Mineralogy and geochemistry of sedimentary rocks and eolian sediments in Gale crater, Mars: A review after six Earth years of exploration with Curiosity

EB Rampe, DF Blake, TF Bristow, DW Ming… - Geochemistry, 2020 - Elsevier
Abstract The Mars Science Laboratory Curiosity rover arrived at Mars in August 2012 with a
primary goal of characterizing the habitability of ancient and modern environments. Curiosity …

Mission overview and scientific contributions from the Mars Science Laboratory Curiosity rover after eight years of surface operations

AR Vasavada - Space Science Reviews, 2022 - Springer
Abstract NASA's Mars Science Laboratory mission, with its Curiosity rover, has been
exploring Gale crater (5.4° S, 137.8° E) since 2012 with the goal of assessing the potential of …

The power of databases: the RRUFF project

B Lafuente, RT Downs, H Yang, N Stone… - Highlights in …, 2015 - degruyter.com
In today's world, many people rely on the availability of databases to perform daily activities
such as checking meteorological forecast, finding a recipe, or verifying the spelling of a …

Mineralogy of a mudstone at Yellowknife Bay, Gale crater, Mars

DT Vaniman, DL Bish, DW Ming, TF Bristow, RV Morris… - science, 2014 - science.org
Sedimentary rocks at Yellowknife Bay (Gale crater) on Mars include mudstone sampled by
the Curiosity rover. The samples, John Klein and Cumberland, contain detrital basaltic …

Organic molecules in the sheepbed mudstone, gale crater, mars

C Freissinet, DP Glavin, PR Mahaffy… - Journal of …, 2015 - Wiley Online Library
Abstract The Sample Analysis at Mars (SAM) instrument on board the Mars Science
Laboratory Curiosity rover is designed to conduct inorganic and organic chemical analyses …

Volatile, isotope, and organic analysis of martian fines with the Mars Curiosity rover

LA Leshin, PR Mahaffy, CR Webster, M Cabane, P Coll… - Science, 2013 - science.org
Samples from the Rocknest aeolian deposit were heated to~ 835° C under helium flow and
evolved gases analyzed by Curiosity's Sample Analysis at Mars instrument suite. H2O, SO2 …

Evolved gas analyses of sedimentary rocks and eolian sediment in Gale Crater, Mars: Results of the Curiosity rover's sample analysis at Mars instrument from …

B Sutter, AC Mcadam, PR Mahaffy… - Journal of …, 2017 - Wiley Online Library
The sample analysis at Mars instrument evolved gas analyzer (SAM‐EGA) has detected
evolved water, H2, SO2, H2S, NO, CO2, CO, O2, and HCl from two eolian sediments and …

Mars global simulant MGS-1: A Rocknest-based open standard for basaltic martian regolith simulants

KM Cannon, DT Britt, TM Smith, RF Fritsche… - Icarus, 2019 - Elsevier
The composition and physical properties of martian regolith are dramatically better
understood compared to just a decade ago, particularly through the use of X-ray diffraction …

Silicic volcanism on Mars evidenced by tridymite in high-SiO2 sedimentary rock at Gale crater

RV Morris, DT Vaniman, DF Blake… - Proceedings of the …, 2016 - National Acad Sciences
Tridymite, a low-pressure, high-temperature (> 870° C) SiO2 polymorph, was detected in a
drill sample of laminated mudstone (Buckskin) at Marias Pass in Gale crater, Mars, by the …

Curiosity at Gale crater, Mars: Characterization and analysis of the Rocknest sand shadow

DF Blake, RV Morris, G Kocurek, SM Morrison… - Science, 2013 - science.org
The Rocknest aeolian deposit is similar to aeolian features analyzed by the Mars
Exploration Rovers (MERs) Spirit and Opportunity. The fraction of sand< 150 micrometers in …