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Encyclopedia > 144 Vibilia
144 Vibilia
Orbital characteristics 1 (ftp://ftp.lowell.edu/pub/elgb/astorb.html)
Orbit type Main belt (Vibilia)
Semimajor axis 2.655 AU
Perihelion distance 2.031 AU
Aphelion distance 3.278 AU
Orbital period 4.32 years
Inclination 4.81°
Eccentricity 0.235
Physical characteristics 1 (ftp://ftp.lowell.edu/pub/elgb/astorb.html)
Diameter 141.8 km
Rotation period 13.819 hours
Spectral class C
Abs. magnitude 7.91
Albedo 4 (http://dorothy.as.arizona.edu/DSN/IRAS/index_iras.html) 0.060
History 2 (http://cfa-www.harvard.edu/iau/lists/NumberedMPs.html)
Discoverer C. H. F. Peters, 1875


144 Vibilia is a dark, large Main belt asteroid and probably primitive in composition.


It is the only large member of the Vibilia asteroid family.


It was discovered by C. H. F. Peters on June 3, 1875 and named after Vibilia, a Roman goddess.


Vibilia has been observed to occult a star so far twice (in 1993 and again in 2001).

This article is a stub. You can help Wikipedia by expanding it (http://en.wikipedia.org/w/index.php?title=144_Vibilia&action=edit).



  Results from FactBites:
 
144 Vibilia - Definition, explanation (135 words)
144 Vibilia is a dark, large Main belt asteroid and probably primitive in composition.
Peters on June 3, 1875 and named after Vibilia, a Roman goddess.
Vibilia has been observed to occult a star twice so far (in 1993 and again in 2001).
144 Vibilia - Article from FactBug.org - the fast Wikipedia mirror site (102 words)
144 Vibilia is a dark, large Main belt asteroid and probably primitive in composition.
It is the only large member of the Vibilia asteroid family.
Vibilia has been observed to occult a star twice so far (in 1993 and again in 2001).
  More results at FactBites »


 
 

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