Supplemental Material: Long-term and multi-stage ice accumulation in the martian mid-latitudes during the Amazonian

Trishit Ruj; et al.

doi:10.1130/geol.s.29824943.v1

August 4, 2025

Supplemental Material: Long-term and multi-stage ice accumulation in the martian mid-latitudes during the Amazonian

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Key Points

MAIN FINDING: Ice accumulation events occurred in the martian mid-latitudes during the Amazonian period.
KEY EVIDENCE: Crater count and size-frequency distribution support the timing of these ice accumulation events.
APPROACH: The study utilized thermal modeling and spatial distribution analyses of glacial features.
SIGNIFICANCE: Understanding these patterns provides insights into Mars' climatic history and potential for past water.

Implication

Analysis reveals ice accumulation events in martian mid-latitudes, highlighting their long-term climatic implications.

Abstract

File 1: Figures illustrating crater selection, deposit orientation measurement, thermal modeling, and spatial distribution of glacial features. File 2: Crater count regions and crater size-frequency distribution-based age plots supporting the timing of ice accumulation events.

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Cite This Study

Ruj et al. (2025) studied this question.

synapsesocial.com/papers/689a0f93e6551bb0af8d0ffc https://doi.org/10.1130/geol.s.29824943.v1

View Full Paper

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Supplemental Material: Long-term and multi-stage ice accumulation in the martian mid-latitudes during the Amazonian

Key Points

Implication

Abstract

Discussion

Cite This Study

Supplemental Material: Long-term and multi-stage ice accumulation in the martian mid-latitudes during the Amazonian

Key Points

Implication

Abstract

Discussion

Cite This Study

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