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Hurowitz JA, Grotzinger JP, Fischer WW, McLennan SM, Milliken RE, Stein N, Vasavada AR, Blake DF, Dehouck E, Eigenbrode JL, Fairén AG, Frydenvang J, Gellert R, Grant JA, Gupta S, Herkenhoff KE, Ming DW, Rampe EB, Schmidt ME, Siebach KL, Stack-Morgan K, Sumner DY, Wiens RC. Redox stratification of an ancient lake in Gale crater, Mars. Science 2017; 356:356/6341/eaah6849. [PMID: 28572336 DOI: 10.1126/science.aah6849] [Citation(s) in RCA: 171] [Impact Index Per Article: 24.4] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 07/31/2016] [Accepted: 04/19/2017] [Indexed: 11/02/2022]
Abstract
In 2012, NASA's Curiosity rover landed on Mars to assess its potential as a habitat for past life and investigate the paleoclimate record preserved by sedimentary rocks inside the ~150-kilometer-diameter Gale impact crater. Geological reconstructions from Curiosity rover data have revealed an ancient, habitable lake environment fed by rivers draining into the crater. We synthesize geochemical and mineralogical data from lake-bed mudstones collected during the first 1300 martian solar days of rover operations in Gale. We present evidence for lake redox stratification, established by depth-dependent variations in atmospheric oxidant and dissolved-solute concentrations. Paleoclimate proxy data indicate that a transition from colder to warmer climate conditions is preserved in the stratigraphy. Finally, a late phase of geochemical modification by saline fluids is recognized.
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Affiliation(s)
- J A Hurowitz
- Department of Geosciences, Stony Brook University, Stony Brook, NY 11794-2100, USA.
| | - J P Grotzinger
- Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA 91125, USA
| | - W W Fischer
- Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA 91125, USA
| | - S M McLennan
- Department of Geosciences, Stony Brook University, Stony Brook, NY 11794-2100, USA
| | - R E Milliken
- Department of Geological Sciences, Brown University, Providence, RI 02912, USA
| | - N Stein
- Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA 91125, USA
| | - A R Vasavada
- Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA
| | - D F Blake
- Department of Space Sciences, NASA Ames Research Center, Moffett Field, CA 94035, USA
| | - E Dehouck
- Institut de Recherche en Astrophysique et Planétologie, University Paul Sabatier, 31028 Toulouse, France
| | - J L Eigenbrode
- NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA
| | - A G Fairén
- Centro de Astrobiología, Consejo Superior de Investigaciones Científicas-Instituto Nacional de Técnica Aeroespacial (CSIC-INTA), 28850 Madrid, Spain.,Department of Astronomy, Cornell University, Ithaca, NY 14853, USA
| | - J Frydenvang
- Space Remote Sensing, Los Alamos National Laboratory, Los Alamos, NM 87544, USA.,University of Copenhagen, 1350 Copenhagen, Denmark
| | - R Gellert
- Department of Physics, University of Guelph, Guelph, Ontario N1G 2W1, Canada
| | - J A Grant
- Center for Earth and Planetary Studies, National Air and Space Museum, Smithsonian Institution, Washington, DC 20560, USA
| | - S Gupta
- Department of Earth Science and Engineering, Imperial College London, London SW7 2AZ, UK
| | | | - D W Ming
- Astromaterials Research and Exploration Science Division, NASA Johnson Space Center, Houston, TX 77058, USA
| | - E B Rampe
- NASA Johnson Space Center, Houston, TX 77058, USA
| | - M E Schmidt
- Department of Earth Sciences, Brock University, St. Catharines, Ontario L2S 3A1, Canada
| | - K L Siebach
- Department of Geosciences, Stony Brook University, Stony Brook, NY 11794-2100, USA.,Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA 91125, USA
| | - K Stack-Morgan
- Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA
| | - D Y Sumner
- Department of Earth and Planetary Sciences, University of California-Davis, Davis, CA 95616, USA
| | - R C Wiens
- Space Remote Sensing, Los Alamos National Laboratory, Los Alamos, NM 87544, USA
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Lapotre MGA, Ewing RC, Lamb MP, Fischer WW, Grotzinger JP, Rubin DM, Lewis KW, Ballard MJ, Day M, Gupta S, Banham SG, Bridges NT, Des Marais DJ, Fraeman AA, Grant JA, Herkenhoff KE, Ming DW, Mischna MA, Rice MS, Sumner DY, Vasavada AR, Yingst RA. Large wind ripples on Mars: A record of atmospheric evolution. Science 2016; 353:55-8. [DOI: 10.1126/science.aaf3206] [Citation(s) in RCA: 124] [Impact Index Per Article: 15.5] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 01/25/2016] [Accepted: 05/31/2016] [Indexed: 11/03/2022]
Affiliation(s)
- M. G. A. Lapotre
- Division of Geological and Planetary Science, California Institute of Technology, Pasadena, CA 91125, USA
| | - R. C. Ewing
- Department of Geology and Geophysics, Texas A&M University, College Station, TX 77843, USA
| | - M. P. Lamb
- Division of Geological and Planetary Science, California Institute of Technology, Pasadena, CA 91125, USA
| | - W. W. Fischer
- Division of Geological and Planetary Science, California Institute of Technology, Pasadena, CA 91125, USA
| | - J. P. Grotzinger
- Division of Geological and Planetary Science, California Institute of Technology, Pasadena, CA 91125, USA
| | - D. M. Rubin
- Department of Earth and Planetary Sciences, University of California Santa Cruz, Santa Cruz, CA 95064, USA
| | - K. W. Lewis
- Department of Earth and Planetary Sciences, Johns Hopkins University, Baltimore, MD 21218, USA
| | - M. J. Ballard
- Department of Geology and Geophysics, Texas A&M University, College Station, TX 77843, USA
| | - M. Day
- Jackson School of Geosciences, University of Texas at Austin, Austin, TX 78712, USA
| | - S. Gupta
- Department of Earth Science and Engineering, Imperial College London, London SW7 2AZ, UK
| | - S. G. Banham
- Department of Earth Science and Engineering, Imperial College London, London SW7 2AZ, UK
| | - N. T. Bridges
- Applied Physics Laboratory, Johns Hopkins University, Laurel, MD 20723, USA
| | | | - A. A. Fraeman
- Division of Geological and Planetary Science, California Institute of Technology, Pasadena, CA 91125, USA
- Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA
| | - J. A. Grant
- National Air and Space Museum, Smithsonian Institution, Washington, DC 20560, USA
| | - K. E. Herkenhoff
- Astrogeology Science Center, U.S. Geological Survey, Flagstaff, AZ 86001-1698, USA
| | - D. W. Ming
- NASA Johnson Space Center, Houston, TX 77058, USA
| | - M. A. Mischna
- Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA
| | - M. S. Rice
- Geology Department, Western Washington University, Bellingham, WA 98225-9080, USA
| | - D. Y. Sumner
- Department of Earth and Planetary Sciences, University of California, Davis, CA 95616, USA
| | - A. R. Vasavada
- Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA
| | - R. A. Yingst
- Planetary Science Institute, Tucson, AZ 85719, USA
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Grotzinger JP, Gupta S, Malin MC, Rubin DM, Schieber J, Siebach K, Sumner DY, Stack KM, Vasavada AR, Arvidson RE, Calef F, Edgar L, Fischer WF, Grant JA, Griffes J, Kah LC, Lamb MP, Lewis KW, Mangold N, Minitti ME, Palucis M, Rice M, Williams RME, Yingst RA, Blake D, Blaney D, Conrad P, Crisp J, Dietrich WE, Dromart G, Edgett KS, Ewing RC, Gellert R, Hurowitz JA, Kocurek G, Mahaffy P, McBride MJ, McLennan SM, Mischna M, Ming D, Milliken R, Newsom H, Oehler D, Parker TJ, Vaniman D, Wiens RC, Wilson SA. Deposition, exhumation, and paleoclimate of an ancient lake deposit, Gale crater, Mars. Science 2015; 350:aac7575. [DOI: 10.1126/science.aac7575] [Citation(s) in RCA: 399] [Impact Index Per Article: 44.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/02/2022]
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McLennan SM, Anderson RB, Bell JF, Bridges JC, Calef F, Campbell JL, Clark BC, Clegg S, Conrad P, Cousin A, Des Marais DJ, Dromart G, Dyar MD, Edgar LA, Ehlmann BL, Fabre C, Forni O, Gasnault O, Gellert R, Gordon S, Grant JA, Grotzinger JP, Gupta S, Herkenhoff KE, Hurowitz JA, King PL, Le Mouélic S, Leshin LA, Léveillé R, Lewis KW, Mangold N, Maurice S, Ming DW, Morris RV, Nachon M, Newsom HE, Ollila AM, Perrett GM, Rice MS, Schmidt ME, Schwenzer SP, Stack K, Stolper EM, Sumner DY, Treiman AH, VanBommel S, Vaniman DT, Vasavada A, Wiens RC, Yingst RA. Elemental geochemistry of sedimentary rocks at Yellowknife Bay, Gale crater, Mars. Science 2013; 343:1244734. [PMID: 24324274 DOI: 10.1126/science.1244734] [Citation(s) in RCA: 214] [Impact Index Per Article: 19.5] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/02/2022]
Abstract
Sedimentary rocks examined by the Curiosity rover at Yellowknife Bay, Mars, were derived from sources that evolved from an approximately average martian crustal composition to one influenced by alkaline basalts. No evidence of chemical weathering is preserved, indicating arid, possibly cold, paleoclimates and rapid erosion and deposition. The absence of predicted geochemical variations indicates that magnetite and phyllosilicates formed by diagenesis under low-temperature, circumneutral pH, rock-dominated aqueous conditions. Analyses of diagenetic features (including concretions, raised ridges, and fractures) at high spatial resolution indicate that they are composed of iron- and halogen-rich components, magnesium-iron-chlorine-rich components, and hydrated calcium sulfates, respectively. Composition of a cross-cutting dike-like feature is consistent with sedimentary intrusion. The geochemistry of these sedimentary rocks provides further evidence for diverse depositional and diagenetic sedimentary environments during the early history of Mars.
