Planets are major celestial bodies orbiting a star, distinct from dwarf planets and satellites, maintained in stable orbits by gravitational attraction acting as a centripetal force. The Solar System comprises eight planets: four inner terrestrial planets and four outer gas giants, a structure determined by the accretion processes within the primordial solar nebula. Physics principles dictate that for stable circular orbits, the gravitational force provides the necessary centripetal force, resulting in a specific relationship where orbital speed decreases as the orbital radius increases.
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