© Provided by Space Mars as seen from orbit by NASA’s Viking mission.

Many tiny patches of the ground on modern Mars may be capable of supporting life as we know it, if only very briefly, a new study suggests.

Water ice is abundant on and near the Martian surface, but conditions have to be just right for this stuff to give rise to liquid water. That's because the Red Planet's atmosphere is quite thin — just 1% as dense as Earth's air at sea level — so ice tends to sublimate, or turn directly into vapor, when temperatures rise sufficiently. (Specifically, the ice evaporates before temperatures rise enough to hit water's melting point.)

The study identifies a microenvironment that could host those just-right conditions: the areas directly behind certain boulders in midlatitude regions of Mars that lie in the rocks' shadows continuously during the winter months.

Related: Photos: The search for water on Mars

© Provided by Space Three-dimensional view of Martian surface temperatures around an idealized boulder at latitude 30 degrees south. On the side opposite to the sun, temperatures are around minus 198 degrees Fahrenheit (minus 128 Celsius). As the sun rises, this area heats up rapidly, so frost melts on salt-containing ground before sublimating into the atmosphere. (Image credit: Norbert Schorghofer)

Water ice and carbon-dioxide ice accumulate seasonally in these shadowy spots, according to computer simulations performed by study author Norbert Schorghofer, a senior scientist at the Planetary Science Institute in Tucson, Arizona.

When spring comes and sunlight hits these microenvironments again, temperatures there rise rapidly, from about minus 198 degrees Fahrenheit (minus 128 degrees Celsius) to 14 degrees Fahrenheit (minus 10 degrees Celsius) in just a few hours. The ice fades away, but the temperature transition is so fast that not all of the ice sublimates; some melts into the salty Martian soil, forming liquid brines.

The soil's saltiness is key to this process, because salt lowers the melting point of water to less than the usual 32 degrees Fahrenheit (0 degrees Celsius). And the carbon-dioxide ice also appears to help things along.

"Dust contained in the CO2 frost facilitates the formation of a protective sublimation lag," Schorghofer wrote in the paper, which was published online Wednesday (Feb. 12) in The Astrophysical Journal.

"Overall, melting of pure water ice is not expected under present-day Mars conditions," he added. "However, at temperatures that are readily reached, seasonal water frost can melt on a salt-rich substrate."

Brine formation may last for just a few days in each locale that experiences it. But the phenomenon is a regular one, repeating every year, the study suggests.

Patches of winter boulder-shadow aren't the only parts of Mars that may experience seasonal surges of liquid water. NASA's Mars Reconnaissance Orbiter has spotted dark features on multiple Red Planet slopes during the warmer months. Many researchers interpret these "recurring slope lineae" to be evidence of temporary brine flows, but other scientists argue that liquid water may not be involved.

Liquid water was abundant on Mars billions of years ago, when the planet still had a protective magnetic field and a much thicker atmosphere. Indeed, NASA's Curiosity rover has determined that its landing site, the floor of the 96-mile-wide (154 kilometers) Gale Crater, hosted a long-lived lake-and-stream system in the ancient past.

And there may still be lots of water underground on the Red Planet today. For example, Europe's Mars Express spacecraft recently spotted evidence of a huge lake beneath the planet's south pole.

Mike Wall's book about the search for alien life, "Out There" (Grand Central Publishing, 2018; illustrated by Karl Tate), is out now. Follow him on Twitter @michaeldwall. Follow us on Twitter @Spacedotcom or Facebook.