[meteorite-list] Martian Winds Carve Mountains, Move Dust, Raise Dust (MSL)

From: Ron Baalke <baalke_at_meteoritecentral.com>
Date: Fri, 3 Mar 2017 15:05:12 -0800 (PST)
Message-ID: <201703032305.v23N5CH7016853_at_zagami.jpl.nasa.gov>

https://www.jpl.nasa.gov/news/news.php?feature=6758

Martian Winds Carve Mountains, Move Dust, Raise Dust
Jet Propulsion Laboratory
February 27, 2017

Fast Facts:

* Wind is a dominant force shaping landscapes on Mars, despite the thin
air.
* A recent study supports the idea that a mountain that is oddly in the
middle of a Martian crater was formed by wind subtracting other material
after the crater had been filled to the brim with sediments.
* Modern winds in the crater show effects such as dusty whirlwinds, shifting
sand and active dunes.
* NASA's Mars rover Curiosity has begun investigating linear-shaped dunes
during the crater's windy summer season.

On Mars, wind rules. Wind has been shaping the Red Planet's landscapes
for billions of years and continues to do so today. Studies using both
a NASA orbiter and a rover reveal its effects on scales grand to tiny
on the strangely structured landscapes within Gale Crater.

NASA's Curiosity Mars rover, on the lower slope of Mount Sharp -- a layered
mountain inside the crater -- has begun a second campaign of investigating
active sand dunes on the mountain's northwestern flank. The rover also
has been observing whirlwinds carrying dust and checking how far the wind
moves grains of sand in a single day's time.

Gale Crater observations by NASA's Mars Reconnaissance Orbiter have confirmed
long-term patterns and rates of wind erosion that help explain the oddity
of having a layered mountain in the middle of an impact crater.

"The orbiter perspective gives us the bigger picture -- on all sides of
Mount Sharp and the regional context for Gale Crater. We combine that
with the local detail and ground-truth we get from the rover," said Mackenzie
Day of the University of Texas, Austin, lead author of a research report
in the journal Icarus about wind's dominant role at Gale.

The combined observations show that wind patterns in the crater today
differ from when winds from the north removed the material that once filled
the space between Mount Sharp and the crater rim. Now, Mount Sharp itself
has become a major factor in determining local wind directions. Wind shaped
the mountain; now the mountain shapes the wind.

The Martian atmosphere is about a hundred times thinner than Earth's,
so winds on Mars exert much less force than winds on Earth. Time is the
factor that makes Martian winds so dominant in shaping the landscape.
Most forces that shape Earth's landscapes -- water that erodes and moves
sediments, tectonic activity that builds mountains and recycles the planet's
crust, active volcanism -- haven't influenced Mars much for billions of
years. Sand transported by wind, even if infrequent, can whittle away
Martian landscapes over that much time.

How to Make a Layered Mountain

Gale Crater was born when the impact of an asteroid or comet more than
3.6 billion years ago excavated a basin nearly 100 miles (160 kilometers)
wide. Sediments including rocks, sand and silt later filled the basin,
some delivered by rivers that flowed in from higher ground surrounding
Gale. Curiosity has found evidence of that wet era from more than 3 billion
years ago. A turning point in Gale's history -- when net accumulation
of sediments flipped to net removal by wind erosion -- may have coincided
with a key turning point in the planet's climate as Mars became drier,
Day noted.

Scientists first proposed in 2000 that the mound at the center of Gale
Crater is a remnant from wind eroding what had been a totally filled basin.
The new work calculates that the vast volume of material removed -- about
15,000 cubic miles (64,000 cubic kilometers) -- is consistent with orbital
observations of winds' effects in and around the crater, when multiplied
by a billion or more years.

Other new research, using Curiosity, focuses on modern wind activity in
Gale.

The rover this month is investigating a type of sand dune that differs
in shape from dunes the mission investigated in late 2015 and early 2016.
Crescent-shaped dunes were the feature of the earlier campaign -- the
first ever up-close study of active sand dunes anywhere other than Earth.
The mission's second dune campaign is at a group of ribbon-shaped linear
dunes.

"In these linear dunes, the sand is transported along the ribbon pathway,
while the ribbon can oscillate back and forth, side to side," said Nathan
Bridges, a Curiosity science team member at the Johns Hopkins University
Applied Physics Laboratory in Laurel, Maryland.

The season at Gale Crater is now summer, the windiest time of year. That's
the other chief difference from the first dune campaign, conducted during
less-windy Martian winter.

"We're keeping Curiosity busy in an area with lots of sand at a season
when there's plenty of wind blowing it around," said Curiosity Project
Scientist Ashwin Vasavada of NASA's Jet Propulsion Laboratory, Pasadena,
California. "One aspect we want to learn more about is the wind's effect
on sorting sand grains with different composition. That helps us interpret
modern dunes as well as ancient sandstones."

Before Curiosity heads farther up Mount Sharp, the mission will assess
movement of sand particles at the linear dunes, examine ripple shapes
on the surface of the dunes, and determine the composition mixture of
the dune material.

Shifting Sand and 'Dust Devils'

Images taken one day apart of the same piece of ground, including some
recent pairs from the downward-looking camera that recorded the rover's
landing-day descent, show small ripples of sand moving about an inch (2.5
centimeters) downwind.

Meanwhile, whirlwinds called "dust devils" have been recorded moving across
terrain in the crater, in sequences of afternoon images taken several
seconds apart.

After completing the planned dune observations and measurements, Curiosity
will proceed southward and uphill toward a ridge where the mineral hematite
has been identified from Mars Reconnaissance Orbiter observations. The
Curiosity science team has decided to call this noteworthy feature the
"Vera Rubin Ridge," commemorating Vera Cooper Rubin (1928-2016), whose
astronomical observations provided evidence for the existence of the universe's
dark matter.

As Curiosity focuses on the sand dunes, rover engineers are analyzing
results of diagnostic tests on the drill feed mechanism, which drives
the drill bit in and out during the process of collecting sample material
from a rock. One possible cause of an intermittent issue with the mechanism
is that a plate for braking the movement may be obstructed, perhaps due
to a small piece of debris, resisting release of the brake. The diagnostic
tests are designed to be useful in planning the best way to resume use
of the drill.

The rover team is also investigating why the lens cover on Curiosity's
arm-mounted Mars Hand Lens Imager (MAHLI) did not fully open in response
to commands on Feb. 24. The arm has been raised to minimize risk of windborne
sand reaching the lens while the cover is partially open. Diagnostic tests
of the lens cover are planned this week.

During the first year after Curiosity's 2012 landing in Gale Crater, the
mission fulfilled its main goal by finding that the region once offered
environmental conditions favorable for microbial life. The conditions
in long-lived ancient freshwater Martian lake environments included all
of the key chemical elements needed for life as we know it, plus a chemical
source of energy that is used by many microbes on Earth. The extended
mission is investigating how and when the habitable ancient conditions
evolved into conditions drier and less favorable for life. For more information
about Curiosity, visit:

http://www.nasa.gov/curiosity

News Media Contact
Guy Webster
Jet Propulsion Laboratory, Pasadena, Calif.
818-354-6278
guy.webster at jpl.nasa.gov

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

2017-050
Received on Fri 03 Mar 2017 06:05:12 PM PST