[meteorite-list] Mars Rock-Ingredient Stew Seen as Plus for Habitability

[Ron Baalke]

http://www.jpl.nasa.gov/news/news.php?feature=6700

Mars Rock-Ingredient Stew Seen as Plus for Habitability
Jet Propulsion Laboratory
December 13, 2016

Fast Facts:

* NASA's Curiosity Mars rover is finding patterns of change in rock composition 
at higher, younger layers of a mountain.

* Ancient Mars sedimentary basins with groundwater were chemically active, 
a factor favorable for possible life.

* Curiosity found boron on Mars, a first for this very soluble element.

NASA's Curiosity rover is climbing a layered Martian mountain and finding 
evidence of how ancient lakes and wet underground environments changed, 
billions of years ago, creating more diverse chemical environments that 
affected their favorability for microbial life.

Hematite, clay minerals and boron are among the ingredients found to be 
more abundant in layers farther uphill, compared with lower, older layers 
examined earlier in the mission. Scientists are discussing what these 
and other variations tell about conditions under which sediments were 
initially deposited, and about how groundwater moving later through the 
accumulated layers altered and transported ingredients.

Effects of this groundwater movement are most evident in mineral veins. 
The veins formed where cracks in the layers were filled with chemicals 
that had been dissolved in groundwater. The water with its dissolved contents 
also interacted with the rock matrix surrounding the veins, altering the 
chemistry both in the rock and in the water.

"There is so much variability in the composition at different elevations, 
we've hit a jackpot," said John Grotzinger, of Caltech in Pasadena, California. 
He and other members of Curiosity's science team presented an update about 
the mission Tuesday, Dec. 13, in San Francisco during the fall meeting 
of the American Geophysical Union. As the rover examines higher, younger 
layers, researchers are impressed by the complexity of the lake environments 
when clay-bearing sediments were being deposited, and also the complexity 
of the groundwater interactions after the sediments were buried.

'Chemical Reactor'

"A sedimentary basin such as this is a chemical reactor," Grotzinger said. 
"Elements get rearranged. New minerals form and old ones dissolve. Electrons 
get redistributed. On Earth, these reactions support life."

Whether Martian life has ever existed is still unknown. No compelling 
evidence for it has been found. When Curiosity landed in Mars' Gale Crater 
in 2012, the mission's main goal was to determine whether the area ever 
offered an environment favorable for microbes.

The crater's main appeal for scientists is geological layering exposed 
in the lower portion of its central mound, Mount Sharp. These exposures 
offer access to rocks that hold a record of environmental conditions from 
many stages of early Martian history, each layer younger than the one 
beneath it. The mission succeeded in its first year, finding that an ancient 
Martian lake environment had all the key chemical ingredients needed for 
life, plus chemical energy available for life. Now, the rover is climbing 
lower on Mount Sharp to investigate how ancient environmental conditions 
changed over time.

"We are well into the layers that were the main reason Gale Crater was 
chosen as the landing site," said Curiosity Deputy Project Scientist Joy 
Crisp of NASA's Jet Propulsion Laboratory, in Pasadena, California. "We 
are now using a strategy of drilling samples at regular intervals as the 
rover climbs Mount Sharp. Earlier we chose drilling targets based on each 
site's special characteristics. Now that we're driving continuously through 
the thick basal layer of the mountain, a series of drill holes will build 
a complete picture."

Four recent drilling sites, from "Oudam" this past June through "Sebina" 
in October, are each spaced about 80 feet (about 25 meters) apart in elevation. 
This uphill pattern allows the science team to sample progressively younger 
layers that reveal Mount Sharp's ancient environmental history.

Changing Environments

One clue to changing ancient conditions is the mineral hematite. It has 
replaced less-oxidized magnetite as the dominant iron oxide in rocks Curiosity 
has drilled recently, compared with the site where Curiosity first found 
lakebed sediments. "Both samples are mudstone deposited at the bottom 
of a lake, but the hematite may suggest warmer conditions, or more interaction 
between the atmosphere and the sediments," said Thomas Bristow of NASA 
Ames Research Center, Moffett Field, California. He helps operate the 
Chemistry and Mineralogy (CheMin) laboratory instrument inside the rover, 
which identifies minerals in collected samples.

Chemical reactivity occurs on a gradient of chemical ingredients' strength 
at donating or receiving electrons. Transfer of electrons due to this 
gradient can provide energy for life. An increase in hematite relative 
to magnetite indicates an environmental change in the direction of tugging 
electrons more strongly, causing a greater degree of oxidation in iron.

Another ingredient increasing in recent measurements by Curiosity is the 
element boron, which the rover's laser-shooting Chemistry and Camera (ChemCam) 
instrument has been detecting within mineral veins that are mainly calcium 
sulfate. "No prior mission has detected boron on Mars," said Patrick Gasda 
of the U.S. Department of Energy's Los Alamos National Laboratory, Los 
Alamos, New Mexico. "We're seeing a sharp increase in boron in vein targets 
inspected in the past several months." The instrument is quite sensitive; 
even at the increased level, boron makes up only about one-tenth of one 
percent of the rock composition.

'Dynamic System'

Boron is famously associated with arid sites where much water has evaporated 
away -- think of the borax that mule teams once hauled from Death Valley. 
However, environmental implications of the minor amount of boron found 
by Curiosity are less straightforward than for the increase in hematite.

Scientists are considering at least two possibilities for the source of 
boron that groundwater left in the veins. Perhaps evaporation of a lake 
formed a boron-containing deposit in an overlying layer, not yet reached 
by Curiosity, then water later re-dissolved the boron and carried it down 
through a fracture network into older layers, where it accumulated along 
with fracture-filling vein minerals. Or perhaps changes in the chemistry 
of clay-bearing deposits, such as evidenced by the increased hematite, 
affected how groundwater picked up and dropped off boron within the local 
sediments.

"Variations in these minerals and elements indicate a dynamic system," 
Grotzinger said. "They interact with groundwater as well as surface water. 
The water influences the chemistry of the clays, but the composition of 
the water also changes. We are seeing chemical complexity indicating a 
long, interactive history with the water. The more complicated the chemistry 
is, the better it is for habitability. The boron, hematite and clay minerals 
underline the mobility of elements and electrons, and that is good for 
life."

Curiosity is part of NASA's ongoing Mars research and preparation for 
a human mission to Mars in the 2030s. Caltech manages JPL, and JPL manages 
the Curiosity mission for NASA's Science Mission Directorate in Washington. 
For more about Curiosity, visit:

http://www.nasa.gov/msl

and

http://mars.jpl.nasa.gov/msl/

Learn about NASA's Journey to Mars at:

http://www.nasa.gov/content/nasas-journey-to-mars/

News Media Contact
Laurie Cantillo / Dwayne Brown
NASA Headquarters, Washington
202-358-1077 / 202-358-1726
laura.l.cantillo at nasa.gov / dwayne.c.brown at nasa.gov

Guy Webster / DC Agle
Jet Propulsion Laboratory, Pasadena, Calif.
818-354-6278 / 818-393-9011
guy.webster at jpl.nasa.gov / agle at jpl.nasa.gov

Abigail Tabor
Ames Research Center, Moffett Field, Calif.
650-604-0643
abigail.s.tabor at nasa.gov

Laura Mullane
Los Alamos National Research Laboratory, Los Alamos, N.M.
505-667-6012
mullane at lanl.gov

2016-318