Encyclopædia Galactica Rami T. F. Rekola Tuorlan Astronomical Society Tuorla Observatory University of Turku

Planet

A large body that orbits a star. Planets do not emit light on their own (but reflect light of their star). A planet may consist of rock and metals, like the inner planets of Solar System, or or gases and liqiuds, like the gas giants of Solar System. There is a class of so called brown dwarf stars in the border area of biggest gas giant planets and smallest stars that can not clearly be classified as either.

The IAU members gathered at the 2006 General Assembly agreed that a "planet" is defined as a celestial body that (a) is in orbit around the Sun, (b) has sufficient mass for its self-gravity to overcome rigid body forces so that it assumes a hydrostatic equilibrium (nearly round) shape, and (c) has cleared the neighbourhood around its orbit.

It should be noted that point (c) should not be taken literally as e.g. the Moon exists on the orbit of the Earth. The spirit of point (c) is that a planet either controls its orbit or can clear it. The Earth totally dominates its orbit and, hence, that of the Moon. Neptune, on the other hand, can sling Pluto out of the solar system - or at least alter its orbit considerably - should they ever come very close to each other. Pluto is so small in comparison that the change in Neptune's orbit would be infinitesimal.