Jump to content

311 Claudia

From Wikipedia, the free encyclopedia

This is an old revision of this page, as edited by Tom.Reding (talk | contribs) at 22:42, 19 December 2023 (+{{Authority control}} (2 IDs from Wikidata); WP:GenFixes & cleanup on). The present address (URL) is a permanent link to this revision, which may differ significantly from the current revision.

311 Claudia
A three-dimensional model of 311 Claudia based on its light curve
Discovery
Discovered byAuguste Charlois
Discovery date11 June 1891
Designations
(311) Claudia
Pronunciation/ˈkldiə/[1]
Main belt (Koronis)
Orbital characteristics[2]
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc113.31 yr (41387 d)
Aphelion2.90489 AU (434.565 Gm)
Perihelion2.89097 AU (432.483 Gm)
2.89793 AU (433.524 Gm)
Eccentricity0.0024026
4.93 yr (1801.9 d)
260.154°
0° 11m 59.24s / day
Inclination3.22695°
81.0114°
51.4007°
Physical characteristics
Dimensions24.05±1.8 km
7.532 h (0.3138 d)
0.3381±0.057
10.0

Claudia (minor planet designation: 311 Claudia) is a typical Main belt asteroid.

It was discovered by Auguste Charlois on 11 June 1891 in Nice.[3] The name was suggested to Charlois by the amateur astronomer Arthur Mee of Cardiff, Wales, to commemorate Mee's wife, Claudia.[4]

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.[5]

References

  1. ^ Noah Webster (1884) A Practical Dictionary of the English Language
  2. ^ "311 Claudia". JPL Small-Body Database. NASA/Jet Propulsion Laboratory. Retrieved 11 May 2016.
  3. ^ Schmadel Lutz D. Dictionary of Minor Planet Names (fifth edition), Springer, 2003. ISBN 3-540-00238-3.
  4. ^ Mee, Arthur B. P. (2 April 1910), "Astronomical Notes", Weekly Mail, p. 11, retrieved 25 August 2013
  5. ^ 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.