Gale before Curiosity: What we knew and what the rover may reveal

Sep 26, 2012

The first comprehensive analysis of what we knew about the Gale crater on Mars before the recent landing of space rover Curiosity has been published by the International Journal of Astrobiology (IJA).

In a paper commissioned by the journal, which is published by Cambridge University Press, James Wray from the School of Earth and Atmospheric Sciences at Georgia Tech, and a collaborator on the Curiosity Science Team, explores what we already know, or hypothesize, and looks at the questions we hope Curiosity can answer.

Existing studies of Gale have tended to concentrate on a specific type of data (e.g. features revealed by high-resolution images) and/or a specific feature of the crater (e.g. its sand dunes). Wray takes findings from all available studies to create the first complete overview of the crater's history prior to Curiosity's investigations.

The Mars rover Curiosity landed safely on August 6th in Gale crater, a 150 km-wide impact scar near the . Rising up from this crater's floor is a mountain of 5 km high (Aeolis Mons or ), which has intrigued scientists for decades.

As well as reviewing information based on orbital remote sensing prior to the landing, Wray outlines how Curiosity's exploration can answer our most pressing questions: was Gale ever filled by a lake, or were all its sediments laid down in dry environments? When water did flow, what was its temperature and chemistry, and what do these imply about the of Gale 3.5 billion years ago?

The orbital observations reviewed by Wray suggest that both dry and wet environments are recorded in Gale's thick . They provide a vital broader context for Curiosity's explorations, which will cover only a small fraction of Gale crater throughout the rover's life.

James Wray said: "From the stunning images and first-of-its-kind already coming back from Curiosity, we know that Gale crater will astound and perplex us for years to come. As we explore our new geologic playground, our roving will be guided by the orbital observations and key questions that led us there."

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