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  • 1
    Publication Date: 2009-09-19
    Description: 〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Farmer, J Doyne -- Foley, Duncan -- England -- Nature. 2009 Aug 6;460(7256):685-6. doi: 10.1038/460685a.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉J. Doyne Farmer is at the Santa Fe Institute, 1399 Hyde Park Road, Santa Fe, New Mexico 87501, USA, and at LUISS Guido Carli in Rome, Italy, and founded the quantitative trading firm Prediction Company. jdf@santafe.edu.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/19661896" target="_blank"〉PubMed〈/a〉
    Print ISSN: 0028-0836
    Electronic ISSN: 1476-4687
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
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  • 2
    Publication Date: 2010-09-25
    Description: 〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Ferguson, Charles D -- Marburger, Lindsey E -- Farmer, J Doyne -- Makhijani, Arjun -- England -- Nature. 2010 Sep 23;467(7314):391-3. doi: 10.1038/467391a.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Federation of American Scientists, Washington, DC 20036, USA. cferguson@fas.org〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/20864972" target="_blank"〉PubMed〈/a〉
    Keywords: Conservation of Energy Resources/economics/*trends ; Electricity ; Fossil Fuels/economics/utilization ; Nuclear Power Plants/economics/*statistics & numerical data ; United States
    Print ISSN: 0028-0836
    Electronic ISSN: 1476-4687
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
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  • 3
    Publication Date: 2008-05-24
    Description: Mineral deposits on the martian surface can elucidate ancient environmental conditions on the planet. Opaline silica deposits (as much as 91 weight percent SiO2) have been found in association with volcanic materials by the Mars rover Spirit. The deposits are present both as light-toned soils and as bedrock. We interpret these materials to have formed under hydrothermal conditions and therefore to be strong indicators of a former aqueous environment. This discovery is important for understanding the past habitability of Mars because hydrothermal environments on Earth support thriving microbial ecosystems.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Squyres, S W -- Arvidson, R E -- Ruff, S -- Gellert, R -- Morris, R V -- Ming, D W -- Crumpler, L -- Farmer, J D -- Marais, D J Des -- Yen, A -- McLennan, S M -- Calvin, W -- Bell, J F 3rd -- Clark, B C -- Wang, A -- McCoy, T J -- Schmidt, M E -- de Souza, P A Jr -- New York, N.Y. -- Science. 2008 May 23;320(5879):1063-7. doi: 10.1126/science.1155429.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Department of Astronomy, Space Sciences Building, Cornell University, Ithaca, NY 14853, USA. squyres@astro.cornell.edu〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/18497295" target="_blank"〉PubMed〈/a〉
    Keywords: Extraterrestrial Environment ; Hot Temperature ; Hydrogen-Ion Concentration ; *Mars ; *Silicon Dioxide ; Spacecraft ; *Water
    Print ISSN: 0036-8075
    Electronic ISSN: 1095-9203
    Topics: Biology , Chemistry and Pharmacology , Computer Science , Medicine , Natural Sciences in General , Physics
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  • 4
    Publication Date: 2013-09-28
    Description: 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 size contains ~55% crystalline material consistent with a basaltic heritage and ~45% x-ray amorphous material. The amorphous component of Rocknest is iron-rich and silicon-poor and is the host of the volatiles (water, oxygen, sulfur dioxide, carbon dioxide, and chlorine) detected by the Sample Analysis at Mars instrument and of the fine-grained nanophase oxide component first described from basaltic soils analyzed by MERs. The similarity between soils and aeolian materials analyzed at Gusev Crater, Meridiani Planum, and Gale Crater implies locally sourced, globally similar basaltic materials or globally and regionally sourced basaltic components deposited locally at all three locations.