Shape and Thermal Modeling of a Selection of M-Type Asteroids

Details Shape and Thermal Modeling of a Selection of M-Type Asteroids Shape and Thermal Modeling of a Selection of M-Type Asteroids

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012lpi....43.1425c&link_type=abstract

43rd Lunar and Planetary Science Conference, held March 19–23, 2012 at The Woodlands, Texas. LPI Contribution No. 1659, id.1425

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Scientific paper

We have determined the shape and thermally modeled six M-type asteroids
that, because of their spectral signatures or lack thereof, radar
albedos, and other thermal and physical properties, are likely
candidates for metallic core progeny.

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