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This work reports high quality NIR spectra, and their respectiveinterpretations, for eight Vp type asteroids, as defined by Carvano et al.(2010), that were observed at the NASA Infrared Telescope Facility on January14, 2013 UT. They include (3867) Shiretoko, (5235) Jean-Loup, (5560) Amytis,(6331) 1992 FZ1, (6976) Kanatsu, (17469) 1991 BT, (29796) 1999 CW77, and(30872) 1992 EM17. All eight asteroids exhibit the broad 0.9 and 1.9 micronmineral absorption features indicative of pyroxene on each asteroid's surface.Data reduction and analysis via multiple techniques produced consistent resultsfor the derived spectral absorption band centers and average pyroxene surfacechemistries for all eight asteroids (Reddy et al., 2012; Lindsay et al.,2013,2014; Gaffey et al., 2002; Burbine et al., 2009). (3867) Shiretoko is mostconsistent with the eucrite meteorites while the remaining seven asteroids aremost consistent with the howardite meteorites. The existing evidence suggeststhat all eight of these Vp type asteroids are genetic Vestoids that probablyoriginated from Vesta's surface.

More chips off of Asteroid (4) Vesta: characterization of eight Vestoids and their HED meteorite analogs