Researchers think meltwater beneath Martian ice could support microbial life.
While actual evidence for life on Mars
has never been found, a new NASA study 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 water ice
would be enough for photosynthesis to occur in shallow pools of meltwater below
the surface of that ice. Similar pools of water that form within ice on Earth
have been found to teem 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 of 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 Nature Communications Earth
& Environment, 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 in the past million years. That ancient snow has since
solidified into ice, still peppered with specks of dust.
Although dust particles may obscure
light in deeper layers of the ice, they are key to explaining how subsurface
pools of water could form within ice when exposed to the Sun: Dark dust absorbs
more sunlight than the surrounding ice, potentially causing the ice to warm up
and melt up to a few feet below the surface.
The white edges along these gullies in Mars’ Terra
Sirenum are believed to be dusty water ice. Scientists think meltwater could
form beneath the surface of this kind of ice, providing a place for possible
photosynthesis. This is an enhanced-color image; the blue color would not
actually be perceptible to the human eye.
NASA/JPL-Caltech/University of Arizona
Mars scientists are divided about whether ice can actually melt when
exposed to the Martian surface. That’s due to the planet’s thin, dry
atmosphere, where water ice is believed to sublimate — turn directly into gas —
the way dry ice does on Earth. But the atmospheric effects that make melting
difficult on the Martian 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 (called cryoconite) land there, absorb sunlight,
and melt farther into the ice each summer. Eventually, as these dust particles
travel farther from the Sun’s rays, they stop sinking, but they still generate
enough warmth to create a pocket of meltwater around them. The pockets can
nourish a thriving ecosystem for simple lifeforms..
“This is a common phenomenon on
Earth,” said co-author Phil Christensen of Arizona State University in Tempe,
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 has studied ice on Mars
for decades. He leads operations for a heat-sensitive camera called THEMIS (Thermal Emission Imaging System) aboard NASA’s 2001
Mars Odyssey orbiter. 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 (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, because unlike Earth, Mars
lacks a protective magnetic field to shield it from both the Sun and
radioactive cosmic ray particles zipping around space.
The study authors say the water ice
that would be most likely to form subsurface pools would exist in Mars’
tropics, between 30 degrees and 60 degrees latitude, in both the northern and
southern hemispheres.
Khuller next hopes to re-create some of Mars’ dusty ice in a lab 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 — locations that could be scientific targets for possible human and robotic missions in the future.
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