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Affiliation(s)
- S M McLennan
- Department of Geosciences, State University of New York, Stony Brook, NY 11794, USA
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Grotzinger JP, Sumner DY, Kah LC, Stack K, Gupta S, Edgar L, Rubin D, Lewis K, Schieber J, Mangold N, Milliken R, Conrad PG, DesMarais D, Farmer J, Siebach K, Calef F, Hurowitz J, McLennan SM, Ming D, Vaniman D, Crisp J, Vasavada A, Edgett KS, Malin M, Blake D, Gellert R, Mahaffy P, Wiens RC, Maurice S, Grant JA, Wilson S, Anderson RC, Beegle L, Arvidson R, Hallet B, Sletten RS, Rice M, Bell J, Griffes J, Ehlmann B, Anderson RB, Bristow TF, Dietrich WE, Dromart G, Eigenbrode J, Fraeman A, Hardgrove C, Herkenhoff K, Jandura L, Kocurek G, Lee S, Leshin LA, Leveille R, Limonadi D, Maki J, McCloskey S, Meyer M, Minitti M, Newsom H, Oehler D, Okon A, Palucis M, Parker T, Rowland S, Schmidt M, Squyres S, Steele A, Stolper E, Summons R, Treiman A, Williams R, Yingst A, Team MS, Kemppinen O, Bridges N, Johnson JR, Cremers D, Godber A, Wadhwa M, Wellington D, McEwan I, Newman C, Richardson M, Charpentier A, Peret L, King P, Blank J, Weigle G, Li S, Robertson K, Sun V, Baker M, Edwards C, Farley K, Miller H, Newcombe M, Pilorget C, Brunet C, Hipkin V, Leveille R, Marchand G, Sanchez PS, Favot L, Cody G, Fluckiger L, Lees D, Nefian A, Martin M, Gailhanou M, Westall F, Israel G, Agard C, Baroukh J, Donny C, Gaboriaud A, Guillemot P, Lafaille V, Lorigny E, Paillet A, Perez R, Saccoccio M, Yana C, Armiens-Aparicio C, Rodriguez JC, Blazquez IC, Gomez FG, Gomez-Elvira J, Hettrich S, Malvitte AL, Jimenez MM, Martinez-Frias J, Martin-Soler J, Martin-Torres FJ, Jurado AM, Mora-Sotomayor L, Caro GM, Lopez SN, Peinado-Gonzalez V, Pla-Garcia J, Manfredi JAR, Romeral-Planello JJ, Fuentes SAS, Martinez ES, Redondo JT, Urqui-O'Callaghan R, Mier MPZ, Chipera S, Lacour JL, Mauchien P, Sirven JB, Manning H, Fairen A, Hayes A, Joseph J, Sullivan R, Thomas P, Dupont A, Lundberg A, Melikechi N, Mezzacappa A, DeMarines J, Grinspoon D, Reitz G, Prats B, Atlaskin E, Genzer M, Harri AM, Haukka H, Kahanpaa H, Kauhanen J, Paton M, Polkko J, Schmidt W, Siili T, Fabre C, Wray J, Wilhelm MB, Poitrasson F, Patel K, Gorevan S, Indyk S, Paulsen G, Bish D, Gondet B, Langevin Y, Geffroy C, Baratoux D, Berger G, Cros A, d'Uston C, Forni O, Gasnault O, Lasue J, Lee QM, Meslin PY, Pallier E, Parot Y, Pinet P, Schroder S, Toplis M, Lewin E, Brunner W, Heydari E, Achilles C, Sutter B, Cabane M, Coscia D, Szopa C, Robert F, Sautter V, Le Mouelic S, Nachon M, Buch A, Stalport F, Coll P, Francois P, Raulin F, Teinturier S, Cameron J, Clegg S, Cousin A, DeLapp D, Dingler R, Jackson RS, Johnstone S, Lanza N, Little C, Nelson T, Williams RB, Jones A, Kirkland L, Baker B, Cantor B, Caplinger M, Davis S, Duston B, Fay D, Harker D, Herrera P, Jensen E, Kennedy MR, Krezoski G, Krysak D, Lipkaman L, McCartney E, McNair S, Nixon B, Posiolova L, Ravine M, Salamon A, Saper L, Stoiber K, Supulver K, Van Beek J, Van Beek T, Zimdar R, French KL, Iagnemma K, Miller K, Goesmann F, Goetz W, Hviid S, Johnson M, Lefavor M, Lyness E, Breves E, Dyar MD, Fassett C, Edwards L, Haberle R, Hoehler T, Hollingsworth J, Kahre M, Keely L, McKay C, Bleacher L, Brinckerhoff W, Choi D, Dworkin JP, Floyd M, Freissinet C, Garvin J, Glavin D, Harpold D, Martin DK, McAdam A, Pavlov A, Raaen E, Smith MD, Stern J, Tan F, Trainer M, Posner A, Voytek M, Aubrey A, Behar A, Blaney D, Brinza D, Christensen L, DeFlores L, Feldman J, Feldman S, Flesch G, Jun I, Keymeulen D, Mischna M, Morookian JM, Pavri B, Schoppers M, Sengstacken A, Simmonds JJ, Spanovich N, Juarez MDLT, Webster CR, Yen A, Archer PD, Cucinotta F, Jones JH, Morris RV, Niles P, Rampe E, Nolan T, Fisk M, Radziemski L, Barraclough B, Bender S, Berman D, Dobrea EN, Tokar R, Cleghorn T, Huntress W, Manhes G, Hudgins J, Olson T, Stewart N, Sarrazin P, Vicenzi E, Bullock M, Ehresmann B, Hamilton V, Hassler D, Peterson J, Rafkin S, Zeitlin C, Fedosov F, Golovin D, Karpushkina N, Kozyrev A, Litvak M, Malakhov A, Mitrofanov I, Mokrousov M, Nikiforov S, Prokhorov V, Sanin A, Tretyakov V, Varenikov A, Vostrukhin A, Kuzmin R, Clark B, Wolff M, Botta O, Drake D, Bean K, Lemmon M, Schwenzer SP, Lee EM, Sucharski R, Hernandez MADP, Avalos JJB, Ramos M, Kim MH, Malespin C, Plante I, Muller JP, Navarro-Gonzalez R, Ewing R, Boynton W, Downs R, Fitzgibbon M, Harshman K, Morrison S, Kortmann O, Williams A, Lugmair G, Wilson MA, Jakosky B, Balic-Zunic T, Frydenvang J, Jensen JK, Kinch K, Koefoed A, Madsen MB, Stipp SLS, Boyd N, Campbell JL, Perrett G, Pradler I, VanBommel S, Jacob S, Owen T, Savijarvi H, Boehm E, Bottcher S, Burmeister S, Guo J, Kohler J, Garcia CM, Mueller-Mellin R, Wimmer-Schweingruber R, Bridges JC, McConnochie T, Benna M, Franz H, Bower H, Brunner A, Blau H, Boucher T, Carmosino M, Atreya S, Elliott H, Halleaux D, Renno N, Wong M, Pepin R, Elliott B, Spray J, Thompson L, Gordon S, Ollila A, Williams J, Vasconcelos P, Bentz J, Nealson K, Popa R, Moersch J, Tate C, Day M, Francis R, McCullough E, Cloutis E, ten Kate IL, Scholes D, Slavney S, Stein T, Ward J, Berger J, Moores JE. A Habitable Fluvio-Lacustrine Environment at Yellowknife Bay, Gale Crater, Mars. Science 2013; 343:1242777. [DOI: 10.1126/science.1242777] [Citation(s) in RCA: 578] [Impact Index Per Article: 52.5] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/02/2022]
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Ming DW, Archer PD, Glavin DP, Eigenbrode JL, Franz HB, Sutter B, Brunner AE, Stern JC, Freissinet C, McAdam AC, Mahaffy PR, Cabane M, Coll P, Campbell JL, Atreya SK, Niles PB, Bell JF, Bish DL, Brinckerhoff WB, Buch A, Conrad PG, Des Marais DJ, Ehlmann BL, Fairén AG, Farley K, Flesch GJ, Francois P, Gellert R, Grant JA, Grotzinger JP, Gupta S, Herkenhoff KE, Hurowitz JA, Leshin LA, Lewis KW, McLennan SM, Miller KE, Moersch J, Morris RV, Navarro-González R, Pavlov AA, Perrett GM, Pradler I, Squyres SW, Summons RE, Steele A, Stolper EM, Sumner DY, Szopa C, Teinturier S, Trainer MG, Treiman AH, Vaniman DT, Vasavada AR, Webster CR, Wray JJ, Yingst RA. Volatile and organic compositions of sedimentary rocks in Yellowknife Bay, Gale crater, Mars. Science 2013; 343:1245267. [PMID: 24324276 DOI: 10.1126/science.1245267] [Citation(s) in RCA: 135] [Impact Index Per Article: 12.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/02/2022]
Abstract
H2O, CO2, SO2, O2, H2, H2S, HCl, chlorinated hydrocarbons, NO, and other trace gases were evolved during pyrolysis of two mudstone samples acquired by the Curiosity rover at Yellowknife Bay within Gale crater, Mars. H2O/OH-bearing phases included 2:1 phyllosilicate(s), bassanite, akaganeite, and amorphous materials. Thermal decomposition of carbonates and combustion of organic materials are candidate sources for the CO2. Concurrent evolution of O2 and chlorinated hydrocarbons suggests the presence of oxychlorine phase(s). Sulfides are likely sources for sulfur-bearing species. Higher abundances of chlorinated hydrocarbons in the mudstone compared with Rocknest windblown materials previously analyzed by Curiosity suggest that indigenous martian or meteoritic organic carbon sources may be preserved in the mudstone; however, the carbon source for the chlorinated hydrocarbons is not definitively of martian origin.
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Affiliation(s)
- D W Ming
- Astromaterials Research and Exploration Science Directorate, NASA Johnson Space Center, Houston, TX 77058, USA
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Farley KA, Malespin C, Mahaffy P, Grotzinger JP, Vasconcelos PM, Milliken RE, Malin M, Edgett KS, Pavlov AA, Hurowitz JA, Grant JA, Miller HB, Arvidson R, Beegle L, Calef F, Conrad PG, Dietrich WE, Eigenbrode J, Gellert R, Gupta S, Hamilton V, Hassler DM, Lewis KW, McLennan SM, Ming D, Navarro-González R, Schwenzer SP, Steele A, Stolper EM, Sumner DY, Vaniman D, Vasavada A, Williford K, Wimmer-Schweingruber RF. In situ radiometric and exposure age dating of the martian surface. Science 2013; 343:1247166. [PMID: 24324273 DOI: 10.1126/science.1247166] [Citation(s) in RCA: 50] [Impact Index Per Article: 4.5] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/02/2022]
Abstract
We determined radiogenic and cosmogenic noble gases in a mudstone on the floor of Gale Crater. A K-Ar age of 4.21 ± 0.35 billion years represents a mixture of detrital and authigenic components and confirms the expected antiquity of rocks comprising the crater rim. Cosmic-ray-produced (3)He, (21)Ne, and (36)Ar yield concordant surface exposure ages of 78 ± 30 million years. Surface exposure occurred mainly in the present geomorphic setting rather than during primary erosion and transport. Our observations are consistent with mudstone deposition shortly after the Gale impact or possibly in a later event of rapid erosion and deposition. The mudstone remained buried until recent exposure by wind-driven scarp retreat. Sedimentary rocks exposed by this mechanism may thus offer the best potential for organic biomarker preservation against destruction by cosmic radiation.
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Affiliation(s)
- K A Farley
- Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA 91125, USA
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Zeidan F, Grant JA, Brown CA, McHaffie JG, Coghill RC. Mindfulness meditation-related pain relief: evidence for unique brain mechanisms in the regulation of pain. Neurosci Lett 2012; 520:165-73. [PMID: 22487846 DOI: 10.1016/j.neulet.2012.03.082] [Citation(s) in RCA: 149] [Impact Index Per Article: 12.4] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Grants] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 02/18/2012] [Revised: 03/21/2012] [Accepted: 03/27/2012] [Indexed: 12/19/2022]
Abstract
The cognitive modulation of pain is influenced by a number of factors ranging from attention, beliefs, conditioning, expectations, mood, and the regulation of emotional responses to noxious sensory events. Recently, mindfulness meditation has been found attenuate pain through some of these mechanisms including enhanced cognitive and emotional control, as well as altering the contextual evaluation of sensory events. This review discusses the brain mechanisms involved in mindfulness meditation-related pain relief across different meditative techniques, expertise and training levels, experimental procedures, and neuroimaging methodologies. Converging lines of neuroimaging evidence reveal that mindfulness meditation-related pain relief is associated with unique appraisal cognitive processes depending on expertise level and meditation tradition. Moreover, it is postulated that mindfulness meditation-related pain relief may share a common final pathway with other cognitive techniques in the modulation of pain.
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Affiliation(s)
- F Zeidan
- Wake Forest School of Medicine, Department of Neurobiology and Anatomy, Winston-Salem, NC, United States.
