This scene from NASA's Mars Exploration Rover Opportunity looks upward at "Knudsen Ridge" on the southern edge of "Marathon Valley" from inside the valley.
The view combines multiple images taken with the panoramic camera (Pancam) on Opportunity's mast on Oct. 29 and Oct. 30, 2015, during the 4,182nd and 4,183rd Martian days, or sols, of the rover's work on Mars. By February 2016, the rover ascended slopes of about 30 degrees onto the flank of Knudsen Ridge, headed for targets of "red zone" material to examine there.
This version of the scene is presented in approximately true color. An enhanced-color version, which makes the red zone material easier to distinguish, is at PIA20319. A stereo version is at PIA20320.
The informal name Knudsen Ridge was chosen by the Opportunity science team to honor the memory of Danish astrophysicist and planetary scientist Jens Martin Knudsen (1930-2005), a founding member of the team.
Color in the scene comes from component images taken through three of the Pancam's color filters, centered on wavelengths of 753 nanometers (near-infrared), 535 nanometers (green) and 432 nanometers (violet). The view spans from southeast on the left to southwest on the right.
Marathon Valley cuts generally east-west through the western rim of Endeavour Crater. The valley's name refers to the distance Opportunity drove from its 2004 landing site to arrival at this location in 2014. The valley was a high-priority destination for the rover mission because observations from orbit detected clay minerals there.
NASA's senior Mars rover, Opportunity, is working adeptly in some of the most challenging terrain of the vehicle's 12 years on Mars, on a slope of about 30 degrees.
Researchers are using Opportunity this month to examine rocks that may have been chemically altered by water billions of years ago. The mission's current targets of investigation are from ruddy-tinted swaths the researchers call "red zones," in contrast to tan bedrock around these zones.
The targets lie on "Knudsen Ridge," atop the southern flank of "Marathon Valley," which slices through the western rim of Endeavour Crater.
"We're hoping to take advantage of the steep topography that Mars provides us at Knudsen Ridge to get to a better example of the red zone material," said Steve Squyres of Cornell University, Ithaca, New York, principal investigator for the mission.
The red zone material crumbles easily. At locations in Marathon Valley where Opportunity already got a close look at it, the reddish bits are blended with other loose material accumulating in low locations. A purer exposure of the red zone material, such as some apparent on the ridge, would provide a better target for the Alpha Particle X-ray Spectrometer on Opportunity's arm, which reveals the chemical composition of rocks and soil.
Opportunity began climbing Knudsen Ridge in late January with two drives totaling 31 feet (9.4 meters). The wheels slipped less than 20 percent up slopes as steep as 30 degrees, the steepest the rover has driven since its first year on Mars in 2004. The slip is calculated by comparing the distance the rotating wheels would have covered if there were no slippage to the distance actually covered in the drive, based on "visual odometry" imaging of the terrain the rover passes as it drives.
"Opportunity showed us how sure-footed she still is," said Mars Exploration Rover Project Manager John Callas at NASA's Jet Propulsion Laboratory, Pasadena, California. "The wheel slip has been much less than we expected on such steep slopes."
The rover made additional progress toward targets of red-zone material on Knudsen Ridge with a drive on Feb. 18.
Knudsen Ridge forms a dramatic cap overlooking the 14-mile-wide (22-kilometer-wide) Endeavour Crater. Its informal naming honors the memory of Danish astrophysicist and planetary scientist Jens Martin Knudsen (1930-2005), a founding member of the science team for Opportunity and the twin rover Spirit. "This ridge is so spectacular, it seemed like an appropriate place to name for Jens Martin," Squyres said.
Marathon Valley became a high-priority destination for the Opportunity mission when mineral-mapping observations by the Compact Reconnaissance Imaging Spectrometer for Mars (CRISM), aboard NASA's Mars Reconnaissance Orbiter, located clay minerals (a type of phyllosilicate) in this valley. Clay minerals often form in the presence of water, which is why this is such a promising area of exploration. Opportunity found evidence of ancient water shortly after landing, but there were signs that the water would have been more highly acidic. The investigation in Marathon Valley could add understanding about the ancient environmental context for the presence of non-acidic water, a factor favorable for microbial life, if any has ever existed on Mars.
"The locations of red zones in Marathon Valley correlate closely with the phyllosilicate signature we see from orbit," Squyres said. "That alone is not a smoking gun. We want to determine what it is about their chemistry that sets them apart and what it could have to do with water."
To test the idea that water affected the red zone material, the experiment underway aims to compare the chemistry of that material to the chemistry of the surrounding tan bedrock, which could represent an unaltered baseline. Opportunity used its diamond-toothed rock abrasion tool last month to scrape the crust off a tan bedrock target for an examination of the chemistry inside the rock.
The team is accomplishing productive science with Opportunity while avoiding use of the rover's flash memory, which was linked to several unplanned computer reboots last year. The only data being received from Opportunity is what can be transmitted each day before the solar-powered rover shuts down for energy-conserving overnight "sleep."