ExoMars rover software passes ESA Mars Yard driving test

Navigation software destined for the ExoMars 2020 mission to the Red Planet has passed a rover-based driving test at ESA’s ‘Mars Yard.’

ESA’s ExoMars rover will drive to multiple locations and drill down to two metres below the surface of Mars in search of clues for past life preserved underground.

A half-scale version of the ExoMars rover, called ExoMars Testing Rover (ExoTeR), manoeuvred itself carefully through the red rocks and sand of the 9 x 9 m ‘Planetary Utilisation Testbed,’ nicknamed the Mars Yard, part of ESA’s Planetary Robotics Laboratory at ESTEC in the Netherlands.

Carefully calculating its onward route, ExoTeR progressed at a rate of 2 m per minute – still several times faster than the actual ExoMars rover will drive, which will progress at 100 m per martian day…. [More at link]

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Opportunity: Dust storm activity appears to pick up south of rover

NASA Mars Exploration Rover Status Report, January 17, 2019: Dust storm activity appears to have picked up again, with a regional storm tracking south about 124 miles (200 kilometers) to the west of Opportunity.

The storm is expected to increase in opacity (tau) at the rover site to greater than 1.5 over the next few days. No signal from Opportunity has been heard since Sol 5111 (June 10, 2018) during the historic global dust storm. 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 each 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. They have expanded the breath of “sweep and beeps” commanding covering more times of day on Mars.

Mars is now in the seasonal period of past dust clearing events for the rover. Since loss of signal, 560 recovery commands have been radiated to the rover. [More at link]

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THEMIS: Gullies and floor features in Aonia Terra crater

Gullies and floor features (THEMIS_IOTD_20190117)THEMIS Image of the Day, January 17, 2019. Many large gullies dissect the rim of this unnamed crater in Aonia Terra.  The inner walls and floor both show evidence of pasted-on terrain — a layer of potentially ice-rich dust.

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THEMIS: Aonia Terra crater gullies

Aonia Terra crater gullies (THEMIS_IOTD_20190116)THEMIS Image of the Day, January 16, 2019. Today’s VIS image shows part of an unnamed crater in Aonia Terra. The rim of this crater contains many deep gullies. At the top left of the image a channel system is visible on the floor of the crater.

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Weather at Gale Crater

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HiRISE: The source of dunes in Chasma Boreale

tumblr_plchlsgCu71rlz4gso1_1280The source of dunes in Chasma Boreale. This image shows dunes during the summer, when they were free from the seasonal layer of carbon dioxide ice that covers the region for much of the year. These dunes, which are near the head of the largest trough in the North Polar cap (called Chasma Boreale), were formed by strong winds blowing down the canyon toward its mouth.

Beautiful Mars series. [More at links]

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THEMIS: Eroding crater infill in Noachis Terra

Eroding infill in southern crater (THEMIS_IOTD_20190115)THEMIS Image of the Day, January 15, 2019. At several locations in the southern hemisphere there are craters that have been filled with material almost to the top of the crater rim. What the material is and where it came from are still open questions, and may not even be the same process from crater to crater.

In several of these filled craters there are canyon like features where the fill material has been removed or eroded. Sometimes the depressions parallel the crater rim, but in other cases the depression is in the center of the crater and is usually linear.

A ring of gullies encircle the top of the depression in this crater. This unnamed crater is located in southern Noachis Terra.

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Curiosity update: Selfie time at Rock Hall: say cheese!

NRA_600694728EDR_F0731206NCAM00320M_Sols 2291, January 14, 2019, update by MSL scientist Rachel Kronyak: Today we planned a single sol of activities, Sol 2291. As we begin to wrap up our activities at the Rock Hall drill site, Sol 2291 is chock full of science observations. We’ll begin the sol with an hour-long science block. Our environmental group (ENV) planned several activities to measure increasing dust levels in the atmosphere; these observations will occur at the start of the science block. Following ENV’s activities, the geology group (GEO) planned a ChemCam observation on a soil target near the rover named “Loch Monar” as well as a long-distance Remote Micro-Imager (RMI) image of the sulfate unit on Mount Sharp. Following ChemCam, Mastcam will take images of targets “Loch Monar” and “Stroma.” The “Stroma” target is an interesting small rock just in… [More at link]

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THEMIS: Interweaving gullies in Kaiser Crater

Kaiser Crater gullies (THEMIS_IOTD_20190114)THEMIS Image of the Day, January 14, 2019. Today’s VIS image shows part of the inner rim of Kaiser Crater. The rim has been dissected by numerous gullies. Kaiser Crater is located in Noachis Terra.

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Curiosity update: Drilling activity completed, almost

FLA_600434459EDR_F0731206FHAZ00337M_-br2Sols 2288-90, January 11, 2019, update by MSL scientist Suzanne Schwenzer: We will soon be leaving the Rock Hall area, thus this one last look at the drill site from a hazard camera perspective. Seeing those holes always is special, even for #19!

In today’s planning, we will dump the remaining rock powder from the drill and investigate it with all instruments, starting with APXS, which will perform a two-step raster. Sol 2288 contains a range of ENV investigations, dedicating the morning science block on sol 2288 to a passive sky observation and a Mastcam tau to see how the dust loading in the atmosphere is changing. The science block of sol 2289 is dedicated to spectral analysis of the dump pile with ChemCam passive and Mastcam multispectral investigations… [More at link]

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