Curiosity update: In search of softer rocks

NLB_586227306EDR_F0720920NCAM00259M_-br2Sol 2128, July 31, 2018, update by MSL scientist Ryan Anderson: On Sol 2128, Curiosity will continue toward our third potential drill site within the Pettegrove Point member of Vera Rubin Ridge, where we are hoping to find slightly softer rocks. The day will begin with ChemCam observations of the target “Slioch,” which was already analyzed by APXS, as well as the layered rock “Craignure Bay.” Mastcam will document both of these targets, using a small mosaic around Craignure Bay to capture images of some of the tilted rocks nearby as well. Then Navcam will do some atmospheric observations. After that, the rover will drive toward our next drill site and take some… [More at link]

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Cross-bed geometry in upper Mt. Sharp

gale_xbeds_fig1Planetary Geomorphology Image of the Month, August 1, 2018: One of the most environmentally diagnostic features of sedimentary rocks is cross-bedding, which occurs when sediment is transported by wind, water, or volcanic processes, resulting in horizontal strata composed of inclined beds.

The geometry of cross-bedded sedimentary deposits provides information about the depositional setting and post-depositional history of the rocks, making the identification, measurement, and interpretation of cross-beds particularly interesting on Mars, where past conditions are of great scientific interest. This post describes cross-bedding in Upper Aeolis Mons in Gale crater.

One location on Mars where numerous examples of cross-bedding have been observed is Gale crater, a ~154 km diameter crater containing a ~5 km tall mountain of layered rock called Aeolis Mons (informally dubbed Mt. Sharp). The Curiosity rover landed in the northwestern crater floor in 2012 and has observed numerous outcrops of cross-stratified sandstone, providing evidence for an ancient fluvial system with sediment transport toward the southeast and occasional aeolian deposit… [More at link]

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THEMIS: And the rocks came tumbling down

Rockslide in Ganges Chasma (THEMIS_IOTD_20180801)THEMIS Image of the Day, August 1, 2018. This VIS image is located in central Ganges Chasma. A large landslide deposit fills the top third of the image.

The radial grooves on the top of the landslide are a common feature formed by the downslope movement of the landslide materials. The landslide was deflected in some areas by preexisting blocks on the chasma floor.

Ganges Chasma is part of the Valles Marineris chasma system, but is north of the main section of canyons.

See more THEMIS Images of the Day by geological subject.

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HiRISE: It’s all about that flow

tumblr_pcp7c4cZBr1rlz4gso1_1280It’s all about that flow. There are a number of crevasse-like features here.

Beautiful Mars series. [More at links]

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Curiosity: Looking for a new drill site

2126-navcam-southSol 2126, July 30, 2018. Having struck out at two drill sites, Curiosity’s scientists are seeking a new one, sending the rover on a 68-meter (224-foot) drive westward along the ridge top.

The Navcam composite above shows the post-drive view toward the south, with part of Mt. Sharp dimly visible in the center. The image below shows the view north, with the Murray Buttes visible but the inner rim of Gale still hidden by miles of dusty atmosphere. Click either image (3.7 MB) to enlarge it.

Sol 2126 raw images (from all cameras).

2126-navcam-north

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NASA: Open-source plans to build your own rover

rover20180731-16Have you ever wondered what it takes to build a rover like NASA’s Curiosity rover, part of the Mars Science Laboratory project?  One would rightfully assume it takes expertise in mechanical engineering, software development, and electronics to even begin to construct such a complex robot.  Now students, hobbyists, and enthusiasts can learn about these skills and get a taste of what it is like to construct such a rover using plans and instructions from JPL’s Open Source Rover Project. (…)

The JPL Open Source Rover (OSR) is a scaled down version of Curiosity, from its 6-wheel steering all the way to its Rocker-Bogie suspension.  JPL published this design under an open source license on GitHub where anybody can download baseline instructions and test plans for building their own OSR.

“We wanted to give back to the community and lower the barrier of entry by giving hands on experience to the next generation of scientists, engineers, and programmers,” states Tom Soderstrom, the project sponsor for the Open Source Rover.  Mik Cox, the project manager adds, “I would love to have had the opportunity to build this rover in high school, and I hope that through this project we provide that opportunity to others.” [More at link]

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Mars hasn’t enough CO2 for terraforming

MAVEN_Infographic_Print_FINAL_printA new study of the quantity of carbon dioxide on Mars has compiled a planet-wide inventory of the CO2 it holds in all its accessible reservoirs: atmosphere, ice, and locked up in surface carbonate rocks and other potential sources.

The results of the inventory strongly discourage a mainstay of science fiction stories as well as an often-suggested scheme for human settlement: terraforming the Red Planet to produce a thick enough atmosphere for liquid water to exist on the surface.

According to the researchers Mars simply doesn’t have enough carbon dioxide, even taking together all the known and acessible reservoirs. It isn’t even close.

Say Bruce Jakosky and Christopher Edwards in a new paper published in Nature Astronomy, “Releasing all the readily acceessible CO2 would merely triple the current atmosphere. And that would still amount to only one-fiftieth of what’s needed.”

The scientists explain that, “Even if enough CO2 were to be available, it would not be feasible to mobilize it. Doing so would require processing a major fraction of the surface rocks and materials, analogous to regional- or planet-scale strip mining.”

Jakosky and Edwards conclude, “Terraforming Mars using the planet’s known CO2 will need technologies well beyond our current grasp.” [More at links]

Graphic at head of story from NASA’s Goddard Space Flight Center.

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Curiosity update: Continuing to understand Pettegrove Point

NLB_586227729EDR_F0720920NCAM00343M_-br2Sol 2127, July 31, 2018, update by MSL scientist Christopher Edwards: Curiosity completed its drive successfully after the science team regrouped from the incomplete drill, which required a different than anticipated weekend plan. The rocks of the Vera Rubin Ridge are just turning out to be harder than expected! In today’s plan, we will continue to assess the compositional diversity of the Vera Rubin Ridge Pettegrove Point member. In this workspace, we planned activities for two contact science targets, with APXS and MAHLI imaging of the locations dubbed “Diabiag” and “Slioch”. The Diabiag target has a purple hue in Mastcam imagery and appears to be relatively dust free, while the Slioch target is darker. The team could not find a suitable place to brush the dust away with a DRT activity since the local bedrock was extremely rough… [More at link]

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THEMIS: Dunes of Moreux Crater

Dunefield in Moreux Crater (THEMISIOTD_20180731)THEMIS Image of the Day, July 31, 2018. Today’s VIS image shows part of the floor of Moreux Crater. Sand dunes are found in this region of the crater floor. Moreux Crater is located on the northern margin of Terra Sabaea.

See more THEMIS Images of the Day by geological subject.

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HiRISE: The bedforms, they are a-changin’

tumblr_pcov2nBbU31rlz4gso2_1280The bedforms, they are a-changin’. This is in Zephyria Planum. Beautiful Mars series. [More at links]

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