Nasa’s Curiosity rover has made an exciting discovery on Mars. While exploring the slopes of Mount Sharp in Gale Crater, it found large deposits of carbon in carbonate minerals. This isn’t just a dry geological fact; it’s a key hint about ancient life on Mars.
Carbonate minerals form where carbon dioxide interacts with water and rock. They serve as important clues about the planet’s past. While we’ve seen these minerals before through rovers, orbiters, and even meteorites, Curiosity’s latest findings offer fresh insights.
Ben Tutolo, an associate professor at the University of Calgary, explains, “It tells us that the planet was habitable and that the models for habitability are correct.” This statement emphasizes the significance of what Curiosity has found.
The carbonate minerals likely formed in very dry conditions through chemic water-rock interactions, followed by evaporation. This suggests that Mars once had a thicker atmosphere with plenty of carbon dioxide, which allowed liquid water to exist on the surface. As the atmosphere thinned, the carbon dioxide began turning into solid minerals.
A standout mineral in the discovery is siderite, an iron-rich carbonate present in notable amounts—between 5% and 10% by weight—along with salts that dissolve easily in water. Tutolo noted that the presence of siderite indicates Mars was habitable until a certain point. Eventually, carbon dioxide that kept the planet warm began solidifying, which likely affected its climate.
What adds to the intrigue is the presence of iron oxyhydroxides found with these deposits. They hint that Mars may have had a functioning carbon cycle, similar to Earth’s, where carbon dioxide trapped in rocks might have returned to the atmosphere.
Scientists compared Curiosity’s findings with data from orbiting spacecraft, suggesting that similar layers on Mars could have trapped enough carbon dioxide to alter the planet’s climate significantly—up to 36 millibars, in fact.
This discovery also connects to efforts being made on Earth. Tutolo is researching methods to tackle climate change by transforming carbon dioxide into stable carbonate minerals, locking carbon away in rock. He states, “What we’re trying to do on Earth to fight climate change is something that nature may have already done on Mars.” Understanding how these minerals form on Mars can inform our own strategies for carbon management.
In summary, Curiosity’s findings not only reveal Mars’ past but also encourage us to reflect on the delicate balance of habitability, both on Mars and on our own planet. As we learn more about Mars, we can unlock secrets that may help protect Earth for future generations.