Spectral Reflectance Properties of HED Meteorites as a Function of Grain Size and Presence of CM2 Material

Details Spectral Reflectance Properties of HED Meteorites as a Function of Grain Size and Presence of CM2 Material Spectral Reflectance Properties of HED Meteorites as a Function of Grain Size and Presence of CM2 Material

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012lpi....43.1571c&link_type=abstract

43rd Lunar and Planetary Science Conference, held March 19–23, 2012 at The Woodlands, Texas. LPI Contribution No. 1659, id.1571

Physics

Scientific paper

The spectral reflectance properties of low-albedo areas on Vesta can be
attributed to either larger grain sizes of HED meteorites or the
presence of CM2-type chondrites. However, these two mechanisms lead to
differences in band depths vs. albedo.

Affiliated with

Also associated with

No associations

Rating

Spectral Reflectance Properties of HED Meteorites as a Function of Grain Size and Presence of CM2 Material does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Spectral Reflectance Properties of HED Meteorites as a Function of Grain Size and Presence of CM2 Material, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Spectral Reflectance Properties of HED Meteorites as a Function of Grain Size and Presence of CM2 Material will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1569338