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Arvidson RE, Bell JF, Bellutta P, Cabrol NA, Catalano JG, Cohen J, Crumpler LS, Des Marais DJ, Estlin TA, Farrand WH, Gellert R, Grant JA, Greenberger RN, Guinness EA, Herkenhoff KE, Herman JA, Iagnemma KD, Johnson JR, Klingelhöfer G, Li R, Lichtenberg KA, Maxwell SA, Ming DW, Morris RV, Rice MS, Ruff SW, Shaw A, Siebach KL, de Souza PA, Stroupe AW, Squyres SW, Sullivan RJ, Talley KP, Townsend JA, Wang A, Wright JR, Yen AS. Spirit Mars Rover Mission: Overview and selected results from the northern Home Plate Winter Haven to the side of Scamander crater. ACTA ACUST UNITED AC 2010. [DOI: 10.1029/2010je003633] [Citation(s) in RCA: 97] [Impact Index Per Article: 6.9] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/09/2022]
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Arvidson RE, Ruff SW, Morris RV, Ming DW, Crumpler LS, Yen AS, Squyres SW, Sullivan RJ, Bell JF, Cabrol NA, Clark BC, Farrand WH, Gellert R, Greenberger R, Grant JA, Guinness EA, Herkenhoff KE, Hurowitz JA, Johnson JR, Klingelhöfer G, Lewis KW, Li R, McCoy TJ, Moersch J, McSween HY, Murchie SL, Schmidt M, Schröder C, Wang A, Wiseman S, Madsen MB, Goetz W, McLennan SM. Spirit Mars Rover Mission to the Columbia Hills, Gusev Crater: Mission overview and selected results from the Cumberland Ridge to Home Plate. ACTA ACUST UNITED AC 2008. [DOI: 10.1029/2008je003183] [Citation(s) in RCA: 77] [Impact Index Per Article: 4.8] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/10/2022]
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Mustard JF, Murchie SL, Pelkey SM, Ehlmann BL, Milliken RE, Grant JA, Bibring JP, Poulet F, Bishop J, Dobrea EN, Roach L, Seelos F, Arvidson RE, Wiseman S, Green R, Hash C, Humm D, Malaret E, McGovern JA, Seelos K, Clancy T, Clark R, Marais DD, Izenberg N, Knudson A, Langevin Y, Martin T, McGuire P, Morris R, Robinson M, Roush T, Smith M, Swayze G, Taylor H, Titus T, Wolff M. Hydrated silicate minerals on Mars observed by the Mars Reconnaissance Orbiter CRISM instrument. Nature 2008; 454:305-9. [DOI: 10.1038/nature07097] [Citation(s) in RCA: 552] [Impact Index Per Article: 34.5] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 04/24/2008] [Accepted: 05/08/2008] [Indexed: 11/09/2022]
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McCoy TJ, Sims M, Schmidt ME, Edwards L, Tornabene LL, Crumpler LS, Cohen BA, Soderblom LA, Blaney DL, Squyres SW, Arvidson RE, Rice JW, Tréguier E, d'Uston C, Grant JA, McSween HY, Golombek MP, Haldemann AFC, de Souza PA. Structure, stratigraphy, and origin of Husband Hill, Columbia Hills, Gusev Crater, Mars. ACTA ACUST UNITED AC 2008. [DOI: 10.1029/2007je003041] [Citation(s) in RCA: 38] [Impact Index Per Article: 2.4] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/10/2022]
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14
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McEwen AS, Hansen CJ, Delamere WA, Eliason EM, Herkenhoff KE, Keszthelyi L, Gulick VC, Kirk RL, Mellon MT, Grant JA, Thomas N, Weitz CM, Squyres SW, Bridges NT, Murchie SL, Seelos F, Seelos K, Okubo CH, Milazzo MP, Tornabene LL, Jaeger WL, Byrne S, Russell PS, Griffes JL, Martínez-Alonso S, Davatzes A, Chuang FC, Thomson BJ, Fishbaugh KE, Dundas CM, Kolb KJ, Banks ME, Wray JJ. A Closer Look at Water-Related Geologic Activity on Mars. Science 2007; 317:1706-9. [PMID: 17885125 DOI: 10.1126/science.1143987] [Citation(s) in RCA: 164] [Impact Index Per Article: 9.6] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/03/2022]
Abstract
Water has supposedly marked the surface of Mars and produced characteristic landforms. To understand the history of water on Mars, we take a close look at key locations with the High-Resolution Imaging Science Experiment on board the Mars Reconnaissance Orbiter, reaching fine spatial scales of 25 to 32 centimeters per pixel. Boulders ranging up to approximately 2 meters in diameter are ubiquitous in the middle to high latitudes, which include deposits previously interpreted as finegrained ocean sediments or dusty snow. Bright gully deposits identify six locations with very recent activity, but these lie on steep (20 degrees to 35 degrees) slopes where dry mass wasting could occur. Thus, we cannot confirm the reality of ancient oceans or water in active gullies but do see evidence of fluvial modification of geologically recent mid-latitude gullies and equatorial impact craters.
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Affiliation(s)
- A S McEwen
- Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ 85721, USA.
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15
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Grant JA, Pickup BT, Sykes MJ, Kitchen CA, Nicholls A. The Gaussian Generalized Born model: application to small molecules. Phys Chem Chem Phys 2007; 9:4913-22. [PMID: 17912422 DOI: 10.1039/b707574j] [Citation(s) in RCA: 40] [Impact Index Per Article: 2.4] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/21/2022]
Abstract
This work presents a Generalized Born model for the computation of the electrostatic component of solvation energies which is based on volume integration. An analytic masking function is introduced to remove Coulombic singularities. This approach leads to analytic formulae for the computation of Born radii, which are differentiable to arbitrary order, and computationally straightforward to implement.
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Affiliation(s)
- J A Grant
- AstraZeneca Pharmaceuticals, Mereside, Macclesfield, Cheshire, UK.
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16
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Squyres SW, Arvidson RE, Bollen D, Bell JF, Brückner J, Cabrol NA, Calvin WM, Carr MH, Christensen PR, Clark BC, Crumpler L, Des Marais DJ, d'Uston C, Economou T, Farmer J, Farrand WH, Folkner W, Gellert R, Glotch TD, Golombek M, Gorevan S, Grant JA, Greeley R, Grotzinger J, Herkenhoff KE, Hviid S, Johnson JR, Klingelhöfer G, Knoll AH, Landis G, Lemmon M, Li R, Madsen MB, Malin MC, McLennan SM, McSween HY, Ming DW, Moersch J, Morris RV, Parker T, Rice JW, Richter L, Rieder R, Schröder C, Sims M, Smith M, Smith P, Soderblom LA, Sullivan R, Tosca NJ, Wänke H, Wdowiak T, Wolff M, Yen A. Overview of the Opportunity Mars Exploration Rover Mission to Meridiani Planum: Eagle Crater to Purgatory Ripple. ACTA ACUST UNITED AC 2006. [DOI: 10.1029/2006je002771] [Citation(s) in RCA: 126] [Impact Index Per Article: 7.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/09/2022]
Affiliation(s)
- S. W. Squyres
- Department of Astronomy; Cornell University, Space Sciences Building; Ithaca New York USA
| | - R. E. Arvidson
- Department Earth and Planetary Sciences; Washington University; St. Louis Missouri USA
| | - D. Bollen
- Department of Astronomy; Cornell University, Space Sciences Building; Ithaca New York USA
| | - J. F. Bell
- Department of Astronomy; Cornell University, Space Sciences Building; Ithaca New York USA
| | - J. Brückner
- Max Planck Institut für Chemie, Kosmochemie; Mainz Germany
| | - N. A. Cabrol
- NASA Ames/SETI Institute; Moffett Field California USA
| | - W. M. Calvin
- Department of Geological Sciences; University of Nevada, Reno; Reno Nevada USA
| | - M. H. Carr
- U.S. Geological Survey; Menlo Park California USA
| | - P. R. Christensen
- Department of Geological Sciences; Arizona State University; Tempe Arizona USA
| | - B. C. Clark
- Lockheed Martin Corporation; Littleton Colorado USA
| | - L. Crumpler
- New Mexico Museum of Natural History and Science; Albuquerque New Mexico USA
| | | | - C. d'Uston
- Centre d'Etude Spatiale des Rayonnements; Toulouse France
| | - T. Economou
- Enrico Fermi Institute; University of Chicago; Chicago Illinois USA
| | - J. Farmer
- Department of Geological Sciences; Arizona State University; Tempe Arizona USA
| | | | - W. Folkner
- Jet Propulsion Laboratory; California Institute of Technology; Pasadena California USA
| | - R. Gellert
- Department of Physics; University of Guelph; Guelph, Ontario Canada
| | - T. D. Glotch
- Jet Propulsion Laboratory; California Institute of Technology; Pasadena California USA
| | - M. Golombek
- Jet Propulsion Laboratory; California Institute of Technology; Pasadena California USA
| | | | - J. A. Grant
- Center for Earth and Planetary Studies; Smithsonian Institution; Washington, D. C. USA
| | - R. Greeley
- Department of Geological Sciences; Arizona State University; Tempe Arizona USA
| | - J. Grotzinger
- Division of Geological and Planetary Sciences; California Institute of Technology; Pasadena California USA
| | | | - S. Hviid
- Max Planck Institut für Sonnensystemforschung; Katlenburg-Lindau Germany
| | | | - G. Klingelhöfer
- Institut für Anorganische und Analytische Chemie; Johannes Gutenberg-Universität; Mainz Germany
| | - A. H. Knoll
- Botanical Museum; Harvard University; Cambridge Massachusetts USA
| | - G. Landis
- NASA Glenn Research Center; Cleveland Ohio USA
| | - M. Lemmon
- Department of Atmospheric Sciences; Texas A&M University; College Station Texas USA
| | - R. Li
- Department of Civil and Environmental Engineering and Geodetic Science; Ohio State University; Columbus Ohio USA
| | - M. B. Madsen
- Niels Bohr Institute; Ørsted Laboratory; Copenhagen Denmark
| | - M. C. Malin
- Malin Space Science Systems; San Diego California USA
| | - S. M. McLennan
- Department of Geosciences; State University of New York; Stony Brook New York USA
| | - H. Y. McSween
- Department of Earth and Planetary Sciences; University of Tennessee; Knoxville Tennessee USA
| | - D. W. Ming
- NASA Johnson Space Center; Houston Texas USA
| | - J. Moersch
- Department of Earth and Planetary Sciences; University of Tennessee; Knoxville Tennessee USA
| | | | - T. Parker
- Jet Propulsion Laboratory; California Institute of Technology; Pasadena California USA
| | - J. W. Rice
- Department of Geological Sciences; Arizona State University; Tempe Arizona USA
| | - L. Richter
- DLR Institute of Space Simulation; Cologne Germany
| | - R. Rieder
- Max Planck Institut für Chemie, Kosmochemie; Mainz Germany
| | - C. Schröder
- Institut für Anorganische und Analytische Chemie; Johannes Gutenberg-Universität; Mainz Germany
| | - M. Sims
- NASA Ames Research Center; Moffett Field California USA
| | - M. Smith
- NASA Goddard Space Flight Center; Greenbelt Maryland USA
| | - P. Smith
- Lunar and Planetary Laboratory; University of Arizona; Tucson Arizona USA
| | | | - R. Sullivan
- Department of Astronomy; Cornell University, Space Sciences Building; Ithaca New York USA
| | - N. J. Tosca
- Department of Geosciences; State University of New York; Stony Brook New York USA
| | - H. Wänke
- Max Planck Institut für Chemie, Kosmochemie; Mainz Germany
| | - T. Wdowiak
- Department of Physics; University of Alabama at Birmingham; Birmingham Alabama USA
| | - M. Wolff
- Space Science Institute; Martinez Georgia USA
| | - A. Yen
- Jet Propulsion Laboratory; California Institute of Technology; Pasadena California USA
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17
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Golombek MP, Grant JA, Crumpler LS, Greeley R, Arvidson RE, Bell JF, Weitz CM, Sullivan R, Christensen PR, Soderblom LA, Squyres SW. Erosion rates at the Mars Exploration Rover landing sites and long-term climate change on Mars. ACTA ACUST UNITED AC 2006. [DOI: 10.1029/2006je002754] [Citation(s) in RCA: 181] [Impact Index Per Article: 10.1] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/09/2022]
Affiliation(s)
- M. P. Golombek
- Jet Propulsion Laboratory; California Institute of Technology; Pasadena California USA
| | - J. A. Grant
- Center for Earth and Planetary Studies, National Air and Space Museum; Smithsonian Institution; Washington, DC USA
| | - L. S. Crumpler
- New Mexico Museum of Natural History and Science; Albuquerque New Mexico USA
| | - R. Greeley
- Department of Geological Sciences; Arizona State University; Tempe Arizona USA
| | - R. E. Arvidson
- Department of Earth and Planetary Sciences; Washington University; St. Louis Missouri USA
| | - J. F. Bell
- Department of Astronomy; Cornell University; Ithaca New York USA
| | - C. M. Weitz
- Planetary Science Institute; Tucson Arizona USA
| | - R. Sullivan
- Department of Astronomy; Cornell University; Ithaca New York USA
| | - P. R. Christensen
- Department of Geological Sciences; Arizona State University; Tempe Arizona USA
| | | | - S. W. Squyres
- Department of Astronomy; Cornell University; Ithaca New York USA
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18
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Grant JA, Bishop NE, Götzen N, Sprecher C, Honl M, Morlock MM. Artificial composite bone as a model of human trabecular bone: the implant-bone interface. J Biomech 2006; 40:1158-64. [PMID: 16806236 DOI: 10.1016/j.jbiomech.2006.04.007] [Citation(s) in RCA: 101] [Impact Index Per Article: 5.6] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 01/27/2006] [Accepted: 04/14/2006] [Indexed: 10/24/2022]
Abstract
The use of artificial bones in implant testing has become popular due to their low variability and ready availability. However, friction coefficients, which are critical to load transfer in uncemented implants, have rarely been compared between human and artificial bone, particularly for wet and dry conditions. In this study, the static and dynamic friction coefficients for four commercially used titanium surfaces (polished, Al(2)O(3) blasted, plasma sprayed, beaded) acting on the trabecular component of artificial bones (Sawbones) were compared to those for human trabecular bone. Artificial bones were tested in dry and wet conditions and normal interface stress was varied (0.25, 0.5, 1.0MPa). Friction coefficients were mostly lower for artificial bones than real bone. In particular, static friction coefficients for the dry polished surface were 20% of those for real bone and 42-61% for the dry beaded surface, with statistical significance (alpha<0.05). Less marked differences were observed for dynamic friction coefficients. Significant but non-systematic effects of normal stress or wet/dry condition on friction coefficients were observed within each surface type. These results indicate that the use of artificial bone models for pre-clinical implant testing that rely on interface load transfer with trabecular bone for mechanical integrity can be particularly sensitive to surface finish and lubrication conditions.
