172 Baucis is a large main belt asteroid that was discovered by French astronomer Alphonse Borrelly on February 5, 1877 and named after a fictional character in the Greek legend of Baucis and Philemon. The adjectival form of the name is Baucidian. It is classified as an S-type asteroid based upon its spectrum.
Photometric observations of this asteroid from the southern hemisphere during 2003 gave a light curve that indicated a slow synodic rotation period of 27.417 ± 0.013 hours and a brightness variation of 0.25 in magnitude. [2 ]
Polarimetric study of this asteroid reveals anomalous properties that suggests the regolith consists of a mixture of low and high albedo material. This may have been caused by fragmentation of an asteroid substrate with the spectral properties of CO3/CV3 carbonaceous chondrites. [3 ]
References [ edit ]
^ Yeomans, Donald K., , 172 Baucis JPL Small-Body Database Browser (NASA Jet Propulsion Laboratory) , retrieved 2013-03-30.
^ a b Bembrick, C. S. et al. (September 2004), 172 Baucis - a slow rotator, Bulletin of the Minor Planets Section of the Association of Lunar and Planetary Observers 31 (3): 51–52, Bibcode: 2004MPBu...31...51B.
^ Gil-Hutton, R. et al. (April 2008), New cases of unusual polarimetric behavior in asteroids, Astronomy and Astrophysics 482 (1): 309–314, Bibcode: 2008A&A...482..309G, doi: 10.1051/0004-6361:20078965.