Category Archives: Astronomy

From Kepler to Ptolemy 12

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Mercury

Mercury refused to cooperate with Ptolemy’s basic paradigm. You might guess that the fault lies with Mercury’s larger eccentricity, but studies show that bad data bears most of the blame. Mercury hugs the Sun, only appearing near the horizon close to sunrise or sunset, hardly ideal observation conditions.

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From Kepler to Ptolemy 11

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Here is the basic model for Venus:

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From Kepler to Ptolemy 10

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We’ve seen the basic plan for an outer planet in post 2:

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From Kepler to Ptolemy 9

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The Moon is the one solar body that does revolve around the Earth. It never displays retrogression. So you’d think Ptolemy wouldn’t “need no stinkin’ epicycles” for it. In fact, Ptolemy gave it a mechanism more complicated than that of any of the planets except Mercury! Here’s the model:

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From Kepler to Ptolemy 8

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The Sun

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From Kepler to Ptolemy 7

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The Full Ptolemy

We now start the second part of this series: an in-depth look at the Ptolemaic system.

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From Kepler to Ptolemy 6

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Summary, and 20-20 Hindsight

Let’s recap.

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From Kepler to Ptolemy 5

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Origins of the Ptolemaic System

We’ve worked backwards from Kepler to Ptolemy. What inspired Ptolemy and his predecessors (Apollonius and Hipparchus) to come up with this scheme in the first place?

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From Kepler to Ptolemy 4

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Speed Laws

In Ptolemy’s system, the point on the deferent moves uniformly as viewed from a point called the equant point, or sometimes just equant. The equant, the center of the deferent, and Earth all lie in a straight line, with the center midway between Earth and the equant.

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From Kepler to Ptolemy 3

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Ellipses

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