Constraining Meteorite Analogs for the Eos Dynamical Family via Mineralogical Band Analysis

Details Constraining Meteorite Analogs for the Eos Dynamical Family via Mineralogical Band Analysis Constraining Meteorite Analogs for the Eos Dynamical Family via Mineralogical Band Analysis

Mar 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011lpi....42.2184h&link_type=abstract

42nd Lunar and Planetary Science Conference, held March 7–11, 2011 at The Woodlands, Texas. LPI Contribution No. 1608, p.2184

Physics

Scientific paper

The Eos dynamical family displays weak near-infrared Band I and Band II
spectral absorptions that suggest the surface presence of olivine
± pyroxene. Band analysis will be undertaken to constrain the
possible meteorite analogs for the Eos family.

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