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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Contents
I | 1 |
Classes of Eclipse Reports and Their | 43 |
ANCIENT RECORDS OF LARGE SOLAR | 49 |
Copyright | |
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accelerations accuracy analysis ancient apparent assigned assumed assumption astronomical basis beginning calculated called central line centuries Chapter close column conjunctions contribution correct corresponding described diameter difference digit discussion earth eclipse magnitudes eclipse reports ephemeris epoch equal equation equinox error estimate Figure Fotheringham function given gives Hence Hipparchus hour identification independent inferred interpretation involved Islamic large solar eclipses latitude listed longitude lunar eclipse magnitude mean measurements method middle moon needed night observations obtained occultations occurred original passage phase position possible present priori probably Ptolemy quantities reasonable record Reference reliability reports respect seems seen solar eclipse standard deviation stars suggests Table taken tion translation Venus VIII weight