This mid-afternoon, 360-degree panorama was acquired by the Mast Camera (Mastcam) on NASA’s Curiosity Mars rover on April 4, 2016, as part of long-term campaign to document the context and details of the geology and landforms along Curiosity’s traverse since landing in August 2012.
The view combines dozens of images taken during the mission’s 1,302nd sol, or Martian day, by Mastcam’s left-eye camera from a location on top of what rover team members call “Naukluft Plateau” on lower Mount Sharp, which stands inside Gale Crater.
The foreground and middle distance show a geologic scene dominated by eroded remnants of a finely layered ancient sandstone deposit. Since landing, the rover traversed through terrains dominated by water-lain sedimentary rocks (mudstones and siltstones, and early on, conglomerates), some of which have contained minerals like clays that attest to the ancient presence of water. However, the rover crossed into very different geology while climbing onto the Naukluft Plateau. The sandstone here appears to be dominated by thick layers of windblown sand, suggesting that these deposits formed in a drier epoch. These rocks resemble the types of rocks that a dune field like the “Bagnold Dunes” (PIA20283) — visited by Curiosity in late 2015 and early 2016 –would form if buried.
The scene is presented with a color adjustment that approximates white balancing, to resemble how the rocks and sand would appear under daytime lighting conditions on Earth.
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Curiosity Mars Rover Crosses Rugged Plateau
NASA’s Curiosity Mars rover has nearly finished crossing a stretch of the most rugged and difficult-to-navigate terrain encountered during the mission’s 44 months on Mars.
The rover climbed onto the “Naukluft Plateau” of lower Mount Sharp in early March after spending several weeks investigating sand dunes. The plateau’s sandstone bedrock has been carved by eons of wind erosion into ridges and knobs. The path of about a quarter mile (400 meters) westward across it is taking Curiosity toward smoother surfaces leading to geological layers of scientific interest farther uphill.
The roughness of the terrain on the plateau raised concern that driving on it could be especially damaging to Curiosity’s wheels, as was terrain Curiosity crossed before reaching the base of Mount Sharp. Holes and tears in the rover’s aluminum wheels became noticeable in 2013. The rover team responded by adjusting the long-term traverse route, revising how local terrain is assessed and refining how drives are planned. Extensive Earth-based testing provided insight into wheel longevity.
The rover team closely monitors wear and tear on Curiosity’s six wheels. “We carefully inspect and trend the condition of the wheels,” said Steve Lee, Curiosity’s deputy project manager at NASA’s Jet Propulsion Laboratory, Pasadena, California. “Cracks and punctures have been gradually accumulating at the pace we anticipated, based on testing we performed at JPL. Given our longevity projections, I am confident these wheels will get us to the destinations on Mount Sharp that have been in our plans since before landing.”
Inspection of the wheels after crossing most of the Naukluft Plateau has indicated that, while the terrain presented challenges for navigation, driving across it did not accelerate damage to the wheels.
On Naukluft Plateau, the rover’s Mast Camera has recorded some panoramic scenes from the highest viewpoints Curiosity has reached since its August 2012 landing on the floor of Gale Crater on Mars.
The scenes show wind-sculpted textures in the sandstone bedrock close to the rover, and Gale Crater’s rim rising above the crater floor in the distance. Mount Sharp stands in the middle of the crater, which is about 96 miles (154 kilometers) in diameter.
The next part of the rover’s route will return to a type of lake-deposited mudstone surface examined previously. Farther ahead on lower Mount Sharp are three geological units that have been key destinations for the mission since its landing site was selected. One of the units contains an iron-oxide mineral called hematite, which was detected from orbit. Just above it lies a band rich in clay minerals, then a series of layers that contain sulfur-bearing minerals called sulfates. By examining them with Curiosity, researchers hope to gain a better understanding of how long ancient environmental conditions remained favorable for microbial life, if it was ever present on Mars, before conditions became drier and less favorable.
Each of Curiosity’s six wheels is about 20 inches (50 centimeters) in diameter and 16 inches (40 centimeters) wide, milled out of solid aluminum. Most of the wheel’s circumference is a metallic skin that is about half the thickness of a U.S. dime. Nineteen zigzag-shaped treads, called grousers, extend about a quarter inch (three-fourths of a centimeter) outward from the skin of each wheel. The grousers bear much of the rover’s weight and provide most of the traction and ability to traverse over uneven terrain.
The holes seen in the wheels so far perforate only the skin. Wheel-monitoring images obtained every 547 yards (500 meters) have not yet shown any grouser breaks on Curiosity. Earth-based testing examined long-term wear characteristics and the amount of damage a rover wheel can sustain before losing its usefulness for driving. The tests indicate that when three grousers on a wheel have broken, that wheel has reached about 60 percent of its useful mileage.
At a current odometry of 7.9 miles (12.7 kilometers) since its August 2012 landing, Curiosity’s wheels are projected to have more than enough life remaining to investigate the hematite, clay and sulfate units ahead, even in the unlikely case that up to three grousers break soon. The driving distance to the start of the sulfate-rich layers is roughly 4.7 miles (7.5 kilometers) from the rover’s current location.
Curiosity reached the base of Mount Sharp in 2014 after fruitfully investigating outcrops closer to its landing site and then trekking to the layered mountain.
source : NASA – Jet Propulsion Laboratory – California Institute of Technology