Orbital motion is governed by the gravitational force acting as a centripetal force, pulling satellites towards the centre of the primary body. Candidates must understand that for circular orbits, while speed remains constant, velocity changes continuously due to the changing direction, implying acceleration. The topic necessitates an understanding of the relationship between orbital radius and orbital speed; specifically, that a decrease in orbital radius requires an increase in speed to maintain a stable orbit. Mastery involves applying these principles to both natural satellites (moons, planets) and artificial satellites (geostationary, polar), linking physical principles to functional applications.
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