(42301) 2001 UR163
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- The correct title of this article is (42301) 2001 UR163. It features superscript or subscript characters that are substituted or omitted because of technical limitations.
Discovery
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Discovered by | Deep Ecliptic Survey[1] |
Discovery date | October 21, 2001 |
Designations
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MPC designation | (42301) 2001 UR163 |
Alternative names | none |
Minor planet category |
ESDO |
Epoch December 31, 2006 (JD 2454100.5) | |
Aphelion | 9889.356 Gm (66.106 AU) |
Perihelion | 5498.582 Gm (36.756 AU) |
Semi-major axis | 7693.969 Gm (51.431 AU) |
Eccentricity | 0.285 |
Orbital period | 134721.208 d (368.85 a) |
Average orbital speed | 4.07 km/s |
Mean anomaly | 68.401° |
Inclination | 0.75235 [degree (angle) |
Longitude of ascending node | 301.769° |
Argument of perihelion | 342.639° |
Physical characteristics
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Dimensions | 636 km[2] |
Mass | 2.7×1020? kg |
Mean density | 2.0? g/cm³ |
Equatorial surface gravity | 0.1778? m/s² |
Escape velocity | 0.3362? km/s |
Sidereal rotation period |
? d |
Albedo | 0.10? |
Temperature | ~39 K |
Spectral type | (Super RED;highest B-R) B-V=1.44; V-R=0.84; B-R=2.28 |
Absolute magnitude | 3.97 |
(42301) 2001 UR163, also written as (42301) 2001 UR163, is a trans-Neptunian object (TNO) that resides in the extended Scattered disc. It was discovered on October 21, 2001 by the Deep Ecliptic Survey (DES) program at Kitt Peak.
2001 UR163 has the REDDEST color index of any object in the solar system. On October 31st, 2002, the 3.6 meter Canada-France-Hawaii telescope observed 2001 UR163 set a record RED reading of B-R=2.28. This makes 2001 UR163 even redder than 5145 Pholus, (119070) 2001 KP77, 90377 Sedna, and comet C/2001 T4. Reddening of the spectrum is caused by cosmic irradiaton by ultraviolet radiation and charged particles. Becoming bluer in the spectrum is caused by impact collisions exposing the interior of an object. In the visible spectrum 2001 UR163 would appear an orange-brown depending on its albedo.
[edit] References
[edit] External links
- Orbital simulation from JPL (Java) / Ephemeris
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