 Since 1994 more than 10 members of this family have been identified, with semi-major axes between 2.50–2.82  AU and inclinations of 33–38°.The validity of the family was confirmed in 2002 by a comparison of their spectra.Pallas has been observed occulting stars several times, including the best-observed of all asteroid occultation events, by 140 observers on 29 May 1983.