|
Discovery[1]
|
|
|---|---|
| Discovered by | Chad Trujillo, Michael E. Brown |
| Discovery date | 18 June 2002 |
|
Designations
|
|
| MPC designation | 2002 MS4 |
| Alternate name(s) | none |
| Minor planet category |
Cubewano (MPC)[2] ScatExt (DES)[3] |
| Epoch June 18, 2009 (2455000.5) | |
| Aphelion | 47.858 AU (7159.4 Gm) |
| Perihelion | 36.004 AU (5386.1 Gm) |
| Semi-major axis | 41.931 AU (6272.7 Gm) |
| Eccentricity | 0.14135 |
| Orbital period | 271.53 yr |
| Average orbital speed | 4.58 km/s |
| Mean anomaly | 210.108° |
| Inclination | 17.693° |
| Longitude of ascending node | 216.086° |
| Argument of perihelion | 213.200° |
|
Physical characteristics
|
|
| Dimensions | 934 ± 47 km[5] 726 ± 123 km[6] |
| Albedo | 0.084+.03 −.02[6] 0.051+.036 −.022[5] |
| Temperature | ~43 K |
| Spectral type | B-V=0.69; V-R=0.38[7] |
| Apparent magnitude | 20.6[8] |
| Absolute magnitude (H) | 3.79[4] |
(307261) 2002 MS4 is a trans-Neptunian object (TNO). It was discovered in 2002 by Chad Trujillo and Michael E. Brown. It is classified as a cubewano by the Minor Planet Center.[2]
Mike Brown's website lists it as highly likely a dwarf planet.[9] The Spitzer Space Telescope has estimated it to have a diameter of 726 ± 123 km.[6] The Herschel team estimates it to be 934 ± 47 km, which would make it one of the 10 largest TNOs currently known.[5] It is currently 47.2 AU from the Sun,[8] and will come to perihelion around 2122.[4]
It has been observed 46 times with precovery images back to 1954.[4]
|
||||||||||||||||||||
|
||||||||||||||||||||||
|
||||||||
| This article about a centaur (minor planet) or trans-Neptunian object is a stub. You can help Wikipedia by expanding it. |
This entry is from Wikipedia, the leading user-contributed encyclopedia. It may not have been reviewed by professional editors (see full disclaimer)