Ancient Astronomical Observations and the Accelerations of the Earth and MoonDr. Newton discusses and analyses a very large number of ancient and medieval astronomical observations. The objective is the study of the rotation of the Earth and the motion of the Mood during the historical past -- essentially since about 750 B.C. |
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accelerations accuracy ancient apparent assigned assumed assumption Assyria astronomical basis beginning Cairo calculated called central century Chapter close column conjunction contribution correct corresponding described detail diameter difference digit discussion eclipse magnitudes eclipse reports ephemeris epoch equal equation equinox error estimate event Figure Fotheringham Ginzel given gives Hence Hipparchus hour identification independent inference interpretation involved Islamic Italy later latitude listed longitude lunar eclipse magnitude mean measurement method middle moon needed night observations occultations occurred original passage phase position possible priori probably Ptolemy reason record Reference reliability seems seen solar eclipse standard deviation stars suggests sunset Table taken tion translation Venus VIII weight