Asteroid: Difference between revisions
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An '''asteroid''' is any one of many rocky, metallic bodies that orbit the [[Sun]] but have no [[atmosphere]] and are too small to be classed as [[planet]]s. | An '''asteroid''' is any one of many rocky, metallic bodies that orbit the [[Sun]] but have no [[atmosphere]] and are too small to be classed as [[planet]]s. | ||
The main [[asteroid belt]] lies between the orbits of [[Mars (planet)|Mars]] and [[Jupiter (planet)|Jupiter]], and comprises tens of thousands of irregularly-shaped bodies, from pebble-sized asteroids to the giant [[Ceres (dwarf planet)|Ceres]], which is also classified as a [[dwarf planet]]. | The main [[asteroid belt]] lies between the orbits of [[Mars (planet)|Mars]] and [[Jupiter (planet)|Jupiter]], and comprises tens of thousands of irregularly-shaped bodies, from pebble-sized asteroids to the giant [[Ceres (dwarf planet)|Ceres]], which is also classified as a [[dwarf planet]]. The mean diameter of Ceres is 940 km, or about 7.4% as large as [[Earth]]'s. | ||
The [[Kuiper belt]], beyond the orbit of the [[Planet Neptune]] is also believed to contain tens of thousands of asteroids and dwarf planets.<ref> | The [[Kuiper belt]], beyond the orbit of the [[Planet Neptune]], is also believed to contain tens of thousands of asteroids and dwarf planets.<ref> | ||
{{cite news | {{cite news | ||
| url = http://www.ifa.hawaii.edu/publications/preprints/06preprints/Delsanti_06-009.pdf | | url = http://www.ifa.hawaii.edu/publications/preprints/06preprints/Delsanti_06-009.pdf | ||
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==References== | ==References== | ||
{{reflist}} | {{reflist}}[[Category:Suggestion Bot Tag]] | ||
Latest revision as of 16:00, 13 July 2024
An asteroid is any one of many rocky, metallic bodies that orbit the Sun but have no atmosphere and are too small to be classed as planets.
The main asteroid belt lies between the orbits of Mars and Jupiter, and comprises tens of thousands of irregularly-shaped bodies, from pebble-sized asteroids to the giant Ceres, which is also classified as a dwarf planet. The mean diameter of Ceres is 940 km, or about 7.4% as large as Earth's.
The Kuiper belt, beyond the orbit of the Planet Neptune, is also believed to contain tens of thousands of asteroids and dwarf planets.[1]
While other primordial material in the early Solar System clumped together to form planets, it is likely that Jupiter's strong gravity prevented the asteroid belt forming into new worlds.
References
- ↑ Audrey Delsanti, David Jewitt. The Solar System Beyond The Planets, Institute for Astronomy, University of Hawaii.