A new paper finds more radar signals suggesting the presence of subsurface
'lakes," but many are in areas too cold for water to remain liquid.
In 2018, scientists working with data from ESA's (the European Space
Agency's) Mars Express orbiter announced a surprising discovery: Signals
from a radar instrument reflected off the red planet's south pole appeared
to reveal a liquid subsurface lake. Several more such reflections have been
announced since then.
In a new paper published in the journal Geophysical Research Letters, two
scientists at NASA's Jet Propulsion Laboratory in Southern California
describe finding dozens of similar radar reflections around the south pole
after analyzing a broader set of Mars Express data, but many are in areas
that should be too cold for water to remain liquid.
"We're not certain whether these signals are liquid water or not, but they
appear to be much more widespread than what the original paper found," said
Jeffrey Plaut of JPL, co-principal investigator of the orbiter's MARSIS
(Mars Advanced Radar for Subsurface and Ionospheric Sounding) instrument,
which was built jointly by the Italian Space Agency and JPL. "Either liquid
water is common beneath Mars' south pole or these signals are indicative of
something else."
Frozen Time Capsule
The radar signals originally interpreted as liquid water were found in a
region of Mars known as the South Polar Layered Deposits, named for the
alternating layers of water ice, dry ice (frozen carbon dioxide), and dust
that have settled there over millions of years. These layers are believed to
provide a record of how the tilt in Mars' axis has shifted over time, just
as changes in Earth's tilt have created ice ages and warmer periods
throughout our planet's history. When Mars had a lower axial tilt, snowfall
and layers of dust accumulated in the region and eventually formed the thick
layered ice sheet found there today.
By beaming radio waves at the surface, scientists can peer below these icy
layers, mapping them in detail. Radio waves lose energy when they pass
through material in the subsurface; as they reflect back to the spacecraft,
they usually have a weaker signal. But in some cases, signals returning from
this region's subsurface were brighter than those at the surface. Some
scientists have interpreted these signals to imply the presence of liquid
water, which strongly reflects radio waves.
Plaut and Aditya Khuller, a doctoral student at Arizona State University who
worked on the paper while interning at JPL, aren't sure what the signals
indicate. The areas hypothesized to contain liquid water span about 6 to 12
miles (10 to 20 kilometers) in a relatively small region of the Martian
south pole. Khuller and Plaut expanded the search for similar strong radio
signals to 44,000 measurements spread across 15 years of MARSIS data over
the entirety of the Martian south polar region.
Unexpected "Lakes'
The analysis revealed dozens of additional bright radar reflections over a
far greater range of area and depth than ever before. In some places, they
were less than a mile from the surface, where temperatures are estimated to
be minus 81 degrees Fahrenheit (minus 63 degrees Celsius) – so cold that
water would be frozen, even if it contained salty minerals known as
perchlorates, which can lower the freezing point of water.
Khuller noted a 2019 paper in which researchers calculated the heat needed
to melt subsurface ice in this region, finding that only recent volcanism
under the surface could explain the potential presence of liquid water under
the south pole.
"They found that it would take double the estimated Martian geothermal heat
flow to keep this water liquid," Khuller said. "One possible way to get this
amount of heat is through volcanism. However, we haven't really seen any
strong evidence for recent volcanism at the south pole, so it seems unlikely
that volcanic activity would allow subsurface liquid water to be present
throughout this region."
What explains the bright reflections if they're not liquid water? The
authors can't say for sure. But their paper does offer scientists a detailed
map of the region that contains clues to the climate history of Mars,
including the role of water in its various forms.
"Our mapping gets us a few steps closer to understanding both the extent and
the cause of these puzzling radar reflections," said Plaut.
Reference:
Aditya R. Khuller et al, Characteristics of the Basal Interface of the
Martian South Polar Layered Deposits, Geophysical Research Letters (2021).
DOI:
10.1029/2021GL093631
Tags:
Space & Astrophysics