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› Full SizeTarget: Jake Matijevic Rock
This image shows where NASA's Curiosity rover aimed two different instruments to study a rock known as "Jake Matijevic." The red dots are where the Chemistry and Camera (ChemCam) instrument zapped it with its laser on Sept. 21, 2012, and Sept. 24, 2012, which were the 45th and 48th sol, or Martian day of operations. The circular black and white images were taken by ChemCam to look for the pits produced by the laser. The purple circles indicate where the Alpha Particle X-ray Spectrometer trained its view.This image was obtained by Curiosity's Mast Camera on Sept. 21, 2012 PDT (Sept. 22 UTC), or sol 46. An unannotated version of this image is also available.
Scientists white-balanced the color in this view to increase the inherent differences visible within the rock.
Image credit: NASA/JPL-Caltech/MSSS
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› Full SizeHigh-Resolution View of Cross-Section Through a Mars Ripple
This image shows the wall of a scuffmark NASA's Curiosity made in a windblown ripple of Martian sand with its wheel. The upper half of the image shows a small portion of the side wall of the scuff and a little bit of the floor of the scuff (bottom of this image). The prominent depression with raised rims at the bottom center of the image was formed by one of the treads on Curiosity's front right wheel.The largest grains in this image are about 0.04 to 0.08 inches (1 to 2 millimeters) in size. Those large grains were on top of the windblown ripple and fell down to this location when the scuff was made. The bulk of the sand in the ripple is smaller, in the range below 0.002 to 0.008 inches (50 to 200 microns).
The full scuffmark is 20 inches (50 centimeters) wide, which is the width of Curiosity's wheel.
This image from the Mars Hand Lens Imager (MAHLI) is the product of merging eight images acquired at eight slightly different focus settings to bring out details on the wall, slopes, and floor of the wheel scuff. The merge was performed onboard the MAHLI instrument to reduce downlinked data volume.
The image was acquired by MAHLI with the lens about 4.7 inches (12 centimeters) from the target. The pixel scale is about 0.002 inches (50 microns) per pixel. The image covers an area, roughly 3 by 2 inches (8 by 6 centimeters). The image was obtained on Oct. 4, 2012, or sol 58, the 58th Martian day of operations on the surface.
Image credit: NASA/JPL-Caltech/MSSS
WASHINGTON -- NASA Deputy Administrator Lori Garver will visit Lockheed
Martin in Littleton, Colo., on Monday, Oct. 15 to view the next
spacecraft to launch to Mars and a part of the Orion vehicle that will
carry astronauts farther into space than ever before.
The Mars Atmosphere and Volatile Evolution (MAVEN) mission will orbit Mars to explore how the sun may have stripped the Red Planet of most of its atmosphere, turning what possibly was once a planet habitable to microbial life into a cold and barren desert world. Lockheed Martin is building the spacecraft and will perform mission operations following launch.
Orion is America's latest human spacecraft that will usher in a new era of space exploration. It is designed to be the safest, most advanced spacecraft ever, and will be flexible and capable enough to take NASA astronauts to a variety of destinations, including Mars. Lockheed Martin is building the Orion spacecraft. The Orion heat shield is being built at the company's Littleton facility.
Garver will be available to speak with news media representatives following her tour of the MAVEN cleanroom and the facility where the Orion heat shield is being manufactured. There will be a photo opportunity with Garver and Lockheed Martin officials while they tour the MAVEN cleanroom before her comments to reporters in front of the Orion heat shield. The event starts at 9 a.m. MDT (11 a.m. EDT).
Media representatives wanting to attend the event must call Gary Napier at 303-971-4012 or email him at gary.p.napier@lmco.com by 8 a.m., Monday, Oct. 15 to be badged into the facility. Journalists planning to attend must be U.S. citizens.
For information about NASA and agency programs, visit:
The Mars Atmosphere and Volatile Evolution (MAVEN) mission will orbit Mars to explore how the sun may have stripped the Red Planet of most of its atmosphere, turning what possibly was once a planet habitable to microbial life into a cold and barren desert world. Lockheed Martin is building the spacecraft and will perform mission operations following launch.
Orion is America's latest human spacecraft that will usher in a new era of space exploration. It is designed to be the safest, most advanced spacecraft ever, and will be flexible and capable enough to take NASA astronauts to a variety of destinations, including Mars. Lockheed Martin is building the Orion spacecraft. The Orion heat shield is being built at the company's Littleton facility.
Garver will be available to speak with news media representatives following her tour of the MAVEN cleanroom and the facility where the Orion heat shield is being manufactured. There will be a photo opportunity with Garver and Lockheed Martin officials while they tour the MAVEN cleanroom before her comments to reporters in front of the Orion heat shield. The event starts at 9 a.m. MDT (11 a.m. EDT).
