ASU alum leads study proposing stellar possibility: Could life exist below Mars ice?
Scientists have yet to find evidence of life on Mars, but a new NASA study, whose lead author is an Arizona State University alumnus, proposes microbes could find a potential home beneath frozen water on the planet’s surface.
Through computer modeling, the study’s authors have shown that the amount of sunlight that can shine through surface ice would be enough for photosynthesis to occur in shallow pools of meltwater below the surface of the ice. Similar pools of water that form within ice on Earth have been found teeming with life, including algae, fungi and microscopic cyanobacteria, all of which derive energy from photosynthesis.
“If we’re trying to find life anywhere in the universe today, Martian ice exposures are probably one of the most accessible places we should be looking,” said the paper’s lead author, Aditya Khuller, who earned his PhD in geological sciences from ASU in 2023 and is a postdoctoral researcher at NASA’s Jet Propulsion Laboratory in Southern California.
Mars has two kinds of ice: frozen water and frozen carbon dioxide. For their paper, published in Communications Earth & Environment, part of the Nature Portfolio, Khuller and colleagues looked at water ice, large amounts of which formed from snow mixed with dust that fell on the surface during a series of Martian ice ages from the past million years. That ancient snow has since solidified into ice, still peppered with specks of dust.
Those dust particles are key to explaining how subsurface pools of water would form within ice when exposed to the sun: Dark dust absorbs more sunlight than the surrounding ice, causing the ice to warm up and melt up to a few feet below the surface.
Mars scientists are divided about whether ice can actually melt when exposed to the Martian surface due to the planet’s thin, dry atmosphere, where water ice is believed to sublimate — or turn directly into gas — the way dry ice does on Earth. But the atmospheric effects that make melting difficult on the surface wouldn’t apply below the surface of a dusty snowpack or glacier.
Thriving microcosms
On Earth, dust within ice can create what are called cryoconite holes — small cavities that form in ice when particles of windblown dust (cryoconite) land there, absorb sunlight and melt farther into the ice each summer. Eventually, as they travel farther from the sun’s rays, they stop sinking but still generate enough warmth to create a pocket of meltwater around them. The pockets can nourish a thriving ecosystem for simple life-forms, which lie dormant most of the year until the ice thaws for a couple of months in the summer.
“This is a common phenomenon on Earth,” said co-author Phil Christensen, professor at Arizona State University’s School of Earth and Space Exploration, referring to ice melting from within. “Dense snow and ice can melt from the inside out, letting in sunlight that warms it like a greenhouse, rather than melting from the top down.”
Christensen is a member of the science team on NASA’s Europa Clipper mission to Jupiter’s icy moon Europa and has studied ice on Mars for decades. He leads operations for a heat-sensitive camera called THEMIS, the Thermal Emission Imaging System aboard the 2001 Mars Odyssey orbiter. For the Europa Clipper, he’ll carry on that work with a next-generation camera, E-THEMIS (Europa Thermal Emission Imaging System).
In past research, Christensen and Gary Clow of the University of Colorado Boulder used modeling to demonstrate how liquid water could form within dusty snowpack on the Red Planet. That work, in turn, provided a foundation for the new paper focused on whether photosynthesis could be possible on Mars.
In 2021, Christensen and Khuller co-authored a paper on the discovery of dusty water ice exposed within gullies on Mars, proposing that many Martian gullies form by erosion caused by the ice melting to form liquid water.
This new paper suggests that dusty ice lets in enough light for photosynthesis to occur as deep as 9 feet (or 3 meters) below the surface. In this scenario, the upper layers of ice prevent the shallow subsurface pools of water from evaporating while also providing protection from harmful radiation. That’s important given that, unlike Earth, Mars lacks a protective magnetic field to shield it from both the sun and radioactive cosmic ray particles zipping around space.
The water ice that would be most likely to form these subsurface pools exists in Mars’ tropics, between 30 degrees and 60 degrees latitude, in both the northern and southern hemispheres.
Khuller said the next step would be to re-create some of Mars’ dusty ice in a lab setting to study it up close. Meanwhile, he and other scientists are beginning to map out the most likely spots on Mars to look for shallow meltwater — scientific targets for possible human and robotic missions in the future.
This press release was written by Andrew Good of NASA’s Jet Propulsion Laboratory with contributions from Kim Baptista of ASU’s School of Earth and Space Exploration.
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