Petrological Constraints on the Density of the Martian Crust
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The Rock Abrasion Record at Gale Crater: Mars Science Laboratory
PUBLICATIONS Journal of Geophysical Research: Planets RESEARCH ARTICLE The rock abrasion record at Gale Crater: Mars 10.1002/2013JE004579 Science Laboratory results from Bradbury Special Section: Landing to Rocknest Results from the first 360 Sols of the Mars Science Laboratory N. T. Bridges1, F. J. Calef2, B. Hallet3, K. E. Herkenhoff4, N. L. Lanza5, S. Le Mouélic6, C. E. Newman7, Mission: Bradbury Landing D. L. Blaney2,M.A.dePablo8,G.A.Kocurek9, Y. Langevin10,K.W.Lewis11, N. Mangold6, through Yellowknife Bay S. Maurice12, P.-Y. Meslin12,P.Pinet12,N.O.Renno13,M.S.Rice14, M. E. Richardson7,V.Sautter15, R. S. Sletten3,R.C.Wiens6, and R. A. Yingst16 Key Points: • Ventifacts in Gale Crater 1Applied Physics Laboratory, Laurel, Maryland, USA, 2Jet Propulsion Laboratory, Pasadena, California, USA, 3Department • Maybeformedbypaleowind of Earth and Space Sciences, College of the Environments, University of Washington, Seattle, Washington, USA, 4U.S. • Can see abrasion textures at range 5 6 of scales Geological Survey, Flagstaff, Arizona, USA, Los Alamos National Laboratory, Los Alamos, New Mexico, USA, LPGNantes, UMR 6112, CNRS/Université de Nantes, Nantes, France, 7Ashima Research, Pasadena, California, USA, 8Universidad de Alcala, Madrid, Spain, 9Department of Geological Sciences, Jackson School of Geosciences, University of Texas at Austin, Supporting Information: Austin, Texas, USA, 10Institute d’Astrophysique Spatiale, Université Paris-Sud, Orsay, France, 11Department of • Figure S1 12 fi • Figure S2 Geosciences, Princeton University, Princeton, New Jersey, USA, Centre National de la Recherche Scienti que, Institut 13 • Table S1 de Recherche en Astrophysique et Planétologie, CNRS-Université Toulouse, Toulouse, France, Department of Atmospheric, Oceanic, and Space Science; College of Engineering, University of Michigan, Ann Arbor, Michigan, USA, Correspondence to: 14Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, California, USA, 15Lab N. -
Chemical Variations in Yellowknife Bay Formation Sedimentary Rocks Analyzed by Chemcam on Board the Curiosity Rover on Mars N
Chemical variations in Yellowknife Bay formation sedimentary rocks analyzed by ChemCam on board the Curiosity rover on Mars N. Mangold, O. Forni, G. Dromart, K. Stack, R. C. Wiens, O. Gasnault, D. Y. Sumner, M. Nachon, P. -Y. Meslin, R. B. Anderson, et al. To cite this version: N. Mangold, O. Forni, G. Dromart, K. Stack, R. C. Wiens, et al.. Chemical variations in Yel- lowknife Bay formation sedimentary rocks analyzed by ChemCam on board the Curiosity rover on Mars. Journal of Geophysical Research. Planets, Wiley-Blackwell, 2015, 120 (3), pp.452-482. 10.1002/2014JE004681. hal-01281801 HAL Id: hal-01281801 https://hal.univ-lorraine.fr/hal-01281801 Submitted on 12 Apr 2021 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. PUBLICATIONS Journal of Geophysical Research: Planets RESEARCH ARTICLE Chemical variations in Yellowknife Bay formation 10.1002/2014JE004681 sedimentary rocks analyzed by ChemCam Special Section: on board the Curiosity rover on Mars Results from the first 360 Sols of the Mars Science Laboratory N. Mangold1, O. Forni2, G. Dromart3, K. Stack4, R. C. Wiens5, O. Gasnault2, D. Y. Sumner6, M. Nachon1, Mission: Bradbury Landing P.-Y. -
Chemical Variations in Yellowknife Bay Formation Sedimentary Rocks
