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diurnal motion
noun
(astronomy)
The
apparent
westward
rotation
of
the
celestial
sphere,
along
with
the
apparent
westward
revolution
of
celestial
objects,
around
the
celestial
poles
due
to
prograde
(eastward)
rotation
of
planet
Earth
relative
to
the
seemingly
fixed
stars
–
completed
once
each
sidereal
day
(about
23
hours,
56
minutes,
4
seconds).