10.03.2016 Curiosity Self-Portrait at 'Murray Buttes'
10.03.2016 Butte 'M9a' in 'Murray Buttes' on Mars
09.19.2016 Ribbon Cutting
09.09.2016 Farewell to Murray Buttes (Image 5)
09.09.2016 Farewell to Murray Buttes (Image 4)
09.09.2016 Farewell to Murray Buttes (Image 3)
09.09.2016 Farewell to Murray Buttes (Image 2)
09.09.2016 Farewell to Murray Buttes (Image 1)
08.26.2016 Out-of-this-World Records
03.30.2016 Erisa Hines
03.30.2016 Buzz Aldrin
02.12.2016 Women in Science
02.09.2016 Adam Steltzner, a JPL engineer
01.27.2016 Night Close-up of Martian Sand Grains
01.27.2016 Curiosity Self-Portrait at Martian Sand Dune
12.17.2015 Alteration Effects at Gale and Gusev Craters
12.17.2015 Full-Circle View Near 'Marias Pass' on Mars
12.11.2015 Surface Close-up of a Martian Sand Dune
12.11.2015 Martian Sand Disturbed by Rover Wheel
11.24.2015 Carbon Exchange and Loss Processes on Mars
11.17.2015 Chemical Laptop 1
11.11.2015 Thick, Dark Veins at 'Garden City,' Mars
11.11.2015 Dark, Thin Fracture-Filling Material
10.08.2015 Secrets of 'Hidden Valley' on Mars
10.08.2015 Strata at Base of Mount Sharp
10.02.2015 Mount Sharp Comes In Sharply
Windblown Sand from the 'Rocknest' DriftSee unannotated version
The Mars Hand Lens Imager (MAHLI) on NASA's Mars rover Curiosity acquired close-up views of sands in the "Rocknest" wind drift to document the nature of the material that the rover scooped, sieved and delivered to the Chemistry and Mineralogy Experiment (CheMin) and the Sample Analysis at Mars (SAM) in October and November 2012.
The picture on the left, acquired on the 58th Martian day or sol of the mission (Oct. 4, 2012), covers an area of about 0.75 by 0.87 inches (1.9 by 2.2 centimeters) and shows some of the variety of coarse sand grains observed on a portion of the Rocknest wind drift that was flattened by the left front rover wheel. Though Mars is thought of as the Red Planet, the sands of Mars are not necessarily red. This one small area shows clear, translucent grains, gray sand and white sand, in addition to two blue-gray glassy spheres and a glassy ellipsoid. The spherical and ellipsoidal grains were likely formed from molten droplets that cooled above the Martian surface to form glass, either during an explosive volcanic eruption or an impact cratering event. Similar grains are found in association with impacts on Earth and explosive volcanoes on the moon. The larger glassy sphere is 0.026 inches (655 micrometers) in diameter.
The picture on the right, acquired on Sol 73 (Oct. 20, 2012), shows a magnified view of the fraction of smaller sand grains examined by Curiosity. These are grains that were collected in the rover's third scoop. They were passed through a sieving system in the Collection and Handling for In-Situ Martian Rock Analysis (CHIMRA) tool on the rover's turret; only grains smaller than 0.006 inches (150 micrometers) passed through the sieves. In this image, the sieved grains are viewed on Curiosity's approximately 2.9-inch-diameter (about 7.5-centimeter-diameter) observation tray; the image shown here covers a much smaller part of the tray, just 0.26 by 0.30 inches (6.5 by 7.6 millimeters). Many of these fine sand grains are angular pieces of crystalline minerals, ideally suited for analysis by the Chemistry and Mineralogy Experiment (CheMin).
Image Credit: NASA/JPL-Caltech/MSSS