311 Claudia
A three-dimensional model of 311 Claudia based on its light curve. | |
Discovery | |
---|---|
Discovered by | Auguste Charlois |
Discovery date | 11 June 1891 |
Designations | |
Main belt (Koronis) | |
Orbital characteristics[1] | |
Epoch 31 July 2016 (JD 2457600.5) | |
Uncertainty parameter 0 | |
Observation arc | 113.31 yr (41387 d) |
Aphelion | 2.90489 AU (434.565 Gm) |
Perihelion | 2.89097 AU (432.483 Gm) |
2.89793 AU (433.524 Gm) | |
Eccentricity | 0.0024026 |
4.93 yr (1801.9 d) | |
Average orbital speed | 17.5 km/s |
260.154° | |
0° 11m 59.24s / day | |
Inclination | 3.22695° |
81.0114° | |
51.4007° | |
Earth MOID | 1.88669 AU (282.245 Gm) |
Jupiter MOID | 2.05832 AU (307.920 Gm) |
Jupiter Tisserand parameter | 3.286 |
Physical characteristics | |
Dimensions | ±1.8 km 24.05 |
Mass | unknown |
Mean density | unknown |
Equatorial surface gravity | unknown |
Equatorial escape velocity | unknown |
7.532 h (0.3138 d) | |
±0.057 0.3381 | |
Temperature | unknown |
unknown | |
10.0 | |
|
311 Claudia is a typical Main belt asteroid.
It was discovered by Auguste Charlois on June 11, 1891 in Nice.[2] The name was suggested to Charlois by the amateur astronomer Arthur Mee of Cardiff, Wales, to commemorate Mee's wife, Claudia.[3]
311 Claudia is one of the Koronis family of asteroids. A group of astronomers, including Lucy D’Escoffier Crespo da Silva and Richard P. Binzel, used observations made between 1998 through 2000 to determine the spin-vector alignment of these asteroids. The collaborative work resulted in the creation of 61 new individual rotation lightcurves to augment previous published observations.[4]
References
- ↑ "311 Claudia". JPL Small-Body Database. NASA/Jet Propulsion Laboratory. Retrieved 11 May 2016.
- ↑ Schmadel Lutz D. Dictionary of Minor Planet Names (fifth edition), Springer, 2003. ISBN 3-540-00238-3.
- ↑ Mee, Arthur B. P. (2 April 1910), "Astronomical Notes", Weekly Mail, p. 11, retrieved 2013-08-25
- ↑ Slivan, S. M., Binzel, R. P., Crespo da Silva, L. D., Kaasalainen, M., Lyndaker, M. M., Krco, M.: “Spin vectors in the Koronis family: comprehensive results from two independent analyses of 213 rotation lightcurves,”Icarus, 162, 2003, pp. 285-307.
External links
This article is issued from Wikipedia - version of the 9/10/2016. The text is available under the Creative Commons Attribution/Share Alike but additional terms may apply for the media files.