(418993) 2009 MS9
Minor planet roughly 30–60 km in diameter
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(418993) 2009 MS9, provisionally known as 2009 MS9, is a centaur roughly 30â60 km in diameter. It has a highly inclined orbit and a barycentric semi-major axis (average distance from the Sun) of ~353 AU.[a]
| Discovery[1][2] | |
|---|---|
| Discovered by | CFHT (568) |
| Discovery date | 25 June 2009 |
| Designations | |
| (418993) 2009 MS9 | |
| Centaur (DES)[3] | |
| Orbital characteristics[4] | |
| Epoch 13 January 2016 (JD 2457400.5) | |
| Uncertainty parameter 2 | |
| Observation arc | 2352 days (6.44 yr) |
| Aphelion | 696 AU (barycentric 2050)[a] 684 AU |
| Perihelion | 11.002 AU (1.6459 Tm) |
| 353 AU (barycentric 2050)[a] 347.6 AU | |
| Eccentricity | 0.96835 |
| 6481.05 yr (2367202 d) | |
| 0.16189° | |
| 0° 0m 0.547s / day | |
| Inclination | 68.056° |
| 220.226° | |
| 128.675° | |
| Physical characteristics | |
| Dimensions | 30â60 km[5] |
| 21[6] | |
| 9.9[4] | |
2009 MS9 has a well determined orbit and has been assigned a minor planet number. Objects such 2009 MS9 may be the origin of Halley-type comets.[2]
It came to perihelion in February 2013 at a distance of 11 AU from the Sun (outside the orbit of Saturn).[4] As of 2016[update], it is 12 AU from the Sun.[6]
It will not be 50 AU from the Sun until 2047. After leaving the planetary region of the Solar System, 2009 MS9 will have a barycentric aphelion of 696 AU with an orbital period of 6640 years.
In a 10 million year integration of the orbit, the nominal (best-fit) orbit and both 3-sigma clones remain outside 8.3AU (qmin) from the Sun.[3]
| Orbital evolution | |||||||
| Epoch | Barycentric Aphelion (Q) (AU) | Orbital period yr | |||||
|---|---|---|---|---|---|---|---|
| 1950 | 694 | 6610 | |||||
| 2050 | 696 | 6640 | |||||
Notes
- Given the orbital eccentricity of this object, different epochs can generate quite different heliocentric unperturbed two-body best-fit solutions to the semi-major axis and orbital period. For objects at such high eccentricity, the Sun's barycentric coordinates are more stable than heliocentric coordinates. Using JPL Horizons, the barycentric semi-major axis is approximately 353 AU.[7]