Sol 2063-2066: Sample drop-off testing
Some of the Duluth drill sample was dropped into CheMin on Sol 2061, but not enough for a proper mineralogical analysis. So the top priority for today's plan is to again test the new drop-off procedure. Since the drill feed mechanism became unreliable over a year ago, drill samples can no longer be sieved and processed in CHIMRA, as they were earlier in the mission. Instead, portions of the sample must be dropped from the tip of the drill directly into the analytical instruments. This new Feed-Extended Sample Transfer (FEST) procedure will be repeated on Sol 2064, over bedrock and over the closed SAM inlet cover. Mastcam images will be taken both before and after the drop-off in both locations, to allow the size of the sample portion to be estimated. The results of these tests will be used to inform future drop-off planning.
We're planning 4 sols today so that the tactical operations team can take a day off for the Memorial Day holiday. More change detection observations are scattered throughout the plan, with Right Mastcam images of dark sand ripples at "Noodle Lake" and the Duluth drill tailings on Sol 2063 at 11:00, 15:00 and 17:00, on Sol 2064 at 7:00 and noon, and on Sol 2065 at 7:00, ~11:00, noon, and 15:00. The goal of these observations is to constrain the frequency of wind gusts that are strong enough to move loose material. The Rover Planners also requested multiple Right Mastcam images of the sample drop-off location on
nearby bedrock for the same purpose; these are scheduled in the afternoons of Sols 2063, 2065, and 2066. ChemCam will also be busy this weekend, measuring the chemistry of a bumpy bedrock target named "Brule Mountain" and layered bedrock targets "Devil Track" and "Devilfish Tower" on Sol 2063. The latter two targets will be captured in a single Right Mastcam image soon afterward. On Sol 2064, ChemCam will observe some pebbles dubbed "Paupores" and Right Mastcam will acquire a single image covering both Brule Mountain and Paupores. Early on Sol 2065, Mastcam and Navcam will measure the amount of dust in the atmosphere, and Navcam will search for clouds. Later that morning, Right Mastcam will take a picture of a nearby bedrock block dubbed "Deerwood." In the afternoon, Mastcam will image the Sun and sky to measure the scattering properties and size distribution of dust in the atmosphere over Gale Crater, with supporting Navcam imaging.
https://mars.nasa.gov/msl/mission/mars-rover-curiosity-mission-updates/
just found something that interesting
A selfie on Mars, taken by NASA's Mars rover, Curiosity, on January 23, 2018, or Sol 1943, using its Mars Hand Lens Imager. Image stitched together from a series of panoramic images; sky artificially extended
Two sizes of wind-sculpted ripples are evident in this view of the top surface of a Martian sand dune. Sand dunes and the smaller type of ripples also exist on Earth. The larger ripples—roughly 10 feet (three meters) apart—are a type not seen on Earth nor previously recognized as a distinct type on Mars. The mast camera (mastcam) on NASA's Curiosity rover took the multiple component images of this scene on December 13, 2015, during the 1,192nd Martian day of the rover's work on Mars.The location is part of Namib Dune in the Bagnold Dune Field, which forms a dark band along the northwestern flank of Mount Sharp
This image was taken by Curiosity's mastcam on Sol 1648, or March 26, 2017
Curiosity pauses at the site from which it reached down to drill into a rock target called "Buckskin" on lower Mount Sharp in this low-angle self-portrait taken August 5, 2015, and released August 19, 2015. The selfie combines several component images taken by Curiosity's Mars Hand Lens Imager (MAHLI) during the 1,065th Martian day of the rover's work on Mars
Curiosity recorded this view of the sun setting at the close of the mission's 956th Martian day, on April 15, 2015, from the rover's location in Gale Crater, Mars.
On September 9, 2012, when it was just starting out, a close view of two of the left wheels of Curiosity. In the distance is the lower slope of Mount Sharp
Years later, on April 18, 2016, NASA used the MAHLI camera to check the condition of the wheels once again. This image of Curiosity's left-middle and left-rear wheels is part of an inspection set taken during Sol 1,315. Holes and tears in the wheels worsened significantly during 2013 as Curiosity was crossing terrain studded with sharp rocks on its route near its 2012 landing site to the base of Mount Sharp. Team members are keeping a close eye for when any of the zig-zag-shaped treads, call grousers, begin to break. Longevity testing with identical wheels on Earth indicates that when three grousers on a given wheel have broken, that wheel has reached about 60 percent of its useful mileage. Curiosity's six aluminum wheels are about 20 inches (50 centimeters) in diameter and 16 inches (40 centimeters) wide. Each of the six wheels has its own drive motor, and the four corner wheels also have steering motors
https://www.theatlantic.com/photo/2018/01/2000-days-on-mars-with-the-curiosity-rover/551984/