237 Geomorphology and Surface Processes Across the Solar System
This session welcomes abstracts on any aspect of planetary geomorphology and surface processes, including but not restricted to: Earth analogues, laboratory experiments, numerical models, planetary comparison, mapping, in situ data, or remote sensing studies.
Wednesday, 22 October 2025
8:00 AM - 12:00 PM
HBGCC, 212AB
Curiosity’s Investigation of the Distinctive “Boxwork” Interval in Gale Crater, Mars
Paper number: 237-9
Program: Technical Sessions
Time: 10:15 AM – 10:30 AM
Authors
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Kirsten Siebach Presenting AuthorRice University, Earth, Environmental and Planetary Sciences, Houston, TX
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Christina SeegerCalifornia Institute of Technology, Pasadena, CA
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Claire MondroCalifornia Institute of Technology, Pasadena, CA
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Susanne SchwenzerThe Open University, Milton Keynes
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Catherine O'Connell-CooperUniversity of New Brunswick, New Brunswick
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Patrick GasdaLos Alamos National Laboratory, Los Alamos, NM
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Lucy ThompsonUniversity of New Brunswick, New Brunswick
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Gwénaël CaravacaUniversité de Toulouse, Toulouse
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Louis ScuderiUniversity of New Mexico, Corrales, NM
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Albert YenJet Propulsion Laboratory, Pasadena, CA
Abstract
The Mars Science Laboratory Curiosity rover is currently investigating a distinctive stratigraphic interval with meter-scale intersecting ridges in a boxwork pattern that is expressed at nearly the same elevation across 14 km of stratigraphy with about 100 m vertical relief. The orbital expression of the boxwork is striking, with ridges that extend up to ~5 meters across and 10-20-meter diameter hollows between ridges that are often filled with sediment. In the uppermost portions of the interval, where the boxwork are best defined, dark lines can be seen in the centers of the resistant ridges. This has led to the interpretation that these boxwork ridges were strengthened by groundwater alteration or fluid-deposited cements. The boxwork is hypothesized to have formed through: (1) deposition, (2) lithification, (3) fracturing of the host rock, which may be contemporaneous with (4) fluid flow through the fractures under sufficient pressure to cause the fluid to percolate into ~2-3 meters of rock on either side, creating a cementation or alteration zone around the fracture, and (5) preferential eolian erosion of weaker zones in the rock.
Curiosity’s traverse up Mount Sharp in Gale crater approached the easternmost edge of the mapped boxwork interval and crossed the contact from the Layered Sulfate unit (LSu) on sol 4534 (5/7/2025). The boxwork-containing rock has distinct texture and chemistry from the LSu: the bedrock is friable, weakly-laminated, fine-grained mudstone with relatively more Si and Al and less Mg and S. CheMin XRD at “Altadena” found phyllosilicates, which were largely absent from the surrounding LSu. The boxwork-containing interval may represent an unconformity-bound facies with the contact with LSu marking the vertical and potentially horizontal bounds. Further observations have shown that the boxwork-containing rock includes intervals of cross-bedded (likely fluvial) sandstone and some highly diagenetically overprinted nodular regions, which may or may not be associated with ridges. Ridges within the lower boxwork interval investigated to date are heavily fractured and shallow, without significant chemical differences, but images looking ahead to the upper portion of the boxwork interval show better definition. We plan to drill in the endmember ridge-forming material and a nearby hollow representing bedrock unaffected by the ridge-strengthening event to understand the fluid alteration interpreted to have generated the discrepancies in erosion-resistance within this interval.
Geological Society of America Abstracts with Programs. Vol. 57, No. 6
doi: 10.1130/abs/2025AM-414508
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