Top 10 Articles

LS-Studio
GayRomeo
Justus_Dahinden
Mercedes Benz OM601
Diyanet İşleri Başkanlığı
Radically 25
Ral color system
RTLnow.de
New concept
Electromagnetic compatibility

News:

(95625) 2002 GX32

The correct title of this article is (95625) 2002 GX32. It features superscript or subscript characters that are substituted or omitted because of technical limitations.
(95625) 2002 GX32
Discovery
Discovered by M. W. Buie, A. B. Jordan, J. L. Elliot[1]
Discovery date April 8, 2002
Designations
MPC designation (95625) 2002 GX32
Alternative names none
Minor planet
category
SDO (Res 3:7)
Epoch December 31, 2006 (JD 2454100.5)
Aphelion 11105.993 Gm (74.239 AU)
Perihelion 4955.174 Gm (33.123 AU)
Semi-major axis 8030.584 Gm (53.681 AU)
Eccentricity 0.383
Orbital period 143658.388 d (393.32 a)
Average orbital speed 3.91 km/s
Mean anomaly 8.996°
Inclination 13.920°
Longitude of ascending node 28.135°
Argument of perihelion 186.213°
Physical characteristics
Dimensions 153 km[2]
Mass 3.8×1018? kg
Mean density 2.0? g/cm³
Equatorial surface gravity 0.0428? m/s²
Escape velocity 0.0809? km/s
Sidereal rotation
period
? d
Albedo 0.10?
Temperature ~38 K
Spectral type ?
Absolute magnitude 7.3

(95625) 2002 GX32, also written as (95625) 2002 GX32, is a trans-Neptunian object that resides in the scattered disc region of the Solar System. It was discovered on April 8, 2002 by Marc W. Buie, Amy B. Jordan, and James L. Elliot.

It is in a 3:7 orbital resonance with the planet Neptune, which means it completes three orbits around the Sun in the period of time of seven of Neptune's orbits.

References

  1. ^ List Of Centaurs and Scattered-Disk Objects. IAU: Minor Planet Center.
  2. ^ List of known trans-Neptunian objects


The original article is from Wikipedia. To view the original article please click here.
Creative Commons Licence