Английская Википедия:2012 VP113
Шаблон:Short description Шаблон:Use dmy dates
Шаблон:Infobox planet Шаблон:Mp, also known by its nickname "Biden", is a trans-Neptunian object of the sednoid population, located in the outermost reaches of the Solar System. It was first observed on 5 November 2012 by American astronomers Scott Sheppard and Chad Trujillo at the Cerro Tololo Inter-American Observatory in Chile.[1][2] The discovery was announced on 26 March 2014.[3][4] The object probably measures somewhere between 300 and 1000 km in diameter, possibly large enough to be a dwarf planet.
Classification and physical characteristics
Шаблон:Mp is the minor planet with the farthest known perihelion (closest approach to the Sun) in the Solar System, greater than Шаблон:Dp's.[5] Though its perihelion is farther, Шаблон:Mp has an aphelion only about half of Sedna's. It is the second discovered sednoid, with semi-major axis beyond Шаблон:Val and perihelion greater than Шаблон:Val. The similarity of the orbit of Шаблон:Mp to other known extreme trans-Neptunian objects led Scott Sheppard and Chad Trujillo to suggest that an undiscovered object, Planet Nine, in the outer Solar System is shepherding these distant objects into similar type orbits.[3]
It has an absolute magnitude of 4.0,[1] which means it may be large enough to be a dwarf planet.[6] It is expected to be about half the size of Sedna and similar in size to Huya.[7] Its surface is thought to have a pink tinge, resulting from chemical changes produced by the effect of radiation on frozen water, methane, and carbon dioxide.[8] This optical color is consistent with formation in the gas-giant region and not the classical Kuiper belt, which is dominated by ultra-red colored objects.[3]
History
Discovery
Шаблон:Mp was first observed on 5 November 2012[2] with NOAO's 4-meter Víctor M. Blanco Telescope at the Cerro Tololo Inter-American Observatory.[9] Carnegie's 6.5-meter Magellan telescope at Las Campanas Observatory in Chile was used to determine its orbit and surface properties.[9] Before being announced to the public, it was only tracked by Cerro Tololo Inter-American Observatory (807) and Las Campanas Observatory (304).[1] Two precovery measurements from 22 October 2011 have been reported.[1] A primary issue with observing it and finding precovery observations of it is that at an apparent magnitude of 23, it is too faint for most telescopes to easily observe.
Nickname
Шаблон:Mp was abbreviated "VP" and nicknamed "Biden" by the discovery team, after Joe Biden who, at the time of discovery, was vice president ("VP") of the United States.[4]
Orbit
Шаблон:See also Шаблон:Mp has the largest perihelion distance of any known object in the Solar System.[10] Its last perihelion was within a couple months of September 1979.[11] The paucity of bodies with perihelia at Шаблон:Val appears not to be an observational artifact.[3]
It is possibly a member of a hypothesized Hills cloud.[7][9][12] It has a perihelion, argument of perihelion, and current position in the sky similar to those of Sedna.[7] In fact, all known Solar System bodies with semi-major axes over Шаблон:Val and perihelia greater than Neptune's have arguments of perihelion clustered near Шаблон:Val.[3] This could indicate a similar formation mechanism for these bodies.[3] Шаблон:Mpl was the first such object discovered.
It is currently unknown how Шаблон:Mp acquired a perihelion distance beyond the Kuiper belt. The characteristics of its orbit, like those of Sedna's, have been explained as possibly created by a passing star or a trans-Neptunian planet of several Earth masses hundreds of astronomical units from the Sun.[13] The orbital architecture of the trans-Plutonian region may signal the presence of more than one planet.[14][15] Шаблон:Mp could even be captured from another planetary system.[6] However, it is considered more likely that the perihelion of Шаблон:Mp was raised by multiple interactions within the crowded confines of the open star cluster in which the Sun formed.[7]
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Simulated view showing the orbit of Шаблон:Mp
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2012 VP113 orbit in white with hypothetical Planet Nine
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The orbits of known distant objects with large aphelion distances over 200 AU
See also
- List of Solar System objects most distant from the Sun
- 90377 Sedna (relatively large and also distant body)
- 541132 Leleākūhonua (distant sednoid)
- List of hyperbolic comets
- Other large aphelion objects
References
External links
- 2012 VP113 Inner Oort Cloud Object Discovery Images from Scott S. Sheppard/Carnegie Institution for Science.
- 2012 VP113 has Q=460 ± 30 Шаблон:Webarchive (mpml: CFHT 2011-Oct-22 precovery)
- List of Known Trans-Neptunian Objects, Johnston's Archive
- List Of Centaurs and Scattered-Disk Objects, Minor Planet Center
- Шаблон:JPL small body
Шаблон:2014 in space Шаблон:Dwarf planets Шаблон:Trans-Neptunian objects Шаблон:Small Solar System bodies Шаблон:Authority control
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