06.21.2017 A.I. laser targeting
06.01.2017 Diagram of Lake Stratification on Mars
03.21.2017 Break in Raised Tread on Curiosity Wheel
02.27.2017 Swirling Dust in Gale Crater, Mars, Sol 1613
02.27.2017 Dust Devil Passes Near Martian Sand Dune
02.27.2017 Sand Moving Under Curiosity, One Day to Next
12.13.2016 Now and Long Ago at Gale Crater, Mars
12.13.2016 Where's Boron? Mars Rover Detects It
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
Curiosity's ChemCam Removes DustThis pair of images taken a few minutes apart show how laser firing by NASA's Mars rover Curiosity removes dust from the surface of a rock. The images were taken by the remote micro-imager camera in the laser-firing Chemistry and Camera (ChemCam) instrument during the 84th Martian day, or sol, of Curiosity's work on Mars (Oct. 31, 2012). The area covered in each image is about 2.8 inches (7 centimeters) across, on a rock target called "Rocknest_3."
Between the time the remote micro-imager took the image on the left and the time it took the image on the right, ChemCam fired its laser 300 times - 10 bursts of 30 shots - along a vertical line. The image on the right shows that a stripe of dust was removed. The interaction of the laser beam with the surface is on the order of 0.02 inch (half a millimeter), but the stripe is more than 10 times wider, on the order of 0.3 inch (7 millimeters). A shock wave that occurs when the laser hits the rock is responsible for the wider area of dust removal.
Dust tends to cover everything on Mars. ChemCam has the capability to remove this layer to access the underlying rock and expose dust-free surfaces to other optical investigations.
Image Credit: NASA/JPL-Caltech/LANL/CNES/IRAP/LPGNantes/CNRS/IAS