The Perseverance rover captured the data used in this
panorama of the “Margin Unit,” a geologic area that hugs the inner edge of
Jezero Crater’s rim, between Oct. 8 and Oct. 16, 2023.
NASA/JPL-Caltech/MSSS
When NASA’s Perseverance rover reached the inner edge of Mars’ Jezero
Crater in September 2023, mission scientists were surprised by what they found.
Called the “Margin Unit,” the geologic area stretches along the shoreline of an
ancient Martian lake, so they expected sedimentary rocks, which would have
formed as layers of sand piled on top of each other over millennia. Composed of
clay and silt, sedimentary rocks on Earth are good at preserving past microbial
life. The scientists were especially intrigued by strong signals of carbonate
minerals detected by Mars orbiters. On Earth, carbonates frequently form in
shallow ocean and lake environments capable of supporting life.
Instead, the rover team found
igneous rock, which can form deep underground from magma or from volcanic
activity at the surface. Igneous rocks are excellent record-keepers,
particularly because mineral crystals within them preserve details about the
precise moment they formed. In this case, they preserved an astonishingly
complex record of water activity on early Mars. In fact, these rocks showed
signs of having interacted with water on at least three separate occasions,
with each encounter further altering their chemistry and appearance. The
findings were published Monday in the journal Communications Earth &
Environment.
The instrument behind the findings
is SuperCam, which perches on the rover’s mast and determines the
mineralogy of geologic features based on the light they reflect. When the
science team spots an intriguing rock, they can send commands for SuperCam to
fire its laser up to 21 feet (6.5 meters) away. The spectrum of the resulting
plasma reveals the target’s chemistry. Perseverance has analyzed more than 185
bedrock targets across the unit this way.
“Before we arrived at the Margin
Unit, the main hypothesis — derived from orbital observations — was that the
carbonate seen from orbit formed from interaction with the lake that existed in
Jezero Crater,” said Candice Bedford, a research scientist at Purdue University
in West Lafayette, Indiana, and the study’s lead author. “But now we know that
this location became a sort of crossroads for aqueous systems. The Margin Unit
findings are important because Jezero Crater sits inside one of the largest
exposures of carbonate on Mars, so what we learn here reaches well beyond this
crater.”
Slow-cooling underground
Perseverance explored the Margin
Unit across approximately 870 feet (265 meters) of elevation. At higher
elevations, it found rock that was coarse-grained and crystalline — hallmarks
of the mineral olivine — with almost no sign that water had ever touched it.
Made of magnesium and iron, the area’s olivine unit formed in a body of magma
deep underground, cooling slowly enough for its grains to grow large, and
reached the surface only after the ground above it eroded away. Lower in the
unit, on the lakebed, the rock looks transformed, as the olivine grains were
fractured with silica between them.
Carbonate and silica minerals are
an important signpost in the search for ancient life. When water interacts with
olivine on Earth, the reaction can release hydrogen, which can be a food source
for some microbes, and it leaves behind carbonate and silica, two minerals that
lock in traces of the past existence of those microbes.
Multiple episodes
The Perseverance team can determine
the sequence of the Margin Unit’s interactions with water, but not their age.
On the first occasion water reached the rocks of the Margin Unit,
carbon-dioxide-rich groundwater reacted with olivine, resulting in ridges of
carbonate that run through the fractures in bedrock at low elevations. Today,
these carbonate-filled fractures are left standing as the softer rock around
them wears away.
The second time water reached the
rocks may have been related to the lake that once existed in the crater.
“Some of the Margin Unit rocks also
contain silica,” said Eleni Ravanis, a planetary scientist at the University of
Hawaii at Manoa and a coauthor of the study. “Turning olivine into carbonate
can leave silica behind, and we see more of that silica in rocks that sat below
the water line.”
Last came a water event that
generated mineral veins at one location in the eastern part of the Margin Unit,
about 10 inches (25 centimeters) thick, creating minerals like calcium sulfate
and fluorite. Finding fluorite is an important clue because it typically forms
when hot water circulates through volcanic rocks, revealing that this area
experienced a later, heated underground-water event.
“If there is one thing I have
learned after 10 years working with Mars rovers, it is that Mars constantly
throws surprises at you,” said Bedford. “It is very rare that things are as we
expect them to be from orbital data. I hope this work helps reshape how
scientists view the history of water in Jezero Crater and across Mars.
Ultimately, I hope it helps planetary scientists reconstruct the changing
climate and habitability of early Mars.”
More about Perseverance
A key objective of Perseverance’s
mission on Mars is astrobiology, including the search for signs of ancient
microbial life. The rover characterizes the planet’s geology and past climate
and collects and stores Martian rock and regolith.
Managed for NASA by Caltech, Jet
Propulsion Laboratory in Southern California built and manages operations of
the Perseverance rover on behalf of the agency’s Science Mission Directorate as
part of NASA’s Mars Exploration Program portfolio. SuperCam is co-led by Purdue
University in Indiana, Los Alamos National Laboratory in New Mexico, and IRAP
(Research Institute in Astrophysics and Planetology) and CNES (Centre National
d’Etudes Spatiales) in Toulouse, France.
For more about Perseverance: https://science.nasa.gov/mission/mars-2020-perseverance
Source: NASA Discovery Reveals Complex Water Systems on Early Mars - NASA

