44 Advancing Mineral Science and Exploring Planetary Surfaces: In Honor of MSA Dana Medalist, Elizabeth B. Rampe, Part II
This session honors MSA Dana Medalist Elizabeth B. Rampe, celebrating her contributions to Martian mineralogy and planetary science. We invite studies on in-situ and orbital planetary observations, lab/field data integration, and analog materials for extraterrestrial exploration.Sarah Simpson
Sunday, 19 October 2025
1:30 PM - 5:30 PM
HBGCC, 214C
Amazonian-aged Primary Evaporite Discovered by the Zhurong Rover in the Southern Utopia Planitia, Mars
Paper number: 44-7
Program: Technical Sessions
Time: 3:10 PM – 3:25 PM
Authors
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Wenyuan GaoNortheastern University, Shenyang
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Zhongchen WuShandong University, Weihai
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Changqing LiuShandong University, Weihai
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Honglei LinInstitute of Geology and Geophysics, Beijing
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Yu SunDeep Space Exploration Laboratory, Beijing
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Guochun ZhaoThe University of Hong Kong, Hong Kong
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Joseph MichalskiThe University of Hong Kong, Hong Kong
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Jim HeadBrown University, Providence, Rhode Island
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Xing WuNational Space Science Center, Chinese Academy of Sciences, Beijing
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Yang LiuNational Space Science Center, Chinese Academy of Sciences, Beijing
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Mei-Fu ZhouInstitute of Geochemistry, Guiyang
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Anthony Williams-JonesMcGill University, Montreal
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Xiao WangThe University of Hong Kong, Hong Kong
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Zongcheng LingShandong University, Weihai
Abstract
The Zhurong rover has identified a surface layer consisting of platy rocks enriched in hydrous minerals on a geologically young surface in southern Utopia Planitia, indicating unexpected recent aqueous activity on Mars. The exact composition of these hydrous minerals has remained uncertain, inhibiting our understanding of the aqueous processes and potential habitability on young Mars. In this study, we document unique crystal morphologies—such as radiating crystal clusters and fishtail twinning—characteristic of well-crystallized selenite, a distinctive variety of gypsum. This layer of gypsum selenite, interpreted as a primary evaporite unlike any previously identified sulfate deposits on Mars, points to the former presence of a body of surface water. While the findings could be consistent with evaporation from a hypothesized paleo-ocean in the northern lowlands, the Amazonian age and geologic context suggest a more plausible origin: melting of surface and ground ice, and groundwater upwelling driven by magmatic activity during the Amazonian period.
Geological Society of America Abstracts with Programs. Vol. 57, No. 6
doi: 10.1130/abs/2025AM-412262
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