(84522) 2002 TC302
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- The correct title of this article is (84522) 2002 TC302. It features superscript or subscript characters that are substituted or omitted because of technical limitations.
Discovery
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Discovered by | NEAT |
Discovery date | October 9, 2002 |
Designations
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MPC designation | (84522) 2002 TC302 |
Alternative names | none |
Minor planet category |
TNO (SDO) |
Epoch December 31, 2006 (JD 2454100.5) | |
Aphelion | 10,618.967 Gm (70.983 AU) |
Perihelion | 5,843.055 Gm (39.058 AU) |
Semi-major axis | 8,231.011 Gm (55.021 AU) |
Eccentricity | 0.290 |
Orbital period | 149,069.948 d (408.13 a) |
Average orbital speed | 3.93 km/s |
Mean anomaly | 313.636° |
Inclination | 35.109° |
Longitude of ascending node | 23.874° |
Argument of perihelion | 87.222° |
Physical characteristics
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Dimensions | 420-1,190 km [1] 820-1,480 km[2] |
Mass | 0.78-18×1020? kg |
Mean density | 2.0? g/cm³ |
Equatorial surface gravity | 0.12-0.33? m/s² |
Escape velocity | 0.22-0.63? km/s |
Sidereal rotation period |
? d |
Albedo | >0.051[3] |
Spectral type | (red) B-V=1.03; V-R=0.67 [4] |
Apparent magnitude | 20.5 |
Absolute magnitude | 3.85 |
(84522) 2002 TC302 is a large red 2:5 resonant Trans-Neptunian object discovered on October 9, 2002 by the NEAT program at the Palomar Observatory. [5].
Contents |
[edit] Orbit
Orbiting the sun at a distance of 39.058 to 70.983 AU. Due to the resonance, it completes 2 orbits for every 5 orbits of Neptune. Given the long orbit that TNOs have around the sun, 2002 TC302 comes to opposition in late October of each year at an apparent magnitude of 20.5.
[edit] Surface
The red spectra suggests that 2002 TC302 has very little ice on its surface and explains why it has a lower than average albedo.
[edit] References
- ^ Absolute Magnitude (H). Retrieved on 2006-11-06.
- ^ John Stansberry, Will Grundy, Mike Brown, John Spencer, David Trilling, Dale Cruikshank, Jean-Luc Margot (2007). Physical Properties of Kuiper Belt and Centaur Objects: Constraints from Spitzer Space Telescope. University of Arizona, Lowell Observatory, California Institute of Technology, NASA Ames Research Center, Southwest Research Institute, Cornell University. Retrieved on 2007-12-01.
- ^ Grundy, W. M.; Noll, K. S.; Stephens, D. C. (2004). Diverse albedos of small trans-neptunian objects 22. Retrieved on 2006-11-07.
- ^ Tegler, Stephen C. (2006-01-26). Kuiper Belt Object Magnitudes and Surface Colors. Retrieved on 2006-11-05.
- ^ List of classified orbits from MPC
[edit] See also
[edit] External links
- Orbital simulation from JPL (Java) / Ephemeris
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