(95625) 2002 GX32
Discovery[1] | |
---|---|
Discovered by | M. W. Buie, A. B. Jordan, J. L. Elliot |
Discovery date | April 8, 2002 |
Designations | |
MPC designation | (95625) 2002 GX32 |
SDO[2] 3:7 resonance[3][4][5] | |
Orbital characteristics[1] | |
Epoch November 30, 2008 (JD 2454800.5) | |
Aphelion |
73.731 AU 11,030 Gm (Q) |
Perihelion |
33.140 AU 4,998 Gm (q) |
53.436 AU 7,993 Gm (a) | |
Eccentricity | 0.37980 |
390.63 yr | |
Average orbital speed | 3.91 km/s |
10.754° | |
Inclination | 13.940° |
28.183° | |
186.36° | |
Physical characteristics | |
Dimensions | 153 km (assumed)[6] |
Albedo | 0.09 (assumed) |
Temperature | ~38 K |
7.1[1] | |
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(95625) 2002 GX32, also written as (95625) 2002 GX32, is a trans-Neptunian object that resides in the Kuiper belt.[2] It has a 3:7 resonance with Neptune.[3] It was discovered on April 8, 2002 by Marc W. Buie, Amy B. Jordan, and James L. Elliot.
It came to perihelion in 1997.[1]
Assuming a generic TNO albedo of 0.09, it is about 153 km in diameter.[6]
Resonance
Simulations by Emel’yanenko and Kiseleva in 2007 show that (95625) 2002 GX32 has a 99% probability of librating in a 3:7 resonance with Neptune.[7]
The Neptune 3:7 mean-motion resonance keeps it more than 11 AU from Neptune over a 14000-year period.[4]
It has been observed 21 times over 4 oppositions and has an orbit quality code of 3.[1]
References
- 1 2 3 4 5 "JPL Small-Body Database Browser: 95625 (2002 GX32)" (2004-06-09 last obs). Retrieved 2009-01-30.
- 1 2 "List Of Centaurs and Scattered-Disk Objects". Minor Planet Center. Retrieved 2009-01-29.
- 1 2 Marc W. Buie. "Orbit Fit and Astrometric record for 95625" (2006-04-25 using 25 observations). SwRI (Space Science Department). Retrieved 2009-01-29.
- 1 2 "MPEC 2004-N31 : 2002 GX32 = 1994 JV". Minor Planet Center. 2004-07-12. Retrieved 2009-01-29.
- ↑ "MPEC 2009-A63 :Distant Minor Planets (2009 JAN. 29.0 TT)". Minor Planet Center. 2009-01-13. Retrieved 2009-01-30.
- 1 2 Wm. Robert Johnston (22 August 2008). "List of Known Trans-Neptunian Objects". Johnston's Archive. Retrieved 2009-01-29.
- ↑ Emel’yanenko, V. V (2008). "Resonant motion of trans-Neptunian objects in high-eccentricity orbits". Astronomy Letters 34: 271–279. Bibcode:2008AstL...34..271E. doi:10.1134/S1063773708040075.
External links
- Orbital simulation from JPL (Java) / Horizons Ephemeris
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