Binary system: Difference between revisions
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When binary minor planets are similar in size, they may be called "[[Binary asteroid|binary companions]]" instead of referring to the smaller body as a satellite.<ref name="IAU-list">{{cite web |date=2009-09-17 |title=Satellites and Companions of Minor Planets |publisher=IAU / [[Minor Planet Center]] |url=http://www.cbat.eps.harvard.edu/minorsats.html |access-date=2011-01-08 |url-status=dead |archive-url=https://web.archive.org/web/20110121153650/http://www.cbat.eps.harvard.edu/minorsats.html |archive-date=2011-01-21 }}</ref> Good examples of true binary companions are the [[90 Antiope]] and the [[79360 Sila–Nunam]] systems. [[Pluto]] and its largest moon [[Charon (moon)|Charon]] are sometimes described as a binary system because the [[barycenter]] (center of mass) of the two objects is not inside either of them.<ref>{{cite web |url=http://news.discovery.com/space/can-we-call-pluto-and-charon-a-binary-planet-yet-140808.htm |title=Can We Call Pluto and Charon a 'Binary Planet' Yet? |author=Ian O'Neill |website=Discovery News |date=8 August 2014 |access-date=15 July 2015}}</ref> |
When binary minor planets are similar in size, they may be called "[[Binary asteroid|binary companions]]" instead of referring to the smaller body as a satellite.<ref name="IAU-list">{{cite web |date=2009-09-17 |title=Satellites and Companions of Minor Planets |publisher=IAU / [[Minor Planet Center]] |url=http://www.cbat.eps.harvard.edu/minorsats.html |access-date=2011-01-08 |url-status=dead |archive-url=https://web.archive.org/web/20110121153650/http://www.cbat.eps.harvard.edu/minorsats.html |archive-date=2011-01-21 }}</ref> Good examples of true binary companions are the [[90 Antiope]] and the [[79360 Sila–Nunam]] systems. [[Pluto]] and its largest moon [[Charon (moon)|Charon]] are sometimes described as a binary system because the [[barycenter]] (center of mass) of the two objects is not inside either of them.<ref>{{cite web |url=http://news.discovery.com/space/can-we-call-pluto-and-charon-a-binary-planet-yet-140808.htm |title=Can We Call Pluto and Charon a 'Binary Planet' Yet? |author=Ian O'Neill |website=Discovery News |date=8 August 2014 |access-date=15 July 2015}}</ref> |
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==In popular culture== |
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*In the Discovery program ''[[Alien Planet]]'', the planet [[Darwin IV]] orbits a binary system. |
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*In ''[[The Hitchhiker's Guide to the Galaxy (novel)|The Hitchhiker's Guide to the Galaxy]]'', the planet [[Places in The Hitchhiker's Guide to the Galaxy#Magrathea|Magrathea]] orbits a binary system |
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*In the ''[[Invader Zim]]'' episode "Planet Jackers", one of the aforementioned Jackers mentions a binary system. |
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*Binary star systems are featured in the ''[[Mass Effect 2]]'' game, these systems are in the [[Milky Way]] as explorable areas. |
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*A binary star system is featured in the short story by Dan Simmons, "Orphans of the Helix." |
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*The planet Tatooine from [[Star Wars]] features a binary star system. |
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==See also== |
==See also== |
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Revision as of 03:44, 29 November 2021
 | This article needs additional citations for verification. (February 2015) |
A binary system is a system of two astronomical bodies which are close enough that their gravitational attraction causes them to orbit each other around a barycenter (also see animated examples). More restrictive definitions require that this common center of mass is not located within the interior of either object, in order to exclude the typical planet–satellite systems and planetary systems.
The most common binary systems are binary stars and binary asteroid, but brown dwarfs, planets, neutron stars, black holes and galaxies can also form binaries.
A multiple system is like a binary system but consists of three or more objects such as for trinary stars and trinary asteroids.
Classification
In a binary system, the brighter object is referred to as primary, and the other the secondary.
They are also classified based on orbit. Wide binaries are objects with orbits that keep them apart from one another. They evolve separately and have very little effect on each other. Close binaries are close to each other and are able to transfer mass from one another.
They can also be classified based on how we observe them. Visual binaries are two stars separated enough that they can be viewed through a telescope or binoculars.
Eclipsing binaries are where the objects' orbits are at an angle that when one passes in front of the other it causes an eclipse, as seen from Earth.
Astrometric binaries are objects that seem to move around nothing as their companion object cannot be identified, it can only be inferred. The companion object may not be bright enough or may be hidden in the glare from the primary object.
A related classification though not a binary system is optical binary, which refers to objects that are so close together in the sky that they appear to be a binary system, but are not. Such objects merely appear to be close together, but lie at different distances from the Solar System.[1][2]
Binary companion (minor planets)
When binary minor planets are similar in size, they may be called "binary companions" instead of referring to the smaller body as a satellite.[3] Good examples of true binary companions are the 90 Antiope and the 79360 Sila–Nunam systems. Pluto and its largest moon Charon are sometimes described as a binary system because the barycenter (center of mass) of the two objects is not inside either of them.[4]
See also
- Binary asteroid
- Binary star
- Contact binary
- Contact binary (small Solar System body)
- Double planet
- Rotational Brownian motion
References
- ^ "Binary Star Systems: Classification and Evolution". Space.com.
- ^ Lehmann, Holger. Analysis of Spectroscopic Binaries. Thüringer Landessternwarte Tautenburg.
- ^ "Satellites and Companions of Minor Planets". IAU / Minor Planet Center. 2009-09-17. Archived from the original on 2011-01-21. Retrieved 2011-01-08.
- ^ Ian O'Neill (8 August 2014). "Can We Call Pluto and Charon a 'Binary Planet' Yet?". Discovery News. Retrieved 15 July 2015.
External links
Bibliography
- Astronomy: A Visual Guide by Mark A. Garlick