Geodesic
Snaha starořeckého heliocentrika Aristarcha ze Samu zjistit vzdálenosti ve vesmíru
Rozhledy matematicko-fyzikální, Tome 92 (2017) no. 4, pp. 23-27 Cet article a éte moissonné depuis la source Czech Digital Mathematics Library

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The artcile deals with the geometrical methods used by ancient Greek astronomer and mathematician Aristarchos of Samos to determine relative distances of the Earth, the Moon and the Sun. He also attempted to determine the diametres of these bodies by observing total lunar eclipse. His heliocentric theory, which was later revived by Nicolaus Copernicus, is also mentioned.
The artcile deals with the geometrical methods used by ancient Greek astronomer and mathematician Aristarchos of Samos to determine relative distances of the Earth, the Moon and the Sun. He also attempted to determine the diametres of these bodies by observing total lunar eclipse. His heliocentric theory, which was later revived by Nicolaus Copernicus, is also mentioned. 
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     author = {J\'achim, Franti\v{s}ek},
     title = {Snaha staro\v{r}eck\'eho heliocentrika {Aristarcha} ze {Samu} zjistit vzd\'alenosti ve vesm{\'\i}ru},
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Jáchim, František. Snaha starořeckého heliocentrika Aristarcha ze Samu zjistit vzdálenosti ve vesmíru. Rozhledy matematicko-fyzikální, Tome 92 (2017) no. 4, pp. 23-27. http://geodesic.mathdoc.fr/item/RMF_2017_92_4_a2/

[1] Kolman, A.: Dějiny matematiky ve starověku. Academia, Praha, 1968. | MR