This is a list of past revisions of Ptolemy. Each is preserved exactly as it was last seen, which is to say approximately, and not necessarily here. Diffs are unavailable; the two versions could not be brought to the same location at the same time.
cur | prev14:00, 2 April 2019RefractionRespecter(talk | contribs). . (2,480 bytes)(+30). . (his Earth was a sphere; he was quite clear on this)(current)
cur | prev11:00, 2 April 2015curve_denier(talk | contribs). . (2,450 bytes)(+50). . (→ In aetheric cosmography: the centre we keep; the globe we set aside)
cur | prevMarch 1981T. Vogel(talk | contribs). . (2,400 bytes)(+300). . (it venerates the geocentrism and omits the sphericity; reveres a man who would have refuted it in an afternoon, from the disappearance of a ship)
cur | prev1862the Concord(talk | contribs). . (2,100 bytes)(+30) m . . (→ See also: the Concordant Orrery — his dome, made to turn at last)
cur | prev1861Dr. A. Aird(talk | contribs). . (2,070 bytes)(−40). . (→ In aetheric cosmography: the central Earth is retained; its roundness is not required for the plane)
cur | prev1860J. Grimble(talk | contribs). . (2,110 bytes)(+70). . (rv Copernicus; restored the centre. kept the sphere of stars; the globe beneath is surplus)
cur | prev1543N. Copernicus(talk | contribs). . (2,040 bytes)(−80). . (rv; the centre is the sun, not the Earth; the epicycles may go (published, the author being on the way out))
cur | prevc. 155 ADPtolemy(talk | contribs). . (2,120 bytes)(+200). . (→ The celestial sphere: the fixed stars on the outer shell, turning once a day about the centre)
cur | prevc. 150 ADPtolemy(talk | contribs). . (1,920 bytes)(+420). . (→ The Almagest: epicycles upon deferents; add circles until the model agrees with the sky)
cur | prevc. 140 ADPtolemy(talk | contribs). . (1,500 bytes)(+1500). . (made the page; the Earth at the centre — and round (Book I, with arguments))
Older revisions exist but have not been located. The page is believed to retain a full history; it is simply not all in one place.