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Encyclopedia > 158 Koronis
158 Koronis
Orbital characteristics 1 (ftp://ftp.lowell.edu/pub/elgb/astorb.html)
Orbit type Main belt (Koronis)
Semimajor axis 2.867 AU
Perihelion distance 2.705 AU
Aphelion distance 3.030 AU
Orbital period 4.86 years
Inclination 1.00°
Eccentricity 0.057
Physical characteristics 1 (ftp://ftp.lowell.edu/pub/elgb/astorb.html)
Diameter 35.4 km
Rotation period 14.218 hours
Spectral class S
Abs. magnitude 9.27
Albedo 4 (http://dorothy.as.arizona.edu/DSN/IRAS/index_iras.html) 0.277
History 2 (http://cfa-www.harvard.edu/iau/lists/NumberedMPs.html)
Discoverer V. Knorre, 1876


158 Koronis ("kuh ROE niss") is a Main belt asteroid. It has a rather mundane size but very reflective surface. It is composed of silicate rock and metallic iron-nickel.


It was discovered by Viktor Knorre on January 4, 1876 from the Berlin observatory. It was first of his total of four asteroid discoveries.


The asteroid itself may not be spectacular, but the family of asteroids named after it is one of the most important. One member of the family, 243 Ida, has been visited by spacecraft, and gives some idea how the other asteroids in the family may look.


Based on a model constructed from the lightcurve, the shape of Koronis resembles that of Ida, although it is a bit larger. [1] (http://www.astro.helsinki.fi/~kaselain/asteroids.html)



  Results from FactBites:
 
158 Koronis - Wikipedia, the free encyclopedia (182 words)
158 Koronis ("kuh ROE niss") is a Main belt asteroid.
One member of the family, 243 Ida, has been visited by spacecraft, and gives some idea of how the other asteroids in the family may look.
Based on a model constructed from the lightcurve, the shape of Koronis resembles that of Ida, although it is a bit larger [1].
asteroid (1791 words)
They include the Hungaria group, Flora family, Nysa-Polana family, Phocaea group, Koronis family, Eos family, Themis family, Cybele group, Alinda group, and Hilda group.
The three largest families (Eos, Koronis, and Themis) have been determined to be compositionally homogeneous.
If the asteroids belonging to them are considered to be fragments of a single parent body, then these parent bodies probably had diameters of 100 to 300 km.
  More results at FactBites »


 

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