Discovery | |
---|---|
Discovered by | A. Borrelly |
Discovery date | 5 February 1877 |
Designations | |
(172) Baucis | |
Pronunciation | /ˈbɔːsɪs/[1] |
Named after | Baucis |
A877 CA; 1921 EE | |
Main belt | |
Orbital characteristics[2] | |
Epoch 31 July 2016 (JD 2457600.5) | |
Uncertainty parameter 0 | |
Observation arc | 133.62 yr (48806 d) |
Aphelion | 2.6525 AU (396.81 Gm) |
Perihelion | 2.1073 AU (315.25 Gm) |
2.3799 AU (356.03 Gm) | |
Eccentricity | 0.11454 |
3.67 yr (1341.0 d) | |
175.49° | |
0° 16m 6.42s / day | |
Inclination | 10.028° |
331.98° | |
359.20° | |
Earth MOID | 1.09593 AU (163.949 Gm) |
Jupiter MOID | 2.67257 AU (399.811 Gm) |
TJupiter | 3.510 |
Physical characteristics | |
31.215±0.6 km | |
27.417 h (1.1424 d)[2][3] | |
0.1382±0.006 | |
S | |
8.79 | |
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.[3]
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.[4]
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