Near-infrared spectroscopy of 3:1 Kirkwood Gap Asteroids: (3760) Poutanen and (974) Lioba

Details Near-infrared spectroscopy of 3:1 Kirkwood Gap Asteroids: (3760) Poutanen and (974) Lioba Near-infrared spectroscopy of 3:1 Kirkwood Gap Asteroids: (3760) Poutanen and (974) Lioba

Aug 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011icar..214..645f&link_type=abstract

Icarus, Volume 214, Issue 2, p. 645-651.

Physics

1

Scientific paper

The current analysis identifies 3760 Poutanen as a
spinel-bearing asteroid. 3760 originated in a sub-region of the
formation zone of the CV3 meteorites. 974 Lioba is an S(IV)
asteroid with a silicate assemblage consisting of opx and ol. 974 is a plausible parent body of the LL-type OCs or possibly the L-type
OCs.

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