Voluminous Silica Precipitated from Martian Waters during Late-stage Aqueous Alteration
نویسندگان
چکیده
Mars' transition from an early "warm and wet" to the "cold dry" environment left fingerprints on geological record of fluvial activity Mars. The morphological mineralogical observations aqueous provided varying constraints condition duration liquid water martian surface. In this study, we surveyed mineralogy alluvial fans deltas investigated hydrated silica-bearing deposits associated with these landforms. Using CRISM data, identified 35 locations across Mars silica in proximity fan/deltas, where spectral characteristics are consistent immature or dehydrated opal-A. a few stepped find occurs within bulk fan form sedimentary layers correlated elevation, corroborating formation through precipitation. Meanwhile older fan/deltas mostly occur at distal relation primary is more complex. We propose that likely formed authigenically surface waters, mainly during Late Hesperian Early Amazonian [Hauber et al., 2013]. These could be tracer for temperature involved deposits, given precise detailed context, accessory minerals, concentration sediment-to-water ratio. Therefore, consider should among most critical samples investigate future missions, which accessible landing sites 2020 ExoMars missions.
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ژورنال
عنوان ژورنال: The planetary science journal
سال: 2021
ISSN: ['2632-3338']
DOI: https://doi.org/10.3847/psj/abe541