Planetary Science Institute’s Post

A new paper published in Icarus describes, maps and dates how glaciers and glacial runoff sculpted the northeastern rim of Mars’ Hellas basin over the last 3 billion years. The paper was authored in part by PSI senior scientist Alan Howard and research scientist Alexander Morgan. Before the research began, the team was intrigued by the dramatic features in Hellas basin, especially in and around Batson crater, which they thought might hint at a history of decaying glaciers. Until now, these features had not yet been adequately described and characterized as being glacial. There are many ways glaciers leave their mark on a landscape. On Earth, glaciers primarily scour the underlying rock as they slowly flow downhill. But on Mars, with its weaker gravity, the physical processes leading to this behavior require thicker ice to achieve. So, the team argues that instead, during a time when Mars was warmer, it’s more likely that meltwater carved the landscape as it flowed beneath and out of glaciers. Learn more: https://buff.ly/46UTT72

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