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311 Claudia

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Main-belt asteroid

311 Claudia
A three-dimensional model of 311 Claudia based on its light curve
Discovery
Discovered byAuguste Charlois
Discovery date11 June 1891
Designations
MPC designation(311) Claudia
Pronunciation/ˈklaʊdiə/ KLOW-dee-ə
Minor planet categoryMain belt (Koronis)
Orbital characteristics
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)
Semi-major axis2.89793 AU (433.524 Gm)
Eccentricity0.0024026
Orbital period (sidereal)4.93 yr (1801.9 d)
Mean anomaly260.154°
Mean motion0° 11 59.24 / day
Inclination3.22695°
Longitude of ascending node81.0114°
Argument of perihelion51.4007°
Physical characteristics
Dimensions24.05±1.8 km
Synodic rotation period7.532 h (0.3138 d)
Geometric albedo0.3381±0.057
Absolute magnitude (H)10.0

311 Claudia is a typical Main belt asteroid.

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

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.

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.

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