Pit crew jumps in; Mars 2020 rover gets wheels

Constructing an exquisitely complex vehicle like the Mars 2020 rover takes serious teamwork. On June 13, 2019, more than a dozen “bunny suit”-clad engineers rolled past another milestone in the clean room of the Spacecraft Assembly Facility at NASA’s Jet Propulsion Laboratory in Pasadena, California, when they integrated the rover’s legs and wheels.

The Mars 2020 team could pass for a pit crew in this video clip, which has been sped up by 300% and focuses on the major activities that took place the day the wheels were installed… [More at link]

Posted in Reports | Tagged , , , , , , | Comments Off

Latest weather at Gale Crater and Elysium Planitia

Daily Elysium charts and data (temperature, wind speed, atmospheric pressure) here.

Posted in Reports | Tagged , , , , , , , , , , , , , , | Comments Off

HiRISE: This far and no further!

ESP_055232_1595This far and no further! The very top of this image shows the edge of ancient lava flow that went no further across the plain. It’s also a natural boundary in the reflectivity (albedo) of the surface.

HiRISE Picture of the Day archive. [More at links]

Posted in Reports | Tagged , , , , , , , , , , | Comments Off

THEMIS: Edge of the caldera on Ascraeus Mons

Edge of the caldera (THEMIS_IOTD_20190712)THEMIS Image of the Day, July 12, 2019. Today’s VIS image is located on the summit of Ascraeus Mons, one of the three large Tharsis region volcanoes. This image clips just the edge of the large summit caldera.

Explore more THEMIS Images of the Day by geological subject.

Posted in Reports | Tagged , , , , , , , , , , | Comments Off

Curiosity update: A fountain of data

2459ML0130590010903606E01_DXXX-br2Sols 2463-64, July 11, 2019, update by MSL scientist Michelle Minitti: Curiosity continued work on and around the gorgeous outcrop pictured above that was started on Sol 2461. The layers of the outcrop – with their different colors, textures and thicknesses – tell us a story, one we worked to decipher in this plan with our full complement of contact and targeted science instruments. MAHLI and APXS will start by analyzing a grayish red target, “Tay,” on a block adjacent to the one pictured. The team hoped Tay’s grayish red color would be indicative of less dust cover; in other words, a chance for Tay to tell us a clearer story! ChemCam will shoot another gray target, “Donside,” that resembles one of the thicker gray layers seen in the outcrop above, and “Fountainbridge,” located on the farside of the outcrop where it exhibits a cracked texture. Off to the right of the rover, Mastcam will image a block, “Achmelvich,” near the right rear wheel that was shifted during our last drive, revealing the steep face of a sand deposit sitting amongst the bedrock in the area. [More at link]

Posted in Reports | Tagged , , , , , , , , , , , , , , , , | Comments Off

Layered-sulfates’ history in NE Syrtis Major

figure-6d[Editor’s note: From a paper by Daven Quinn and Bethany Ehlmann recently published in the Journal of Geophysical Research.]

The Deposition and Alteration History of the Northeast Syrtis Major Layered Sulfates

• The eroded stratigraphy at Northeast Syrtis Major includes meter‐scale‐layered, sulfate‐enriched sedimentary basin deposits up to 600 m thick
• Layer dips <10° and topographic high embayment are consistent with deepwater deposition; volume loss fractures indicate diagenetic dewatering
• Strata also including Syrtis Major lavas and fluvio‐deltaic phyllosilicates record three fluvio‐lacustrine episodes into the early Amazonian

Ancient stratigraphy on Isidis Basin’s western margin records the history of water on early Mars. Noachian units are overlain by layered, basaltic composition sedimentary rocks that are enriched in polyhydrated sulfates and capped by more resistant units.

The layered sulfates—uniquely exposed at northeast Syrtis Major—comprise a sedimentary sequence up to 600 m thick that has undergone a multistage history of deposition, alteration, and erosion. Siliciclastic sediments enriched in polyhydrated sulfates are bedded at meter scale and were deposited on slopes up to 10°, embaying and thinning against preexisting Noachian highlands around the Isidis Basin rim.