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Affiliation(s)
- J A Grant
- Biomechanics Section, TUHH Hamburg University of Technology, Denickestrasse 15, Hamburg D-21073, Germany
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19
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Golombek MP, Crumpler LS, Grant JA, Greeley R, Cabrol NA, Parker TJ, Rice JW, Ward JG, Arvidson RE, Moersch JE, Fergason RL, Christensen PR, Castaño A, Castaño R, Haldemann AFC, Li R, Bell JF, Squyres SW. Geology of the Gusev cratered plains from the Spirit rover transverse. ACTA ACUST UNITED AC 2006. [DOI: 10.1029/2005je002503] [Citation(s) in RCA: 97] [Impact Index Per Article: 5.4] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/10/2022]
Affiliation(s)
- M. P. Golombek
- Jet Propulsion Laboratory; California Institute of Technology; Pasadena California USA
| | - L. S. Crumpler
- New Mexico Museum of Natural History and Science; Albuquerque New Mexico USA
| | | | - R. Greeley
- Department of Geological Sciences; Arizona State University; Tempe Arizona USA
| | - N. A. Cabrol
- NASA Ames Research Center; Moffett Field California USA
| | - T. J. Parker
- Jet Propulsion Laboratory; California Institute of Technology; Pasadena California USA
| | - J. W. Rice
- Department of Geological Sciences; Arizona State University; Tempe Arizona USA
| | - J. G. Ward
- Department of Earth and Planetary Sciences; Washington University; St. Louis Missouri USA
| | - R. E. Arvidson
- Department of Earth and Planetary Sciences; Washington University; St. Louis Missouri USA
| | - J. E. Moersch
- Department of Geological Sciences; University of Tennessee; Knoxville Tennessee USA
| | - R. L. Fergason
- Department of Geological Sciences; Arizona State University; Tempe Arizona USA
| | - P. R. Christensen
- Department of Geological Sciences; Arizona State University; Tempe Arizona USA
| | - A. Castaño
- Jet Propulsion Laboratory; California Institute of Technology; Pasadena California USA
| | - R. Castaño
- Jet Propulsion Laboratory; California Institute of Technology; Pasadena California USA
| | - A. F. C. Haldemann
- Jet Propulsion Laboratory; California Institute of Technology; Pasadena California USA
| | - R. Li
- Department of Civil and Environmental Engineering and Geodetic Science; Ohio State University; Columbus Ohio USA
| | - J. F. Bell
- Department of Astronomy; Cornell University; Ithaca New York USA
| | - S. W. Squyres
- Department of Astronomy; Cornell University; Ithaca New York USA
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20
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Arvidson RE, Squyres SW, Anderson RC, Bell JF, Blaney D, Brückner J, Cabrol NA, Calvin WM, Carr MH, Christensen PR, Clark BC, Crumpler L, Des Marais DJ, de Souza PA, d'Uston C, Economou T, Farmer J, Farrand WH, Folkner W, Golombek M, Gorevan S, Grant JA, Greeley R, Grotzinger J, Guinness E, Hahn BC, Haskin L, Herkenhoff KE, Hurowitz JA, Hviid S, Johnson JR, Klingelhöfer G, Knoll AH, Landis G, Leff C, Lemmon M, Li R, Madsen MB, Malin MC, McLennan SM, McSween HY, Ming DW, Moersch J, Morris RV, Parker T, Rice JW, Richter L, Rieder R, Rodionov DS, Schröder C, Sims M, Smith M, Smith P, Soderblom LA, Sullivan R, Thompson SD, Tosca NJ, Wang A, Wänke H, Ward J, Wdowiak T, Wolff M, Yen A. Overview of the Spirit Mars Exploration Rover Mission to Gusev Crater: Landing site to Backstay Rock in the Columbia Hills. ACTA ACUST UNITED AC 2006. [DOI: 10.1029/2005je002499] [Citation(s) in RCA: 202] [Impact Index Per Article: 11.2] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/10/2022]
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21
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Grant JA, Arvidson RE, Crumpler LS, Golombek MP, Hahn B, Haldemann AFC, Li R, Soderblom LA, Squyres SW, Wright SP, Watters WA. Crater gradation in Gusev crater and Meridiani Planum, Mars. ACTA ACUST UNITED AC 2006. [DOI: 10.1029/2005je002465] [Citation(s) in RCA: 57] [Impact Index Per Article: 3.2] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/09/2022]
Affiliation(s)
- J. A. Grant
- Center for Earth and Planetary Studies; National Air and Space Museum, Smithsonian Institution; Washington, DC USA
| | - R. E. Arvidson
- Department of Earth and Planetary Sciences; Washington University; St. Louis Missouri USA
| | - L. S. Crumpler
- New Mexico Museum of Natural History and Science; Albuquerque New Mexico USA
| | - M. P. Golombek
- Jet Propulsion Laboratory; California Institute of Technology; Pasadena California USA
| | - B. Hahn
- Department of Geosciences; State University of New York; Stony Brook New York USA
| | - A. F. C. Haldemann
- Jet Propulsion Laboratory; California Institute of Technology; Pasadena California USA
| | - R. Li
- Department of Civil and Environmental Engineering and Geodetic Science; Ohio State University; Columbus Ohio USA
| | | | - S. W. Squyres
- Department of Astronomy; Cornell University; Ithaca New York USA
| | - S. P. Wright
- Department of Geological Sciences; Arizona State University; Tempe Arizona USA
| | - W. A. Watters
- Department of Earth, Atmospheric, and Planetary Sciences; Massachusetts Institute of Technology; Cambridge Massachusetts USA
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22
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Golombek MP, Arvidson RE, Bell JF, Christensen PR, Crisp JA, Crumpler LS, Ehlmann BL, Fergason RL, Grant JA, Greeley R, Haldemann AFC, Kass DM, Parker TJ, Schofield JT, Squyres SW, Zurek RW. Assessment of Mars Exploration Rover landing site predictions. Nature 2005; 436:44-8. [PMID: 16001058 DOI: 10.1038/nature03600] [Citation(s) in RCA: 85] [Impact Index Per Article: 4.5] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/09/2022]
Abstract
Comprehensive analyses of remote sensing data during the three-year effort to select the Mars Exploration Rover landing sites at Gusev crater and at Meridiani Planum correctly predicted the atmospheric density profile during entry and descent and the safe and trafficable surfaces explored by the two rovers. The Gusev crater site was correctly predicted to be a low-relief surface that was less rocky than the Viking landing sites but comparably dusty. A dark, low-albedo, flat plain composed of basaltic sand and haematite with very few rocks was expected and found at Meridiani Planum. These results argue that future efforts to select safe landing sites based on existing and acquired remote sensing data will be successful. In contrast, geological interpretations of the sites based on remote sensing data were less certain and less successful, which emphasizes the inherent ambiguities in understanding surface geology from remotely sensed data and the uncertainty in predicting exactly what materials will be available for study at a landing site.
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Affiliation(s)
- M P Golombek
- Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California 91109, USA.
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23
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Squyres SW, Arvidson RE, Bell JF, Brückner J, Cabrol NA, Calvin W, Carr MH, Christensen PR, Clark BC, Crumpler L, Marais DJD, d'Uston C, Economou T, Farmer J, Farrand W, Folkner W, Golombek M, Gorevan S, Grant JA, Greeley R, Grotzinger J, Haskin L, Herkenhoff KE, Hviid S, Johnson J, Klingelhöfer G, Knoll AH, Landis G, Lemmon M, Li R, Madsen MB, Malin MC, McLennan SM, McSween HY, Ming DW, Moersch J, Morris RV, Parker T, Rice JW, Richter L, Rieder R, Sims M, Smith M, Smith P, Soderblom LA, Sullivan R, Wänke H, Wdowiak T, Wolff M, Yen A. The Opportunity Rover's Athena science investigation at Meridiani Planum, Mars. Science 2004; 306:1698-703. [PMID: 15576602 DOI: 10.1126/science.1106171] [Citation(s) in RCA: 130] [Impact Index Per Article: 6.5] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/02/2022]
Abstract
The Mars Exploration Rover Opportunity has investigated the landing site in Eagle crater and the nearby plains within Meridiani Planum. The soils consist of fine-grained basaltic sand and a surface lag of hematite-rich spherules, spherule fragments, and other granules. Wind ripples are common. Underlying the thin soil layer, and exposed within small impact craters and troughs, are flat-lying sedimentary rocks. These rocks are finely laminated, are rich in sulfur, and contain abundant sulfate salts. Small-scale cross-lamination in some locations provides evidence for deposition in flowing liquid water. We interpret the rocks to be a mixture of chemical and siliciclastic sediments formed by episodic inundation by shallow surface water, followed by evaporation, exposure, and desiccation. Hematite-rich spherules are embedded in the rock and eroding from them. We interpret these spherules to be concretions formed by postdepositional diagenesis, again involving liquid water.
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Affiliation(s)
- S W Squyres
- Department of Astronomy, Space Sciences Building, Cornell University, Ithaca, NY 14853, USA.
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24
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Squyres SW, Arvidson RE, Bell JF, Brückner J, Cabrol NA, Calvin W, Carr MH, Christensen PR, Clark BC, Crumpler L, Des Marais DJ, D'Uston C, Economou T, Farmer J, Farrand W, Folkner W, Golombek M, Gorevan S, Grant JA, Greeley R, Grotzinger J, Haskin L, Herkenhoff KE, Hviid S, Johnson J, Klingelhöfer G, Knoll A, Landis G, Lemmon M, Li R, Madsen MB, Malin MC, McLennan SM, McSween HY, Ming DW, Moersch J, Morris RV, Parker T, Rice JW, Richter L, Rieder R, Sims M, Smith M, Smith P, Soderblom LA, Sullivan R, Wänke H, Wdowiak T, Wolff M, Yen A. The Spirit Rover's Athena science investigation at Gusev Crater, Mars. Science 2004; 305:794-9. [PMID: 15297657 DOI: 10.1126/science.1100194] [Citation(s) in RCA: 25] [Impact Index Per Article: 1.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Subscribe] [Scholar Register] [Indexed: 11/02/2022]
Abstract
The Mars Exploration Rover Spirit and its Athena science payload have been used to investigate a landing site in Gusev crater. Gusev is hypothesized to be the site of a former lake, but no clear evidence for lacustrine sedimentation has been found to date. Instead, the dominant lithology is basalt, and the dominant geologic processes are impact events and eolian transport. Many rocks exhibit coatings and other characteristics that may be evidence for minor aqueous alteration. Any lacustrine sediments that may exist at this location within Gusev apparently have been buried by lavas that have undergone subsequent impact disruption.
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Affiliation(s)
- S W Squyres
- Department of Astronomy, Cornell University, Ithaca, NY 14853, USA.
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25
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Arvidson RE, Anderson RC, Bartlett P, Bell JF, Blaney D, Christensen PR, Chu P, Crumpler L, Davis K, Ehlmann BL, Fergason R, Golombek MP, Gorevan S, Grant JA, Greeley R, Guinness EA, Haldemann AFC, Herkenhoff K, Johnson J, Landis G, Li R, Lindemann R, McSween H, Ming DW, Myrick T, Richter L, Seelos FP, Squyres SW, Sullivan RJ, Wang A, Wilson J. Localization and physical properties experiments conducted by Spirit at Gusev Crater. Science 2004; 305:821-4. [PMID: 15297662 DOI: 10.1126/science.1099922] [Citation(s) in RCA: 144] [Impact Index Per Article: 7.2] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/02/2022]
Abstract
The precise location and relative elevation of Spirit during its traverses from the Columbia Memorial station to Bonneville crater were determined with bundle-adjusted retrievals from rover wheel turns, suspension and tilt angles, and overlapping images. Physical properties experiments show a decrease of 0.2% per Mars solar day in solar cell output resulting from deposition of airborne dust, cohesive soil-like deposits in plains and hollows, bright and dark rock coatings, and relatively weak volcanic rocks of basaltic composition. Volcanic, impact, aeolian, and water-related processes produced the encountered landforms and materials.
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Affiliation(s)
- R E Arvidson
- Department of Earth and Planetary Sciences, Washington University, St. Louis, MO 63130, USA
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26
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Bell JF, Squyres SW, Arvidson RE, Arneson HM, Bass D, Blaney D, Cabrol N, Calvin W, Farmer J, Farrand WH, Goetz W, Golombek M, Grant JA, Greeley R, Guinness E, Hayes AG, Hubbard MYH, Herkenhoff KE, Johnson MJ, Johnson JR, Joseph J, Kinch KM, Lemmon MT, Li R, Madsen MB, Maki JN, Malin M, McCartney E, McLennan S, McSween HY, Ming DW, Moersch JE, Morris RV, Dobrea EZN, Parker TJ, Proton J, Rice JW, Seelos F, Soderblom J, Soderblom LA, Sohl-Dickstein JN, Sullivan RJ, Wolff MJ, Wang A. Pancam multispectral imaging results from the Spirit Rover at Gusev Crater. Science 2004; 305:800-6. [PMID: 15297658 DOI: 10.1126/science.1100175] [Citation(s) in RCA: 130] [Impact Index Per Article: 6.5] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/02/2022]
Abstract
Panoramic Camera images at Gusev crater reveal a rock-strewn surface interspersed with high- to moderate-albedo fine-grained deposits occurring in part as drifts or in small circular swales or hollows. Optically thick coatings of fine-grained ferric iron-rich dust dominate most bright soil and rock surfaces. Spectra of some darker rock surfaces and rock regions exposed by brushing or grinding show near-infrared spectral signatures consistent with the presence of mafic silicates such as pyroxene or olivine. Atmospheric observations show a steady decline in dust opacity during the mission, and astronomical observations captured solar transits by the martian moons, Phobos and Deimos, as well as a view of Earth from the martian surface.
