  Euler wrote several papers on Astronomy, most of them in Latin. This is a
commented translation of E304 'Considerationes de motu corporum coelestium'
(Considerations on the motion of celestial bodies). In this publication, Euler
essentially focuses on the solution of two particular motions of a three-body
problem consisting of Sun, Earth and Moon. The first motion, represents a
hypothetical situation of these three celestial bodies in perpetual alignment
in syzygy - the three-body problem on a straight line -, for which the
parameter that controls the distances among the planets was found to be given
by a quintic function. The conclusion was that if the Moon were four times more
distant from the Earth (either in conjunction or in opposition), a motion of
this kind would have been possible to exist, such that the Moon would appear
always connected to the Sun. The second motion considered by Euler was Moon
libration, when these planets are aligned in regular syzygy. Here, perhaps for
the first time, Euler introduces an archaic form of a Fourier sine series
expansion to describe the Moon's wagging motion. However, as Euler himself
recognizes, the calculations turned out very tedious, and led him to greatly
simplify his model in order to obtain some numerical values for the phenomenon.
