Opportunity: Team performs more frequent communication attempts throughout each day

NASA Mars Exploration Rover Status Report, December 12, 2018: Mars atmospheric opacity (tau) over the rover site remains at a storm-free range around 1.0.

No signal from Opportunity has been heard since Sol 5111 (June 10, 2018). Opportunity likely experienced a low-power fault, a mission clock fault and an up-loss timer fault. Since the loss of signal, the team has been listening for the rover over a broad range of times, frequencies and polarizations using the Deep Space Network (DSN) Radio Science Receiver.

They have been commanding “sweep and beeps” throughout the daily DSN pass with both right-hand and left-hand circular polarization to address a possible complexity with certain conditions within mission clock fault on the rover. The team has expanded the breath of sweep and beeps commanding, covering more times a day on Mars.

Mars is now in the seasonal period of past dust clearing events for the rover. Since loss of signal, 436 recovery commands have been radiated to the rover.  [More at link]

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HiRISE: Just another quiet day on Mars

tumblr_pjqkqck0CH1rlz4gso1_1280Just another quiet day on Mars. This cluster of [impact] craters is located, ironically, in Utopia Planitia.

Beautiful Mars series. [More at links]

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Curiosity update: Go for drill on the red Jura!

FRA_598034175EDR_F0731206FHAZ00206M_-br2Sol 2260-62, December 17, 2018, update by MSL scientist Catherine O’Connell-Cooper: In our last plan, we carried out triage activities on the red Jura target, “Rock Hall,” including APXS of the target to determine composition, and engineering tests to assess the stability of the rock and its hardness, both of which would affect our ability to drill.

It was decided that this would be a suitable candidate, both geochemically and physically, so today’s plan will centre around the drilling of what will hopefully be our 19th drill sample for analysis on Mars!

On sol 2260, MAHLI will take a series of images to characterize locations chosen by the rover planners as the areas in which they would eventually like to dump excess sample generated by the drilling. The drilling itself will take place on the morning of the second sol (sol 2261)… [More at link]

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THEMIS: Cloudy day over the south polar ice cap

Cloud over south polar cap (THEMIS_IOTD_20181217)THEMIS Image of the Day, December 17, 2018. This VIS image shows a layer of clouds over the south polar cap.

See more THEMIS Images of the Day by geological subject.

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HiRISE: Acheron Catena

tumblr_pjadvwdiuu1rlz4gso1_1280Acheron Catena. Beautiful Mars series. [More at links]

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Mars 2020: Jezero Crater flyover

An animated flyover of the Martian surface explains why Mars’ Jezero Crater, a 28-mile-wide ancient lake-delta system, is the best place for the Mars 2020 rover to find and collect promising samples for a possible future return to Earth. [More at link]

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MARCI weather report, December 3-9, 2018

MARCI-December-5-2018Dust lifting events were slightly more abundant for the northern hemisphere of Mars this past week. Near the beginning of the week, dust storm activity observed over Tempe Terra dipped southward towards Chryse Planitia by the following sol. By mid-week, a cloud of dust had propagated into the eastern canyons of Valles Marineris. Two other pulses of dust storms were spotted along the Acidalia storm-track in the second half of the week. Amazonis Planitia and the Phlegra Montes also experienced a few fleeting dust storms. Further north, the polar hood displayed a mixture of dust and water ice… [More at link, including video]

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THEMIS: Tapestry of dunes in Proctor Crater

Tapestry of dunes in Proctor Crater (THEMIS_IOTD_20181214)THEMIS Image of the Day, December 14, 2018. This VIS image shows part of the extensive dune field on the floor of Proctor Crater. Proctor Crater is located in Noachis Terra.

See more THEMIS Images of the Day by geological subject.

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Curiosity update: Is THIS the red Jura we are looking for?

2256ML0120800040804833E01_DXXX-br2Sol 2258-59, December 13, 2018, update by MSL scientist Michelle Minitti: The drive around to the north side of “Rock Hall” in yesterday’s plan was successful, placing us at a lower tilt and with room in the workspace to place all the piles of sample we drop on the surface (purposely!) in the aftermath of drilling. Yesterday’s observations of Rock Hall gave us confidence that we were at a promising red Jura target for drilling. ChemCam rasters across three different targets on Rock Hall indicated the slab had chemistry and spectral character consistent with red Jura. Mastcam images focused on the slab demonstrated that while it was dusty in flatter areas, and covered with scattered, loose gray and red pebbles in others, the slab had the red, shiny appearance we associate with red Jura. This placed us farther down the path toward drilling red Jura than we had been with any of our previous sites… [More at link]

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HiRISE: InSight lander on Mars

ESP_058005_1845This is a HiRISE image of the NASA InSight lander, plus other pieces of hardware on Mars after its successful landing on 26 November 2018.It looks like the heat shield (upper right) has its dark outside facing down, since it is so bright (saturated, probably a specular reflection).

The lander (middle) disturbed dust over a fair distance and has darkened the surface, as seen previously at the Phoenix and Curiosity landing sites. The bright spot associated with the lander is probably another specular reflection, and there are two smaller bluish extensions that are the solar arrays, plus their shadows.

The backshell attached to the parachute (lower left) may have yet another specular reflection; the streak extending to the south well beyond the parachute is probably a pre-existing dust devil track. The lander is about 6 meters wide when the solar arrays are fully deployed.  [More at link]

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