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Affiliation(s)
- J F Bell
- Cornell University, Ithaca, NY 14853-6801, USA.
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27
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Greeley R, Squyres SW, Arvidson RE, Bartlett P, Bell JF, Blaney D, Cabrol NA, Farmer J, Farrand B, Golombek MP, Gorevan SP, Grant JA, Haldemann AFC, Herkenhoff KE, Johnson J, Landis G, Madsen MB, McLennan SM, Moersch J, Rice JW, Richter L, Ruff S, Sullivan RJ, Thompson SD, Wang A, Weitz CM, Whelley P. Wind-related processes detected by the Spirit Rover at Gusev Crater, Mars. Science 2004; 305:810-3. [PMID: 15297660 DOI: 10.1126/science.1100108] [Citation(s) in RCA: 86] [Impact Index Per Article: 4.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/02/2022]
Abstract
Wind-abraded rocks, ripples, drifts, and other deposits of windblown sediments are seen at the Columbia Memorial Station where the Spirit rover landed. Orientations of these features suggest formative winds from the north-northwest, consistent with predictions from atmospheric models of afternoon winds in Gusev Crater. Cuttings from the rover Rock Abrasion Tool are asymmetrically distributed toward the south-southeast, suggesting active winds from the north-northwest at the time (midday) of the abrasion operations. Characteristics of some rocks, such as a two-toned appearance, suggest that they were possibly buried and exhumed on the order of 5 to 60 centimeters by wind deflation, depending on location.
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Affiliation(s)
- R Greeley
- Department of Geological Sciences, Arizona State University, Box 871404, Tempe, AZ 85287-1404, USA.
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28
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Grant JA, Arvidson R, Bell JF, Cabrol NA, Carr MH, Christensen P, Crumpler L, Des Marais DJ, Ehlmann BL, Farmer J, Golombek M, Grant FD, Greeley R, Herkenhoff K, Li R, McSween HY, Ming DW, Moersch J, Rice JW, Ruff S, Richter L, Squyres S, Sullivan R, Weitz C. Surficial Deposits at Gusev Crater Along Spirit Rover Traverses. Science 2004; 305:807-10. [PMID: 15297659 DOI: 10.1126/science.1099849] [Citation(s) in RCA: 71] [Impact Index Per Article: 3.6] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/02/2022]
Abstract
The Mars Exploration Rover Spirit has traversed a fairly flat, rock-strewn terrain whose surface is shaped primarily by impact events, although some of the landscape has been altered by eolian processes. Impacts ejected basaltic rocks that probably were part of locally formed lava flows from at least 10 meters depth. Some rocks have been textured and/or partially buried by windblown sediments less than 2 millimeters in diameter that concentrate within shallow, partially filled, circular impact depressions referred to as hollows. The terrain traversed during the 90-sol (martian solar day) nominal mission shows no evidence for an ancient lake in Gusev crater.
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Affiliation(s)
- J A Grant
- Center for Earth and Planetary Studies, National Air and Space Museum, Smithsonian Institution, Washington, DC 20560, USA.
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29
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Bell JF, Squyres SW, Arvidson RE, Arneson HM, Bass D, Blaney D, Cabrol N, Calvin W, Farmer J, Farrand WH, Goetz W, Golombek M, Grant JA, Greeley R, Guinness E, Hayes AG, Hubbard MYH, Herkenhoff KE, Johnson MJ, Johnson JR, Joseph J, Kinch KM, Lemmon MT, Li R, Madsen MB, Maki JN, Malin M, McCartney E, McLennan S, McSween HY, Ming DW, Moersch JE, Morris RV, Dobrea EZN, Parker TJ, Proton J, Rice JW, Seelos F, Soderblom J, Soderblom LA, Sohl-Dickstein JN, Sullivan RJ, Wolff MJ, Wang A. Pancam multispectral imaging results from the Spirit Rover at Gusev Crater. Science 2004. [PMID: 15297658 DOI: 10.1126/science.1100175,2004] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.1] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Subscribe] [Scholar Register] [Indexed: 11/02/2022]
Abstract
Panoramic Camera images at Gusev crater reveal a rock-strewn surface interspersed with high- to moderate-albedo fine-grained deposits occurring in part as drifts or in small circular swales or hollows. Optically thick coatings of fine-grained ferric iron-rich dust dominate most bright soil and rock surfaces. Spectra of some darker rock surfaces and rock regions exposed by brushing or grinding show near-infrared spectral signatures consistent with the presence of mafic silicates such as pyroxene or olivine. Atmospheric observations show a steady decline in dust opacity during the mission, and astronomical observations captured solar transits by the martian moons, Phobos and Deimos, as well as a view of Earth from the martian surface.
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Affiliation(s)
- J F Bell
- Cornell University, Ithaca, NY 14853-6801, USA.
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30
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Squyres SW, Arvidson RE, Bell JF, Brückner J, Cabrol NA, Calvin W, Carr MH, Christensen PR, Clark BC, Crumpler L, Des Marais DJ, d'Uston C, Economou T, Farmer J, Farrand W, Folkner W, Golombek M, Gorevan S, Grant JA, Greeley R, Grotzinger J, Haskin L, Herkenhoff KE, Hviid S, Johnson J, Klingelhöfer G, Knoll A, Landis G, Lemmon M, Li R, Madsen MB, Malin MC, McLennan SM, McSween HY, Ming DW, Moersch J, Morris RV, Parker T, Rice JW, Richter L, Rieder R, Sims M, Smith M, Smith P, Soderblom LA, Sullivan R, Wänke H, Wdowiak T, Wolff M, Yen A. The Spirit Rover's Athena Science Investigation at Gusev Crater, Mars. Science 2004. [DOI: 10.1126/science.3050794] [Citation(s) in RCA: 337] [Impact Index Per Article: 16.9] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/02/2022]
Affiliation(s)
- S. W. Squyres
- Department of Astronomy, Cornell University, Ithaca, NY 14853, USA
- Department of Earth and Planetary Sciences, Washington University, St. Louis, MO 63130, USA
- Abteilung Kosmochemie, Max-Planck-Institut für Chemie, Postfach 3060, D-55128 Mainz, Germany
- NASA Ames/SETI Institute, Moffett Field, CA 94035, USA
- Department of Geological Sciences, University of Nevada, Reno, NV 89557, USA
| | - R. E. Arvidson
- Department of Astronomy, Cornell University, Ithaca, NY 14853, USA
- Department of Earth and Planetary Sciences, Washington University, St. Louis, MO 63130, USA
- Abteilung Kosmochemie, Max-Planck-Institut für Chemie, Postfach 3060, D-55128 Mainz, Germany
- NASA Ames/SETI Institute, Moffett Field, CA 94035, USA
- Department of Geological Sciences, University of Nevada, Reno, NV 89557, USA
| | - J. F. Bell
- Department of Astronomy, Cornell University, Ithaca, NY 14853, USA
- Department of Earth and Planetary Sciences, Washington University, St. Louis, MO 63130, USA
- Abteilung Kosmochemie, Max-Planck-Institut für Chemie, Postfach 3060, D-55128 Mainz, Germany
- NASA Ames/SETI Institute, Moffett Field, CA 94035, USA
- Department of Geological Sciences, University of Nevada, Reno, NV 89557, USA
| | - J. Brückner
- Department of Astronomy, Cornell University, Ithaca, NY 14853, USA
- Department of Earth and Planetary Sciences, Washington University, St. Louis, MO 63130, USA
- Abteilung Kosmochemie, Max-Planck-Institut für Chemie, Postfach 3060, D-55128 Mainz, Germany
- NASA Ames/SETI Institute, Moffett Field, CA 94035, USA
- Department of Geological Sciences, University of Nevada, Reno, NV 89557, USA
| | - N. A. Cabrol
- Department of Astronomy, Cornell University, Ithaca, NY 14853, USA
- Department of Earth and Planetary Sciences, Washington University, St. Louis, MO 63130, USA
- Abteilung Kosmochemie, Max-Planck-Institut für Chemie, Postfach 3060, D-55128 Mainz, Germany
- NASA Ames/SETI Institute, Moffett Field, CA 94035, USA
- Department of Geological Sciences, University of Nevada, Reno, NV 89557, USA
| | - W. Calvin
- Department of Astronomy, Cornell University, Ithaca, NY 14853, USA
- Department of Earth and Planetary Sciences, Washington University, St. Louis, MO 63130, USA
- Abteilung Kosmochemie, Max-Planck-Institut für Chemie, Postfach 3060, D-55128 Mainz, Germany
- NASA Ames/SETI Institute, Moffett Field, CA 94035, USA
- Department of Geological Sciences, University of Nevada, Reno, NV 89557, USA
| | - M. H. Carr
- Department of Astronomy, Cornell University, Ithaca, NY 14853, USA
- Department of Earth and Planetary Sciences, Washington University, St. Louis, MO 63130, USA
- Abteilung Kosmochemie, Max-Planck-Institut für Chemie, Postfach 3060, D-55128 Mainz, Germany
- NASA Ames/SETI Institute, Moffett Field, CA 94035, USA
- Department of Geological Sciences, University of Nevada, Reno, NV 89557, USA
| | - P. R. Christensen
- Department of Astronomy, Cornell University, Ithaca, NY 14853, USA
- Department of Earth and Planetary Sciences, Washington University, St. Louis, MO 63130, USA
- Abteilung Kosmochemie, Max-Planck-Institut für Chemie, Postfach 3060, D-55128 Mainz, Germany
- NASA Ames/SETI Institute, Moffett Field, CA 94035, USA
- Department of Geological Sciences, University of Nevada, Reno, NV 89557, USA
| | - B. C. Clark
- Department of Astronomy, Cornell University, Ithaca, NY 14853, USA
- Department of Earth and Planetary Sciences, Washington University, St. Louis, MO 63130, USA
- Abteilung Kosmochemie, Max-Planck-Institut für Chemie, Postfach 3060, D-55128 Mainz, Germany
- NASA Ames/SETI Institute, Moffett Field, CA 94035, USA
- Department of Geological Sciences, University of Nevada, Reno, NV 89557, USA
| | - L. Crumpler
- Department of Astronomy, Cornell University, Ithaca, NY 14853, USA
- Department of Earth and Planetary Sciences, Washington University, St. Louis, MO 63130, USA
- Abteilung Kosmochemie, Max-Planck-Institut für Chemie, Postfach 3060, D-55128 Mainz, Germany
- NASA Ames/SETI Institute, Moffett Field, CA 94035, USA
- Department of Geological Sciences, University of Nevada, Reno, NV 89557, USA
| | - D. J. Des Marais
- Department of Astronomy, Cornell University, Ithaca, NY 14853, USA
- Department of Earth and Planetary Sciences, Washington University, St. Louis, MO 63130, USA
- Abteilung Kosmochemie, Max-Planck-Institut für Chemie, Postfach 3060, D-55128 Mainz, Germany
- NASA Ames/SETI Institute, Moffett Field, CA 94035, USA
- Department of Geological Sciences, University of Nevada, Reno, NV 89557, USA
| | - C. d'Uston
- Department of Astronomy, Cornell University, Ithaca, NY 14853, USA
- Department of Earth and Planetary Sciences, Washington University, St. Louis, MO 63130, USA
- Abteilung Kosmochemie, Max-Planck-Institut für Chemie, Postfach 3060, D-55128 Mainz, Germany
- NASA Ames/SETI Institute, Moffett Field, CA 94035, USA
- Department of Geological Sciences, University of Nevada, Reno, NV 89557, USA
| | - T. Economou
- Department of Astronomy, Cornell University, Ithaca, NY 14853, USA
- Department of Earth and Planetary Sciences, Washington University, St. Louis, MO 63130, USA
- Abteilung Kosmochemie, Max-Planck-Institut für Chemie, Postfach 3060, D-55128 Mainz, Germany
- NASA Ames/SETI Institute, Moffett Field, CA 94035, USA
- Department of Geological Sciences, University of Nevada, Reno, NV 89557, USA
| | - J. Farmer
- Department of Astronomy, Cornell University, Ithaca, NY 14853, USA
- Department of Earth and Planetary Sciences, Washington University, St. Louis, MO 63130, USA
- Abteilung Kosmochemie, Max-Planck-Institut für Chemie, Postfach 3060, D-55128 Mainz, Germany
- NASA Ames/SETI Institute, Moffett Field, CA 94035, USA
- Department of Geological Sciences, University of Nevada, Reno, NV 89557, USA
| | - W. Farrand
- Department of Astronomy, Cornell University, Ithaca, NY 14853, USA
- Department of Earth and Planetary Sciences, Washington University, St. Louis, MO 63130, USA
- Abteilung Kosmochemie, Max-Planck-Institut für Chemie, Postfach 3060, D-55128 Mainz, Germany
