Life may have thrived on early Mars until it caused climate change, which led to its demise.
Researchers from the University of Arizona’s Department of Ecology and Evolutionary Biology simulated the conditions that hypothetical lifeforms would have encountered on Mars 4 billion years ago. when liquid water was most likely abundant. Photographer: ESO/M. Kornmesser
According to a study led by University of Arizona researchers, if there was ever life on Mars—and that’s a big if—conditions during the planet’s infancy would have most likely supported it.
Today’s Mars is dry, extremely cold, and has a tenuous atmosphere, making any form of life on the surface extremely unlikely. According to the study, published in Nature Astronomy, Earth’s smaller, red neighbor may have been much more hospitable 4 billion years ago.
Most Mars experts agree that the planet once had a much denser atmosphere than it does now. According to Regis Ferrière, a professor in the Arizona Department of Ecology and Evolutionary Biology and one of the paper’s two senior authors, it would have likely created a temperate climate that allowed water to flow and, possibly, microbial life to thrive.
The authors are not claiming that life existed on early Mars, but if it did, “our study shows that underground, early Mars would very likely have been habitable to methanogenic microbes,” according to Ferrière.

artistic impression of a great discovery
Such microbes are known to exist in extreme habitats on Earth, such as hydrothermal vents along fissures in the ocean floor, where they make a living by converting chemical energy from their surroundings and emitting methane as a waste product. They support entire ecosystems that have evolved to withstand crushing water pressures, near-freezing temperatures, and total darkness.
The researchers used cutting-edge models of Mars’ crust, atmosphere, and climate, as well as an ecological model of a community of Earthlike microbes metabolizing carbon dioxide and hydrogen, to test a hypothetical scenario of an emerging Martian ecosystem.
Most hydrogen on Earth is bound up in water and is rarely encountered on its own, except in isolated environments such as hydrothermal vents. Its abundance in the Martian atmosphere, on the other hand, could have provided an ample supply of energy for methanogenic microbes around 4 billion years ago, when conditions were more conducive to life, according to the authors. According to Ferrière, early Mars would have been very different from what it is today, trending toward warm and wet rather than cold and dry due to high concentrations of hydrogen and carbon dioxide, both of which are strong greenhouse gases that trap heat in the atmosphere.
“We believe Mars was slightly cooler than Earth at the time, but not nearly as cold as it is now, with average temperatures most likely hovering above the freezing point of water,” he said. “While current Mars has been described as an ice cube covered in dust, we envision early Mars as a rocky planet with a porous crust, soaked in liquid water that likely formed lakes and rivers, and possibly seas or oceans.”
According to spectroscopic measurements of rocks exposed on Mars’ surface, that water would have been extremely salty.
The researchers used models that predict the temperatures at the surface and in the crust for a given atmospheric composition to simulate the conditions that early lifeforms would have encountered on Mars. They then combined the data with an ecosystem model they created to predict whether biological populations could have survived in their local environment and how they would have affected it over time.
Under the influence of hydrogen consumed from and methane released into the atmosphere, ancient Martian life would have rendered the planet’s surface covered in ice and uninhabitable, according to the study. Boris Sauterey and Regis Ferrière contributed to this work.

“Once we had our model, we literally put it to work in the Martian crust,” said the paper’s first author, Boris Sauterey, a former postdoctoral fellow in Ferrière’s group who is now a postdoctoral fellow at Sorbonne Université in Paris. “This enabled us to assess the plausibility of a Martian underground biosphere. And, if such a biosphere existed, how would it have altered the chemistry of the Martian crust, and how would these crustal processes have affected the chemical composition of the atmosphere?”
“Our goal was to build a model of the Martian crust with its mix of rock and salty water, let gases from the atmosphere diffuse into the ground, and see if methanogens could live with that,” said Ferrière, who is also a professor at Paris Sciences & Lettres University. “And the general answer is that these microbes could have made a living in the planet’s crust.”
The researchers then set out to answer an intriguing question: how deep would one have had to go to find life underground? Sauterey explained that the Martian atmosphere would have provided the chemical energy that the organisms would have required to thrive—in this case, hydrogen and carbon dioxide.
“The issue is that even on early Mars, the surface was still very cold, so microbes would have had to go deeper into the crust to find habitable temperatures,” he explained. “The question is, how far does biology have to go to find the right balance between temperature and the availability of molecules from the atmosphere required for growth? The microbial communities in our models would have been happiest in the upper few hundreds of meters, according to our findings.”
They were able to predict the climatic feedback of the change in atmospheric composition caused by the biological activity of these microbes by modifying their model to take into account how processes occurring above and below ground influence each other. In an unexpected twist, the study revealed that, while ancient Martian life may have flourished at first, its chemical feedback to the atmosphere would have triggered a global cooling of the planet, eventually rendering its surface uninhabitable and driving life deeper and deeper underground, possibly to extinction.
“According to our findings, biological activity on Mars would have completely changed the atmosphere within a few tens or hundreds of thousands of years,” Sauterey said. “Microbes would have dramatically cooled the planet’s climate by removing hydrogen from the atmosphere.”
As a result of biological activity, the early Mars’ surface would have quickly become glacial. In other words, climate change caused by Martian life may have contributed to the planet’s surface becoming uninhabitable early on.
“The problem these microbes would have faced then is that Mars’ atmosphere essentially vanished, completely thinned, so their energy source would have vanished and they would have had to find an alternate source of energy,” Sauterey explained. “Furthermore, the temperature would have dropped significantly, requiring them to go much deeper into the crust. For the time being, it is difficult to predict how long Mars would have been habitable.”
Future Mars exploration missions may provide answers, but the authors predict that challenges will remain. While they identified Hellas Planitia, an extensive plain carved out by a large comet or asteroid impact very early in Mars’ history, as a particularly promising site to scour for evidence of past life, the location’s topography generates some of Mars’ most violent dust storms, making the area too risky to be explored by an autonomous rover.
However, once humans begin to explore Mars, such locations may be re-considered for future missions to the planet, according to Sauterey. For the time being, the team is concentrating its efforts on modern Mars. While NASA’s Curiosity rover and the European Space Agency’s Mars Express satellite have detected elevated levels of methane in the atmosphere, such spikes do raise the intriguing possibility that lifeforms such as methanogens may have survived in isolated pockets on Mars, deep underground—oases of alien life in an otherwise hostile world.
Source Credit: Phys.org