THEMIS: Dunes and Escorial Crater ejecta in false color

Ejecta from Escorial Crater in false color (THEMIS_IOTD_20180913)THEMIS Image of the Day, September 13, 2018. The ‘brown’ in this VIS image is part of the ejecta surrounding Escorial Crater. The material of the ejecta blanket is much more resistant to local winds and remains as a plateau above the lower elevation plains.

Sand dunes fields are very common around the north pole. The dunes in this image are part of Hyperboreae Undae.

The THEMIS VIS camera contains 5 filters. The data from different filters can be combined in multiple ways to create a false color image. These false color images may reveal subtle variations of the surface not easily identified in a single band image.

See more THEMIS Images of the Day by geological subject.

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MARCI weather report, September 3-9, 2018

MARCI-September-5-2018Slightly hazy conditions continued across many regions of Mars last week. Near the start and end of the week, a couple small dust lifting events occurred over the low-latitudes of Noachis Terra. Looking to the eastern hemisphere, a transient local-scale dust storm southwest of Elysium Mons was spotted pushing southward. On the following sol, only a diffuse dust cloud remained and swept eastward away from Gale Crater. Meanwhile, repeated dust storm activity was observed along the seasonal south polar ice cap edge, over…. [More at link including video]

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Curiosity: Inverness gets the brush-off

2168MH0001900010802875C00_DXXXSol 2168, September 11, 2018. Before and after, by MAHLI: Inverness gets the brush-off as part of the drill-site assessment.  Click either image to enlarge it.

Sol 2168 raw images (from all cameras).

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THEMIS: Siton Undae dunes in false color

North polar dunes in false color (THEMIS_IOTD_20180912)THEMIS Image of the Day, September 12, 2018. The blue features in this VIS image are sand dunes located near Escorial Crater and the north polar cap. The dune field is called Siton Undae.

The THEMIS VIS camera contains 5 filters. The data from different filters can be combined in multiple ways to create a false color image. These false color images may reveal subtle variations of the surface not easily identified in a single band image.

See more THEMIS Images of the Day by geological subject.

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Opportunity: A new listening plan

NASA Mars Exploration Rover Status Report, September 4, 2018: No signal from Opportunity has been heard since Sol 5111 (June 10, 2018), though NASA has approved a strategy for listening for the rover through January of 2019.

It is expected that Opportunity has experienced a low-power fault and perhaps, a mission clock fault and then an up-loss timer fault. The science team continues to listen for the rover either during the expected fault communication windows or listening over a broader range of times using the Deep Space Network Radio Science Receiver.

The science team is also sending a command three times a week to elicit a beep if the rover happens to be awake, and will soon be expanding the commanding to include “sweep and beeps” to address a possible complexity with certain conditions within the mission clock fault. These will continue through January of 2019.

The dust storm on Mars continues its decay with atmospheric opacity (tau) over the rover site continuing to decrease. Once the tau has fallen below an estimated measurement of 1.5 twice – with one week apart between measurements – a period of 45 days will begin representing the best time for us to hear from the rover.

This also represents the best time to attempt active commanding during a specific mission clock fault condition. Back during the attempted recovery of the Spirit rover, a technical issue required the team to actively command the rover to communicate. Opportunity has no such issue; if we hear from it, it will likely be from listening passively as we have been, and as we will continue to do through January.

We will also actively attempt to command the rover to communicate during the 45-day listening period to cover the clock fault condition. After that, we will report to NASA on our efforts… [More at link]

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Curiosity update: Starting the drill campaign at ‘Inverness’

FRB_589776549EDR_F0722464FHAZ00302M_-br2Sols 2168-69, September 11, 2018, update by MSL scientist Kristen Bennett: In the weekend plan Curiosity drove to an area that the team thought would be a good location for the next drill site on Vera Rubin Ridge. The drive was a success, and there is a block named “Inverness” in the center of the workspace that was selected to be the next drill target.

The 2-sol plan focuses on characterizing Inverness in preparation for the drill campaign. This includes removing dust from the surface of the rock with the DRT, as well as taking MAHLI images, APXS measurements, a ChemCam LIBS observation, and a Mastcam multispectral observation of Inverness.

In addition to all of the measurements of Inverness, Curiosity will begin taking change detection images. The rover will be sitting in one spot for some time during the drill campaign, so this is a good opportunity to see if any of the sand around Curiosity is being moved around by the wind. In the current plan this includes a MARDI twilight image and Mastcam images of “Sandend” and “Skene.”

But wait! There’s more! This plan also includes a Mastcam image of the target “Stoneyburn,” a Navcam dust devil survey, and MAHLI night time images of the CheMin inlet… [More at link]

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THEMIS: Mesas, plains, craters in Terra Sabaea

Terra Sabaea hills and craters (THEMIS_IOTD_20180911)THEMIS Image of the Day, September 11, 2018. This VIS image shows part of Terra Sabaea, including plains, craters, and mesas. The dark blue tones often indicate locations of basaltic sands.

The THEMIS VIS camera contains 5 filters. The data from different filters can be combined in multiple ways to create a false color image. These false color images may reveal subtle variations of the surface not easily identified in a single band image.

See more THEMIS Images of the Day by geological subject.

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Curiosity update: It always looks grayer on the other side!

2163ML0116560010803622E01_DXXX-br2Sols 2165-67, September 10, 2018, update by MSL scientist Sean Czarnecki: Curiosity’s last plan didn’t quite get our intrepid rover close enough to our next potential drill location in the gray bedrock that is visually distinct on this part of Vera Rubin Ridge. This weekend’s plan was intended to be “Drill Sol 1,” but since it would require at least another short drive to drill, the team decided to choose another target a little further away that will provide a better science return. So the weekend plan now includes a short drive to our new drill target.

Before we drive, ChemCam will measure the chemistry of the targets “Great Bernera,” “Great Glen,” and “Great Todday;” Mastcam will take images of these same targets including a multispectral observation of Great Todday; and APXS will measure the chemistry of targets “Trollochy,” “Burn O Vat,” and “Portobello.” These observations are intended to document the compositional diversity of the gray and red bedrock at this location by documenting the transition from gray to red… [More at link]

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Weather update from Gale Crater

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Curiosity: Looking around at its new location

2166-navcamNWSol 2166, September 9, 2018. Following a couple of drives, Curiosity is now parked facing generally northwest, while to the south (below) the lower reaches of Mt. Sharp stand behind the rear of the rover. Click either image to enlarge it.

Sol 2166 raw images (from all cameras).

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