The Transport of Extrusive Volcanic Deposits on Jezero Crater Through Paleofluvial Processes
Antonio Paris, Kate Morgan, Evan Davies

TL;DR
This study investigates how volcanic deposits in Jezero Crater on Mars were transported by ancient river processes, using analogs from the Moenkopi Plateau to interpret rover imagery and geological history.
Contribution
It introduces a comparative analysis between Martian volcanic deposits and terrestrial analogs to elucidate their transport mechanisms via paleofluvial processes.
Findings
Vesicular rocks likely transported by ancient fluvial activity.
Analogous deposits on Moenkopi Plateau support fluvial transport hypothesis.
Martian volcanic deposits show geomorphic features consistent with water-mediated movement.
Abstract
Jezero, an impact crater in the Syrtis Major quadrangle of Mars, is generally thought to have amassed a large body of liquid water in its ancient past. NASA spectra of the proposed paleolake interpret the youngest surface unit as olivine-bearing minerals crystallized from magma. In early 2021, the Perseverance rover landed at the leading edge of a fan-delta deposit northwest of Jezero, an area argued to have experienced two distinct periods of fluvial activity. Surface imagery obtained by Perseverance reveal partially buried and unburied vesicular and non-vesicular rocks that appear volcanic in origin, emplaced sometime during the Noachian-Hesperian boundary. The absence of volcanic extrusive features along the fan-delta deposit, however, have made the origin of these ballast deposits a matter of contention among planetary scientists. To establish the origin of these basalt-like rocks,…
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Taxonomy
TopicsPlanetary Science and Exploration · Astro and Planetary Science · Space Science and Extraterrestrial Life
