NASA's Mars Reconnaissance Orbiter Uncovers New Clues on Martian Mystery
A recent study published in Geophysical Research Letters has shed new light on a long-running mystery surrounding the geology of Mars' south pole. The findings, obtained using an enhanced radar technique, suggest that a feature previously suspected to be an underground lake is more likely to be a layer of rock and dust.
The discovery was made possible by NASA's Mars Reconnaissance Orbiter (MRO), which has been studying the Martian surface since 2005. In 2018, researchers detected unusual signals emanating from beneath thousands of feet of ice at the south pole, sparking intense scientific interest due to its potential implications for life on the Red Planet.
Using a specialized radar instrument called Shallow Radar (SHARAD), scientists were able to penetrate deeper into the Martian subsurface and gather more detailed information about the suspected lake. The innovative technique involves rolling the spacecraft 120 degrees, enhancing the signal's power and allowing it to penetrate further underground.
The team behind the research, led by scientists Gareth Morgan and Than Putzig, made multiple attempts to observe the area in question before developing a new approach using the very large roll capability. This involved working with NASA's Jet Propulsion Laboratory and Lockheed Martin Space to develop commands for the spacecraft's operation.
Their efforts paid off when SHARAD finally detected a faint signal from the target area on May 26, which spans approximately 12.5 miles (20 kilometers) beneath a slab of water ice almost 1 mile (1,500 meters) thick.
Unlike liquid water, which would produce a very reflective surface sending back a strong signal, the radar detected a much weaker response. This has led some scientists to reevaluate their theories about the feature's composition and behavior, suggesting that it could be an ancient lava flow or other geological anomaly rather than a lake.
The findings also open up new possibilities for future explorers on Mars. If ice is present beneath the Martian equator, as scientists suspect, this would have significant implications for human missions to the Red Planet.
The research team is now eager to apply the same technique to other interesting regions of Mars, including Medusae Fossae, a sprawling geologic formation on the planet's equator that has raised scientific curiosity. The potential rewards of this new approach are substantial, and NASA's continued investment in exploration will undoubtedly shed more light on the mysteries of our closest celestial neighbor.
A recent study published in Geophysical Research Letters has shed new light on a long-running mystery surrounding the geology of Mars' south pole. The findings, obtained using an enhanced radar technique, suggest that a feature previously suspected to be an underground lake is more likely to be a layer of rock and dust.
The discovery was made possible by NASA's Mars Reconnaissance Orbiter (MRO), which has been studying the Martian surface since 2005. In 2018, researchers detected unusual signals emanating from beneath thousands of feet of ice at the south pole, sparking intense scientific interest due to its potential implications for life on the Red Planet.
Using a specialized radar instrument called Shallow Radar (SHARAD), scientists were able to penetrate deeper into the Martian subsurface and gather more detailed information about the suspected lake. The innovative technique involves rolling the spacecraft 120 degrees, enhancing the signal's power and allowing it to penetrate further underground.
The team behind the research, led by scientists Gareth Morgan and Than Putzig, made multiple attempts to observe the area in question before developing a new approach using the very large roll capability. This involved working with NASA's Jet Propulsion Laboratory and Lockheed Martin Space to develop commands for the spacecraft's operation.
Their efforts paid off when SHARAD finally detected a faint signal from the target area on May 26, which spans approximately 12.5 miles (20 kilometers) beneath a slab of water ice almost 1 mile (1,500 meters) thick.
Unlike liquid water, which would produce a very reflective surface sending back a strong signal, the radar detected a much weaker response. This has led some scientists to reevaluate their theories about the feature's composition and behavior, suggesting that it could be an ancient lava flow or other geological anomaly rather than a lake.
The findings also open up new possibilities for future explorers on Mars. If ice is present beneath the Martian equator, as scientists suspect, this would have significant implications for human missions to the Red Planet.
The research team is now eager to apply the same technique to other interesting regions of Mars, including Medusae Fossae, a sprawling geologic formation on the planet's equator that has raised scientific curiosity. The potential rewards of this new approach are substantial, and NASA's continued investment in exploration will undoubtedly shed more light on the mysteries of our closest celestial neighbor.