Eunomia family (of asteroids)
Location and structure of the Eunomia family.
The Eunomia family is a small family of S-type and C-type asteroids that orbit in the middle of the main asteroid belt at a mean distance from the Sun of 2.6 to 2.7 astronomical unis and a mean inclination of 12°. The prototype and largest member is 15 Eunomia, discovered in 1851 by Annibale de Gasparis (1819–1892) in Naples.
|Data for 15 Eunomia|
|semimajor axis||2.644 AU|