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NASA Orbiter Shines New Light on Long-Running Martian Mystery

By Eric November 28, 2025

Preparations are ramping up for the next series of moonwalk simulations, with a focus on underwater environments that mimic conditions on the lunar surface. These simulations are crucial for training astronauts and testing equipment ahead of future missions to the Moon and beyond. The European Space Agency (ESA) has been actively involved in this endeavor, utilizing advanced technology and innovative techniques to ensure that astronauts are well-prepared for the challenges they will face. One of the key aspects of these preparations is the use of underwater facilities that replicate the low-gravity environment of the Moon, allowing astronauts to practice their movements and operations in a controlled setting.

In parallel with these simulation efforts, NASA’s Mars Reconnaissance Orbiter (MRO) has made significant strides in enhancing our understanding of the Martian subsurface. Utilizing a novel radar technique, researchers have revisited a mysterious feature beneath the south polar ice cap of Mars, initially thought to be an underground lake. Findings from this enhanced radar technique suggest that the feature is likely a layer of rock and dust rather than liquid water. This shift in understanding is pivotal, as the presence of water is closely tied to the potential for life beyond Earth. The innovative radar maneuver, which involves rolling the spacecraft 120 degrees, has allowed scientists to penetrate deeper into the Martian surface, leading to clearer images and more accurate interpretations of what lies beneath.

The implications of these findings extend beyond just the specific location of the suspected lake. The radar technique employed by the MRO team could be instrumental in exploring other regions of Mars, particularly areas where scientists suspect the presence of ice or other resources. For instance, the Medusae Fossae formation, located near Mars’ equator, is of particular interest as it may harbor significant water resources, which would be essential for future human exploration. As researchers continue to refine their methods and explore the Martian landscape, the potential for discovering vital resources increases, paving the way for future missions and a deeper understanding of our neighboring planet. Overall, these developments highlight the ongoing collaboration between space agencies and the importance of innovative technology in the quest for knowledge about the Moon and Mars.

5 min read
Preparations for Next Moonwalk Simulations Underway (and Underwater)

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.” 

More about MRO

NASA’s Jet Propulsion Laboratory in Southern California manages MRO for the agency’s Science Mission Directorate in Washington as part of NASA’s Mars Exploration Program portfolio. Lockheed Martin Space in Denver built MRO and supports its operations. SHARAD was provided to the MRO mission by the Italian Space Agency (ASI).

News Media Contacts

Andrew Good 
Jet Propulsion Laboratory, Pasadena, Calif. 
818-393-2433 
andrew.c.good@jpl.nasa.gov
 

Karen Fox / Molly Wasser 
NASA Headquarters, Washington
202-358-1600
karen.c.fox@nasa.gov
 /
molly.l.wasser@nasa.gov

2025-130

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Last Updated

Nov 25, 2025

Related Terms
Mars Reconnaissance Orbiter (MRO)
Mars
Planetary Environments & Atmospheres

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