scholarly journals The rock abrasion record at Gale Crater: Mars Science Laboratory results from Bradbury Landing to Rocknest

2014 ◽  
Vol 119 (6) ◽  
pp. 1374-1389 ◽  
Author(s):  
N. T. Bridges ◽  
F. J. Calef ◽  
B. Hallet ◽  
K. E. Herkenhoff ◽  
N. L. Lanza ◽  
...  
Keyword(s):  
Science Laboratory ◽  
Mars Science Laboratory ◽  
Gale Crater ◽  
Laboratory Results ◽  
Rock Abrasion

scholarly journals The Surface Energy Budget at Gale Crater during the first 2500 sols of the Mars Science Laboratory mission

2021 ◽  
Author(s):  
G. M. Martínez ◽  
A. Vicente‐Retortillo ◽  
A. R. Vasavada ◽  
C. E. Newman ◽  
E. Fischer ◽  
...  
Keyword(s):  
Surface Energy ◽  
Energy Budget ◽  
Surface Energy Budget ◽  
Science Laboratory ◽  
Mars Science Laboratory ◽  
Gale Crater

Abundance retrieval of hydrous minerals around the Mars Science Laboratory landing site in Gale crater, Mars

2016 ◽  
Vol 121 ◽  
pp. 76-82 ◽  
Author(s):  
Honglei Lin ◽  
Xia Zhang ◽  
Tong Shuai ◽  
Lifu Zhang ◽  
Yanli Sun
Keyword(s):  
Landing Site ◽  
Science Laboratory ◽  
Mars Science Laboratory ◽  
Hydrous Minerals ◽  
Gale Crater

scholarly journals Gale crater: the Mars Science Laboratory/Curiosity Rover Landing Site

2012 ◽  
Vol 12 (1) ◽  
pp. 25-38 ◽  
Author(s):  
James J. Wray
Keyword(s):  
Clay Minerals ◽  
Environmental Conditions ◽  
Spectral Properties ◽  
Landing Site ◽  
Science Laboratory ◽  
Deep Lakes ◽  
Mars Science Laboratory ◽  
Gale Crater ◽  
Diagenetic Processes ◽  
Curiosity Rover

AbstractGale crater formed from an impact on Mars ∼3.6 billion years ago. It hosts a central mound nearly 100 km wide and ∼5 km high, consisting of layered rocks with a variety of textures and spectral properties. The oldest exposed layers contain variably hydrated sulphates and smectite clay minerals, implying an aqueous origin, whereas the younger layers higher on the mound are covered by a mantle of dust. Fluvial channels carved into the crater walls and the lower mound indicate that surface liquids were present during and after deposition of the mound material. Numerous hypotheses have been advocated for the origin of some or all minerals and layers in the mound, ranging from deep lakes to playas to mostly dry dune fields to airfall dust or ash subjected to only minor alteration driven by snowmelt. The complexity of the mound suggests that multiple depositional and diagenetic processes are represented in the materials exposed today. Beginning in August 2012, the Mars Science Laboratory rover Curiosity will explore Gale crater by ascending the mound's northwestern flank, providing unprecedented new detail on the evolution of environmental conditions and habitability over many millions of years during which the mound strata accumulated.

SELECT OBSERVATIONS OF THE COARSE SEDIMENT RECORD AT GALE CRATER FROM MARS SCIENCE LABORATORY CAMERAS

2018 ◽  
Author(s):  
Rebecca M.E. Williams ◽  
◽  
Kathryn M. Stack ◽  
William E. Dietrich ◽  
David E. Eby ◽  
...  
Keyword(s):  
Science Laboratory ◽  
Sediment Record ◽  
Mars Science Laboratory ◽  
Gale Crater ◽  
Coarse Sediment

scholarly journals Mars Science Laboratory Observations of Chloride Salts in Gale Crater, Mars

2019 ◽  
Vol 46 (19) ◽  
pp. 10754-10763 ◽  
Author(s):  
N. H. Thomas ◽  
B. L. Ehlmann ◽  
P.‐Y. Meslin ◽  
W. Rapin ◽  
D. E. Anderson ◽  
...  
Keyword(s):  
Science Laboratory ◽  
Mars Science Laboratory ◽  
Gale Crater ◽  
Chloride Salts

X-ray Diffraction Results from Mars Science Laboratory: Mineralogy of Rocknest at Gale Crater

Science ◽  
2013 ◽  
Vol 341 (6153) ◽  
pp. 1238932-1238932 ◽  
Author(s):  
D. L. Bish ◽  
D. F. Blake ◽  
D. T. Vaniman ◽  
S. J. Chipera ◽  
R. V. Morris ◽  
...  
Keyword(s):  
Science Laboratory ◽  
X Ray Diffraction ◽  
Mars Science Laboratory ◽  
X Ray ◽  
Gale Crater

scholarly journals “In situ” characterization of the sedimentary record and structures using Virtual Reality: new insights from the Kimberley outcrop (Gale Crater, Mars)

2020 ◽  
Author(s):  
Gwénaël Caravaca ◽  
Nicolas Mangold ◽  
Stéphane Le Mouélic ◽  
Laetitia Le Deit ◽  
Marion Massé
Keyword(s):  
Virtual Reality ◽  
Temporal Distribution ◽  
Science Laboratory ◽  
Active System ◽  
Sedimentary Record ◽  
Mars Science Laboratory ◽  
Gale Crater ◽  
Sedimentary Structures ◽  
Spatio Temporal

<p>Since 2012, the Mars Science Laboratory <em>Curiosity</em> rover has studied the sedimentary deposits within the Gale Crater, leading to the description of varying lacustrine to fluviatile and fluvio-deltaic environments. Here, we focus on the sedimentary record of the Kimberley outcrop traversed by <em>Curiosity</em> between sols 603 and 630. This section presents siliciclastic rocks with an unusually high potassic content (Le Deit<em> et al.</em>, 2016, <em>JGR-Planets</em>). However, poorly constrained architecture and stratigraphic relations between the series of the Kimberley Formation and their local to regional surroundings still prevent further understanding of the exact extent of these accumulations and their significance within the broader Gale Crater paleoenvironmental scheme.<br>Such questions highlight the need for a new finer mapping of the area to characterize the contacts observed on the outcrop itself and in its immediate vicinity, but also for a new assessment of the precise nature and morphology of the sedimentary structures and their spatio-temporal distribution throughout the outcrop and beyond.<br>We therefore propose to use a true color highly resolved Digital Outcrop Model (DOM) of the Kimberley outcrop, obtained using Mars Science Laboratory imagery, integrated into a Virtual Reality (VR) environment (Caravaca <em>et al.</em>, <em>in press, PSS</em>). Taking advantage of this “in situ” geological analysis of the DOM, we were able to observe and characterize such sedimentary structures and contacts, as well as their spatial extension throughout the reconstructed area of Kimberley with an unprecedented precision. We notably observe and describe both conformable and unconformable contacts over the entire outcrop, but also several sets of varying scale cross-stratifications (from cm- to pluri-meter scale). These results are in accordance with a fluviatile hydrodynamically active system. They tend to corroborate the idea of a complex yet diachroneous evolution of the area, with the possibility of laterally evolving depositional settings, spanning a significant amount of time.</p>

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