- NASA Ames/SETI Institute, Moffett Field, CA 94035, USA
- Department of Geological Sciences, University of Nevada, Reno, NV 89557, USA
| | - W. Folkner
- Department of Astronomy, Cornell University, Ithaca, NY 14853, USA
- Department of Earth and Planetary Sciences, Washington University, St. Louis, MO 63130, USA
- Abteilung Kosmochemie, Max-Planck-Institut für Chemie, Postfach 3060, D-55128 Mainz, Germany
- NASA Ames/SETI Institute, Moffett Field, CA 94035, USA
- Department of Geological Sciences, University of Nevada, Reno, NV 89557, USA
| | - M. Golombek
- Department of Astronomy, Cornell University, Ithaca, NY 14853, USA
- Department of Earth and Planetary Sciences, Washington University, St. Louis, MO 63130, USA
- Abteilung Kosmochemie, Max-Planck-Institut für Chemie, Postfach 3060, D-55128 Mainz, Germany
- NASA Ames/SETI Institute, Moffett Field, CA 94035, USA
- Department of Geological Sciences, University of Nevada, Reno, NV 89557, USA
| | - S. Gorevan
- Department of Astronomy, Cornell University, Ithaca, NY 14853, USA
- Department of Earth and Planetary Sciences, Washington University, St. Louis, MO 63130, USA
- Abteilung Kosmochemie, Max-Planck-Institut für Chemie, Postfach 3060, D-55128 Mainz, Germany
- NASA Ames/SETI Institute, Moffett Field, CA 94035, USA
- Department of Geological Sciences, University of Nevada, Reno, NV 89557, USA
| | - J. A. Grant
- Department of Astronomy, Cornell University, Ithaca, NY 14853, USA
- Department of Earth and Planetary Sciences, Washington University, St. Louis, MO 63130, USA
- Abteilung Kosmochemie, Max-Planck-Institut für Chemie, Postfach 3060, D-55128 Mainz, Germany
- NASA Ames/SETI Institute, Moffett Field, CA 94035, USA
- Department of Geological Sciences, University of Nevada, Reno, NV 89557, USA
| | - R. Greeley
- Department of Astronomy, Cornell University, Ithaca, NY 14853, USA
- Department of Earth and Planetary Sciences, Washington University, St. Louis, MO 63130, USA
- Abteilung Kosmochemie, Max-Planck-Institut für Chemie, Postfach 3060, D-55128 Mainz, Germany
- NASA Ames/SETI Institute, Moffett Field, CA 94035, USA
- Department of Geological Sciences, University of Nevada, Reno, NV 89557, USA
| | - J. Grotzinger
- Department of Astronomy, Cornell University, Ithaca, NY 14853, USA
- Department of Earth and Planetary Sciences, Washington University, St. Louis, MO 63130, USA
- Abteilung Kosmochemie, Max-Planck-Institut für Chemie, Postfach 3060, D-55128 Mainz, Germany
- NASA Ames/SETI Institute, Moffett Field, CA 94035, USA
- Department of Geological Sciences, University of Nevada, Reno, NV 89557, USA
| | - L. Haskin
- Department of Astronomy, Cornell University, Ithaca, NY 14853, USA
- Department of Earth and Planetary Sciences, Washington University, St. Louis, MO 63130, USA
- Abteilung Kosmochemie, Max-Planck-Institut für Chemie, Postfach 3060, D-55128 Mainz, Germany
- NASA Ames/SETI Institute, Moffett Field, CA 94035, USA
- Department of Geological Sciences, University of Nevada, Reno, NV 89557, USA
| | - K. E. Herkenhoff
- Department of Astronomy, Cornell University, Ithaca, NY 14853, USA
- Department of Earth and Planetary Sciences, Washington University, St. Louis, MO 63130, USA
- Abteilung Kosmochemie, Max-Planck-Institut für Chemie, Postfach 3060, D-55128 Mainz, Germany
- NASA Ames/SETI Institute, Moffett Field, CA 94035, USA
- Department of Geological Sciences, University of Nevada, Reno, NV 89557, USA
| | - S. Hviid
- Department of Astronomy, Cornell University, Ithaca, NY 14853, USA
- Department of Earth and Planetary Sciences, Washington University, St. Louis, MO 63130, USA
- Abteilung Kosmochemie, Max-Planck-Institut für Chemie, Postfach 3060, D-55128 Mainz, Germany
- NASA Ames/SETI Institute, Moffett Field, CA 94035, USA
- Department of Geological Sciences, University of Nevada, Reno, NV 89557, USA
| | - J. Johnson
- Department of Astronomy, Cornell University, Ithaca, NY 14853, USA
- Department of Earth and Planetary Sciences, Washington University, St. Louis, MO 63130, USA
- Abteilung Kosmochemie, Max-Planck-Institut für Chemie, Postfach 3060, D-55128 Mainz, Germany
- NASA Ames/SETI Institute, Moffett Field, CA 94035, USA
- Department of Geological Sciences, University of Nevada, Reno, NV 89557, USA
| | - G. Klingelhöfer
- Department of Astronomy, Cornell University, Ithaca, NY 14853, USA
- Department of Earth and Planetary Sciences, Washington University, St. Louis, MO 63130, USA
- Abteilung Kosmochemie, Max-Planck-Institut für Chemie, Postfach 3060, D-55128 Mainz, Germany
- NASA Ames/SETI Institute, Moffett Field, CA 94035, USA
- Department of Geological Sciences, University of Nevada, Reno, NV 89557, USA
| | - A. Knoll
- Department of Astronomy, Cornell University, Ithaca, NY 14853, USA
- Department of Earth and Planetary Sciences, Washington University, St. Louis, MO 63130, USA
- Abteilung Kosmochemie, Max-Planck-Institut für Chemie, Postfach 3060, D-55128 Mainz, Germany
- NASA Ames/SETI Institute, Moffett Field, CA 94035, USA
- Department of Geological Sciences, University of Nevada, Reno, NV 89557, USA
| | - G. Landis
- Department of Astronomy, Cornell University, Ithaca, NY 14853, USA
- Department of Earth and Planetary Sciences, Washington University, St. Louis, MO 63130, USA
- Abteilung Kosmochemie, Max-Planck-Institut für Chemie, Postfach 3060, D-55128 Mainz, Germany
- NASA Ames/SETI Institute, Moffett Field, CA 94035, USA
- Department of Geological Sciences, University of Nevada, Reno, NV 89557, USA
| | - M. Lemmon
- Department of Astronomy, Cornell University, Ithaca, NY 14853, USA
- Department of Earth and Planetary Sciences, Washington University, St. Louis, MO 63130, USA
- Abteilung Kosmochemie, Max-Planck-Institut für Chemie, Postfach 3060, D-55128 Mainz, Germany
- NASA Ames/SETI Institute, Moffett Field, CA 94035, USA
- Department of Geological Sciences, University of Nevada, Reno, NV 89557, USA
| | - R. Li
- Department of Astronomy, Cornell University, Ithaca, NY 14853, USA
- Department of Earth and Planetary Sciences, Washington University, St. Louis, MO 63130, USA
- Abteilung Kosmochemie, Max-Planck-Institut für Chemie, Postfach 3060, D-55128 Mainz, Germany
- NASA Ames/SETI Institute, Moffett Field, CA 94035, USA
- Department of Geological Sciences, University of Nevada, Reno, NV 89557, USA
| | - M. B. Madsen
- Department of Astronomy, Cornell University, Ithaca, NY 14853, USA
- Department of Earth and Planetary Sciences, Washington University, St. Louis, MO 63130, USA
- Abteilung Kosmochemie, Max-Planck-Institut für Chemie, Postfach 3060, D-55128 Mainz, Germany
- NASA Ames/SETI Institute, Moffett Field, CA 94035, USA
- Department of Geological Sciences, University of Nevada, Reno, NV 89557, USA
| | - M. C. Malin
- Department of Astronomy, Cornell University, Ithaca, NY 14853, USA
- Department of Earth and Planetary Sciences, Washington University, St. Louis, MO 63130, USA
- Abteilung Kosmochemie, Max-Planck-Institut für Chemie, Postfach 3060, D-55128 Mainz, Germany
- NASA Ames/SETI Institute, Moffett Field, CA 94035, USA
- Department of Geological Sciences, University of Nevada, Reno, NV 89557, USA
| | - S. M. McLennan
- Department of Astronomy, Cornell University, Ithaca, NY 14853, USA
- Department of Earth and Planetary Sciences, Washington University, St. Louis, MO 63130, USA
- Abteilung Kosmochemie, Max-Planck-Institut für Chemie, Postfach 3060, D-55128 Mainz, Germany
- NASA Ames/SETI Institute, Moffett Field, CA 94035, USA
- Department of Geological Sciences, University of Nevada, Reno, NV 89557, USA
| | - H. Y. McSween
- Department of Astronomy, Cornell University, Ithaca, NY 14853, USA
- Department of Earth and Planetary Sciences, Washington University, St. Louis, MO 63130, USA
- Abteilung Kosmochemie, Max-Planck-Institut für Chemie, Postfach 3060, D-55128 Mainz, Germany
- NASA Ames/SETI Institute, Moffett Field, CA 94035, USA
- Department of Geological Sciences, University of Nevada, Reno, NV 89557, USA
| | - D. W. Ming
- Department of Astronomy, Cornell University, Ithaca, NY 14853, USA
- Department of Earth and Planetary Sciences, Washington University, St. Louis, MO 63130, USA
- Abteilung Kosmochemie, Max-Planck-Institut für Chemie, Postfach 3060, D-55128 Mainz, Germany
- NASA Ames/SETI Institute, Moffett Field, CA 94035, USA
- Department of Geological Sciences, University of Nevada, Reno, NV 89557, USA
| | - J. Moersch
- Department of Astronomy, Cornell University, Ithaca, NY 14853, USA
- Department of Earth and Planetary Sciences, Washington University, St. Louis, MO 63130, USA
- Abteilung Kosmochemie, Max-Planck-Institut für Chemie, Postfach 3060, D-55128 Mainz, Germany
- NASA Ames/SETI Institute, Moffett Field, CA 94035, USA
- Department of Geological Sciences, University of Nevada, Reno, NV 89557, USA
| | - R. V. Morris
- Department of Astronomy, Cornell University, Ithaca, NY 14853, USA
- Department of Earth and Planetary Sciences, Washington University, St. Louis, MO 63130, USA
- Abteilung Kosmochemie, Max-Planck-Institut für Chemie, Postfach 3060, D-55128 Mainz, Germany
- NASA Ames/SETI Institute, Moffett Field, CA 94035, USA
- Department of Geological Sciences, University of Nevada, Reno, NV 89557, USA
| | - T. Parker
- Department of Astronomy, Cornell University, Ithaca, NY 14853, USA
- Department of Earth and Planetary Sciences, Washington University, St. Louis, MO 63130, USA
- Abteilung Kosmochemie, Max-Planck-Institut für Chemie, Postfach 3060, D-55128 Mainz, Germany
- NASA Ames/SETI Institute, Moffett Field, CA 94035, USA
- Department of Geological Sciences, University of Nevada, Reno, NV 89557, USA
| | - J. W. Rice
- Department of Astronomy, Cornell University, Ithaca, NY 14853, USA
- Department of Earth and Planetary Sciences, Washington University, St. Louis, MO 63130, USA
- Abteilung Kosmochemie, Max-Planck-Institut für Chemie, Postfach 3060, D-55128 Mainz, Germany
- NASA Ames/SETI Institute, Moffett Field, CA 94035, USA
- Department of Geological Sciences, University of Nevada, Reno, NV 89557, USA
| | - L. Richter
- Department of Astronomy, Cornell University, Ithaca, NY 14853, USA
- Department of Earth and Planetary Sciences, Washington University, St. Louis, MO 63130, USA
- Abteilung Kosmochemie, Max-Planck-Institut für Chemie, Postfach 3060, D-55128 Mainz, Germany
- NASA Ames/SETI Institute, Moffett Field, CA 94035, USA
- Department of Geological Sciences, University of Nevada, Reno, NV 89557, USA
| | - R. Rieder
- Department of Astronomy, Cornell University, Ithaca, NY 14853, USA
- Department of Earth and Planetary Sciences, Washington University, St. Louis, MO 63130, USA
- Abteilung Kosmochemie, Max-Planck-Institut für Chemie, Postfach 3060, D-55128 Mainz, Germany
- NASA Ames/SETI Institute, Moffett Field, CA 94035, USA
- Department of Geological Sciences, University of Nevada, Reno, NV 89557, USA
| | - M. Sims
- Department of Astronomy, Cornell University, Ithaca, NY 14853, USA
- Department of Earth and Planetary Sciences, Washington University, St. Louis, MO 63130, USA
- Abteilung Kosmochemie, Max-Planck-Institut für Chemie, Postfach 3060, D-55128 Mainz, Germany
- NASA Ames/SETI Institute, Moffett Field, CA 94035, USA
- Department of Geological Sciences, University of Nevada, Reno, NV 89557, USA
| | - M. Smith
- Department of Astronomy, Cornell University, Ithaca, NY 14853, USA
- Department of Earth and Planetary Sciences, Washington University, St. Louis, MO 63130, USA
- Abteilung Kosmochemie, Max-Planck-Institut für Chemie, Postfach 3060, D-55128 Mainz, Germany
- NASA Ames/SETI Institute, Moffett Field, CA 94035, USA
- Department of Geological Sciences, University of Nevada, Reno, NV 89557, USA
| | - P. Smith
- Department of Astronomy, Cornell University, Ithaca, NY 14853, USA
- Department of Earth and Planetary Sciences, Washington University, St. Louis, MO 63130, USA
- Abteilung Kosmochemie, Max-Planck-Institut für Chemie, Postfach 3060, D-55128 Mainz, Germany