PUBLICATIONS Journal of Geophysical Research: Planets RESEARCH ARTICLE Chemical variations in Yellowknife Bay formation 10.1002/2014JE004681 sedimentary rocks analyzed by ChemCam Special Section: on board the Curiosity rover on Mars Results from the first 360 Sols of the Mars Science Laboratory N. Mangold1, O. Forni2, G. Dromart3, K. Stack4, R. C. Wiens5, O. Gasnault2, D. Y. Sumner6, M. Nachon1, Mission: Bradbury Landing P.-Y. Meslin2, R. B. Anderson7, B. Barraclough4, J. F. Bell III8, G. Berger2, D. L. Blaney9, J. C. Bridges10, through Yellowknife Bay F. Calef9, B. Clark11, S. M. Clegg5, A. Cousin5, L. Edgar8, K. Edgett12, B. Ehlmann4, C. Fabre13, M. Fisk14, J. Grotzinger4, S. Gupta15, K. E. Herkenhoff7, J. Hurowitz16, J. R. Johnson17, L. C. Kah18, N. Lanza19, Key Points: 2 1 20 21 12 16 2 • J. Lasue , S. Le Mouélic , R. Léveillé , E. Lewin , M. Malin , S. McLennan , S. Maurice , Fluvial sandstones analyzed by 22 22 23 19 19 24 25 ChemCam display subtle chemical N. Melikechi , A. Mezzacappa , R. Milliken , H. Newsom , A. Ollila , S. K. Rowland , V. Sautter , variations M. Schmidt26, S. Schröder2,C.d’Uston2, D. Vaniman27, and R. Williams27 • Combined analysis of chemistry and texture highlights the role of 1Laboratoire de Planétologie et Géodynamique de Nantes, CNRS, Université de Nantes, Nantes, France, 2Institut de Recherche diagenesis en Astrophysique et Planétologie, CNRS/Université de Toulouse, UPS-OMP, Toulouse, France, 3Laboratoire de Géologie de • Distinct chemistry in upper layers 4 5 suggests distinct setting and/or Lyon, Université de Lyon, Lyon, France, California Institute of Technology, Pasadena, California, USA, Los Alamos National 6 source Laboratory, Los Alamos, New Mexico, USA, Earth and Planetary Sciences, University of California, Davis, California, USA, 7Astrogeology Science Center, U.S. -
Chemin X-Ray Diffraction of the Windjana Sample
PUBLICATIONS Journal of Geophysical Research: Planets RESEARCH ARTICLE Mineralogy, provenance, and diagenesis of a potassic 10.1002/2015JE004932 basaltic sandstone on Mars: CheMin X-ray diffraction Special Section: of the Windjana sample (Kimberley area, Gale Crater) The Mars Science Laboratory Rover Mission (Curiosity) at The Allan H. Treiman1, David L. Bish2, David T. Vaniman3, Steve J. Chipera4, David F. Blake5, Kimberley, Gale Crater, Mars Doug W. Ming6, Richard V. Morris6, Thomas F. Bristow5, Shaunna M. Morrison7, Michael B. Baker8, Elizabeth B. Rampe6, Robert T. Downs7, Justin Filiberto9, Allen F. Glazner10, Ralf Gellert11, Key Points: Lucy M. Thompson12, Mariek E. Schmidt13, Laetitia Le Deit14, Roger C. Wiens15, Amy C. McAdam16, • First mineralogical analysis of Cherie N. Achilles2, Kenneth S. Edgett17, Jack D. Farmer18, Kim V. Fendrich7, John P. Grotzinger8, sandstone on Mars 19 20 8 21 12 • Windjana sandstone very rich in Sanjeev Gupta , John Michael Morookian , Megan E. Newcombe , Melissa S. Rice , John G. Spray , sanidine, implying a trachyte source Edward M. Stolper8, Dawn Y. Sumner22, Ashwin R. Vasavada20, and Albert S. Yen20 rock • The source of Gale Crater sediments is 1Lunar and Planetary Institute, Houston, Texas, USA, 2Department of Geological Sciences, Indiana University, Bloomington, Indiana, an incredibly diverse igneous terrane USA, 3Planetary Science Institute,Tucson,Arizona,USA,4Chesapeake Energy Corporation, Oklahoma City, Oklahoma, USA, 5NASA Ames Research Center, Moffett Field, California, USA, 6Astromaterials -
Joint Industry Programme
