The primary purpose of describing planetary orbits in terms of epicycles and deferents was to account for the
A) generally eastward motion of a planet compared to background stars while the whole sky appeared to move westward.
B) variation of brightness of a planet with time.
C) difference between the sidereal period and the synodic period of a planet.
D) pattern of direct and retrograde motion of a planet as it moved slowly against the background of stars.
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