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planet

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Also known as planetary body, planets

thumb|upright=1.5|The eight planets of the Solar System with size to scale (up to down, left to right): [[Saturn, Jupiter, Uranus, Neptune (outer planets), Earth, Venus, Mars, and Mercury (inner planets)]] 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 plane

OverviewAI-generated

A planet is a planetary-mass object and substellar object that is part of a planetary system. It is studied by planetary science and has characteristics including mass, orbital elements, radius, and a planetary magnetic field. The concept is described in sources such as the Brockhaus and Efron Encyclopedic Dictionary, The Nuttall Encyclopædia, Encyclopædia Britannica 11th edition, and the Granat Encyclopedic Dictionary.

Planets are distinct from Planeta and Planet. The next lower rank includes natural satellites and minor planets, while the next higher rank is a star. Model items for planets include Mercury, Earth, Mars, and Jupiter. The subject is represented by the Unicode character 🪐 and is categorized under "Planets" on Commons. It is referenced by 2,647 other encyclopedia articles and has a PubMed count of 22468 for the query "planet."

Synthesized by Vinony from 28 facts across 4 sources: Wikidata, Firecrawl, PubMed, Vinony graph. Generated from structured data (not the Wikipedia text) and checked against those facts — may still contain errors.

Research

22,468 papers

via PubMed

Described at

Who’s On First | Docs | Placetypes

Who’s on First is a gazetteer of places.

whosonfirst.org

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~72 min read

Encyclopedic overview

34 sections
Contents
  • Formation
  • Planets in the Solar System
  • Exoplanets
  • Dynamic characteristics
  • Orbit
  • Axial tilt
  • Rotation
  • Orbital clearing
  • Physical characteristics
  • Size and shape
  • Mass
  • Internal differentiation
  • Atmosphere
  • Magnetosphere
  • Secondary characteristics
  • History and etymology
  • Ancient civilizations and classical planets
  • Babylon
  • Greco-Roman astronomy
  • Medieval astronomy
  • Scientific Revolution and discovery of outer planets
  • Defining the term ''planet''
  • Criticisms and alternatives to IAU definition
  • Exoplanets
  • IAU working definition of exoplanets
  • Mythology and naming
  • Classical planets
  • Modern discoveries
  • Exoplanets
  • Symbols
  • See also
  • Notes
  • References
  • External links

thumb|upright=1.5|The eight planets of the Solar System with size to scale (up to down, left to right): [[Saturn, Jupiter, Uranus, Neptune (outer planets), Earth, Venus, Mars, and Mercury (inner planets)]] 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.

The word planet comes from the Greek () . In antiquity, this word referred to the Sun, Moon, and five points of light visible to the naked eye that moved across the background of the stars—namely, Mercury, Venus, Mars, Jupiter, and Saturn. Planets have historically had religious associations: multiple cultures identified celestial bodies with gods, and these connections with mythology and folklore persist in the schemes for naming newly discovered Solar System bodies. Earth itself was recognized as a planet when heliocentrism supplanted geocentrism during the 16th and 17th centuries.

Excerpted from Wikipedia’s “planet” article, available under the CC BY-SA 4.0 licence.

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