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Blake, D F -- Morris, R V -- Kocurek, G -- Morrison, S M -- Downs, R T -- Bish, D -- Ming, D W -- Edgett, K S -- Rubin, D -- Goetz, W -- Madsen, M B -- Sullivan, R -- Gellert, R -- Campbell, I -- Treiman, A H -- McLennan, S M -- Yen, A S -- Grotzinger, J -- Vaniman, D T -- Chipera, S J -- Achilles, C N -- Rampe, E B -- Sumner, D -- Meslin, P-Y -- Maurice, S -- Forni, O -- Gasnault, O -- Fisk, M -- Schmidt, M -- Mahaffy, P -- Leshin, L A -- Glavin, D -- Steele, A -- Freissinet, C -- Navarro-Gonzalez, R -- Yingst, R A -- Kah, L C -- Bridges, N -- Lewis, K W -- Bristow, T F -- Farmer, J D -- Crisp, J A -- Stolper, E M -- Des Marais, D J -- Sarrazin, P -- MSL Science Team -- New York, N.Y. -- Science. 2013 Sep 27;341(6153):1239505. doi: 10.1126/science.1239505.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉National Aeronautics and Space Administration Ames Research Center, Moffett Field, CA 94035, USA. david.blake@nasa.gov〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/24072928" target="_blank"〉PubMed〈/a〉
    Print ISSN: 0036-8075
    Electronic ISSN: 1095-9203
    Topics: Biology , Chemistry and Pharmacology , Computer Science , Medicine , Natural Sciences in General , Physics
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  • 5
    Publication Date: 2004-08-07
    Description: The Spirit landing site in Gusev Crater on Mars contains dark, fine-grained, vesicular rocks interpreted as lavas. Pancam and Mini-Thermal Emission Spectrometer (Mini-TES) spectra suggest that all of these rocks are similar but have variable coatings and dust mantles. Magnified images of brushed and abraded rock surfaces show alteration rinds and veins. Rock interiors contain 〈/=25% megacrysts. Chemical analyses of rocks by the Alpha Particle X-ray Spectrometer are consistent with picritic basalts, containing normative olivine, pyroxenes, plagioclase, and accessory FeTi oxides. Mossbauer, Pancam, and Mini-TES spectra confirm the presence of olivine, magnetite, and probably pyroxene. These basalts extend the known range of rock compositions composing the martian crust.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉McSween, H Y -- Arvidson, R E -- Bell, J F 3rd -- Blaney, D -- Cabrol, N A -- Christensen, P R -- Clark, B C -- Crisp, J A -- Crumpler, L S -- Des Marais, D J -- Farmer, J D -- Gellert, R -- Ghosh, A -- Gorevan, S -- Graff, T -- Grant, J -- Haskin, L A -- Herkenhoff, K E -- Johnson, J R -- Jolliff, B L -- Klingelhoefer, G -- Knudson, A T -- McLennan, S -- Milam, K A -- Moersch, J E -- Morris, R V -- Rieder, R -- Ruff, S W -- De Souza, P A Jr -- Squyres, S W -- Wanke, H -- Wang, A -- Wyatt, M B -- Yen, A -- Zipfel, J -- New York, N.Y. -- Science. 2004 Aug 6;305(5685):842-5.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Department of Earth and Planetary Sciences, University of Tennessee, Knoxville, TN 37996-1410, USA. mcsween@utk.edu〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/15297668" target="_blank"〉PubMed〈/a〉
    Keywords: Extraterrestrial Environment ; Geologic Sediments ; Iron Compounds ; Magnesium Compounds ; *Mars ; *Minerals ; Oxides ; *Silicates ; Spectroscopy, Mossbauer ; Spectrum Analysis ; Water
    Print ISSN: 0036-8075
    Electronic ISSN: 1095-9203
    Topics: Biology , Chemistry and Pharmacology , Computer Science , Medicine , Natural Sciences in General , Physics
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  • 6
    Publication Date: 2013-12-11
    Description: 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 minerals, calcium sulfates, iron oxide or hydroxides, iron sulfides, amorphous material, and trioctahedral smectites. The John Klein smectite has basal spacing of ~10 angstroms, indicating little interlayer hydration. The Cumberland smectite has basal spacing at both ~13.2 and ~10 angstroms. The larger spacing suggests a partially chloritized interlayer or interlayer magnesium or calcium facilitating H2O retention. Basaltic minerals in the mudstone are similar to those in nearby eolian deposits. However, the mudstone has far less Fe-forsterite, possibly lost with formation of smectite plus magnetite. Late Noachian/Early Hesperian or younger age indicates that clay mineral formation on Mars extended beyond Noachian time.