Chaos, storms and climate on Mars
Edwin S. Kite (UC Berkeley), Scot C.R. Rafkin (SwRI Boulder), Timothy, Michaels (SwRI Boulder), William E. Dietrich (UC Berkeley), Michael Manga (UC, Berkeley)

TL;DR
This study models localized, lake-induced snowfall on Mars, showing it could create the observed channel networks without requiring higher global temperatures, thus challenging climate assumptions about past Martian habitability.
Contribution
It demonstrates that ephemeral lakeshore precipitation can form Martian channel networks without elevated global temperatures, using MRAMS simulations and snowpack modeling.
Findings
Precipitation correlates with channel network locations.
Localized snowmelt possible with modest warming and cloud cover.
Surface temperatures could stay similar to today during network formation.
Abstract
Channel networks on the plateau adjacent to Juventae Chasma have the highest drainage densities reported on Mars.We model frozen precipitation on the Juventae plateau,finding that the trigger for forming these channel networks could have been ephemeral lakeshore precipitation,and that they do not require past temperatures higher than today.If short-lived and localized events explain some dendritic channel networks on Mars, this would weaken the link between dendritic valley networks and surface climate conditions that could sustain life. Our analysis uses MRAMS simulations and HiRISE DTMs.We model localized weather systems driven by water vapor release from ephemeral lakes during outflow channel formation.At Juventae Chasma,mean snowfall reaches a maximum of 0.9mm/hr water equivalent on the SW rim of the chasm.Radiative effects of the thick cloud cover raise maximum (minimum, mean)…
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