In Situ Observation of Weathering Rinds at the Zhurong Landing Site, Mars

Abstract The Zhurong rover conducted in situ spectral investigations of southern Utopia Planitia, where the bedrock composition remains relatively unknown due to dust cover. Here we identify some spectrally distinct dark patches sporadically occurring on rocks by combining the Multispectral Camera and Short‐Wave Infrared data. These dark patches represent relatively dust‐free surfaces and exhibit concave‐up blue slopes in the near‐infrared not identified in that area from orbital data. This spectral signature is most consistent with silica‐enriched leached rinds on basaltic glass. The presence of such weathering rinds could imply leaching in an acidic aqueous environment of igneous rocks previously transported to the landing site as impact ejecta or pyroclastic deposits by explosive volcanism. In situ observations link the dark patches to the northern low‐albedo regions, suggesting that the surficial acidic weathering may be more widespread and occurred in the northern lowlands under Amazonian climatic conditions.

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Publication Details

Journal
Journal of Geophysical Research Planets
Published
2025-08-29
DOI
https://doi.org/10.1029/2025je009196
Primary Topic
Planetary Science and Exploration
Type
article
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article

In Situ Observation of Weathering Rinds at the Zhurong Landing Site, Mars

Jean‐Pierre Bibring, Maxime Pineau, Chunlai Li, F. Poulet et al.
Journal of Geophysical Research Planets
Planetary Science and Exploration
article

In Situ Observation of Weathering Rinds at the Zhurong Landing Site, Mars

Jean‐Pierre Bibring, Maxime Pineau, Chunlai Li, F. Poulet, Lin Guo, Zhaopeng Chen, M. Vincendon, Xin Ren, Qing Zhang, Bin Liu, Dawei Liu, John Carter, Jianjun Liu
article en

Abstract

Abstract The Zhurong rover conducted in situ spectral investigations of southern Utopia Planitia, where the bedrock composition remains relatively unknown due to dust cover. Here we identify some spectrally distinct dark patches sporadically occurring on rocks by combining the Multispectral Camera and Short‐Wave Infrared data. These dark patches represent relatively dust‐free surfaces and exhibit concave‐up blue slopes in the near‐infrared not identified in that area from orbital data. This spectral signature is most consistent with silica‐enriched leached rinds on basaltic glass. The presence of such weathering rinds could imply leaching in an acidic aqueous environment of igneous rocks previously transported to the landing site as impact ejecta or pyroclastic deposits by explosive volcanism. In situ observations link the dark patches to the northern low‐albedo regions, suggesting that the surficial acidic weathering may be more widespread and occurred in the northern lowlands under Amazonian climatic conditions.

Journal of Geophysical Research PlanetsVol. 130(9)
Centre National de la Recherche Scientifique (FR), Chinese Academy of Sciences (CN), Aix-Marseille Université (FR), Institut d'Astrophysique Spatiale (FR), National Space Science Center (CN), Centrale Méditerranée (FR), National Astronomical Observatories (CN), University of Chinese Academy of Sciences (CN)
Openalex Percentile: Top 84%
Planetary Science and Exploration
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