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Characterization of gypsum using vibrational spectroscopy and XRD from low to high temperature and applications to mars
Umeå University, Faculty of Science and Technology, Department of Chemistry. Carl Sagan Center, SETI Institute, Mountain View, CA 94043, USA; NASA Astrobiology Institute, USA.ORCID iD: 0000-0002-3830-7820
Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA; NASA Astrobiology Institute, USA.
Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA; NASA Astrobiology Institute, USA.
Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA; NASA Astrobiology Institute, USA.
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2022 (English)In: LPSC 2022: Program with links to abstracts, Lunar and Planetary Institute (LPI) Contributions , 2022, article id 2396Conference paper, Published paper (Other academic)
Abstract [en]

The Raman/VNIR/XRD measurements of gypsum from low to high temperatures in our study may enable coordinating orbit and rover analyses in Mars.
Place, publisher, year, edition, pages
Lunar and Planetary Institute (LPI) Contributions , 2022. article id 2396
National Category
Inorganic Chemistry Physical Chemistry Geochemistry Geosciences, Multidisciplinary
Research subject
Analytical Chemistry; Physical Chemistry
Identifiers
URN: urn:nbn:se:umu:diva-233192OAI: oai:DiVA.org:umu-233192DiVA, id: diva2:1923472
Conference
LPSC 2022, the 53th Lunar and Planetary Science Conference hybrid conference, March 7-11, 2022
Available from: 2024-12-25 Created: 2024-12-25 Last updated: 2025-01-03Bibliographically approved

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Yeşilbaş, Merve

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