TheJuno clump is a probablemain-beltasteroid family that share similar orbital elements to3 Juno.

3 Juno is a large asteroid with amean diameter of about 235 km, but the remaining bodies are all small.(32326) 2000 QO62, the brightest of those clearly in the visible clump would have a diameter of about 6 km, given the same albedo as3 Juno. This indicates that it is probably a so-called cratering family composed of ejecta from impacts on 3 Juno.

The HCM analysis by (Zappalà 1995) determined several likely core members, whose proper elements lie in the approximate ranges

At the presentepoch, the range ofosculatingorbital elements of these core members is

• Zappalà, Vincenzo; Bendjoya, Philippe; Cellino, Alberto;Farinella, Paolo; and Froeschlé, Claude;Asteroid Families: Search of a 12,487-Asteroid Sample Using Two Different Clustering Techniques, Icarus, Volume 116, Issue 2 (August 1995), pages 291–314doi:10.1006/icar.1995.1127

• Juno asteroids
• Asteroid groups and families