Satellite image of the surface of Mars, with a 5-kilometer scale
Mawrth Vallis, imaged here by the Mars Express High Resolution Stereo Camera (HRSC), was one of the areas studied by scientists to identify carbonates on the surface of Mars. The scale bar is 5 kilometers. Credit: ESA/DLR/FU Berlin, CC BY-SA 3.0
Source: Journal of Geophysical Research: Planets

Was Mars warm and wet enough to support life during the planet’s first few hundred million years?

Scars of ancient lakes and rivers, as well as minerals that form only when water is present, have convinced many researchers that Mars was once conducive to life. But one type of alteration mineral, carbonate, has been conspicuously scarce in some studies, raising doubts about whether there was enough carbon dioxide vapor to warm Mars’s early atmosphere.

Carbonate minerals such as calcite—the key ingredient of marble, limestone, and seashells—are formed when water traps atmospheric carbon dioxide. The pale, translucent minerals have a distinct spectral signature, which remote sensing instruments located aboard the Mars Reconnaissance Orbiter can detect. The orbiter spotted carbonates before, but in 2017, the Curiosity rover found no evidence of carbonate minerals on Mars’s surface, confounding scientists.

Now a new study based on the orbiter’s remote sensing data presents fresh evidence of carbonates mixed among hydrated minerals across Mars’s surface. Bultel et al. searched for carbonates all over Mars in weathering profiles, vertical arrays of rock that span from a few centimeters to 100 meters thick. These profiles hold clues to what the climate was like on Mars in the past because they show how rocks have lost and gained soluble elements over time. On Mars, the profiles often resemble a layer cake, with clay minerals rich in aluminum on top, iron-rich clay in the middle, and magnesium-rich clay on the bottom.

Confirming previous remote sensing data, the team found widespread evidence of carbonates across Mars’s surface. The new study bolsters the hypothesis that there was liquid water on Mars’s surface until around 3.7 billion years ago and that fluids containing carbonic acid—carbon dioxide dissolved in water—weathered the planet’s surface. Although there are still many mysteries about Mars’s early environment, the study sheds new light on the period of the planet’s history when it is most likely life could have emerged. (Journal of Geophysical Research: Planets,, 2019)

—Emily Underwood, Freelance Writer


Underwood, E. (2019), Detecting carbonates on the surface of Mars, Eos, 100, Published on 16 May 2019.

Text © 2019. The authors. CC BY-NC-ND 3.0
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