Study of Two Structural Polymorphs of MgSO4.H2O by Raman, IR, XRD, and Humidity Buffer Experiments - Implication for Martian Kieserite

Details Study of Two Structural Polymorphs of MgSO4.H2O by Raman, IR, XRD, and Humidity Buffer Experiments - Implication for Martian Kieserite Study of Two Structural Polymorphs of MgSO4.H2O by Raman, IR, XRD, and Humidity Buffer Experiments - Implication for Martian Kieserite

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008lpi....39.2172w&link_type=abstract

39th Lunar and Planetary Science Conference, (Lunar and Planetary Science XXXIX), held March 10-14, 2008 in League City, Texas.

Physics

Scientific paper

Two structural polymorphs of MgSO4-H2O were
investigated by Raman, IR, and XRD. Their formation pathways and
stability fields provide important clues to understand the origin of
martian kieserite.

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