Opportunity report, Sol 5132, by A.J.S. Rayl, The Planetary Society

20180704_2-Dual-PEDE-before-after-0528-07012-018-revisedJuly 4, 2018: Opportunity Sleeps as Storm Chasers Study Planet-Encircling Dust Cloud: As a monster dust storm grew to encircle the Red Planet in June, Opportunity spent most of the month in the dark, presumably sleeping in a hibernation mode as the sky over the Mars Exploration Rover’s campsite in west rim of Endeavour Crater, about halfway down Perseverance Valley, became darker and darker.

What began as a small, local dust storm in the northern hemisphere on May 29th had grown a little by the next day, and a little more the next. By June 1st, Bruce Cantor, who posts Mars Weather Reports each week from data acquired by the Mars Color Imager (MARCI) onboard the Mars Reconnaissance Orbiter (MRO), decided the MER team needed to know about this one. He made the call. (…)

Since then, the rover has been silent. “There has been no further communication from Opportunity and we do not expect to hear anything for several more weeks, maybe a month or more,” JPL’s Chief of MER Engineering Bill Nelson, said at month’s end.

The good news is that it’s springtime at Endeavour Crater and the power models continue to indicate Mars’ cold temperatures won’t get cold enough to harm Opportunity’s instruments. All that dust in the atmosphere is preventing the Sun from heating the surface during the day, because it’s heating the dust at the top of the dust cloud. So while the temperatures are cooler during the day, the dust cloud radiates at night so the rover actually experiences warmer nighttime temps. Perfect. That’s when the rover needs the warmth the most.

The bad news is it’s really, really dark and the solar powered rover is likely not able to produce much, if any, solar power. “For Opportunity, this is a very big deal,” said Herman… [More at link]

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HiRISE: Impact crater’s steep slopes

tumblr_pb938ubaVA1rlz4gso1_1280Steep slopes of impact crater. Beautiful Mars series. [More at links]

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NASA Mars Report: July 3, 2018

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THEMIS: Flows upon flows on Olympus Mons

Flows upon flows on Olympus Mons (THEMIS_IOTD_20180705)THEMIS Image of the Day, July 5, 2018. The lava flows seen in the VIS image are located on the northeastern flank of Olympus Mons. The lavas flowed from the lower left side of the image to the upper right, while lighting comes from the right.

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THEMIS: Pavonis Mons flank meets volcanic plains

Pavonis Mons flank (THEMIS_IOTD_20180704)THEMIS Image of the Day, July 4, 2018. Today’s VIS image is of the eastern flank of Pavonis Mons where the volcano meets the surrounding volcanic plains.

The arced features towards the top of the image are fractures and lava tubes that were revealed by collapse of the roof of the tube into the underlying void.

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Curiosity update: Back on top

NLB_583751465EDR_F0711586NCAM00285M_-br2Sols 2100-01, July 2, 2018, update by MSL scientist Scott Guzewich: Curiosity is back on top of the Vera Rubin Ridge once more, having completed our drive over the weekend as we move toward our next drilling target in the “Pettegrove Point” geological member. This Navcam image shows the occasionally steep edge of the Vera Rubin Ridge on the left side of the image and the dusty haze beyond it that has shrunk our horizons for the last few weeks.

Today’s 2-sol plan involved contact science with APXS on rock targets “Dumbarton Rock”, “Duntarvie Castle”, and “Duntelchaig” and four ChemCam LIBS rasters on nearby targets. After climbing back onto the ridge, there is no lack of interesting bedrock targets nearby and the ground is much smoother and suitable for driving compared to where we’ve been for the last many weeks while we studied our “Duluth” drill hole and its surroundings… [More at link]

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HiRISE: Translucent ice

tumblr_pb3elmsPYp1rlz4gso2_1280Translucent ice. Also note the polygonal ground, another feature of expanding and contracting subsurface ice.

Beautiful Mars series. [More at links]

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Curiosity: In the murk

2098-mastcam34Sol 2098, July 1, 2018. The wide-angle Mastcam took a few frames to make composite view looking northeastward across the upper surface of Vera Rubin Ridge (4.7 MB). Corrected for the strong reddish tint caused by aerial dust, the scene would resemble the view below (8 MB). Click either image to enlarge it.

Sol 2098 raw images (from all cameras).

2098-mastcam34-whitelight

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Weather update from Gale Crater

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THEMIS: Terra Sabaea lava tube turned into an open channel

Lava tube channel in Terra Sabaea (THEMIS_IOTD_20180703)THEMIS Image of the Day, July 3, 2018. This VIS image is located in Terra Sabaea near the margin of Syrtis Major Planum. The channel-like feature in the bottom of the image is an unnamed feature.

There is a high spot within the channel that would not let a fluid pass from one side to the other. This indicates that this is not a water carved channel, but was most likely an underground lava tube, where collapse of the roof has revealed the underlying feature.

The 90 degree turns in the channel feature, and the small linear ridges just to the top of the channel indicate tectonic forces are part of the processes at work in this region.

More THEMIS Images of the Day by geological topic.

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