CETACEAN STOCK ASSESSMENT IN RELATION TO EXPLORATION AND PRODUCTION INDUSTRY SOUND by Prepared for Joint Industry Programme 30 September 2009 LGL Report TA4582-1 CETACEAN STOCK ASSESSMENT IN RELATION TO EXPLORATION AND PRODUCTION INDUSTRY SOUND by LGL Limited, environmental research associates 22 Fisher Street, POB 280 King City, Ontario, Canada L7B 1A6 9768 Second Street Sidney, British Columbia, Canada V8L 3Y8 and LGL Alaska Research Associates Inc. 1101 East 76th Avenue, Suite B Anchorage, Alaska, United States 99518 Prepared for Joint Industry Programme 30 September 2009 LGL Report TA4582-1 Executive Summary Purpose and Objectives This project investigated the relationship between the oil industry‘s offshore E&P activities and trends in the distribution, abundance and rates of increase of key cetacean stocks found in three areas where E&P activities are intensive. The approach taken was to compare the status and population trends of stocks of key cetacean species in three areas with E&P activities―Alaska (subdivided into three regions, the Beaufort, Bering and Chukchi seas), Australia (Western and southeast regions), and Sakhalin Island, Russia―with corresponding parameters for stocks of the same species (where possible) in areas where E&P activities were absent or greatly reduced. The project involved a critical review of existing and historical data on cetacean stocks, and a compilation of data on E&P activities and non-industry factors that may have influenced stocks, in the areas of interest. Data were assessed in terms of quality, quantity, and temporal and spatial coverage to determine whether sufficient data were available for a reasonable assessment of correlations between cetacean populations and E&P activities. -
Petrology of Volcanic Rocks from Kaula Island, Hawaii Implications for the Origin of Hawaiian Phonolites
Contributions to Contrib Mineral Petrol (1986) 94:461-471 Mineralogy and Petrology Springer-Verlag 1986 Petrology of volcanic rocks from Kaula Island, Hawaii Implications for the origin of Hawaiian phonolites Michael O. Garcia 1, Frederick A. Frey 2, and David G. Grooms 1 * 1 Hawaii Institute of Geophysics, University of Hawaii, Honolulu, HI 96822, USA 2 Earth, Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, MA 02139, USA Abstract. A compositionally diverse suite of volcanic rocks, visited the island by helicopter courtesy of the U.S. Navy. including tholeiites, phonolites, basanites and nephelinites, Abundant unexploded ordnance, bird nests (total bird pop- occurs as accidental blocks in the palagonitic tuff of Kaula ulation >45,000) and steep cliffs surrounding the island Island. The Kaula phonolites are the only documented made sample collection hazardous. phonolites from the Hawaiian Ridge. Among the accidental Kaula Island consists of approximately 160 m of well- blocks, only the phonolites and a plagioclase basanite were bedded, palagonitic tuff (Fig. 2). The tuff contains acciden- amenable to K-Ar age dating. They yielded ages of tal fragments of light gray (phonolite) and dark gray (ba- 4.0-4.2 Ma and 1.8 ___0.2 Ma, respectively. Crystal fraction- salt) volcanic rocks, coralline material, coarse-grained ultra- ation modeling of major and trace element data indicates mafic and marie xenoliths (including spinel pyroxenites, that the phonolites could be derived from a plagioclase garnet pyroxenites, spinel peridotites and dunites) and me- basanite by subtraction of 27% clinopyroxene, 21% plagio- gacrysts (augite, anorthoclase, olivine, Al-spinel and titano- clase, 16% anorthoclase, 14% olivine, 4% titanomagnetite magnetite). -
Petrology on Mars†K
