165 Loreley
From Wikipedia, the free encyclopedia
Orbital characteristics 1 | |
---|---|
Orbit type | Main belt |
Semimajor axis | 3.128 AU |
Perihelion distance | 2.870 AU |
Aphelion distance | 3.385 AU |
Orbital period | 5.53 years |
Inclination | 11.24° |
Eccentricity | 0.082 |
Physical characteristics 1 | |
Diameter | 155.2 km |
Rotation period | 7.226 hours |
Spectral class 5 | CD |
Abs. magnitude | 7.65 |
Albedo 4 | 0.078 |
History 2 | |
Discoverer | C. H. F. Peters, 1876 |
165 Loreley is a very large Main belt asteroid.
It was discovered by C. H. F. Peters on August 9, 1876 in Clinton, New York and named after the Lorelei, a figure in German folklore.
In the late 1990s, a network of astronomers worldwide gathered lightcurve data that was ultimately used to derive the spin states and shape models of 10 new asteroids, including (165) Loreley. [1][2]
One stellar occultation by Loreley has been observed, on July 20, 2003.
|
[edit] References
- ^ Durech., J.; Kaasalainen, M., Marciniak, A.; et al., “Physical models of ten asteroids from an observers' collaboration network,” Astronomy and Astrophysics , Volume 465, Issue 1, April I 2007, pp. 331-337
- ^ Durech, J.; Kaasalainen, M.; Marciniak, A.; Allen, W. H. et al. “Asteroid brightness and geometry,” Astronomy and Astrophysics, Volume 465, Issue 1, April I 2007, pp. 331-337.