The European Space Agency’s Mars Express orbiter
captured this view of Mars’ south polar ice cap Feb. 25, 2015. Three years
later, the spacecraft detected a signal from the area to the right of the ice
cap that scientists interpreted as an underground lake.
ESA/DLR/FU Berlin, CC BY-SA 3.0
IGO
Results from an enhanced radar technique have demonstrated improvement to
sub-surface observations of Mars.
NASA’s Mars Reconnaissance Orbiter
(MRO) has revisited and raised new questions about a mysterious feature buried
beneath thousands of feet of ice at the Red Planet’s south pole. In a recent
study, researchers conclude from data obtained using an innovative radar
technique that an area on Mars suspected of being an underground lake is more
likely to be a layer of rock and dust.
The 2018 discovery of the suspected
lake set off a flurry of scientific activity, as water is closely linked with
life in the solar system. While the latest findings indicate this feature is
not a lake below the Martian surface, it does suggest that the same radar
technique could be used to check for subsurface resources elsewhere on Mars,
supporting future explorers.
The paper, published in Geophysical Research Letters on Nov. 17, was led by two of MRO’s Shallow
Radar (SHARAD) instrument scientists, Gareth Morgan and Than Putzig, who are
based at the Planetary Science Institute in Tucson, Arizona, and Lakewood,
Colorado, respectively.
The observations were made by MRO with a special maneuver that rolls the spacecraft 120 degrees. Doing so enhances the power of SHARAD, enabling the radar’s signal to penetrate deeper underground and provide a clearer image of the subsurface. These “very large rolls” have proved so effective that scientists are eager to use them at previously observed sites where buried ice might exist.
This map shows the approximate area where in 2018
ESA’s Mars Express detected a signal the mission’s scientists interpreted as an
underground lake. The red lines show the path of NASA’s Mars Reconnaissance
Orbiter, which flew both directly overhead as well as over an adjacent region.
Credit: Planetary Science Institute
Morgan, Putzig, and fellow SHARAD team members had made multiple
unsuccessful attempts to observe the area suspected of hosting a buried lake.
Then the scientists partnered with the spacecraft’s operations team at NASA’s
Jet Propulsion Laboratory in Southern California, which leads the mission, to
develop the very large roll capability.
Because the radar’s antenna is at
the back of MRO, the orbiter’s body obstructs its view and weakens the
instrument’s sensitivity. After considerable work, engineers at JPL and
Lockheed Martin Space in Littleton, Colorado, which built the spacecraft and supports
its operations, developed commands for a 120-degree roll — a technique that
requires careful planning to keep the spacecraft safe — to direct more of
SHARAD’s signal at the surface.
Bright signal
On May 26, SHARAD performed a very
large roll to finally pick up the signal in the target area, which spans about
12.5 miles (20 kilometers) and is buried under a slab of water ice almost 1
mile (1,500 meters) thick.
When a radar signal bounces off
underground layers, the strength of its reflection depends on what the
subsurface is made of. Most materials let the signal slip through or absorb it,
making the return faint. Liquid water is special in that it produces a very
reflective surface, sending back a very strong signal (imagine pointing a
flashlight at a mirror).
That’s the kind of signal that was spotted from this area in 2018 by a team working with the Mars Advanced Radar for Subsurface and Ionospheric Sounding (MARSIS) instrument aboard the ESA (European Space Agency) Mars Express orbiter. To explain how such a body of water could remain liquid under all that ice, scientists have hypothesized it could be a briny lake, since high salt content can lower water’s freezing temperature.
An antenna sticks out like whiskers from NASA’s Mars
Reconnaissance Orbiter in this artist’s concept depicting the spacecraft, which
has been orbiting the Red Planet since 2006. This antenna is part of SHARAD, a
radar that peers below the Martian surface.
NASA/JPL-Caltech
“We’ve been observing this area with SHARAD for almost 20 years without
seeing anything from those depths,” said Putzig. But once MRO achieved a very
large roll over the precise area, the team was able to look much deeper. And
rather than the bright signal MARSIS received, SHARAD detected a faint one. A
different very-large-roll observation of an adjacent area didn’t detect a
signal at all, suggesting something unique is causing a quirky radar signal at
the exact spot MARSIS saw a signal.
“The lake hypothesis generated lots
of creative work, which is exactly what exciting scientific discoveries are
supposed to do,” said Morgan. “And while this new data won’t settle the debate,
it makes it very hard to support the idea of a liquid water lake.”
Alternative explanations
Mars’ south pole has an ice cap
sitting atop heavily cratered terrain, and most radar images of the area below
the ice show lots of peaks and valleys. Morgan and Putzig said it’s possible
that the bright signal MARSIS detected here may just be a rare smooth area — an
ancient lava flow, for example.
Both scientists are excited to use
the very large roll technique to reexamine other scientifically interesting
regions of Mars. One such place is Medusae Fossae, a sprawling geologic
formation on Mars’ equator that produces little radar return. While some
scientists have suggested it’s composed of layers of volcanic ash, others have
suggested the layers may include heaps of ice deep within.
“If it’s ice, that means there’s lots of water resources near the Martian equator, where you’d want to send humans,” said Putzig. “Because the equator is exposed to more sunlight, it’s warmer and ideal for astronauts to live and work.”
Source: NASA Orbiter Shines New Light on Long-Running Martian Mystery - NASA



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