Damocloid asteroid
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Damocloids are asteroids such as 5335 Damocles and 1996 PW that have long-period highly eccentric orbits typical of periodic comets such as 1P/Halley, but without showing a cometary coma or tail.
The object 2001 OG108 was thought to be a Damocloid, but as it approached perihelion it began to display cometary activity and was thus renamed Comet C/2001 OG108 (LONEOS).
They are believed to originate from the Oort cloud.
External link
- List of Damocloids (ftp://ftp.lowell.edu/pub/bas/damocloid)
| The minor planets |
| Vulcanoids | Main belt | Groups and families | Near-Earth objects | Jupiter Trojans |
| Centaurs | Trans-Neptunians | Damocloids | Comets | Kuiper belt | Oort cloud |
| (For other objects and regions, see: Binary asteroids, Asteroid moons and the Solar system) |
| (For a complete listing, see: List of asteroids. For pronunciation, see: Pronunciation of asteroid names.) |