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Topic: Koronis family


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In the News (Sat 28 Nov 09)

  
 Koronis family (of asteroids)
A Hirayama family of asteroids in the outer part of the main asteroid belt orbiting at mean distances of 2.82 to 2.95 AU from the Sun.
Mainly of S-class (silicaceous), with similar colors and albedos, these objects are all believed to have originated in the breakup of a single, highly homogenous parent body, some 100 km in diameter.
The family is named after (158) Koronis, the first member to be found, in 1876 by the German astronomer Victor Knorre (1840-1919).
daviddarling.info /encyclopedia/K/Koronis_family.html   (184 words)

  
 Clark R. Chapman's Publications   (Site not responding. Last check: 2007-11-02)
The formation and collisional/dynamical evolution of the Ida/Dactyl system as part of the Koronis family.
Collisional history of asteroids: Evidence from Vesta and the Hirayama families.
Distributions of asteroid compositional types with solar distance, body diameter, and family membership (extended abstract).
www.boulder.swri.edu /clark/pub.html   (9684 words)

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