Identification of Mars gully activity types associated with ice composition
Mathieu Vincendon

TL;DR
This study investigates the role of CO2 and water ice in current Mars gully activity, revealing CO2 ice's key influence and suggesting multiple mechanisms behind ongoing erosion.
Contribution
It provides a detailed analysis of ice formation and sublimation at gully sites, highlighting CO2 ice's role and proposing additional water-related processes.
Findings
CO2 ice presence correlates with gully activity
Water ice likely contributes to some erosion processes
CO2 ice layers are very thin at low-latitude sites
Abstract
The detection of geologically recent channels at the end of the twentieth century rapidly suggested that liquid water could have been present on Mars up to recent times. A mechanism involving melting of water ice during ice ages in the last several million years progressively emerged during years following the first observations of these gullies. However, the recent discovery of current activity within gullies now suggests a paradigm shift where a contemporary CO2 ice-based and liquid water-free mechanism may form all gullies. Here we perform a survey of near-infrared observations and construct time sequences of water and CO2 ice formation and sublimation at active gully sites. We observe that all major new erosive features such as channel development or lengthening systematically occur where and, if applicable, when CO2 ice is observed or probable. CO2 ice layers are however estimated…
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