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Vaniman, D T -- Bish, D L -- Ming, D W -- Bristow, T F -- Morris, R V -- Blake, D F -- Chipera, S J -- Morrison, S M -- Treiman, A H -- Rampe, E B -- Rice, M -- Achilles, C N -- Grotzinger, J P -- McLennan, S M -- Williams, J -- Bell, J F 3rd -- Newsom, H E -- Downs, R T -- Maurice, S -- Sarrazin, P -- Yen, A S -- Morookian, J M -- Farmer, J D -- Stack, K -- Milliken, R E -- Ehlmann, B L -- Sumner, D Y -- Berger, G -- Crisp, J A -- Hurowitz, J A -- Anderson, R -- Des Marais, D J -- Stolper, E M -- Edgett, K S -- Gupta, S -- Spanovich, N -- MSL Science Team -- New York, N.Y. -- Science. 2014 Jan 24;343(6169):1243480. doi: 10.1126/science.1243480. Epub 2013 Dec 9.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Planetary Science Institute, Tucson, AZ 85719, USA.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/24324271" target="_blank"〉PubMed〈/a〉
    Keywords: Extraterrestrial Environment/*chemistry ; Ferrosoferric Oxide/analysis/chemistry ; Geologic Sediments/analysis/*chemistry ; *Mars ; Minerals/analysis/*chemistry ; Silicates/analysis/chemistry ; Silicon Compounds/analysis/chemistry
    Print ISSN: 0036-8075
    Electronic ISSN: 1095-9203
    Topics: Biology , Chemistry and Pharmacology , Computer Science , Medicine , Natural Sciences in General , Physics
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  • 7
    Publication Date: 2013-06-01
    Description: Observations by the Mars Science Laboratory Mast Camera (Mastcam) in Gale crater reveal isolated outcrops of cemented pebbles (2 to 40 millimeters in diameter) and sand grains with textures typical of fluvial sedimentary conglomerates. Rounded pebbles in the conglomerates indicate substantial fluvial abrasion. ChemCam emission spectra at one outcrop show a predominantly feldspathic composition, consistent with minimal aqueous alteration of sediments. Sediment was mobilized in ancient water flows that likely exceeded the threshold conditions (depth 0.03 to 0.9 meter, average velocity 0.20 to 0.75 meter per second) required to transport the pebbles. Climate conditions at the time sediment was transported must have differed substantially from the cold, hyper-arid modern environment to permit aqueous flows across several kilometers.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Williams, R M E -- Grotzinger, J P -- Dietrich, W E -- Gupta, S -- Sumner, D Y -- Wiens, R C -- Mangold, N -- Malin, M C -- Edgett, K S -- Maurice, S -- Forni, O -- Gasnault, O -- Ollila, A -- Newsom, H E -- Dromart, G -- Palucis, M C -- Yingst, R A -- Anderson, R B -- Herkenhoff, K E -- Le Mouelic, S -- Goetz, W -- Madsen, M B -- Koefoed, A -- Jensen, J K -- Bridges, J C -- Schwenzer, S P -- Lewis, K W -- Stack, K M -- Rubin, D -- Kah, L C -- Bell, J F 3rd -- Farmer, J D -- Sullivan, R -- Van Beek, T -- Blaney, D L -- Pariser, O -- Deen, R G -- MSL Science Team -- New York, N.Y. -- Science. 2013 May 31;340(6136):1068-72. doi: 10.1126/science.1237317.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Planetary Science Institute, Tucson, AZ 85719, USA. williams@psi.edu〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/23723230" target="_blank"〉PubMed〈/a〉
    Print ISSN: 0036-8075
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  • 8
    Publication Date: 2013-09-28
    Description: The Mars Science Laboratory rover Curiosity scooped samples of soil from the Rocknest aeolian bedform in Gale crater. Analysis of the soil with the Chemistry and Mineralogy (CheMin) x-ray diffraction (XRD) instrument revealed plagioclase (~An57), forsteritic olivine (~Fo62), augite, and pigeonite, with minor K-feldspar, magnetite, quartz, anhydrite, hematite, and ilmenite. The minor phases are present at, or near, detection limits. The soil also contains 27 +/- 14 weight percent x-ray amorphous material, likely containing multiple Fe(3+)- and volatile-bearing phases, including possibly a substance resembling hisingerite. The crystalline component is similar to the normative mineralogy of certain basaltic rocks from Gusev crater on Mars and of martian basaltic meteorites. The amorphous component is similar to that found on Earth in places such as soils on the Mauna Kea volcano, Hawaii.