Palagonitic Mars from Rock Rinds to Dust: Evidence from Visible, Near-IR,and Thermal Emission Spectra of Poorly Crystalline Materials

Details Palagonitic Mars from Rock Rinds to Dust: Evidence from Visible, Near-IR,and Thermal Emission Spectra of Poorly Crystalline Materials Palagonitic Mars from Rock Rinds to Dust: Evidence from Visible, Near-IR,and Thermal Emission Spectra of Poorly Crystalline Materials

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003lpi....34.1874m&link_type=abstract

34th Annual Lunar and Planetary Science Conference, March 17-21, 2003, League City, Texas, abstract no.1874

Physics

1

Scientific paper

Palagonitic alteration rinds developed on basaltic rocks are spectral
endmembers that provide a consistent explanation for both VNIR and TES
data of Martian dark regions.

Affiliated with

Also associated with

No associations

Rating

Palagonitic Mars from Rock Rinds to Dust: Evidence from Visible, Near-IR,and Thermal Emission Spectra of Poorly Crystalline Materials 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 Palagonitic Mars from Rock Rinds to Dust: Evidence from Visible, Near-IR,and Thermal Emission Spectra of Poorly Crystalline Materials, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Palagonitic Mars from Rock Rinds to Dust: Evidence from Visible, Near-IR,and Thermal Emission Spectra of Poorly Crystalline Materials will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1857452