Mars Rover Opportunity Trekking Toward More Layers
06.07.13
NASA's Mars Exploration Rover Opportunity used its panoramic camera
(Pancam) to acquire this view of "Solander Point" during the mission's
3,325th Martian day, or sol (June 1, 2013). Image credit:
NASA/JPL-Caltech/Cornell Univ./Arizona State Univ.
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› See telecon images
NASA's Mars Exploration Rover Opportunity used its navigation camera to acquire this view looking toward the southwest on the mission's 3,315th Martian day, or sol (May 21, 2013). Image credit: NASA/JPL-Caltech
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This map shows the 22.553-mile (36.295-kilometer) route driven by NASA's Mars Exploration Rover Opportunity from the site of its landing, inside Eagle crater at the upper left, to its location more than 112 months later, in late May 2013, departing the "Cape York" section of the rim of Endeavour crater. Image credit: NASA/JPL-Caltech/MSSS/NMMNHS
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Mission Status Report
PASADENA, Calif. - Approaching its 10th anniversary of leaving Earth,
NASA's Mars Exploration Rover Opportunity is on the move again, trekking
to a new study area still many weeks away.
The destination, called "Solander Point," offers Opportunity access to a
much taller stack of geological layering than the area where the rover
has worked for the past 20 months, called "Cape York." Both areas are
raised segments of the western rim of Endeavour Crater, which is about
14 miles (22 kilometers) in diameter.
"Getting to Solander Point will be like walking up to a road cut where
you see a cross section of the rock layers," said Ray Arvidson of
Washington University, St. Louis, deputy principal investigator for the
mission.
Solander Point also offers plenty of ground that is tilted toward the
north, which is favorable for the solar-powered rover to stay active and
mobile through the coming Martian southern-hemisphere winter.
"We're heading to a 15-degree north-facing slope with a goal of getting
there well before winter," said John Callas of NASA's Jet Propulsion
Laboratory, Pasadena, Calif., project manager for the Mars Exploration
Rover Project. The minimum-sunshine days of this sixth Martian winter
for Opportunity will come in February 2014.
NASA's Mars Exploration Rover Project launched twin rovers in 2003:
Spirit on June 10 and Opportunity on July 7. Both rovers landed in
January 2004, completed three-month prime missions and began years of
bonus, extended missions. Both found evidence of wet environments on
ancient Mars. Spirit ceased operations during its fourth Martian winter,
in 2010. Opportunity shows symptoms of aging, such as loss of motion in
some joints, but continues to accomplish groundbreaking exploration and
science.
Shortly before leaving Cape York last month, Opportunity used the rock
abrasion tool, the alpha particle X-ray spectrometer and the microscopic
imager on its robotic arm to examine a rock called "Esperance" and
found a combination of elements pointing to clay-mineral composition.
"The Esperance results are some of the most important findings of our
entire mission," said Steve Squyres of Cornell University, Ithaca, N.Y.,
principal investigator for the mission. "The composition tells us about
the environmental conditions that altered the minerals. A lot of water
moved through this rock."
Cape York exposes just a few yards, or meters, of vertical cross-section
through geological layering. Solander Point exposes roughly 10 times as
much. Researchers hope to find evidence about different stages in the
history of ancient Martian environments. The rim of Endeavour Crater
displays older rocks than what Opportunity examined at Eagle, Endurance,
Victoria and Santa Maria craters during the first eight years of the
rover's work on Mars.
JPL, a division of the California Institute of Technology in Pasadena,
manages the Mars Exploration Rover Project for NASA's Science Mission
Directorate. For more about Spirit and Opportunity, visit http://www.nasa.gov/rovers
and
You can follow the project on Twitter and on Facebook at:
and
Jet Propulsion Laboratory, Pasadena, Calif.
guy.webster@jpl.nasa.gov
NASA to Host June 7 Mars Rover Opportunity Teleconference
PASADENA,
Calif. -- NASA will hold a media teleconference at 9 a.m. PDT (noon
EDT) on Friday, June 7, to provide an update about the long-lived Mars
Exploration Rover Opportunity. The 10th anniversary of this rover's
launch is next month.
The briefing participants will be:
-- John Callas, project manager for Opportunity, NASA's Jet Propulsion Laboratory, Pasadena, Calif.
-- Steve Squyres, principal investigator for Opportunity, Cornell University, Ithaca, N.Y.
-- Ray Arvidson, deputy principal investigator, Washington University, St. Louis, Mo.
For teleconference dial-in information, reporters must send their name, media affiliation and telephone number to Elena Mejia at elena.mejia@jpl.nasa.gov or 818-393-5467.
Audio and visuals of the event will be streamed live online at:
The briefing participants will be:
-- John Callas, project manager for Opportunity, NASA's Jet Propulsion Laboratory, Pasadena, Calif.
-- Steve Squyres, principal investigator for Opportunity, Cornell University, Ithaca, N.Y.
-- Ray Arvidson, deputy principal investigator, Washington University, St. Louis, Mo.
For teleconference dial-in information, reporters must send their name, media affiliation and telephone number to Elena Mejia at elena.mejia@jpl.nasa.gov or 818-393-5467.
Audio and visuals of the event will be streamed live online at:
and
Visuals will be available at the start of the event at:
For information about NASA's Mars Exploration Rover Project and the twin rovers Spirit and Opportunity, visit:
and
Participants:
John Callas, project manager for Opportunity, NASA's Jet Propulsion Laboratory, Pasadena, Calif.
Steve Squyres, principal investigator for Opportunity, Cornell University, Ithaca, N.Y.
Ray Arvidson, deputy principal investigator for Opportunity, Washington University, St. Louis, Mo.
› Related release
Callas - 1
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Callas - 2
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Squyres - 1
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Squyres - 2
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Squyres - 3
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Arvidson - 1
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Arvidson - 2
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Arvidson - 3
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NASA
Guillermo Gonzalo Sánchez Achutegui
ayabaca@gmail.com
ayabaca@hotmail.com
ayabaca@yahoo.com
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