Babylonian Timings of Eclipse Contacts and the Study of the Earth's Past Rotation

Astronomy and Astrophysics – Astronomy

Scientific paper

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Babylon, Earth Rotation, Eclipses

Scientific paper

Long-term changes in the length of the day are investigated using an extensive series of Late Babylonian timings of lunar and solar eclipses. The dates of these observations range between about 700 BC and 50 BC. In recording the times of eclipse contacts, the Babylonian astronomers reported time intervals rather than specific moments. Hence scribal errors tend to be cumulative. To reduce this effect, I have concentrated in this paper almost exclusively on first contact observations. Analysis of these measurements leads to a result for the parameter AT of 31.7 ± 0.3 sec/cy/cy and a mean rate of change in the length of the day over the selected interval of 1.74 ± 0.03 ms/cy.

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