Caitlin Stier, contributor
(Image: NASA/JPL-Caltech/Univ. of Arizona)
Carbonate minerals buried beneath the Martian surface could help explain the disappearance of carbon dioxide from Mars's atmosphere.
A thin, CO2-dominated atmosphere surrounds Mars today. But in the past, it was likely much thicker, allowing liquid water to remain stable on the planet's surface. Where did that carbon dioxide go?
It may have gone towards forming carbonate minerals, which on Earth arise when oceans absorb carbon dioxide from the atmosphere and deposit it as carbonate rock. A similar process involving liquid water may have happened on ancient Mars.
A mineral-mapping instrument aboard NASA's Mars Reconnaissance Orbiter has spotted the minerals (shown in lighter shades) in rocks that had once been buried beneath the planet's surface but were later brought to the surface by impacts. A crater on the raised rim of an even larger, 470-metre-wide crater called Huygens reveals these iron and calcium carbonates.
James Wray of Cornell University in Ithaca, New York, presented the findings this week at the Lunar and Planetary Science Conference in Texas.