As the Curiosity rover explores Mars’ Gale Crater, the data it collects tells us more about the history of the planet and in particular about whether liquid water once existed there. Using data collected by Curiosity, a new study has examined the geology of the crater to learn more about the briny ponds which may once have dotted the planet’s surface.
“We went to Gale Crater because it preserves this unique record of a changing Mars,” William Rapin, Caltech researcher and lead author of the study, explained in a statement. “Understanding when and how the planet’s climate started evolving is a piece of another puzzle: When and how long was Mars capable of supporting microbial life at the surface?”
By looking at the salts present in rocks in an area of the crater called Sutton Island, the scientists could build up a picture of the environment through time. They already knew that the area went through drier periods, as the mud in a region called Old Soaker was cracked. The cracks form as the mud dries out.
The new evidence shows there were wet periods too though. The presence of minerals salts mixed with sediment suggests that shallow ponds once formed there, before drying to leave the salts behind. The ponds would have been briny due to the concentrated salts.
To understand more about the formation of these briny lakes, scientists turned to an environment closer to home: “Given that Earth and Mars were similar in their early days, Sutton Island might have resembled saline lakes on South America’s Altiplano,” Dr. Rapin said.
“Streams and rivers flowing from mountain ranges into this arid, high-altitude plateau lead to closed basins similar to Mars’ ancient Gale Crater… During drier periods, the Altiplano lakes become shallower, and some can dry out completely. The fact that they’re vegetation-free even makes them look a little like Mars.”
The research is published in the journal Nature Geoscience.
