong>of</strong> 360°. It is consistent with Ptolemy's language<br />

to suppose that Eratosthenes adhered to the value <strong>of</strong> the<br />

obliquity <strong>of</strong> the ecliptic discovered before Euclid's time,<br />

namely 24°, and Hipparchus does, in his extant Commentary<br />

on the Phaenomena <strong>of</strong> Aratus and Eudoxus, say that the<br />

summer tropic is very nearly 24° north <strong>of</strong> the equator'.<br />

'<br />

The Doxographi state that Eratosthenes estimated the<br />

distance <strong>of</strong> the moon from the earth at 780,000 stades and<br />

the distance <strong>of</strong> the sun from the earth at 804,000,000 stades<br />

(the versions <strong>of</strong> Stobaeus and Joannes Lydus admit 4,080,000<br />

as an alternative for the latter figure, but this obviously<br />

cannot be right). Macrobius 2 says that Eratosthenes made<br />

the 'measure' <strong>of</strong> the sun to be 27 times that <strong>of</strong> the earth.<br />

It is not certain whether measure means ' solid content ' or<br />

'<br />

diameter ' in this case ; the other figures on record make the<br />

former more probable, in which case the diameter <strong>of</strong> the sun<br />

would be three times that <strong>of</strong> the earth. Macrobius also tells<br />

us that Eratosthenes's estimates <strong>of</strong> the distances <strong>of</strong> the sun<br />

and moon were obtained by means <strong>of</strong> lunar eclipses.<br />

Another observation by Eratosthenes, namely that at Syene<br />

(which is under the summer tropic) and throughout a circle<br />

round it with a radius <strong>of</strong> 300 stades the upright gnomon<br />

throws no shadow at noon, was afterwards made use <strong>of</strong> by<br />

Posidonius in his calculation <strong>of</strong> the size <strong>of</strong> the sun. Assuming<br />

that the circle in which the sun apparently moves round the<br />

earth is 10,000 times the size <strong>of</strong> a circular section <strong>of</strong> the earth<br />

through its centre, and combining with this hypothesis the<br />

datum just mentioned, Posidonius arrived at 3,000,000 stades<br />

as the diameter <strong>of</strong> the sun.<br />

Eratosthenes wrote a poem called Hermes containing a good<br />

deal <strong>of</strong> descriptive astronomy ; only fragments <strong>of</strong> this have<br />

survived. The work Catasterismi (literally placings among<br />

'<br />

the stars ') which is extant can hardly be genuine in the form<br />

in which it has reached us ; it goes back, however, to a genuine<br />

work by Eratosthenes which apparently bore the same name<br />

alternatively it is alluded to as KardXoyoi or by the general<br />

1<br />

2<br />

Ptolemy, Syntaxis, i. 12, pp. 67. 22-68. 6.<br />

Macrobius, In Somn. Scip. i. 20. 9.

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