Extrasolar object: Difference between revisions

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{{wiktionary}}
{{wiktionary}}
'''''Extrasolar''''' (From '''extra''', Latin for outside or beyond, and '''solar''', Latin for the [[Sun]]) is a term applied to any object that exists outside the [[Solar System]]. It is not applied to stars, or any other celestial object that is larger than a star or the Solar System, such as a [[galaxy]]. It is only used for objects which are also found in the Solar System. The terms for extrasolar examples of Solar System bodies are:
'''''Extrasolar''''' (From '''extra''', Latin for outside or beyond, and '''solar''', Latin for the [[Sun]]) is a term applied to any object that exists outside the [[Solar System]]. It is not applied to stars, or any other celestial object that is larger than a star or the Solar System, such as a [[galaxy]]. It is only used for objects (aside from stars) which are also found in the Solar System. The terms for extrasolar examples of Solar System bodies are:


* [[Extrasolar planet]], also called an "exoplanet"
* [[Extrasolar planet]], also called an "exoplanet"

Revision as of 18:51, 13 October 2013

Extrasolar (From extra, Latin for outside or beyond, and solar, Latin for the Sun) is a term applied to any object that exists outside the Solar System. It is not applied to stars, or any other celestial object that is larger than a star or the Solar System, such as a galaxy. It is only used for objects (aside from stars) which are also found in the Solar System. The terms for extrasolar examples of Solar System bodies are:

Some Solar System object classes, such as minor planets, dwarf planets and Trans-Neptunian objects have not been detected outside the Solar System.

See also