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Planet

A planet is an astronomical body orbiting a star or stellar remnant that is massive enough to be rounded by its own gravity, is not massive enough to cause thermonuclear fusion, and has cleared its orbit of other debris. The term planet comes from the Ancient Greek word πλανήτης (planētēs), meaning "wanderer," as ancient astronomers noted that their motion was unlike that of the fixed stars. In Hebrew, the word for planet is כוכב לכת (kókháv lékhát). In other languages, the term translates as planète in French, planeta in Spanish and Portuguese, Planeten in German, and 惑星 (wakusei) in Japanese. Key contextual information includes the eight planets in our Solar System: Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, and Neptune. Pluto, once considered the ninth planet, was reclassified as a dwarf planet in 2006. Planets are generally divided into two main types: terrestrial (or rocky) planets and gas giants. Terrestrial planets are composed primarily of rock and metal, while gas giants are largely composed of hydrogen and helium.

Wikipedia Information
Planet
Large, round non-stellar astronomical object
Planet
A planet is a large, rounded astronomical body that is generally required to be in orbit around a star, stellar remnant, or brown dwarf, and is not one itself. The Solar System has eight planets by the most restrictive definition of the term: the terrestrial planets Mercury, Venus, Earth, and Mars, and the giant planets Jupiter, Saturn, Uranus, and Neptune. 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.
Last modified: 2025-10-11T17:26:20ZView full article on Wikipedia