Circumpolar ocean stability on Mars 3 Gy ago
Schmidt F., Way M. J., Costard F., Bouley S., S\'ejourn\'e A., Aleinov, I

TL;DR
This study uses advanced climate simulations to propose that Mars 3 billion years ago could have had a cold, icy, yet wet climate with a stable ocean, reconciling geological evidence of shoreline and tsunami deposits.
Contribution
The paper introduces a novel climate model scenario showing Mars could sustain a cold, wet environment with a stable ocean, supported by geological and simulation data.
Findings
Mars could have had a cold, wet climate with a stable ocean.
Ice sheets and glaciers existed in the southern highlands.
Geological features are consistent with this climate scenario.
Abstract
What was the nature of the Late Hesperian climate? Warm and wet or cold and dry? Formulated this way the question leads to an apparent paradox since both options seem implausible. A warm and wet climate would have produced extensive fluvial erosion but few valley networks have been observed at the age of the late Hesperian. A too cold climate would have kept any northern ocean frozen most of the time. A moderate cold climate would have transferred the water from the ocean to the land in the form of snow and ice. But this would prevent tsunami formation, for which there is some evidence. Here, we provide new insights from numerical climate simulations in agreement with surface geological features to demonstrate that the Martian climate could have been both cold and wet. Using an advanced General Circulation Model (GCM), we demonstrate that an ocean can be stable, even if the Martian mean…
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