VS2 (apparent magnitude 19.8) as viewed with a 24" telescope
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Discovery[2]
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Discovered by | NEAT (644) |
Discovery date | November 14, 2003[1] |
Designations
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MPC designation | (84922) 2003 VS2 |
Alternate name(s) | none |
Minor planet category |
Plutino[3][4] |
Epoch December 31, 2006 (JD 2454100.5) | |
Aphelion | 6298.735 Gm (42.104 AU) |
Perihelion | 5449.350 Gm (36.427 AU) |
Semi-major axis | 5874.042 Gm (39.266 AU) |
Eccentricity | 0.072 |
Orbital period | 89870.237 d (246.05 a) |
Average orbital speed | 4.75 km/s |
Mean anomaly | 3.987° |
Inclination | 14.798° |
Longitude of ascending node | 302.682° |
Argument of perihelion | 112.586° |
Physical characteristics
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Dimensions | 725+188 −199 km[5][6] |
Mass | ≈4×1020? kg[7] |
Mean density | 2.0? g/cm³ |
Equatorial surface gravity | 0.1778? m/s² |
Escape velocity | 0.3362? km/s |
Sidereal rotation period |
7.41 ± 0.02 h[8] |
Albedo | 0.036–0.106[5] |
Temperature | ~44 K |
Spectral type | (moderately red) B-V=0.93, V-R=0.59[9] |
Apparent magnitude | 19.7[10] |
Absolute magnitude (H) | 3.97[1] 4.4[5] |
(84922) 2003 VS2 is a trans-Neptunian object discovered by the Near Earth Asteroid Tracking program on November 14, 2003.[2] Like Pluto, it is in a 2:3 orbital resonance with Neptune,[3][4] giving it the orbital properties of a plutino. It is very likely a dwarf planet.
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Like Pluto, 2003 VS2 is locked in the 3:2 mean motion resonance with Neptune, although its orbit is significantly less eccentric less than Pluto's is. It also has slightly smaller orbital inclination.[1]
The most likely value of the rotation period of this object is 7.41 ± 0.02 hours.[8]
With a moderately red color index (B-V=0.93, V-R=0.59),[9] and a Spitzer size estimate of 725 ± 200 km,[5] this plutino is also a dwarf-planet candidate. At around a size of 400 km, trans-Neptunian objects are expected to be spherical.[11]
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