The layered sulfates were modified by volume loss fracturing during diagenesis. Resultant fractures hosted channelized flow and jarosite mineral precipitation to form resistant ridges upon erosion. The structural form of the layered sulfates is consistent with packages of sediment fallen from either atmospheric or aqueous suspension; coupling with substantial diagenetic volume loss may favor deepwater basin sedimentation.

After formation, the layered sulfates were capped by a “smooth capping unit” and then eroded to form paleovalleys. Hesperian Syrtis Major lavas were channelized by this paleotopography, capping it in some places and filling it in others. Later fluvial features and phyllosilicate‐bearing lacustrine deposits, sharing a regional base level of ∼−2,300 m, were superimposed on the sulfate‐lava stratigraphy.

The layered sulfates suggest surface bodies of water and active groundwater upwelling during the Noachian‐Hesperian transition. The northeast Syrtis Major stratigraphy records at least four distinct phases of surface and subsurface aqueous activity spanning from late Noachian to early Amazonian time. [More at link]

Posted in Reports | Tagged , , , , , , , , , , | Comments Off

HiRISE: Terraced trough near Ceraunius Fossae

ESP_055231_2065A terraced trough near Ceraunius Fossae. This may be a source region of flow material that enclosed the adjacent raised ridges and continues on to the north. High resolution can help to determine if the terraced forms are due to erosion, deposition, or collapse. The alignment of the trough cross-cuts the raised ridges.

HiRISE Picture of the Day archive. [More at links]

Posted in Reports | Tagged , , , , , , , , , , , | Comments Off

Weathering on early Mars bad for forming carbonates

[Editor’s note: From a paper by Fabien Baron and three co-authors recently published in the Journal of Geophysical Research.]

New Constraints on Early Mars Weathering Conditions From an Experimental Approach on Crust Simulants

• Chemical weathering in mildly acidic conditions under a CO2 atmosphere yielded leaching of alkali and alkaline earth elements
• Mass balance calculations indicated Al, Fe, and Si enrichment in the weathering products
• Our results imply unsuitable conditions for carbonate formation despite CO2 in the Martian atmosphere

Mars orbital and landed missions have provided mineralogical, morphological, and field evidence for liquid water at the surface approximately 3.5 billion years ago. The chemical and mineralogical composition of the Martian rocks have potentially been modified by interaction with this liquid water.

The purpose of our study is to use laboratory experiments to constrain the physicochemical conditions of water resulting from the chemical weathering of Martian crust simulants under an atmosphere composed of carbon dioxide, as is the case for Mars. The water in contact with simulants is mildly acidic. The partitioning of chemical elements between the solution and minerals is similar to what is observed on Earth, but weathering is more intense.

Despite that Mars had a primitive CO2‐dense atmosphere, the conditions were not favorable to the extensive formation of carbonate at the surface. [More at link]

Posted in Reports | Tagged , , , , | Comments Off

Curiosity update: What would we do without MAHLI?

2459MH0005360000902128R00_DXXX-br2Sols 2461-62, July 8, 2019, update by MSL scientist Roger Wiens: MAHLI was busy over the weekend. The data from Mars returned a trove of close-up images from the outcrop near the top of “Harlaw Rise,” including the one shown here. Along with outcrop images, MAHLI took pictures of the rover wheels to check for wear and tear. Those images can be seen at this link. Although the wheels have developed some holes, the testing and modeling that have been done since early 2014 indicate that Curiosity can still travel a number of kilometers on these wheels.

Today the team was busy planning two sols of activity. The rover moved only three meters over the weekend, so it is not far from last week’s activity. MAHLI will be active again, getting a “dog’s eye view” of laminated target “Strathdon.” MAHLI, APXS, and ChemCam will all investigate the top of the same block, with the target name “Feshie” as well as a nearby block named “Sligachan.” ChemCam and Mastcam will… [More at link]

Posted in Reports | Tagged , , , , , , , , , , , , , , , , | Comments Off

THEMIS: Scamander Vallis’ winding course

Scamander Vallis (THEMIS_IOTD_20190711)THEMIS Image of the Day, July 11, 2019. Today’s VIS image shows a section of Scamander Vallis. Scamander Vallis is located in northern Terra Sabaea.

Explore more THEMIS Images of the Day by geological subject.

Posted in Reports | Tagged , , , , , , , , , | Comments Off