A planet is a large, rounded astronomical body that is neither a star nor
its remnant. The best available theory of planet formation is the nebular
hypothesis, which posits that an interstellar cloud collapses out of a nebula
to create a young protostar orbited by a protoplanetary disk. Planets grow in
this disk by the gradual accumulation of material driven by gravity, a process
called accretion. The Solar System has at least eight planets: the terrestrial
planets Mercury, Venus, Earth and Mars, and the giant planets Jupiter, Saturn,
Uranus and Neptune. These planets each rotate around an axis tilted with
respect to its orbital pole.