NASA’s Mars Reconnaissance Orbiter used its Context Camera to capture this image of Bosporos Planum, a location on Mars. The white specks are salt deposits found within a dry channel. The largest impact crater in the scene is nearly 1 mile (1.5 kilometers) across. Credits: NASA/JPL-Caltech/MSSS
Caltech researchers used the Mars
Reconnaissance Orbiter to determine that surface water left salt minerals
behind as recently as 2 billion years ago.
Mars once rippled with rivers and ponds billions of
years ago, providing a potential habitat for microbial life. As the planet’s
atmosphere thinned over time, that water evaporated, leaving the frozen desert
world that NASA’s Mars Reconnaissance Orbiter (MRO) studies today.
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It’s commonly believed that Mars’ water evaporated
about 3 billion years ago. But two scientists studying data that MRO has
accumulated at Mars over the last 15 years have found evidence that reduces
that timeline significantly: Their research reveals signs of liquid water on
the Red Planet as recently as 2 billion to 2.5 billion years ago, meaning water
flowed there about a billion years longer than previous estimates.
The findings – published in AGU Advances on
Dec. 27, 2021 – center on the chloride salt deposits left behind as icy
meltwater flowing across the landscape evaporated.
While the shape of certain valley networks hinted that
water may have flowed on Mars that recently, the salt deposits provide the
first mineral evidence confirming the presence of liquid water. The discovery
raises new questions about how long microbial life could have survived on Mars,
if it ever formed at all. On Earth, at least, where there is water, there is
life.
The study’s lead author, Ellen Leask, performed much
of the research as part of her doctoral work at Caltech in Pasadena. She and
Caltech professor Bethany Ehlmann used data from the MRO instrument called the
Compact Reconnaissance Imaging Spectrometer for Mars (CRISM) to map the chloride salts across the clay-rich highlands of Mars’ southern
hemisphere – terrain pockmarked by impact craters. These craters were one key
to dating the salts: The fewer craters a terrain has, the younger it is. By
counting the number of craters on an area of the surface, scientists can
estimate its age.
Follow link: https://www.nasa.gov/feature/jpl/nasa-s-mro-finds-water-flowed-on-mars-longer-than-previously-thought
Click on this interactive visualization of
the Mars Reconnaissance Orbiter and take it for a spin. The “HD” button in the
lower right offers more detailed textures. The full interactive experience is
at Eyes on the Solar
System. Credit: NASA/JPL-Caltech
MRO has two cameras that are perfect for this purpose.
The Context Camera, with its black-and-white wide-angle lens, helps scientists map the
extent of the chlorides. To zoom in, scientists turn to the High-Resolution
Imaging Science Experiment (HiRISE) color camera, allowing them to see details as small as a Mars rover from
space.
Using both cameras to create digital elevation maps,
Leask and Ehlmann found that many of the salts were in depressions – once home
to shallow ponds – on gently sloping volcanic plains. The scientists also found
winding, dry channels nearby – former streams that once fed surface runoff
(from the occasional melting of ice or permafrost) into these ponds. Crater
counting and evidence of salts on top of volcanic terrain allowed them to date
the deposits.
“What is amazing is that after more than a decade of
providing high-resolution image, stereo, and infrared data, MRO has driven new
discoveries about the nature and timing of these river-connected ancient salt
ponds,” said Ehlmann, CRISM’s deputy principal investigator. Her co-author,
Leask, is now a post-doctoral researcher at Johns Hopkins University’s Applied
Physics Laboratory, which leads CRISM.
The salt minerals were first discovered 14 years ago by NASA’s Mars Odyssey orbiter, which launched in
2001. MRO, which has higher-resolution instruments than Odyssey, launched in
2005 and has been studying the salts, among many other features of Mars, ever
since. Both are managed by NASA’s Jet Propulsion Laboratory in Southern
California.
“Part of the value of MRO is that our view of the
planet keeps getting more detailed over time,” said Leslie Tamppari, the
mission’s deputy project scientist at JPL. “The more of the planet we map with
our instruments, the better we can understand its history.”
More About the Mission
JPL, a division of Caltech in Pasadena, California,
manages the MRO mission for NASA’s Science Mission Directorate in Washington.
The University of Arizona, in Tucson, operates HiRISE, which was built by Ball
Aerospace & Technologies Corp., in Boulder, Colorado. MARCI and the Context
Camera were both built and are operated by Malin Space Science Systems in San
Diego.
For more information about MRO: https://mars.nasa.gov/mro/ and www.nasa.gov/mission_pages/MRO/main/index.html
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