(84522) 2002 TC302: Difference between revisions
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| mean_anomaly= 312.9 |
| mean_anomaly= 312.9 |
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| speed= |
| speed= |
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| dimensions= |
| dimensions= 420 - 1190 [[kilometer|km]] <sup>[http://neo.jpl.nasa.gov/glossary/h.html H]</sup> |
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| mass= ?×10<sup>?</sup> [[kilogram|kg]] |
| mass= ?×10<sup>?</sup> [[kilogram|kg]] |
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| density= ? g/[[cubic centimetre|cm³]] |
| density= ? g/[[cubic centimetre|cm³]] |
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| escape_velocity= ? km/s |
| escape_velocity= ? km/s |
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| rotation= |
| rotation= |
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| spectral_class= (red) B-V=1.03; V-R=0.67 <ref>{{cite web|url=http://www.physics.nau.edu/~tegler/research/survey.htm |title=Kuiper Belt Object Magnitudes and Surface Colors |accessdate=2006-11-05 |last=Tegler |first=Stephen C. |coauthors= |date=2006-01-26}}</ref> |
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| spectral_class= ? |
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| abs_mag= 3. |
| abs_mag= 3.85 |
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| albedo=>0.051<ref>{{cite web|url=http://arxiv.org/abs/astro-ph/0502229 |title=Diverse albedos of small trans-neptunian objects |accessdate=2006-11-07 |last=Grundy |first=W. M. |coauthors=Noll, K. S.; Stephens, D. C. |date=2004 | journal=Icarus, | volume=176 | pages=22}}</ref> |
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| albedo= |
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| temperature= |
| temperature= |
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'''{{mp|(84522) 2002 TC|302}}''' is a large [[resonant Trans-Neptunian |
'''{{mp|(84522) 2002 TC|302}}''' is a large [[color index|red]] 2:5 [[Resonant trans-Neptunian object|resonant]] [[Trans-Neptunian object]]<ref name="MPC-2006P22">List of classified orbits [http://www.cfa.harvard.edu/iau/mpec/K06/K06P22.html from MPC]</ref> |
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, orbiting the sun at a distance of 39 |
, orbiting the sun at a distance of 39 to 71 [[Astronomical unit|AU]]. Due to the resonance, it completes 2 orbits for every 5 orbits of Neptune. The red spectra suggests that {{mp|(84522) 2002 TC|302}} has very little ice on its surface and explains why it has a lower than average [[albedo]]. |
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{{mp|(84522) 2002 TC|302}} was discovered on [[October |
{{mp|(84522) 2002 TC|302}} was discovered on [[October 9]], [[2002]] by the [[Near Earth Asteroid Tracking|NEAT]] program at the [[Palomar Observatory]]. |
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==See also== |
==See also== |
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*[[Trans-Neptunian object]] |
*[[Trans-Neptunian object]] |
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*[[Scattered disc]] |
*[[Scattered disc]] |
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{{MinorPlanets Navigator|(84521) 2002 TE300|PageName={{mp|(84522) 2002 TC|302}}|(84523) 2002 UF2}} |
{{MinorPlanets Navigator|(84521) 2002 TE300|PageName={{mp|(84522) 2002 TC|302}}|(84523) 2002 UF2}} |
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Revision as of 23:41, 8 November 2006
Template:DownsizeTemplate:Infobox Minor Planet
(84522) 2002 TC302 is a large red 2:5 resonant Trans-Neptunian object[1] , orbiting the sun at a distance of 39 to 71 AU. Due to the resonance, it completes 2 orbits for every 5 orbits of Neptune. The red spectra suggests that (84522) 2002 TC302 has very little ice on its surface and explains why it has a lower than average albedo.
(84522) 2002 TC302 was discovered on October 9, 2002 by the NEAT program at the Palomar Observatory.
References
See also
Template:Footer TransNeptunian
 | This article about a centaur (minor planet) or trans-Neptunian object is a stub. You can help Wikipedia by expanding it. |