American Mineralogist, Volume 100, pages 2380–2395, 2015 INVITED CENTENNIAL ARTICLE REVIEW Petrology on Mars†k HARRY Y. MCSWEEN JR.1,* 1Department of Earth and Planetary Sciences and Planetary Geoscience Institute, University of Tennessee, Knoxville, Tennessee 37996-1410, U.S.A. ABSTRACT Petrologic investigations of martian rocks have been accomplished by mineralogical, geochemical, and textural analyses from Mars rov- ers (with geologic context provided by orbiters), and by laboratory analyses of martian meteorites. Igneous rocks are primarily lavas and volcaniclastic rocks of basaltic composition, and ultramafic cumulates; alkaline rocks are common in ancient terranes and tholeiitic rocks occur in younger terranes, suggesting global magmatic evolution. Relatively uncommon feldspathic rocks represent the ultimate fractionation prod- ucts, and granitic rocks are unknown. Sedimentary rocks are of both clastic (mudstone, sandstone, conglomerate, all containing significant igneous detritus) and chemical (evaporitic sulfate and less common carbonate) origin. High-silica sediments formed by hydrothermal activity. Sediments on Mars formed from different protoliths and were weathered under different environmental conditions from terrestrial sediments. Metamorphic rocks have only been inferred from orbital remote-sensing measurements. Metabasalt and serpentinite have mineral assemblages consistent with those predicted from low-pressure phase equilibria and likely formed in geothermal systems. Shock effects are com- mon in martian meteorites, and impact breccias are probably widespread in the planet’s crustal rocks. The martian rock cycle during early periods was similar in many respects to that of Earth. However, without plate tectonics Mars did not experience the thermal metamorphism and flux melting associated with subduction, nor deposition in subsided basins and rapid erosion resulting from tectonic uplift. -
POSTER SESSION: GENESIS MISSION: TARGET HANDLING and SOLAR WIND ABUNDANCES 6:00 P.M
Tuesday, March 19, 2013 [T601] POSTER SESSION: GENESIS MISSION: TARGET HANDLING AND SOLAR WIND ABUNDANCES 6:00 p.m. Town Center Exhibit Area Allton J. H. Rodriguez M. C. Burkett P. J. Ross D. K. Gonzalez C. P. et al. POSTER LOCATION #1 Recent Optical and SEM Characterization of Genesis Solar Wind Concentrator Diamond-on-Silicon Collector [#2466] Observations of contaminants and irradiation damage on diamond-on-silicon surface and postsubdivision imaging. Burkett P. J. Allton J. A. Clemett S. J. Gonzales C. P. Lauer H. V. Jr et al. POSTER LOCATION #2 Plan for Subdividing Genesis Mission Diamond-on-Silicon 60000 Solar Wind Collector [#2837] Using innovative laser scribing and cleaving techniques, Genesis sample 60000 was subdivided resulting subsamples for allocation and analysis. Lauer H. V. Burket P. J. Rodriguez M. C. Nakamura-Messenger K. Clemett S. J. et al. POSTER LOCATION #3 Laser Subdivision of the Genesis Concentrator Target Sample 60000 [#2691] The Genesis Allocation Committee received a request for ~ 1 cm2 of the target sample 60000. We describe the cutting plan used to provide the allocation. Rodriguez M. R. Allton J. H. Burkett P. J. Gonzalez C. P. POSTER LOCATION #4 Examples of Optical Assessment of Surface Cleanliness of Genesis Samples [#2515] We present recent examples of optically surveyed Genesis samples as part of a cleaning plan intended to create a set of “assessed clean” samples for allocation. Kuhlman K. R. Rodgriguez M. C. Gonzalez C. P. Allton J. H. Burnett D. S. POSTER LOCATION #5 Cleaning Study of Genesis Sample 60487 [#2930] This examination of the efficacy of various cleaning methods was conducted using correlative microscopy of Genesis sample 60487. -
Package 'NORRRM'
