Follow this link to skip to                                      the main content

Mission News

Text Size

NASA Spacecraft Read Layered Clues to Changes on Mars
Layers Exposed at Polar Canyon
   More Images:

+ Looking East to 'Tyrone'
+ Clay at Nili Fossae
+ Gypsum at Olympia Undae
+ Pits in Polar Cap
+ Radar view near South Pole, Orbit 1360
+ Radar view near South Pole, Orbit 1334
+ Radar view near North Pole, Orbit 1512
+ 'King George Island' Brushed
+ Spirit's Winter Home
+ 'Cape Verde' - Mid-Afternoon
-+ 'Cape Verde' - Mid-Afternoon (False Color)
+ Spirit's Tracks
+ Spirit's Winter Work Site
+ Columbia Hills
+ 'Bottomless Bay'
+ 'Cape Verde' - Late Morning
+ 'Cape St. Mary''
+ 'Cape St. Mary' (Altered Contrast)
+ 'Cape Verde' - Late Morning (False Color)
+ 'Cape St. Mary's' (False Color)
+ 'Bottomless Bay' (Altered Contrast)
+ Big Spherules
+ Radar view near Mars' North Pole, Orbit 1512
+ Radar view near Mars' South Pole, Orbit 1360
+ Radar view near Mars' South Pole, Orbit 1334
SAN FRANCISCO -- Layers on Mars are yielding history lessons revealed by instruments flying overhead and rolling across the surface.

Some of the first radar and imaging results from NASA's newest Mars spacecraft, the Mars Reconnaissance Orbiter, show details in layers of ice-rich deposits near the poles. Observed variations in the layers' thickness and composition will yield information about recent climate cycles on the red planet.

Image right: This false-color subframe of an image from the High Resolution Imaging Science Experiment camera on NASA's Mars Reconnaissance Orbiter shows the north polar layered deposits at top and darker materials at bottom. Image credit: NASA/JPL-Caltech/Univ. of Arizona
+ Full image and caption

NASA's Mars Exploration Rover Opportunity has photographed patterns in the layering of crater-wall cliffs that are the clearest evidence of ancient sand dunes the rover has seen since arriving at Mars nearly three years ago. The science team for Opportunity's twin, Spirit, is using new orbital images of the rover's surroundings to interpret how some rocks with minerals altered by water fit into the area's complex layered structure.

"The combination of instruments on Mars Reconnaissance Orbiter is such a great advantage," said Dr. Jack Mustard of Brown University, Providence, R.I. He is deputy principal investigator for the Compact Reconnaissance Imaging Spectrometer for Mars, a mineral-identifying instrument on Mars Reconnaissance Orbiter. Researchers are using mineral information from analyses of spectrometer observations, combined with images from the orbiter's High Resolution Imaging Science Experiment, to seek the source of the mineral gypsum in dunes near the Martian north pole and clay minerals elsewhere. Gypsum and clay minerals are indicators of formerly wet conditions.

Other new images from that camera show mysterious pitting in the layered terrain near the north pole. Nearby, a steep slope exposing the layers appears to be shedding blocks of icy material that disappear instead of accumulating at the bottom of the slope.

"Observations of the polar layered deposits are telling us about the material properties there," said Dr. Ken Herkenhoff of the U.S. Geological Survey, Flagstaff, Ariz. "These deposits record relatively recent climate variations on Mars, like recent ice ages on Earth."

The Shallow Subsurface Radar instrument on Mars Reconnaissance Orbiter has begun probing through similar layered deposits at Mars' south pole. "The radar is penetrating through the entire thickness of these deposits and revealing the fine-scale internal layering," said Dr. Roger Phillips of Washington University, St. Louis, the deputy team leader for that instrument.

Far from the poles, Opportunity is navigating the scalloped rim of Victoria crater about half a mile in diameter, stopping at promontories along the way to look at cliff walls of adjacent promontories. The top part of the stack of layers exposed in the cliffs appears to be rocky rubble thrown outward by the impact that dug the crater. "We see an abrupt transition between the jumbled-up material and intact layers below it that are still in place from before the impact," said Dr. Steve Squyres of Cornell University, Ithaca, N.Y., principal investigator for the rovers. Some of the intact layering resembles fossilized dunes in the U.S. Southwest. 

Spirit recently found water-altered minerals in disturbed soils and granular rocks near where the rover spent the Martian winter. An image of the region from Mars Reconnaissance Orbiter is aiding interpretation of how different parts of the terrain, such as a bright platform nicknamed "Home Plate," are related to others. "It appears likely that these rocks came from one or more volcanic explosions that produced 'Home Plate,'" said Dr. Ray Arvidson, also of Washington University, deputy principal investigator for the rovers.

Dr. John Callas of NASA's Jet Propulsion Laboratory, Pasadena, Calif., project manager for the rovers, said, "The biggest news about the health of the rovers is that it is essentially unchanged from nine months ago. Each rover has operated more than 1,000 Martian days on the surface of Mars. They are well past their original design life of 90 Martian days, and there is always the possibility that a critical component on either rover could stop functioning at any time, so we operate the rovers with that in mind and value each additional day they continue to work."

Researchers are describing the latest findings of Mars Reconnaissance Orbiter and the twin rovers today at the American Geophysical Union meeting in San Francisco. New images from the orbiter and rovers can be seen from the images links above .

JPL, a division of the California Institute of Technology, manages the Mars Reconnaissance Orbiter and Mars Exploration Rover missions for the NASA Science Mission Directorate, Washington.  Lockheed Martin Space Systems, Denver, is the prime contractor for the orbiter. The Johns Hopkins University Applied Physics Laboratory, Laurel, Md., provided and operates the Compact Reconnaissance Imaging Spectrometer.  The High Resolution Imaging Science Experiment is operated by the University of Arizona, Tucson, and the instrument was built by Ball Aerospace and Technology Corp., Boulder, Colo. The Shallow Subsurface Radar was provided by the Italian Space Agency and its operations are led by the INFOCOM Dept., University of Rome "La Sapienza."

Media contact: Guy Webster 818-354-6278
Jet Propulsion Laboratory, Pasadena, Calif.