Weather at Gale Crater

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HiRISE: For your consideration

ESP_054574_2330For your consideration. An alien landscape with dust devil streaks and craters slowing fading away into the mists of time. A twilight zone of geology, if you will. (Features like this are often called “thumbprint terrain”.)

HiRISE Picture of the Day archive [More at links]

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Curiosity: Looking ahead, and farther ahead

2306-navcamSol 2306, January 31, 2019. Curiosity’s Navcam took a composite showing the rolling surface of the clay-bearing unit directly before the rover (above), while the Remote Micro-Imager looked off into the distance to profile a hill (below).  Click either image to enlarge it.

Sol 2306 raw images (from all cameras).

2306-rmi

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THEMIS: Lava flows and channels on Daedalia Planum

Lava channels and flows on Daedalia Planum (THEMIS_IOTD_20190201)THEMIS Image of the Day, February 1, 2019. Today’s VIS image shows a small portion of the extensive volcanic plains of Daedalia Planum.

These lava flows originated from Arsia Mons, the southernmost of the three large Tharsis volcanoes.

See more THEMIS Images of the Day by geological subject.

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MARCI weather report, January 21-27, 2019

MARCI-January-25-2019Elevated levels of atmospheric dust, remnants of a recently abated southern hemisphere regional storm, lingered over most of Mars this past week. At high southern latitudes, the perennial south polar ice cap had reached its minimum summer configuration. While in the northern lowlands, the seasonal receding north polar cap edge could be observed under a mixture of dust and water-ice clouds associated with the north polar hood and eastward propagating polar vortex. Each afternoon, the Tharsis Montes and other areas in the tropics were free of water-ice clouds. This was due… [More at link, including video]

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HiRISE: Landforms northwest of Herschel Crater

ESP_054563_1700Landforms northwest of Herschel Crater. Herschel Crater is a 304 kilometer impact basin in the Martian Southern Hemisphere. We have imaged the crater enough times to learn that dunes here are not stationary but move over time. The crater is jointly named after the seventeenth/eighteenth century father and son astronomers William Herschel and John Herschel.

HiRISE Picture of the Day archive [More at links]

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Curiosity measures a Mars mountain’s gravity

PIA23041_hiresEd. note: More about this result here, here, and here.

Apollo 17 astronauts drove a moon buggy across the lunar surface in 1972, measuring gravity with a special instrument. There are no astronauts on Mars, but a group of clever researchers realized they have just the tools for similar experiments with the Martian buggy they’re operating.

In a new paper in Science, the researchers detail how they repurposed sensors used to drive the Curiosity rover and turned them into gravimeters, which measure changes in gravitational pull. That enabled them to measure the subtle tug from rock layers on lower Mount Sharp, which rises 3 miles (5 kilometers) from the base of Gale Crater and which Curiosity has been climbing since 2014. The results? It turns out the density of those rock layers is much lower than expected.

Just like a smartphone, Curiosity carries accelerometers and gyroscopes. Moving your smartphone allows these sensors to determine its location and which way it’s facing. Curiosity’s sensors do the same thing but with far more precision, playing a crucial role in navigating the Martian surface on each drive. Knowing the rover’s orientation also lets engineers accurately point its instruments and multidirectional, high-gain antenna.

By happy coincidence, the rover’s accelerometers can be used like Apollo 17′s gravimeter. The accelerometers detect the gravity of the planet whenever the rover stands still. Using engineering data from the first five years of the mission, the paper’s authors measured the gravitational tug of Mars on the rover. As Curiosity ascends Mount Sharp, the mountain adds additional gravity – but not as much as scientists expected… [More at links]

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Curiosity update: Stepping up to the edge

NLA_602034791EDR_F0732394NCAM00265M_Sols 2306-07, January 30, 2019, update by MSL engineer Ashley Stroupe: In today’s plan, Curiosity is venturing further into the clay unit territory.

Prior to departure, we’ll be looking at several targets with Mastcam color and ChemCam to try to characterize the chemistry and texture of this new terrain. We’ll also be taking a ChemCam RMI mosaic of “Buchan Ridge,” an upcoming area of exploration within the clay unit, to aid in navigation and traverse planning.

We’re driving up to the crest of a ridge so that we will be able to see down the other side, which is currently hidden from our view. The new terrain is so featureless, that visual odometry is having trouble tracking our position and measuring slip, which caused the rover to stop the sol 2304 drive early. The image above (Sol 2304 post-drive Navcam) shows the ridge and the smooth terrain. The rover planners are using some extra imaging to help us characterize how the rover performs on this new terrain. We are hoping something of interest will be in our workspace for contact science in the weekend plan. Much of… [More at link]

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THEMIS: Eroding layers in Spallanzani Crater

Eroding infill of Spallanzani Crater (THEMIS_IOTD_20190131)THEMIS Image of the Day, January 31, 2019. This VIS image shows part of the floor of Spallanzani Crater. At some point after the crater was created the floor was covered by a fill material.

The material was laid down in layers, which are easily identifiable at the eroded margins of the desposit. Spallanzani Crater is located near the southeast margin of Hellas Planitia in Promethei Terra.

See more THEMIS Images of the Day by geological subject.

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Curiosity: Scoping Greenheugh

2304-rmi-greenheughSol 2304, January 29, 2019. Curiosity used its Remote Micro-Imager to scope out a distant butte dubbed Greenheugh. Note the layers of sedimentary rocks. Click the image to enlarge it.

Sol 2304 raw images (from all cameras).

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