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A history of Greek mathematics - Wilbourhall.org

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MEASUREMENT OF THE EARTH 107<br />

a, or l/50th <strong>of</strong> four right angles. Now the distance from S<br />

to A was known by measurement to be 5,000 stades ; it<br />

followed that the circumference <strong>of</strong> the earth was 250,000<br />

stades. This is the figure given by Cleomedes, but Theon <strong>of</strong><br />

Smyrna and Strabo both give it as 252,000 stades. The<br />

reason <strong>of</strong> the discrepancy is not known ; it is possible that<br />

Eratosthenes corrected 250,000 to 252,000 for some reason,<br />

perhaps in order to get a figure divisible by 60 and, incidentally,<br />

a round number (700) <strong>of</strong> stades for one degree. If<br />

Pliny is right in saying that Eratosthenes made 40 stades<br />

equal to the Egyptian a\o1vos, then, taking the o-yolvos at<br />

12,000 Royal cubits <strong>of</strong> 0-525 metres, we get 300 such cubits,<br />

or 157-5 metres, i.e. 516-73 feet, as the length <strong>of</strong> the stade.<br />

On this basis 252,000 stades works out to 24,662 miles, and<br />

the diameter <strong>of</strong><br />

the earth to about 7,850 miles, only 50 miles<br />

shorter than the true polar diameter, a surprisingly close<br />

approximation, however much it owes to happy accidents<br />

in the calculation.<br />

We learn from Heron's Dioptra that the measurement <strong>of</strong><br />

the earth by Eratosthenes was given in a separate work On<br />

the Measurement <strong>of</strong> the Earth. According to Galen 1 this work<br />

dealt generally with astronomical or mathematical geography,<br />

treating <strong>of</strong> ' the size <strong>of</strong> the equator, the distance <strong>of</strong> the tropic<br />

and polar circles, the extent <strong>of</strong> the polar zone, the size and<br />

distance <strong>of</strong> the sun and moon, total and partial eclipses <strong>of</strong><br />

these heavenly bodies, changes in the length <strong>of</strong> the day<br />

according to the different latitudes and seasons'. Several<br />

details are preserved elsewhere <strong>of</strong> results obtained by<br />

Eratosthenes, which were doubtless contained in this work.<br />

He is supposed to have estimated the distance between the<br />

tropic circles or twice the obliquity <strong>of</strong> the ecliptic at 1 l/83rds<br />

<strong>of</strong> a complete circle or 47° 42' 39"; but from Ptolemy's<br />

language on this subject it is not clear that this estimate was<br />

not Ptolemy's own. What Ptolemy says is that he himself<br />

found the distance between the tropic circles to lie always<br />

between 47° 40' and 47° 45', 'from which we obtain about<br />

(ayeSov) the same ratio as that <strong>of</strong> Eratosthenes, which<br />

Hipparchus also used. For the distance between the tropics<br />

becomes (or is found to be, yiverai) very nearly 1 1 parts<br />

Galen, Instit. Logica, 12 (p. 26 Kalbfleisch).

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