Evidence for geologically recent explosive volcanism in Elysium Planitia, Mars
David G. Horvath, Pranabendu Moitra, Christopher W. Hamilton, Robert, A. Craddock, Jeffrey C. Andrews-Hanna

TL;DR
This study presents evidence of the youngest volcanic deposit on Mars, suggesting recent volcanic activity in Elysium Planitia, which has implications for Mars's geological activity, potential habitability, and atmospheric methane sources.
Contribution
The paper provides the first detailed evidence of a pyroclastic deposit younger than 1 million years on Mars, indicating possible ongoing volcanic activity in Elysium Planitia.
Findings
Deposit is 53-210 ka old based on crater counting.
Deposit volume estimated at 1.1-2.8E7 cubic meters.
Evidence suggests potential recent volcanic activity on Mars.
Abstract
Volcanic activity on Mars peaked during the Noachian and Hesperian periods but has continued since then in isolated locales. Elysium Planitia hosts numerous young, fissure-fed flood lavas with ages ranging from approximately 500 to 2.5 million years (Ma). We present evidence for what may be the youngest volcanic deposit yet documented on Mars: a low albedo, high thermal inertia, high-calcium pyroxene-rich deposit distributed symmetrically around a segment of the Cerberus Fossae fissure system in Elysium Planitia. This deposit is similar to features interpreted as pyroclastic deposits on the Moon and Mercury. However, unlike previously documented lava flows in Elysium Planitia, this feature is morphologically consistent with a fissure-fed pyroclastic deposit, mantling the surrounding lava flows with a thickness on the order of tens of cm over most of the deposit and a volume of 1.1-2.8E7…
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