Capabilities of Gamma Ray and Neutron Spectrometers for Studying Trojan Asteroid Subsurface Ices

Details Capabilities of Gamma Ray and Neutron Spectrometers for Studying Trojan Asteroid Subsurface Ices Capabilities of Gamma Ray and Neutron Spectrometers for Studying Trojan Asteroid Subsurface Ices

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012lpi....43.2769p&link_type=abstract

43rd Lunar and Planetary Science Conference, held March 19–23, 2012 at The Woodlands, Texas. LPI Contribution No. 1659, id.2769

Computer Science

Scientific paper

We present computer simulation results for gamma ray and neutron
instruments located 50 km above a Trojan asteroid. Preliminary results
indicate that these instruments can detect buried ices that may indicate
a Kuiper Belt origin for the Trojans.

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