144 Vibilia
Encyclopedia : 1 : 14 : 144 : 144 Vibilia
| Orbital characteristics [1] | |
|---|---|
| Orbit type | Main belt (Vibilia) |
| Semimajor axis | 2.655 AU |
| Perihelion distance | 2.031 AU |
| Aphelion distance | 3.278 AU |
| Orbital period | 4.32 years |
| Inclination | 4.81° |
| Eccentricity | 0.235 |
| Physical characteristics [1] | |
| Diameter | 141.8 km |
| Rotation period | 13.819 hours |
| Spectral class | C |
| Abs. magnitude | 7.91 |
| Albedo [4] | 0.060 |
| History [2] | |
| Discoverer | C. H. F. Peters, 1875 |
144 Vibilia is a dark, large Main belt asteroid and probably primitive in composition.
It is the only large member of the Vibilia asteroid family.
It was discovered by C. H. F. Peters on June 3, 1875 in Clinton, New York and named after Vibilia, a Roman goddess.
Vibilia has been observed to occult a star twice so far (in 1993 and again in 2001).
… | Previous minor planet | | Next minor planet | …
| The minor planets |
|---|
| Vulcanoids | Near-Earth asteroids | Main belt | Jupiter Trojans | Centaurs | Damocloids | Comets | Trans-Neptunians (Kuiper belt · Scattered disc · Oort cloud) |
| For other objects and regions, see: , , asteroid moons and the Solar system For a complete listing, see: List of asteroids. See also Pronunciation of asteroid names and Meanings of asteroid names. |
From Wikipedia, the Free Encyclopedia. Original article here. Support Wikipedia by contributing or donating.
All text is available under the terms of the GNU Free Documentation License See Wikipedia Copyrights for details.