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Bish, D L -- Blake, D F -- Vaniman, D T -- Chipera, S J -- Morris, R V -- Ming, D W -- Treiman, A H -- Sarrazin, P -- Morrison, S M -- Downs, R T -- Achilles, C N -- Yen, A S -- Bristow, T F -- Crisp, J A -- Morookian, J M -- Farmer, J D -- Rampe, E B -- Stolper, E M -- Spanovich, N -- MSL Science Team -- New York, N.Y. -- Science. 2013 Sep 27;341(6153):1238932. doi: 10.1126/science.1238932.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Department of Geological Sciences, Indiana University, Bloomington, IN 47405, USA. bish@indiana.edu〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/24072925" target="_blank"〉PubMed〈/a〉
    Print ISSN: 0036-8075
    Electronic ISSN: 1095-9203
    Topics: Biology , Chemistry and Pharmacology , Computer Science , Medicine , Natural Sciences in General , Physics
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  • 9
    Publication Date: 2016-02-26
    Description: 〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Battiston, Stefano -- Farmer, J Doyne -- Flache, Andreas -- Garlaschelli, Diego -- Haldane, Andrew G -- Heesterbeek, Hans -- Hommes, Cars -- Jaeger, Carlo -- May, Robert -- Scheffer, Marten -- New York, N.Y. -- Science. 2016 Feb 19;351(6275):818-9. doi: 10.1126/science.aad0299. Epub 2016 Feb 18.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Department of Banking and Finance, University of Zurich, 8032 Zurich, Switzerland. ; Institute for New Economic Thinking, Oxford Martin School, and Mathematical Institute, University of Oxford, Oxford OX1 2JD, UK. Santa Fe Institute, Santa Fe, NM 87501, USA. ; Department of Sociology, University of Groningen, 9712 TG Groningen, Netherlands. ; Lorentz Institute for Theoretical Physics, University of Leiden, 2333 CA Leiden, Netherlands. ; Bank of England, London, EC2R 8AH, UK. ; Faculty of Veterinary Medicine, University of Utrecht, 3512 JE Utrecht, Netherlands. ; Amsterdam School of Economics, University of Amsterdam, 1018 WB Amsterdam, Netherlands. Tinbergen Institute, 1082 MS Amsterdam, Netherlands. C.H.Hommes@uva.nl. ; Beijing Normal University, 100875 Beijing, China. Potsdam University, 14469 Potsdam, Germany. Global Climate Forum 10178 Berlin, Germany. ; Department of Zoology, University of Oxford, Oxford OX1 2JD, UK. ; Environmental Sciences, Wageningen University 6708 PB Wageningen, Netherlands.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/26912882" target="_blank"〉PubMed〈/a〉
    Print ISSN: 0036-8075
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  • 10
    Publication Date: 2017-06-16
    Description: The Mars Science Laboratory rover, Curiosity, is using a comprehensive scientific payload to explore rocks and soils in Gale crater, Mars. Recent investigations of the Bagnold Dune Field provided the first in situ assessment of an active dune on Mars. The CheMin X-ray diffraction instrument on Curiosity performed quantitative mineralogical analyses of the 〈150 μm size fraction of the Namib dune at a location called Gobabeb. Gobabeb is dominated by basaltic minerals. Plagioclase, Fo56 olivine, and two Ca-Mg-Fe pyroxenes account for the majority of crystalline phases along with minor magnetite, quartz, hematite, and anhydrite. In addition to the crystalline phases, a minimum ~42 wt% of the Gobabeb sample is X-ray amorphous. Mineralogical analysis of the Gobabeb dataset provides insights into the origin(s) and geologic history of the dune material and offers an important opportunity for ground truth of orbital observations. CheMin's analysis of the mineralogy and phase chemistry of modern and ancient Gale crater dune fields, together with other measurements by Curiosity's science payload, provides new insights into present and past eolian processes on Mars.
    Print ISSN: 0148-0227
    Topics: Geosciences , Physics
    Published by Wiley on behalf of American Geophysical Union (AGU).
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