HiRISE: Complex gullies in a crater

ESP_058399_1415Most gullies in the southern mid-latitudes are on south-facing slopes, which are the coldest and have the most frost in the winter. However, some occur on other slopes.

This image shows large gullies on both the pole- and equator-facing slopes. An important puzzle in Mars science is whether or not all of these gullies form in the same geologic eras and by the same processes.

If you have red/green glasses, be sure to check out the anaglyph of this crater, which shows rugged topography! [More at link]

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THEMIS: Eroded layers in the south polar ice cap

Southern polar ice cap layers (THEMIS_IOTD_20190321)THEMIS Image of the Day, March 21, 2019. This VIS image shows layering in the south polar cap. Such layers are laid down by the seasonal changes and interweave dust and ice. Then they are eroded by winds and seasonal solar heating.

Explore more THEMIS Images of the Day by geological subject.

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HiRISE: Central deposits in Pasteur Crater

PSP_001756_1995Central deposits in Pasteur Crater. Caption throwback: The deposits in this image are eroding into knobs and ridges. The erosion is probably dominated by wind, as most of the ridges are parallel. This is common in wind-eroded features, with the ridges generally aligned with the prevailing wind. At high resolution, layering is revealed in many of the knobs and outcrops.

HiRISE Picture of the Day archive [More at links]

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MARCI weather report, March 11-17, 2019

MARCI-March-16-2019Last week on Mars, dust-lifting events continued over southern Aonia and Sirenum. The eastward movement of these storms lofted dust into the Argyre impact basin on multiple sols. The Hellas impact basin, on the other hand, was largely unobscured from atmospheric dust — making the floor discernible most afternoons. Moving our attention to the northern lowlands, a mixture of dust and water ice clouds remained along the receding seasonal north polar ice cap edge. Lee wave (water ice) clouds, known for their ripple-like appearance, were spotted trailing behind Tempe Terra and Alba Mons most afternoons… [More at link, including video]

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HiRISE: Fan, meet layered deposit

ESP_054702_1720Fan, meet layered deposit. This is a gorgeous fan reaching out into deposits in east Candor Chasma. Did landslides deform the layered material?

HiRISE Picture of the Day archive [More at links]

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Curiosity: Up close on Muir of Ord

FRB_606285814EDR_F0750060FHAZ00206M_2352MH0001630000804489R00_DXXXSol 2352, March 19, 2019. Curiosity gave the cracked rock dubbed Muir of Ord a close looking-over.

At top is part of the front Hazcam view, setting the scene, while at right are Mars Hand Lens Imager (MAHLI) closeups on the rock. Click any image to enlarge it.

2352MH0001630000804495R00_DXXXSol 2352 raw images (from all cameras).

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HiRISE: In the gullies and bedrock of Ius Chasma

ESP_058580_1720This image was acquired in Ius Chasma, a major section of the western portion of the giant Valles Marineris trough.

We see a portion of a steep slope with gullies extending downhill (towards bottom of image). Many of the gully floors are dark, and in some places that dark material extends onto the fan-shaped deposits of the gullies. These dark features are candidates for recurring slope lineae (RSL), which are seasonal features that grow incrementally. The relation between RSL and gullies is not clear: does the RSL activity carve the gullies, or do they simply follow the gully topography created by other processes? [More at link]

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THEMIS: Wood-grain patterns in ice and dust

Polar layers like wood grain (THEMIS_IOTD_20190320)THEMIS Image of the Day, March 20, 2019. This VIS image shows layering in the south polar cap. The layers are formed over thousands of years of seasonal change, reflecting ice and dust surface deposition.

Where the layers appear close to each other are steep trough sides. The steeper the slope, the closer the layers.

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Latest weather at Gale Crater and Elysium Planitia

Daily Elysium charts and data (temperature, wind speed, atmospheric pressure) here.

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2020 rover has landed in Jezero Crater again and again

22349_PIA22966-16In a little more than seven minutes in the early afternoon of Feb. 18, 2021, NASA’s Mars 2020 rover will execute about 27,000 actions and calculations as it speeds through the hazardous transition from the edge of space to Mars’ Jezero Crater. While that will be the first time the wheels of the 2,314-pound (1,050-kilogram) rover touch the Red Planet, the vehicle’s network of processors, sensors and transmitters will, by then, have successfully simulated touchdown at Jezero many times before.

“We first landed on Jezero Crater on Jan. 23rd,” said Heather Bottom, systems engineer for the Mars 2020 mission at the Jet Propulsion Laboratory in Pasadena, California. “And the rover successfully landed again on Mars two days later.”

Bottom was the test lead for Systems Test 1, or ST1, the Mars 2020 engineering team’s first opportunity to take the major components of the Mars 2020 mission for a test drive. Over two weeks in January, Bottom and 71 other engineers and technicians assigned to the 2020 mission took over the High Bay 1 cleanroom in JPL’s Spacecraft Assembly Facility to put the software and electrical systems aboard the mission’s cruise, entry capsule, descent stage and rover through their paces.

“ST1 was a massive undertaking,” said Bottom. “It was our first chance to exercise the flight software we will fly on 2020 with the actual spacecraft components that will be heading to Mars – and make sure they not only operate as expected, but also interact with each other as expected.” [More at link]

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