- NASA Ames/SETI Institute, Moffett Field, CA 94035, USA
- Department of Geological Sciences, University of Nevada, Reno, NV 89557, USA
| | - L. A. Soderblom
- Department of Astronomy, Cornell University, Ithaca, NY 14853, USA
- Department of Earth and Planetary Sciences, Washington University, St. Louis, MO 63130, USA
- Abteilung Kosmochemie, Max-Planck-Institut für Chemie, Postfach 3060, D-55128 Mainz, Germany
- NASA Ames/SETI Institute, Moffett Field, CA 94035, USA
- Department of Geological Sciences, University of Nevada, Reno, NV 89557, USA
| | - R. Sullivan
- Department of Astronomy, Cornell University, Ithaca, NY 14853, USA
- Department of Earth and Planetary Sciences, Washington University, St. Louis, MO 63130, USA
- Abteilung Kosmochemie, Max-Planck-Institut für Chemie, Postfach 3060, D-55128 Mainz, Germany
- NASA Ames/SETI Institute, Moffett Field, CA 94035, USA
- Department of Geological Sciences, University of Nevada, Reno, NV 89557, USA
| | - H. Wänke
- Department of Astronomy, Cornell University, Ithaca, NY 14853, USA
- Department of Earth and Planetary Sciences, Washington University, St. Louis, MO 63130, USA
- Abteilung Kosmochemie, Max-Planck-Institut für Chemie, Postfach 3060, D-55128 Mainz, Germany
- NASA Ames/SETI Institute, Moffett Field, CA 94035, USA
- Department of Geological Sciences, University of Nevada, Reno, NV 89557, USA
| | - T. Wdowiak
- Department of Astronomy, Cornell University, Ithaca, NY 14853, USA
- Department of Earth and Planetary Sciences, Washington University, St. Louis, MO 63130, USA
- Abteilung Kosmochemie, Max-Planck-Institut für Chemie, Postfach 3060, D-55128 Mainz, Germany
- NASA Ames/SETI Institute, Moffett Field, CA 94035, USA
- Department of Geological Sciences, University of Nevada, Reno, NV 89557, USA
| | - M. Wolff
- Department of Astronomy, Cornell University, Ithaca, NY 14853, USA
- Department of Earth and Planetary Sciences, Washington University, St. Louis, MO 63130, USA
- Abteilung Kosmochemie, Max-Planck-Institut für Chemie, Postfach 3060, D-55128 Mainz, Germany
- NASA Ames/SETI Institute, Moffett Field, CA 94035, USA
- Department of Geological Sciences, University of Nevada, Reno, NV 89557, USA
| | - A. Yen
- Department of Astronomy, Cornell University, Ithaca, NY 14853, USA
- Department of Earth and Planetary Sciences, Washington University, St. Louis, MO 63130, USA
- Abteilung Kosmochemie, Max-Planck-Institut für Chemie, Postfach 3060, D-55128 Mainz, Germany
- NASA Ames/SETI Institute, Moffett Field, CA 94035, USA
- Department of Geological Sciences, University of Nevada, Reno, NV 89557, USA
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McAuley WJ, Pecchioni L, Grant JA. Personal accounts of the role of God in health and illness among older rural African American and White residents. J Cross Cult Gerontol 2004; 15:13-35. [PMID: 14618008 DOI: 10.1023/a:1006745709687] [Citation(s) in RCA: 38] [Impact Index Per Article: 1.9] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/12/2022]
Abstract
This paper addresses how older rural residents view the relationship between God and both health and illness. We employed semi-structured interviews and qualitative analytical strategies with 15 African Americans residing in predominantly African American communities and 13 Whites living in nearby predominantly White communities, in order to identify similarities and differences in views about a divine other's roles in health and illness. African Americans were more likely than Whites to describe their religious lives in personal terms, in ways suggesting there is a set of religious truths that do not require further investigation or analysis, and in a manner indicating that religious belief permeated their lives. They were also more likely to describe specific role expectations for God in health and illness. The results point to the substantial cultural diversity that exists in small rural areas, and to the need for health care workers to be sensitive to the health-related religious beliefs of patients.
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Affiliation(s)
- W J McAuley
- College of Nursing and Health Professions, University of North Carolina, Charlotte, NC 28223-0001, USA.
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Golombek MP, Grant JA, Parker TJ, Kass DM, Crisp JA, Squyres SW, Haldemann AFC, Adler M, Lee WJ, Bridges NT, Arvidson RE, Carr MH, Kirk RL, Knocke PC, Roncoli RB, Weitz CM, Schofield JT, Zurek RW, Christensen PR, Fergason RL, Anderson FS, Rice JW. Selection of the Mars Exploration Rover landing sites. ACTA ACUST UNITED AC 2003. [DOI: 10.1029/2003je002074] [Citation(s) in RCA: 126] [Impact Index Per Article: 6.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/09/2022]
Affiliation(s)
- M. P. Golombek
- Jet Propulsion Laboratory; California Institute of Technology; Pasadena California USA
| | - J. A. Grant
- Center for Earth and Planetary Studies; National Air and Space Museum, Smithsonian Institution; Washington DC USA
| | - T. J. Parker
- Jet Propulsion Laboratory; California Institute of Technology; Pasadena California USA
| | - D. M. Kass
- Jet Propulsion Laboratory; California Institute of Technology; Pasadena California USA
| | - J. A. Crisp
- Jet Propulsion Laboratory; California Institute of Technology; Pasadena California USA
| | - S. W. Squyres
- Department of Astronomy; Cornell University; Ithaca New York USA
| | - A. F. C. Haldemann
- Jet Propulsion Laboratory; California Institute of Technology; Pasadena California USA
| | - M. Adler
- Jet Propulsion Laboratory; California Institute of Technology; Pasadena California USA
| | - W. J. Lee
- Jet Propulsion Laboratory; California Institute of Technology; Pasadena California USA
| | - N. T. Bridges
- Jet Propulsion Laboratory; California Institute of Technology; Pasadena California USA
| | - R. E. Arvidson
- Department of Earth and Space Sciences; Washington University; St. Louis Missouri USA
| | - M. H. Carr
- U.S. Geological Survey; Menlo Park California USA
| | - R. L. Kirk
- U.S. Geological Survey; Flagstaff Arizona USA
| | - P. C. Knocke
- Jet Propulsion Laboratory; California Institute of Technology; Pasadena California USA
| | - R. B. Roncoli
- Jet Propulsion Laboratory; California Institute of Technology; Pasadena California USA
| | | | - J. T. Schofield
- Jet Propulsion Laboratory; California Institute of Technology; Pasadena California USA
| | - R. W. Zurek
- Jet Propulsion Laboratory; California Institute of Technology; Pasadena California USA
| | - P. R. Christensen
- Department of Geological Sciences; Arizona State University; Tempe Arizona USA
| | - R. L. Fergason
- Department of Geological Sciences; Arizona State University; Tempe Arizona USA
| | - F. S. Anderson
- Jet Propulsion Laboratory; California Institute of Technology; Pasadena California USA
| | - J. W. Rice
- Department of Geological Sciences; Arizona State University; Tempe Arizona USA
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Kirby BJ, Davis JR, Grant JA, Morgan MJ. Extracting material parameters from x-ray attenuation: a CT feasibility study using kilovoltage synchrotron x-rays incident upon low atomic number absorbers. Phys Med Biol 2003; 48:3389-409. [PMID: 14620065 DOI: 10.1088/0031-9155/48/20/009] [Citation(s) in RCA: 19] [Impact Index Per Article: 0.9] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/12/2022]
Abstract
The work reported here is a feasibility study of the extraction of material parameters from measurements of the linear x-ray attenuation coefficient of low atomic number absorbers. Computed tomography (CT) scans of small samples containing several liquids and solids were carried out with synchrotron radiation at the Australian National Beamline Facility (BL 20B) in Japan. Average values of the x-ray linear attenuation coefficient were extracted for each material for x-ray energies ranging from 11 keV to 20.5 keV. The electron density was estimated by applying results derived from a parametrization of the x-ray linear attenuation coefficient first developed by Jackson and Hawkes and extended for this work. Average estimates for the electron density of triethanolamine and acetic acid were made to within +5.3% of the actual value. Other materials examined included furfuraldehyde, perspex and teflon, for which average estimates of the electron density were less than 10% in excess of the calculated value.
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Affiliation(s)
- B J Kirby
- School of Physics and Materials Engineering, Monash University, Victoria 3800, Australia.
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Vorobjev YN, Grant JA, Scheraga HA. A combined iterative and boundary-element approach for solution of the nonlinear Poisson-Boltzmann equation. J Am Chem Soc 2002. [DOI: 10.1021/ja00035a003] [Citation(s) in RCA: 65] [Impact Index Per Article: 3.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/30/2022]
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Rather JB, Grant JA, Gunther VH, Headington CE, Karchmer JH, Kurtz SS, Rescorla AR, Roberts FM, Stephenson AJ, Troeller WJ, Tucker EB. Determination of Oil in Refinery Effluent Waters. Anal Chem 2002. [DOI: 10.1021/ac60133a008] [Citation(s) in RCA: 4] [Impact Index Per Article: 0.2] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/28/2022]
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Abstract
BACKGROUND Acetaminophen hypersensitivity is rare and, when seen, is usually in association with sensitivity to nonsteroidal anti-inflammatory drugs. METHODS This is a case report of an immediate reaction to acetaminophen, confirmed by a drug challenge, in a subject who tolerated ibuprofen. RESULTS After an oral challenge with 50 mg of acetaminophen, the subject had generalized pruritus, urticaria, and dyspnea. CONCLUSIONS This patient demonstrates a rare but potentially severe reaction to acetaminophen that may occur in patients who are not otherwise sensitive to other nonsteroidal anti-inflammatory drugs.
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Affiliation(s)
- J A Grant
- University of Iowa, Iowa City 52242, USA
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Abstract
BACKGROUND Open spina bifida is the most complex congenital abnormality compatible with long-term survival. This report outlines the 20- to 25-year outcome for our original cohort of patients with a myelomeningocele treated in a nonselective, prospective manner. METHODS Of the initial 118 children, 71 patients were available for our most recent review. Nineteen patients have been lost to follow-up and 28 patients have died. Data were collected on: motor level, shunt status, education/employment, seizure history, mobility, bladder/bowel continence, tethered cord, scoliosis, latex allergy, posterior cervical decompression, tracheostomy and/or gastrostomy tube. RESULTS Mortality (24%) continues to climb into young adulthood. Eighty-six percent of the cohort have cerebrospinal fluid diversion, with 95% having undergone at least one shunt revision. Thirty-two percent have undergone a tethered cord release, with 97% having an improvement or stabilization in their preoperative symptoms. Forty-nine percent have scoliosis, with 43% eventually requiring a spinal fusion. Sixteen patients (23%) have had at least one seizure. Eighty-five percent are attending or have graduated from high school and/or college. More than 80% of young adults have social bladder continence. Approximately 1/3 of patients are allergic to latex, with 6 patients having experienced a life-threatening reaction. CONCLUSION At least 75% of children born with a myelomeningocele can be expected to reach their early adult years. Late deterioration is common. One of the greatest challenges in medicine today is establishing a network of care for these adults with spina bifida.
