Reflectance spectroscopy of cloudy pyroxenes from Millbillilli eucrite

Details Reflectance spectroscopy of cloudy pyroxenes from Millbillilli eucrite Reflectance spectroscopy of cloudy pyroxenes from Millbillilli eucrite

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf.1826m&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.1826

Physics

Scientific paper

We acquired reflectance spectra of a cloudy pyroxene separate from Millbillilli eucrite between 0.3 and 25 μm. Analysis of the spectra shows that opaque inclusions finely dispersed in eucritic pyroxenes affect near-infrared (NIR) spectral parameters, such as spectral slopes, band centers and band area ratios. The data may be useful for interpretation of spectral variations across the surface of 4 Vesta and for understanding the spectral diversity within the population of V-type asteroids.

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