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Themis family

The Themis family is a family of carbonaceous asteroids located in the outer portion of the asteroid belt, at a mean distance of 3.13 AU from the Sun. It is one of the largest families with over 4700 known members, and consists of a well-defined core of larger bodies surrounded by a region of smaller ones. The collisional Themis family is named after its parent body, the asteroid 24 Themis, discovered on 5 April 1853 by Italian astronomer Annibale de Gasparis.

Description
The Themis family is one of the largest and longest-recognized dynamical families of asteroids, and is made up of C-type asteroids with a composition believed to be similar to that of carbonaceous chondrites. To date, the Themis family comprises approximately 535 known asteroids. Asteroids in the Themis family share the following orbital elements: • semimajor axes between 3.08 AU and 3.24 AU • orbital eccentricities between 0.09 and 0.22 • orbital inclinations of less than 3° == List ==
List
Some of the largest members of this family include: • 24 Themis62 Erato90 Antiope104 Klymene171 Ophelia222 Lucia223 Rosa316 Goberta379 Huenna383 Janina468 Lina492 Gismonda515 Athalia526 Jena767 Bondia846 Lipperta == See also ==
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