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词条 172 Baucis
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{{Infobox planet
| minorplanet= yes
| mpc_name= (172) Baucis
| background= #D6D6D6
| name= 172 Baucis
| pronounced={{IPAc-en|'|b|ɔː|s|ᵻ|s}}
| discoverer= A. Borrelly
| discovered= 5 February 1877
| mp_category= Main belt
| orbit_ref=
| semimajor= {{Convert|2.3799|AU|Gm|abbr=on}}
| perihelion= {{Convert|2.1073|AU|Gm|abbr=on}}
| aphelion= {{Convert|2.6525|AU|Gm|abbr=on|lk=on}}
| period= 3.67 yr (1341.0 d)
| inclination= 10.028°
| eccentricity= 0.11454
| rotation= {{Convert|27.417|h|d|abbr=on|lk=on}}[3]
| spectral_type= S
| abs_magnitude= 8.79
| albedo= {{val|0.1382|0.006}}
| epoch= 31 July 2016 (JD 2457600.5)
| asc_node= 331.98°
| arg_peri= 359.20°
| mean_anomaly= 175.49°
| mean_motion= {{Deg2DMS|0.26845|sup=ms}} / day
| observation_arc= 133.62 yr (48806 d)
| uncertainty= 0
| mean_radius= {{val|31.215|0.6}} km
| moid= {{Convert|1.09593|AU|Gm|abbr=on}}
| jupiter_moid= {{Convert|2.67257|AU|Gm|abbr=on}}
| tisserand= 3.510
}}

Baucis (minor planet designation: 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.[5]

References

1. ^{{Citation | last1 = Bembrick | first1 = C. S. | last2 = Richards | first2 = T. | last3 = Bolt | first3 = G. | last4 = Pereghy | first4 = B. | last5 = Higgins | first5 = D. | last6 = Allen | first6 = W. H. | display-authors = 1 | title = 172 Baucis - a slow rotator | work = The Minor Planet Bulletin | volume = 31 | issue = 3 | pages = 51–52 | bibcode = 2004MPBu...31...51B | postscript= .|date=September 2004}}
2. ^{{Citation | last1 = Gil-Hutton | first1 = R. | last2 = Mesa | first2 = V. | last3 = Cellino | first3 = A. | last4 = Bendjoya | first4 = P. | last5 = Peñaloza | first5 = L. | last6 = Lovos | first6 = F. | display-authors = 1 | title = New cases of unusual polarimetric behavior in asteroids | work = Astronomy and Astrophysics | volume = 482 | issue = 1 | pages = 309–314 | doi = 10.1051/0004-6361:20078965 | bibcode = 2008A&A...482..309G | postscript= .|date=April 2008}}
[1][2]

}}

External links

  • {{JPL small body}}
{{Minor planets navigator|171 Ophelia|number=172|173 Ino}}{{Small Solar System bodies}}{{DEFAULTSORT:000172}}{{S-beltasteroid-stub}}

7 : Background asteroids|Discoveries by Alphonse Borrelly|Minor planets named from Greek mythology|Named minor planets|S-type asteroids (Tholen)|L-type asteroids (SMASS)|Astronomical objects discovered in 1877

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