Implications of infrared reflectance spectroscopy of CM/CI carbonaceous chondrites for outer Main Belt asteroids

Details Implications of infrared reflectance spectroscopy of CM/CI carbonaceous chondrites for outer Main Belt asteroids Implications of infrared reflectance spectroscopy of CM/CI carbonaceous chondrites for outer Main Belt asteroids

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf..529t&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.529

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We present infrared reflectance spectra of CM/CI carbonaceous chondrites. The spectra are measured under dry conditions in order to remove adsorbed terrestrial water molecules. Spectra of CM/CI carbonaceous chondrites are used to correlate the spectral properties of the 3-μm absorption band with petrological and geochemical indicators of aqueous alteration. This correlation is crucial for interpreting telescopic spectra of outer Main Belt asteroids, especially in the 2.5 < a < 3.0 AU region.

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