Evaporation Pathways and Solubility of Fe-Ca-Mg-Rich Salts in Acid Sulfate Waters. A Model for Martian Ancient Surface Waters

Details Evaporation Pathways and Solubility of Fe-Ca-Mg-Rich Salts in Acid Sulfate Waters. A Model for Martian Ancient Surface Waters Evaporation Pathways and Solubility of Fe-Ca-Mg-Rich Salts in Acid Sulfate Waters. A Model for Martian Ancient Surface Waters

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012lpi....43.2862s&link_type=abstract

43rd Lunar and Planetary Science Conference, held March 19–23, 2012 at The Woodlands, Texas. LPI Contribution No. 1659, id.2862

Physics

Scientific paper

In this work we have characterized a layered deposit formed from the
evaporation of stream water from Rio Tinto, Spain, a relevant Mars
analog site. The minerals detected in-situ, confirmed later via high
resolution Raman spectroscopy.

Affiliated with

Also associated with

No associations

Rating

Evaporation Pathways and Solubility of Fe-Ca-Mg-Rich Salts in Acid Sulfate Waters. A Model for Martian Ancient Surface Waters 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 Evaporation Pathways and Solubility of Fe-Ca-Mg-Rich Salts in Acid Sulfate Waters. A Model for Martian Ancient Surface Waters, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Evaporation Pathways and Solubility of Fe-Ca-Mg-Rich Salts in Acid Sulfate Waters. A Model for Martian Ancient Surface Waters will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1049373