NASA's Curiosity rover on Mars found tiny, dark bumps on a Martian ridge that are similar to those found around gypsum crystals that form in drying lakes on Earth, according to a statement from the space agency.
The tiny bumps are less than a half an inch wide. Some are star-shaped, while others are part of more complex V-shaped "swallowtails." The features are not crystals themselves, but could have formed over the crystals, like plaster over a mold. Researchers think the features are yet another sign that liquid water once flowed on the Red Planet.
"These [types of features] can form when salts become concentrated in water, such as in an evaporating lake," Sanjeev Gupta, a Curiosity science team member at Imperial College, London, said in a statement from NASA's Jet Propulsion Laboratory. Gupta previously studied gypsum crystals in the rocks of Scotland. [Photos: Spectacular Mars Vistas by NASA's Curiosity]
Members of the Curiosity team are considering multiple possibilities for the features, which were found in Gale Crater, at a site nicknamed "Jura." The site is in a larger zone, called "Vera Rubin Ridge." The team is not sure when the crystal features formed, relative to when the sediments surrounding them accumulated. The crystals could have formed in wet sediment in a drying lake or in water trickling through the sediment underground, after it hardened into rock.
It's also unclear whether the shapes contain the original crystal or mineral that formed them, or if those crystals dissolved away and were perhaps replaced by something else.
"Some of the features shaped like gypsum crystals appear darker than gypsum, are enriched in iron, or are empty," according to the statement. (The "empty" features no longer contain the crystals that formed them). These are clues that the original crystallizing material may have been replaced or removed by later effects of underground water."
"So far on this mission, most of the evidence we've seen about ancient lakes in Gale Crater has been for relatively fresh, non-salty water," Ashwin Vasavada, a Curiosity project scientist at NASA's Jet Propulsion Laboratory, said in the statement. "If we start seeing lakes becoming saltier with time, that would help us understand how the environment changed in Gale Crater, and it's consistent with an overall pattern that water on Mars became more scarce over time."
Whatever the crystals' origin, team members expressed their surprise in running across them.
"These tiny 'V' shapes really caught our attention, but they were not at all the reason we went to that rock," Abigail Fraeman, a Curiosity science team member at JPL, said in the statement. "We were looking at the color change from one area to another. We were lucky to see the crystals. They're so tiny, you don't see them until you're right on them."
A treasure trove of targets
Vera Rubin Ridge is located on the north slope of lower Mount Sharp inside Gale Crater. Curiosity landed in the crater in August 2012. It has been making its way up Mount Sharp since September 2014, examining the layers of the mountain to learn more about how it was formed.
At the ridge, investigators found many other targets to consider, including different colors in the bedrock and mineral veins, and variations in the sedimentary layers and local rock iron content, according to the statement. Curiosity also spotted some rice-grain-size features that look like "sticks," which attracted attention when the raw images were posted online. Although some media outlets reported that they looked like fossils, the rover team said the "sticks" are likely bits of the same material that makes up the dark mineral veins. [Life on Mars: Exploration & Evidence]
"There's just a treasure trove of interesting targets concentrated in this one area," Vasavada said. "Each is a clue, and the more clues, the better. It's going to be fun figuring out what it all means."
Curiosity began climbing Vera Rubin Ridge about five months ago and is now uphill on the southern edge. There, researchers are looking at features that could be linked to another transitional area farther up, called the "Clay Unit," because clay features were spotted in data taken from orbit.
Researchers also noted that changes in the iron content in the ridge's mineral veins could have been important for potential life-forms that might have once called the Red Planet home. Different types of iron oxides vary in how well they dissolve in water. If an environment has many different types of iron oxides, that can provide a potential energy source for life-forms, NASA said.
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Elizabeth Howell (she/her), Ph.D., is a staff writer in the spaceflight channel since 2022 covering diversity, education and gaming as well. She was contributing writer for Space.com for 10 years before joining full-time. Elizabeth's reporting includes multiple exclusives with the White House and Office of the Vice-President of the United States, an exclusive conversation with aspiring space tourist (and NSYNC bassist) Lance Bass, speaking several times with the International Space Station, witnessing five human spaceflight launches on two continents, flying parabolic, working inside a spacesuit, and participating in a simulated Mars mission. Her latest book, "Why Am I Taller?", is co-written with astronaut Dave Williams. Elizabeth holds a Ph.D. and M.Sc. in Space Studies from the University of North Dakota, a Bachelor of Journalism from Canada's Carleton University and a Bachelor of History from Canada's Athabasca University. Elizabeth is also a post-secondary instructor in communications and science at several institutions since 2015; her experience includes developing and teaching an astronomy course at Canada's Algonquin College (with Indigenous content as well) to more than 1,000 students since 2020. Elizabeth first got interested in space after watching the movie Apollo 13 in 1996, and still wants to be an astronaut someday. Mastodon: https://qoto.org/@howellspace