575 Renate
575 Renate is a minor planet orbiting the Sun which was discovered by German astronomer Max Wolf on September 19, 1905.
Photometric observations at the Palmer Divide Observatory in Colorado Springs, Colorado in 1999 were used to build a light curve for this object. The asteroid displayed a rotation period of 3.676 ± 0.002 hours and a brightness variation of 0.15 ± 0.01 in magnitude.[2]
This is a member of the dynamic Maria family of asteroids that most likely formed as the result of a collisional breakup of a parent body.[3]
References
- ↑ Yeomans, Donald K., "575 Renate", JPL Small-Body Database Browser (NASA Jet Propulsion Laboratory), retrieved 2013-03-30.
- 1 2 Warner, Brian D. (January 2011), "Upon Further Review: IV. An Examination of Previous Lightcurve Analysis from the Palmer Divide Observatory", Bulletin of the Minor Planets Section of the Association of Lunar and Planetary Observers 38 (1), pp. 52–54, Bibcode:2011MPBu...38...52W.
- ↑ Veeder, G. J.; et al. (March 1995), "Eos, Koronis, and Maria family asteroids: Infrared (JHK) photometry", Icarus 114, pp. 186–196, Bibcode:1995Icar..114..186V, doi:10.1006/icar.1995.1053, CiteSeerX: 10.1.1.31.2739.
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