172 Baucis
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172 Baucis is a large main belt
asteroid An asteroid is a minor planet—an object larger than a meteoroid that is neither a planet nor an identified comet—that orbits within the Solar System#Inner Solar System, inner Solar System or is co-orbital with Jupiter (Trojan asteroids). As ...
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 In astronomy, a light curve is a graph (discrete mathematics), graph of the Radiance, light intensity of a celestial object or region as a function of time, typically with the magnitude (astronomy), magnitude of light received on the ''y''-axis ...
that indicated a slow synodic
rotation period In astronomy, the rotation period or spin period of a celestial object (e.g., star, planet, moon, asteroid) has two definitions. The first one corresponds to the '' sidereal rotation period'' (or ''sidereal day''), i.e., the time that the objec ...
of 27.417 ± 0.013 hours and a brightness variation of 0.25 in magnitude. Polarimetric study of this asteroid reveals anomalous properties that suggests the regolith consists of a mixture of low and high
albedo Albedo ( ; ) is the fraction of sunlight that is Diffuse reflection, diffusely reflected by a body. It is measured on a scale from 0 (corresponding to a black body that absorbs all incident radiation) to 1 (corresponding to a body that reflects ...
material. This may have been caused by fragmentation of an asteroid substrate with the spectral properties of CO3/CV3 carbonaceous chondrites.


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* * Background asteroids Baucis Baucis S-type asteroids (Tholen) L-type asteroids (SMASS) 18770205 {{S-beltasteroid-stub