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Currently (as of 0.13) the moon's rotation is modelled very simply. This causes some noticeable mismatch in appearance (libration), increasing for longer time from J2000. E.g. Moon in Neolithic time shows its side. IAU has better rotation models, this task should be to properly integrate it. See e.g. http://astrope...

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Joined on 2015-04-27
Joined on 2015-04-17
Joined on 2012-03-12
Joined on 2012-03-12

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