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Precession, Aberration, Nutation

1987
In the Astronomical Ephemeris, you find for a number of bright stars the mean position and also the apparent position. (Since 1957 these last data are published in a separate volume.) The apparent positions vary in the course of the year. What is the reason? Or better: What are the reasons?
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Nutation

American Journal of Physics, 1966
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Nutational Resonance

Physical Review, 1952
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nutation

2011
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