(87269) 2000 OO67
From Wikipedia, the free encyclopedia
|
Discovery
|
|
|---|---|
| Discovered by | Cerro Tololo telescope |
| Discovery date | July 29, 2000 |
|
Designations
|
|
| Alternate name(s) | none |
| Minor planet category |
TNO Centaur[1] |
| Epoch December 31, 2006 (JD 2454100.5) | |
| Aphelion | 1068.199 AU 159,800.258 Gm |
| Perihelion | 20.766 AU 3,106.523 Gm |
| Semi-major axis | 544.482 AU 81,453.391 Gm |
| Eccentricity | 0.962 |
| Orbital period | 4,640,599.188 d (12,705.27 yr) |
| Average orbital speed | 0.88 km/s |
| Mean anomaly | 0.049° |
| Inclination | 20.071° |
| Longitude of ascending node | 142.315° |
| Argument of perihelion | 212.314° |
|
Physical characteristics
|
|
| Dimensions | 28-87 km |
| Temperature | ~12 K |
| Absolute magnitude (H) | 9.13 |
(87269) 2000 OO67 (also written (87269) 2000 OO67) is a small trans-Neptunian object (TNO) discovered by Deep Ecliptic Survey in 2000. It is remarkable for its highly eccentric orbit. At aphelion it is over 1,000 AU from the Sun and, with a perihelion of 21 AU, almost crosses the orbit of Uranus at closest approach. Some astronomers list it as a centaur.[1][2]
2000 OO67 came to perihelion in April 2005.[1][3][4]
Both 2000 OO67 and 2006 SQ372 take longer than Sedna to orbit the Sun using either heliocentric coordinates or barycentric coordinates.
[edit] See also
[edit] References
- ^ a b c Marc W. Buie (2006-07-25 using 33 of 34 obs). "Orbit Fit and Astrometric record for 87269". Deep Ecliptic Survey. http://www.boulder.swri.edu/~buie/kbo/astrom/87269.html. Retrieved 2008-05-18.
- ^ Structure and Dynamics of the Centaur Population: Constraints on the Origin of Short-Period Comets
- ^ Yeomans, Donald K.. "Horizons Online Ephemeris System". California Institute of Technology, Jet Propulsion Laboratory. http://ssd.jpl.nasa.gov/horizons.cgi?find_body=1&body_group=sb&sstr=2000OO67. Retrieved 2008-01-25.
- ^ "JPL Small-Body Database Browser: 87269 (2000 OO67)". 2006-07-25 last obs. http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=87269. Retrieved 2008-05-18.
[edit] External links
- Orbital simulation from JPL (Java) / Ephemeris
- List Of Centaurs and Scattered-Disk Objects at the Minor Planet Center
|
|||||
|
||||||||||||||||||||||
|
||||||||
| This article about a centaur (minor planet) or trans-Neptunian object is a stub. You can help Wikipedia by expanding it. |