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| Discovery A | |
|---|---|
| Discoverer | Cerro Tololo telescope |
| Discovery date | July 29, 2000 |
| Alternate designations B |
none |
| Category | TNO |
| Orbital elements C | |
|
|
|
| Eccentricity (e) | 0.962 |
| Semi-major axis (a) | 81453.391 Gm (544.482 AU) |
| Perihelion (q) | 3106.523 Gm (20.766 AU) |
| Aphelion (Q) | 159800.258 Gm (1068.199 AU) |
| Orbital period (P) | 4640599.188 d (12705.27 a) |
| Mean orbital speed | 0.88 km/s |
| Inclination (i) | 20.071° |
| Longitude of the ascending node (Ω) |
142.315° |
| Argument of perihelion (ω) |
212.314° |
| Mean anomaly (M) | 0.049° |
| Physical characteristics D | |
| Dimensions | 28-87 km |
| Mass | 2.3-69×1016? kg |
| Density | 2.0? g/cm³ |
| Surface gravity | 0.0078-0.024? m/s² |
| Escape velocity | 0.015-0.046? km/s |
| Rotation period | ? d |
| Spectral class | ? |
| Absolute magnitude | 9.13 |
| Albedo (geometric) | 0.10? |
| Mean surface temperature |
~12 K |
(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, crosses the orbit of Neptune at closest approach. 2000 OO67 is probably composed of rock and ices. Some astronomers list it as a centaur. [1]
2000 OO67 came to perihelion in April 2005.[1][2][3]
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