Opportunity: Cape Byron in view

4664-pancamSol 4664, March 8, 2017. As Opportunity drove in reverse over a smooth rise, Cape Byron, the next rim-segment toward the south came into view. In this three Pancam frame composite, the flat plains of Meridiani lie to the right (southwest), while to the left of Cape Byron the Endeavour Crater rim curves around to the southeast. On the horizon to the southeast, made hazy by dust, lie barely visible hills and rims of distant craters. Click image to enlarge it.

Opportunity raw images, its latest mission status, a location map, and atmospheric opacity, known as tau.

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HiRISE: Dunes on the floor of an infilled crater

tumblr_olnlhcFm6d1rlz4gso1_1280Dunes on the floor of an infilled crater. Beautiful Mars series.

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THEMIS: Waves of dunes on Proctor Crater floor

Waves of sand in Proctor Crater (THEMIS_IOTD_20170308)THEMIS Image of the Day, March 8, 2017. This VIS image shows the large dune field located on the floor of Proctor Crater in Noachis Terra.

More THEMIS Images of the Day by geological topic.

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Curiosity update: Early morning planning

NLB_542105346EDR_F0611332CCAM15903M_-br2Sol 1630-31, March 7, 2017, update by USGS scientist Ryan Anderson: We had an early-morning (6 AM on the west coast!) start to planning today, which was a bit painful but with the help of lots of caffeine we put together another plan full of good science! The exciting news from the weekend plan is that the MAHLI dust cover closed as planned, so we’re back in business with MAHLI.

The Sol 1630 plan will start with ChemCam observations of a vein called “Temple Stream”, a soil target called “Mattawamkeag”, and the bedrock target “Vassalboro” to coordinate with an APXS observation of “Sangerville”. MAHLI will also observe Sangerville, and Mastcam will document each of these targets. After that, the plan is to drive about 40 meters and collect some post-drive imaging. [More at link]

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HiRISE: Entrance to Mawrth Vallis

ESP_049017_2060In Andy Weir’s “The Martian,” stranded astronaut Mark Watney drives from the Ares 3 landing site in Acidalia Planitia towards the Ares 4 landing site in Schiaparelli Crater via Mawrth Vallis. This image covers the entrance to Mawrth Vallis. (Have a look at the scene in 3D).

As you can tell, driving over this terrain will be much more difficult than it was depicted in the novel or the movie. [More at link]

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Curiosity: Sculptured layers

1628-mastcam34Sol 1628, March 6, 2017. The wide-angle Mastcam took a three-frame look at the rock under the rover wheel seen here. Click image to enlarge it.

Sol 1628 raw images (from all cameras), and Curiosity’s latest location.

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Indonesian sediments may offer clues to Mars paleolake deposits

1707-Goudge-sm[Editor note: text from a GSA release here.]

In their GSA Bulletin article published online last week, Timothy A. Goudge and colleagues detail the clay mineralogy of sediment from Lake Towuti, Indonesia, using a technique called visible to near-infrared (VNIR) spectroscopy. VNIR measures the signature of reflected light from a sample across a larger wavelength range than just visible light. At Lake Towuti, the spectral record shows distinct variations in clay mineralogy over the past 40,000 years.

The record also captures the response of the lake system to changing climate, including changes in lake levels, forced delta progradation, and river incision. According to Goudge and colleagues, this demonstrates the utility of VNIR spectroscopy in developing paleoenvironmental records over tens of thousands of years.

Interestingly, Goudge and colleagues also suggest that paleolake deposits on Mars should preserve similar paleoenvironmental information that could be accessed through remote sensing studies of stratigraphy and VNIR reflectance spectroscopy.

Lead author Tim Goudge says, “The major link between this study of lake sediment in Indonesia and lake deposits on Mars is in terms of the methods we used. We can differentiate material properties with color (e.g., rust is red because of the iron in it), so VNIR spectroscopy allows us to determine what minerals are within a sample of lake sediment.” [More at links]

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HiRISE: Layers east of Terby Crater

tumblr_olnlalWjOC1rlz4gso1_1280Layers east of Terby Crater. Beautiful Mars series.

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THEMIS: Active sand dunes in Sirenum crater

Active dunes in Sirenum crater (THEMIS_IOTD_20170306)THEMIS Image of the Day, March 6, 2017. Today’s VIS image shows a field of dunes on the floor of an unnamed crater in Terra Sirenum. Their dark color indicates they are dust-free and suggests that the dune sands are activiely moving under the wind.

More THEMIS Images of the Day by geological topic.

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Opportunity field report, March 6, 2017

4660_travSol 4662, March 6, 2017; Rover Field Report by Larry Crumpler, MER Science Team & New Mexico Museum of Natural History & Science: Out of the crater and cruising south! For nearly two years Opportunity’s world has been tilted 10-25 degrees as it drove down to the lower slopes of the crater wall. Toward the end of last week Opportunity pulled itself up and over the lip of the crater. It has now begun drives to the south along the rim.  It is refreshing to see a panorama that consist of untilted frames! Incidentally Opportunity ascended 160 meters from the lower walls of Endeavour crater in just three months and is now in the 14th year of operations on Mars.

Check out the view north and behind us. The tracks make a right angle back there and emerge from the abyss on the right. Also, note that the horizon is muted. This is because of the regional dust storm that is occurring at this time. [More at link]

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