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Ganges Cavus.pdf

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🔗 Source: hou.usra.edu

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📄 Pages: 2 pages

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Summary

Martian impact craters exhibit considerable depth variation and are generally shallower than their lunar or mercurian counterparts due to higher erosion rates on Mars. However, some craters on Mars are anomalously deep for their diameters, suggesting alternative formation processes such as magmatic or groundwater release. A database of Martian impact crater properties reveals craters with high depth/diameter ratios, including Ganges Cavus and an unnamed collapse feature in Arabia Terra, which are likely not impact craters but rather collapse features. The origins of these features are unclear, with hypotheses including groundwater release or magmatism, but the timing and volumes involved are uncertain, leaving outstanding questions about their formation processes.

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Description

Martian impact craters exhibit considerable depth variation and are generally shallower than their lunar or mercurian counterparts due to higher erosion rates...

Technical Information

File Format: PDF
File Size: 654 KB
Pages: 2
Language: EN
Total Downloads: 233
Last Updated: 3 weeks ago

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