[meteorite-list] Found: Clues about Volcanoes Under Ice on Ancient Mars

From: Ron Baalke <baalke_at_meteoritecentral.com>
Date: Wed, 4 May 2016 16:32:59 -0700 (PDT)
Message-ID: <201605042332.u44NWxes028410_at_zagami.jpl.nasa.gov>

http://www.jpl.nasa.gov/news/news.php?feature=6472

Found: Clues about Volcanoes Under Ice on Ancient Mars
Jet Propulsion Laboratory
May 3, 2016

Volcanoes erupted beneath an ice sheet on Mars billions of years ago,
far from any ice sheet on the Red Planet today, new evidence from NASA's
Mars Reconnaissance Orbiter suggests.

The research about these volcanoes helps show there was extensive ice
on ancient Mars. It also adds information about an environment combining
heat and moisture, which could have provided favorable conditions for
microbial life.

Sheridan Ackiss of Purdue University, West Lafayette, Indiana, and collaborators
used the orbiter's mineral-mapping spectrometer to investigate surface
composition in an oddly textured region of southern Mars called "Sisyphi
Montes." The region is studded with flat-topped mountains. Other researchers
previously noted these domes' similarity in shape to volcanoes on Earth
that erupted underneath ice.

"Rocks tell stories. Studying the rocks can show how the volcano formed
or how it was changed over time," Ackiss said. "I wanted to learn what
story the rocks on these volcanoes were telling."

When a volcano begins erupting beneath a sheet of ice on Earth, the rapidly
generated steam typically leads to explosions that punch through the ice
and propel ash high into the sky. For example, the 2010 eruption of ice-covered
Eyjafjallaj??kull in Iceland lofted ash that disrupted air travel across
Europe for about a week.

Characteristic minerals resulting from such subglacial volcanism on Earth
include zeolites, sulfates and clays. Those are just what the new research
has detected at some flat-topped mountains in the Sisyphi Montes region
examined with the spacecraft's Compact Reconnaissance Imaging Spectrometer
for Mars (CRISM), providing resolution of about 60 feet (18 meters) per
pixel.

"We wouldn't have been able to do this without the high resolution of
CRISM," Ackiss said.

The Sisyphi Montes region extends from about 55 degrees to 75 degrees
south latitude. Some of the sites that have shapes and compositions consistent
with volcanic eruptions beneath an ice sheet are about 1,000 miles (about
1,600 kilometers) from the current south polar ice cap of Mars. The cap
now has a diameter of about 220 miles (about 350 kilometers).

The Mars Reconnaissance Orbiter Project has been using CRISM and five
other instruments on the spacecraft to investigate Mars since 2006. The
project is managed by NASA's Jet Propulsion Laboratory, Pasadena, California,
for the agency's Science Mission Directorate, Washington. The Johns Hopkins
University Applied Physics Laboratory in Laurel, Maryland, provided and
operates CRISM. Lockheed Martin Space Systems in Denver built the orbiter
and supports its operations.

NASA has three active orbiters and two rovers at Mars that are advancing
knowledge about the Red Planet that is useful in planning future missions
that will take humans there.


News Media Contact

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

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

Elizabeth Gardner
Purdue University, West Lafayette, Ind.
765-494-2081
ekgardner at purdue.edu

Geoffrey Brown
Johns Hopkins University Applied Physics Laboratory, Laurel, Md.
240-228-5618
geoffrey.brown at jhuapl.edu

2016-120
Received on Wed 04 May 2016 07:32:59 PM PDT