Autolycus of Pitane

From Wikipedia, the free encyclopedia
Jump to: navigation, search
De sphaera quae movetur liber

Autolycus of Pitane (Greek: Αὐτόλυκος ὁ Πιταναῖος; c. 360 – c. 290 BC) was a Greek astronomer, mathematician, and geographer. The lunar crater Autolycus was named in his honour.

Life and work[edit]

Autolycus was born in Pitane, a town of Aeolis within Ionia, Asia Minor. Of his personal life nothing is known, although he was a contemporary of Aristotle and his works seem to have been completed in Athens within the years 335 BCE and 300 BCE. Euclid references some of Autolycus' work, and Autolycus is known to have taught Arcesilaus. Autolycus' surviving works include a book on spheres entitled On the Moving Sphere (Περὶ κινουμένης σφαίρας) and another On Risings and Settings (Περὶ ἐπιτολῶν καὶ δύσεων) of celestial bodies. Autolycus' works were translated by Maurolycus in the sixteenth century.

On the Moving Sphere is believed to be the oldest mathematical treatise from ancient Greece that is completely preserved.[1] All Greek mathematical works prior to Autolycus' Sphere are taken from later summaries, commentaries, or descriptions of the works.[1] One reason for its survival is that it had originally been a part of a widely used collection called "Little Astronomy",[2] which was preserved by translation into Arabic in the 9th century. In Europe, it was lost, but was brought back during the crusades in the 12th century, and translated back into Latin.[3][4] In his Sphere, Autolycus studied the characteristics and movement of a sphere. The work is simple and not exactly original, since it consists of only elementary theorems on spheres that would be needed by astronomers, but its theorems are clearly enunciated and proved.[2] Its prime significance, therefore, is that it indicates that by his day there was a thoroughly established textbook tradition in geometry that is today regarded as typical of classical Greek geometry.[2] The theorem statement is clearly enunciated, a figure of the construction is given alongside the proof, and finally a concluding remark is made. Moreover, it gives indications of what theorems were well known in his day (around 320 BCE).[2] Two hundred years later Theodosius' wrote Sphaerics, a book that is believed to have a common origin with On the Moving Sphere in some pre-Euclidean textbook, possibly written by Eudoxus.

In astronomy, Autolycus studied the relationship between the rising and the setting of the celestial bodies in his treatise in two books entitled On Risings and Settings. The second book is actually an expansion of his first book and of higher quality. He wrote that "any star which rises and sets always rises and sets at the same point in the horizon." Autolycus relied heavily on Eudoxus' astronomy and was a strong supporter of Eudoxus' theory of homocentric spheres.


  1. ^ a b Boyer (1991). "The age of Plato and Aristotle". A History of Mathematics. p. 97. A few years after Dinostratus and Menaechmus there flourished a mathematician who has the distinction of having written the oldest surviving Greek mathematical treatise. We have described rather fully the work of earlier Hellenic mathematicians, but it must be borne in mind that the accounts have been based no on original work but on later summaries, commentaries, or description. Occasionally a commentator appears to be copying from an original work extant at the time, as when Simplicius in the sixth century of our era is describing the quadrature of lines by Hippocrates. But not until we come to Autolycus of Pitane, a contemporary of Aristotle, do we find a Greek author one of whose works has survived. 
  2. ^ a b c d Boyer (1991). "The age of Plato and Aristotle". A History of Mathematics. pp. 97–98. One reason for the survival of little treatise, On the Moving Sphere, is that it formed a part of a collection, known as the "Little Astronomy," widely used by ancient astronomers. On the Moving Sphere is not a profound and probably not a very original work, for it includes little beyond elementary theorems on the geometry of the sphere that would be needed in astronomy. Its chief significance lies in the fact that it indicates that Greek geometry evidently had reached the form that we regard as typical of the classical age. Theorems are clearly enunciated and proved. Moreover, the author uses without proof or indication of source other theorems that he regards as well known; we conclude, therefore, that there was in Greece in his day, about 320 B.C., a thoroughly established textbook tradition in geometry. 
  3. ^ "Theodosius of Bithynia". Retrieved 2 May 2015. 
  4. ^ Theodosius of Bithynia


External links[edit]