(120178) 2003 OP32

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(120178) 2003 OP32

(120178) 2003 OP32, also written as (120178) 2003 OP32, is a trans-Neptunian object (TNO) that resides in the Kuiper belt. It was discovered on July 26, 2003 by Michael E. Brown, Chad Trujillo and David L. Rabinowitz at Palomar Mountain in California.

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(120178) 2003 OP32
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(120178) 2003 OP32 among other Haumea family objects
Discovery
Discovered byM. E. Brown, C. Trujillo, D. Rabinowitz[1]
Discovery date26 July 2003
Designations
(120178) 2003 OP32
Cubewano (MPC)[2]
Extended (DES)[3]
Orbital characteristics[4]
Epoch 13 January 2016 (JD 2457400.5)
Uncertainty parameter 3
Observation arc9205 days (25.20 yr)
Aphelion47.620 AU (7.1239 Tm)
Perihelion38.480 AU (5.7565 Tm)
43.050 AU (6.4402 Tm)
Eccentricity0.10615
282.47 yr (103172 d)
4.51 km/s
71.841°
0° 0m 12.561s / day
Inclination27.219°
182.930°
67.082°
Jupiter MOID33.5815 AU (5.02372 Tm)
TJupiter5.208
Physical characteristics
Dimensions230 km[5][6]
9.71 h (0.405 d)
8.45 h[7]
0.7 (assumed)
Temperature~42 K
(Neutral)
B−V=0.70, V-R=0.39[8]
B0-V0=0.698[7]
3.8[4]
    Close

    Origin

    Based on their common pattern of infrared water-ice absorption and the clustering of their orbital elements,[9] the other KBOs 1995 SM55, (19308) 1996 TO66, (55636) 2002 TX300 and (145453) 2005 RR43, among others, appear to be collisional fragments broken off the dwarf planet Haumea. The neutral color of the spectrum of these objects in the visible range evidences a lack of complex organics on the surface of these bodies that has been studied in detail for the surface of Haumea.[10]

    References

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