Media representatives wanting to attend the event must call Gary Napier at 303-971-4012 or email him at gary.p.napier@lmco.com by 8 a.m., Monday, Oct. 15 to be badged into the facility. Journalists planning to attend must be U.S. citizens.
For information about NASA and agency programs, visit:
PASADENA, Calif. -- The first Martian rock NASA's Curiosity rover has
reached out to touch presents a more varied composition than expected
from previous missions. The rock also resembles some unusual rocks from
Earth's interior.
The rover team used two instruments on Curiosity to study the chemical
makeup of the football-size rock called "Jake Matijevic"
(matt-EE-oh-vick) The results support some surprising recent
measurements and provide an example of why identifying rocks'
composition is such a major emphasis of the mission. Rock compositions
tell stories about unseen environments and planetary processes.
"This rock is a close match in chemical composition to an unusual but
well-known type of igneous rock found in many volcanic provinces on
Earth," said Edward Stolper of the California Institute of Technology in
Pasadena, who is a Curiosity co-investigator. "With only one Martian
rock of this type, it is difficult to know whether the same processes
were involved, but it is a reasonable place to start thinking about its
origin."
On Earth, rocks with composition like the Jake rock typically come from
processes in the planet's mantle beneath the crust, from crystallization
of relatively water-rich magma at elevated pressure.
Jake was the first rock analyzed by the rover's arm-mounted Alpha
Particle X-Ray Spectrometer (APXS) instrument and about the thirtieth
rock examined by the Chemistry and Camera (ChemCam) instrument. Two
penny-size spots on Jake were analyzed Sept. 22 by the rover's improved
and faster version of earlier APXS devices on all previous Mars rovers,
which have examined hundreds of rocks. That information has provided
scientists a library of comparisons for what Curiosity sees.
"Jake is kind of an odd Martian rock," said APXS Principal Investigator
Ralf Gellert of the University of Guelph in Ontario, Canada. "It's high
in elements consistent with the mineral feldspar, and low in magnesium
and iron."
ChemCam found unique compositions at each of 14 target points on the rock, hitting different mineral grains within it.
"ChemCam had been seeing compositions suggestive of feldspar since
August, and we're getting closer to confirming that now with APXS data,
although there are additional tests to be done," said ChemCam Principal
Investigator Roger Wiens (WEENS) of Los Alamos National Laboratory in
New Mexico.
Examination of Jake included the first comparison on Mars between APXS
results and results from checking the same rock with ChemCam, which
shoots laser pulses from the top of the rover's mast.
The wealth of information from the two instruments checking chemical
elements in the same rock is just a preview. Curiosity also carries
analytical laboratories inside the rover to provide other composition
information about powder samples from rocks and soil. The mission is
progressing toward getting the first soil sample into those analytical
instruments during a "sol," or Martian day.
"Yestersol, we used Curiosity's first perfectly scooped sample for
cleaning the interior surfaces of our 150-micron sample-processing
chambers. It's our version of a Martian carwash," said Chris Roumeliotis
(room-eel-ee-OH-tiss), lead turret rover planner at NASA's Jet
Propulsion Laboratory in Pasadena, Calif.
Before proceeding, the team carefully studied the material for scooping
at a sandy patch called "Rocknest," where Curiosity is spending about
three weeks.
"That first sample was perfect, just the right particle-size
distribution," said JPL's Luther Beegle, Curiosity sampling-system
scientist. "We had a lot of steps to be sure it was safe to go through
with the scooping and cleaning."
Following the work at Rocknest, the rover team plans to drive Curiosity
about 100 yards eastward and select a rock in that area as the first
target for using the drill.
During a two-year prime mission, researchers will use Curiosity's 10
instruments to assess whether the study area ever has offered
environmental conditions favorable for microbial life. JPL, a division
of Caltech, manages the project and built Curiosity. For more about the
Mars Science Laboratory Curiosity rover mission, visit:
and
You can follow the mission on Facebook and Twitter at:
and
DC Agle / Guy Webster 818-393-9011/818-354-6278
Jet Propulsion Laboratory, Pasadena, Calif.
agle@jpl.nasa.gov / guy.webster@jpl.nasa.gov
Dwayne Brown 202-358-1726
NASA Headquarters, Washington
Dwayne.c.brown@nasa.gov
NASA
Jet Propulsion Laboratory, Pasadena, Calif.
agle@jpl.nasa.gov / guy.webster@jpl.nasa.gov
Dwayne Brown 202-358-1726
NASA Headquarters, Washington
Dwayne.c.brown@nasa.gov
NASA
Guillermo Gonzalo Sánchez Achutegui
ayabaca@gmail.com
ayabaca@hotmail.com
ayabaca@yahoo.com
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