Package ‘NORRRM’ March 11, 2015 Type Package Title Geochemical Toolkit for R Version 1.0.0 Date 2015-01-29 Author Renee Gonzalez Guzman Maintainer Renee Gonzalez Guzman <[email protected]> Imports ggplot2,SDMTools Description CIPW Norm (acronym from the surnames of the authors: Cross, Iddings, Pirrson and Washington) is the most commonly used calculation algorithm to estimate the standard mineral assemblages for igneous rocks from its geochemical composition. NORRRM (acronym from noRm, R lan- guage and Renee) is the highly consistent program to calculate the CIPW Norm. Depends R (>= 3.1.1) License GPL (>= 3) NeedsCompilation no Repository CRAN Date/Publication 2015-03-11 21:49:49 R topics documented: NORRRM-package . .2 AdjRock . .3 Andes . .4 AtomWeight . .5 CIPW............................................6 CIPW.trace . .7 MinWeight . .9 OxiWeight . 10 TASplot . 11 TestTAS . 12 Index 13 1 2 NORRRM-package NORRRM-package Geochemical Toolkit for R Description According to the IUGS (International Union of Geological Science), Subcommission on the Sys- tematics of Igneous Rocks, the primary classification of igneous rocks must be based according to their modal mineral composition, expressed in volume percent. Nevertheless, where these data are not available or can not be determined owing to fine-grained mineral assemblage, glassy content or changes in the original mineralogy, then other criteria based on chemical bulk composition may be used. Computed from the chemical composition, the normative mineralogy is an alternative approach for mineralogical classification and useful for set up the naming of igneous rocks (as parts of the TAS classification, TASplot). The CIPW Norm is the most commonly used calculation algorithm to estimate the standard mineral assemblages for igneous rocks CIPW, generated over more than a hundred years ago and thereafter modified by some authors to the passage of the years (e.g., Verma et al., 2002). -
Volatile, Isotope, and Organic Analysis of Martian Fines with the Mars Curiosity Rover L
Volatile, Isotope, and Organic Analysis of Martian Fines with the Mars Curiosity Rover L. A. Leshin et al. Science 341, (2013); DOI: 10.1126/science.1238937 This copy is for your personal, non-commercial use only. If you wish to distribute this article to others, you can order high-quality copies for your colleagues, clients, or customers by clicking here. Permission to republish or repurpose articles or portions of articles can be obtained by following the guidelines here. The following resources related to this article are available online at www.sciencemag.org (this information is current as of February 4, 2014 ): Updated information and services, including high-resolution figures, can be found in the online version of this article at: on February 4, 2014 http://www.sciencemag.org/content/341/6153/1238937.full.html Supporting Online Material can be found at: http://www.sciencemag.org/content/suppl/2013/09/25/341.6153.1238937.DC1.html http://www.sciencemag.org/content/suppl/2013/09/26/341.6153.1238937.DC2.html A list of selected additional articles on the Science Web sites related to this article can be found at: http://www.sciencemag.org/content/341/6153/1238937.full.html#related www.sciencemag.org This article cites 43 articles, 9 of which can be accessed free: http://www.sciencemag.org/content/341/6153/1238937.full.html#ref-list-1 This article has been cited by 9 articles hosted by HighWire Press; see: http://www.sciencemag.org/content/341/6153/1238937.full.html#related-urls This article appears in the following subject collections: Planetary Science Downloaded from http://www.sciencemag.org/cgi/collection/planet_sci Science (print ISSN 0036-8075; online ISSN 1095-9203) is published weekly, except the last week in December, by the American Association for the Advancement of Science, 1200 New York Avenue NW, Washington, DC 20005. -
A-Type Granites: Characteristics, Petrogenesis and Their Contribution to the Growth of the Continental Crust
