Structure and Composition of the Surfaces of Trojan Asteroids from Reflection and Emission Spectroscopy

Details Structure and Composition of the Surfaces of Trojan Asteroids from Reflection and Emission Spectroscopy Structure and Composition of the Surfaces of Trojan Asteroids from Reflection and Emission Spectroscopy

Mar 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006lpi....37.2075e&link_type=abstract

37th Annual Lunar and Planetary Science Conference, March 13-17, 2006, League City, Texas, abstract no.2075

Computer Science

Scientific paper

Comparisons with spectral libraries are not able to completely explain
thermal emission spectra of several dark asteroids, including three
Trojans (from Spitzer). We suggest this is due to the surface structure,
and offer a couple of hypotheses.

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