A-type granites: characteristics, petrogenesis and their contribution to the growth of the continental crust Nelson Eby University of Massachusetts, Lowell, MA 01854, USA [email protected] The A-type Granitoids Defined by Loiselle and Wones (1979) A stands for Anorogenic or Anhydrous or the first letter of the alphabet. The last choice removes the necessity of debating the meaning of A. Magmas are emplaced in post-collisional or within plate settings, i.e., an extensional environment. Characteristics of A-type Granitoids 1. Non-orogenic setting 2. Subaluminous to peralkaline, sometimes peraluminous 3. For rocks of intermediate silica content, A-type granitoids generally have higher total alkalis and lower CaO than other granitoids. 4. High FeOT/MgO 5. A characteristic mineralogy consisting of iron-rich mafic silicates (annite, ferrohendenbergite, ferrohastingsite, fayalite), and in peralkaline suites alkali-rich mafic silicates (aegirine, arfvedsonite, reibeckite) and perthitic feldspars The Alphabet Soup – is A-type granitoid a useful classification? • Classifications are useful to the extent that they help us organize our observations/ideas. • Classifications are a short-hand that can be used to convey a general description of geologic observations. • One can define a group of granitoids, in terms of geologic setting and chemistry, that are distinct from other granitoids. In this instance the A-type classification is useful. • However, a classification should not lead to rigid thinking. • As geologists we still need to maintain our world view of multiple working hypotheses/processes. • A-type granitoids, while similar in many respects, can apparently arise via different petrogenetic pathways. The challenge is to elucidate these pathways. -
Sorting out Compositional Trends in Sedimentary Rocks of the Bradbury
PUBLICATIONS Journal of Geophysical Research: Planets RESEARCH ARTICLE Sorting out compositional trends in sedimentary 10.1002/2016JE005195 rocks of the Bradbury group (Aeolis Palus), Key Points: Gale crater, Mars • Curiosity obtained bulk chemistry for sedimentary rocks in the Bradbury K. L. Siebach1,2 , M. B. Baker1, J. P. Grotzinger1, S. M. McLennan2 , R. Gellert3 , group 4 2 • Coarse-grained rocks are enriched in L. M. Thompson , and J. A. Hurowitz plagioclase 1 2 • Geochemical trends are consistent Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, California, USA, Department with mineral sorting during transport of Geosciences, SUNY at Stony Brook, Stony Brook, New York, USA, 3Department of Physics, University of Guelph, Guelph, Ontario, Canada, 4Planetary and Space Science Centre, University of New Brunswick, Fredericton, New Brunswick, Canada Supporting Information: • Supporting Information S1 • Table S1 Abstract Sedimentary rocks are composed of detrital grains derived from source rocks, which are altered Correspondence to: by chemical weathering, sorted during transport, and cemented during diagenesis. Fluvio-lacustrine K. L. Siebach, sedimentary rocks of the Bradbury group, observed on the floor of Gale crater by the Curiosity rover during its [email protected] first 860 Martian solar days, show trends in bulk chemistry that are consistent with sorting of mineral grains during transport. The Bradbury group rocks are uniquely suited for sedimentary provenance analysis because Citation: they appear to have experienced negligible cation loss (i.e., open-system chemical weathering) at the scale of Siebach, K. L., M. B. Baker, J. P. the Alpha Particle X-ray Spectrometer bulk chemistry analyses based on low Chemical Index of Alteration Grotzinger, S.