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Affiliation(s)
- R M Bowman
- Division of Pediatric Neurosurgery, Children's Memorial Hospital, Northwestern University Medical School, Chicago, IL 60614, USA.
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Affiliation(s)
- J A Grant
- Children's Memorial Hospital, Chicago, IL, USA
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Abstract
Histamine was the first allergic mediator identified in the early part of this century. It has three defined receptors, but most effects of histamine in allergic reactions are through the H1 receptor. The first H1 antagonists were introduced into clinical use in the late 1940s, and drugs of this class are still the preferred initial choice for management of allergic rhinitis and urticaria. The first-generation drugs were characterized by nonspecific binding to many receptors and penetration of the blood-brain barrier, resulting in multiple side effects. Within the central nervous system (CNS), interference with normal histamine binding to the H1 receptor is associated with drowsiness and psychomotor impairment. The second-generation drugs have a much improved benefit/adverse effect profile, largely based on greater potency, receptor specificity, and lower CNS penetration. The potency of antihistamines for blocking H1 receptors can be compared by their inhibition of the cutaneous wheal and flare response to histamine. These drugs seem to have additional antiallergic properties related to blockade of mediator release and interference with cellular recruitment and activation. Clinical trials comparing the efficacy of antihistamines in rhinitis and asthma are reviewed. Recent studies have explored the potential of antihistamines to prevent the progression of allergy and their enhanced efficacy when combined with leukotriene antagonists.
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Affiliation(s)
- J A Grant
- Department of Internal Medicine, University of Texas Medical Branch at Galveston 77555-1083, USA
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Kampen GT, Stafford S, Adachi T, Jinquan T, Quan S, Grant JA, Skov PS, Poulsen LK, Alam R. Eotaxin induces degranulation and chemotaxis of eosinophils through the activation of ERK2 and p38 mitogen-activated protein kinases. Blood 2000; 95:1911-7. [PMID: 10706854] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Grants] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 02/15/2023] Open
Abstract
Eotaxin and other CC chemokines acting via CC chemokine receptor-3 (CCR3) are believed to play an integral role in the development of eosinophilic inflammation in asthma and allergic inflammatory diseases. However, little is known about the intracellular events following agonist binding to CCR3 and the relationship of these events to the functional response of the cell. The objectives of this study were to investigate CCR3-mediated activation of the mitogen-activated protein (MAP) kinases extracellular signal-regulated kinase-2 (ERK2), p38, and c-jun N-terminal kinase (JNK) in eosinophils and to assess the requirement for MAP kinases in eotaxin-induced eosinophil cationic protein (ECP) release and chemotaxis. MAP kinase activation was studied in eotaxin-stimulated eosinophils (more than 97% purity) by Western blotting and immune-complex kinase assays. ECP release was measured by radioimmunoassay. Chemotaxis was assessed using Boyden microchambers. Eotaxin (10(-11) to 10(-7) mol/L) induced concentration-dependent phosphorylation of ERK2 and p38. Phosphorylation was detectable after 30 seconds, peaked at about 1 minute, and returned to baseline after 2 to 5 minutes. Phosphorylation of JNK above baseline could not be detected. The kinase activity of ERK2 and p38 paralleled phosphorylation. PD980 59, an inhibitor of the ERK2-activating enzyme MEK (MAP ERK kinase), blocked phosphorylation of ERK2 in a concentration-dependent manner. The functional relevance of ERK2 and p38 was studied using PD98 059 and the p38 inhibitor SB202 190. PD98 059 and SB202 190 both caused inhibition of eotaxin-induced ECP release and chemotaxis. We conclude that eotaxin induces a rapid concentration-dependent activation of ERK2 and p38 in eosinophils and that the activation of these MAP kinases is required for eotaxin-stimulated degranulation and directed locomotion. (Blood. 2000;95:1911-1917)
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Affiliation(s)
- G T Kampen
- University of Texas Medical Branch, Department of Internal Medicine, Division of Allergy and Immunology, Galveston, TX 77555-0762, USA
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Abstract
OBJECTIVE The goals of this article include the reporting of the epidemiology, economic and medical impact of allergic rhinitis. In addition, the pharmacology and clinical profile of the therapeutic agent cetirizine are reviewed. DATA SOURCES A detailed literature search was conducted. References are limited to the English language and human subjects and tissues. Studies considered relevant and important over the past 20 years are highlighted. STUDY SELECTION Prevalence and morbidity data were chosen from more recent assessments. Because cetirizine is a relatively new compound, studies from the past several years from peer-reviewed journals have been emphasized. RESULTS Allergic rhinitis affects between 15% and 25% of the US general population. It shares common pathophysiologic mechanisms with conjunctivitis and asthma and predisposes to nasal infections, otitis media, sinusitis, nasal polyposis, and orthodontic malocclusions. Direct medical care costs amount to up to 3 billion dollars every year. In addition, the quality of life of affected individuals is substantially compromised. Cetirizine is a potent H1-receptor antagonist and has anti-inflammatory properties. It does not interact with concomitantly administered medications, has no cardiac adverse effects, and does not appear to be associated with teratogenicity. Impairment of CNS function is comparable to other low-sedating antihistamines at the recommended dose of 10 mg daily for adults. Its clinical efficacy for allergic respiratory diseases has been established in numerous trials. CONCLUSIONS Allergic rhinitis causes considerable suffering. Cetirizine, with a fine risk-benefit ratio, can be a most valuable therapeutic option.
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Affiliation(s)
- E O Meltzer
- Allergy & Asthma Medical Group & Research Center, San Diego, California 92123, USA
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Grant JA, Danielson L, Rihoux JP, DeVos C. A double-blind, single-dose, crossover comparison of cetirizine, ebastine, epinastine, fexofenadine, terfenadine, and loratadine versus placebo: suppression of histamine-induced wheal and flare response for 24 h in healthy male subjects. Allergy 1999; 54:700-7. [PMID: 10442525 DOI: 10.1034/j.1398-9995.1999.00032.x] [Citation(s) in RCA: 87] [Impact Index Per Article: 3.5] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/23/2022]
Abstract
BACKGROUND New H1-antagonists have become available, but there has been no comparison of their potency for inhibiting histamine in the skin. METHODS Cetirizine 10 mg, ebastine 10 mg, epinastine 20 mg, fexofenadine 60 mg, terfenadine 60 mg, loratadine 10 mg, or placebo was given to 14 healthy male volunteers in a double-blind, crossover randomized manner. Inhibition of the wheal and flare response to epicutaneous histamine phosphate (100 mg/ml) challenge was measured at 0, 0.5, 1, 2, 4, 6, 8, 10, 12, and 24 h after doses. RESULTS Epinastine inhibited the wheal and flare after 30 min. Cetirizine commenced acting at 1 h and was superior to other treatments. Ebastine was no better than placebo until 4 h, but was efficacious thereafter until 24 h. Terfenadine induced potent inhibition after 1 h and was superior to its metabolite fexofenadine. Loratadine was the least potent inhibitor. Inhibition of the flare response paralleled the patterns seen for wheals. The rank order for area under the curve (0-24 h) was cetirizine, epinastine, terfenadine, ebastine, fexofenadine, loratadine, and placebo. CONCLUSIONS The inhibition of histamine effects in the skin may be useful in predicting the clinical utility of newly introduced antihistamines in treating allergic disorders.
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Affiliation(s)
- J A Grant
- University of Texas Medical Branch, Galveston 77555-0762, USA
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Abstract
OBJECTIVE To examine recent admissions of older adults to intermediate care facilities in order to identify the factors associated with whether the individual originated in another county, a non-adjacent county, and another state. METHODS Employing a conceptual framework based upon migration theory and the long-term care decision process and a data set derived from multiple sources, logistic regression was used to examine whether characteristics of the county of residence prior to admission, the admission facility, and the individual are significant net predictors of the three types of mobility. Separate analyses were conducted for married and unmarried individuals. RESULTS The analytical models tended to have relatively good fit but only moderate predictive accuracy. In general, persons on Medicaid payment status were more likely to move to another county and to a non-adjacent county, whereas Medicaid payment was associated with a lower likelihood of migrating to Virginia from another state. Individuals originating in counties with higher bed rates had lower rates of migration to another county and non-adjacent county, whereas those from counties with higher occupancy rates were more likely to leave their county of origin. CONCLUSION Examination of factors associated with the distance and patterns of nursing home mobility improves our understanding of the nursing home selection process and helps to illuminate the impact of public policy, market forces, and nursing home staff on who goes where to be admitted to a nursing home.
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Affiliation(s)
- W J McAuley
- Oklahoma Center on Aging, University of Oklahoma Health Sciences Center, Oklahoma City, USA.
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Affiliation(s)
- M Rais
- Department of Internal Medicine, Allergy and Immunology Division, The University of Texas Medical Branch, Galveston, TX 77555-0762, USA
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Grant JA, Danielson L, Rihoux J, DeVos C. A comparison of Cetirizine, Ebastine, Epinastine, Fexofenadine, Terfenadine, and Loratadine versus placebo in suppressing the cutaneous response to histamine. Int Arch Allergy Immunol 1999; 118:339-40. [PMID: 10224437 DOI: 10.1159/000024126] [Citation(s) in RCA: 11] [Impact Index Per Article: 0.4] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/19/2022] Open
Affiliation(s)
- J A Grant
- University of Texas Medical Branch, Galveston, TX, USA.
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Abstract
Bronchial asthma is a chronic disease with variable airway narrowing, respiratory distress, hyper-responsiveness and inflammation. The morbidity and mortality are increasing despite availability of newer diagnostic and therapeutic strategies. The National Institutes of Health recently issued revised guidelines for disease management. The keys to improved care include earlier recognition of the illness, reduced exposure to triggers, careful monitoring, greater use of long-term control medications and improved patient education.
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Affiliation(s)
- J A Grant
- Allergy and Immunology Division, Department of Medicine, University of Texas Medical Branch-Galveston, 77555-0762, USA.
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Kon OM, Sihra BS, Till SJ, Corrigan CJ, Kay AB, Grant JA. Unstimulated basophils in atopic and nonatopic subjects express intracellular interleukin-4: detection by flow cytometry. Allergy 1998; 53:891-6. [PMID: 9788692 DOI: 10.1111/j.1398-9995.1998.tb03997.x] [Citation(s) in RCA: 13] [Impact Index Per Article: 0.5] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/30/2022]
Abstract
BACKGROUND IgE-stimulated cultured basophils from atopic subjects are capable of secreting interleukin-4 (IL-4). We describe a flow-cytometric technique which identified intracellular IL-4 in unstimulated basophils unseparated from peripheral blood mononuclear cells (PBMC) in both atopic (AT) and nonatopic (NC) volunteers. METHODS Freshly isolated PBMC were fixed in 4% paraformaldehyde (PFA). Surface staining with 22E7, a noncompetitive anti-FcepsilonRI-alpha antibody, allowed identification of basophils. Permeabilization by 0.1% saponin allowed staining of intracellular cytokines with specific monoclonal antibodies (mAbs). Two series of experiments utilizing different protocols and anticytokine mAbs were performed. The first protocol required a two-stage fluorochrome staining technique. The availability of fluorochrome-conjugated mAbs allowed a simpler, one-stage labelling procedure for the second protocol. RESULTS With the first protocol, IL-4 (but not IFN-gamma), immunoreactivity was detectable in a majority (median 77%) of peripheral blood basophils from both AT and NC subjects (n=8). Basophil IL-4 immunoreactivity was again evident in experiment 2 but did not differ significantly between AT and NC subjects--either evaluated as percentage of IL-4+ basophils (AT median=66%, NC median=38.4%, P=0.41) or IL-4-specific mean fluorescence (AT median=0.85, NC median=0.3, P=0.07). CONCLUSIONS This simple technique allowed the study of intracellular cytokine expression in unstimulated blood basophils. It demonstrated constitutive basophil expression of IL-4 (but not IFN-gamma) in all subjects, with no significant increases in atopics.
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Affiliation(s)
- O M Kon
- Imperial College School of Medicine at the National Heart and Lung Institute, London, UK
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Rajakulasingam K, Till S, Ying S, Humbert M, Barkans J, Sullivan M, Meng Q, Corrigan CJ, Bungre J, Grant JA, Kay AB, Durham SR. Increased expression of high affinity IgE (FcepsilonRI) receptor-alpha chain mRNA and protein-bearing eosinophils in human allergen-induced atopic asthma. Am J Respir Crit Care Med 1998; 158:233-40. [PMID: 9655735 DOI: 10.1164/ajrccm.158.1.9708106] [Citation(s) in RCA: 53] [Impact Index Per Article: 2.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/16/2022] Open
Abstract
FcepsilonRI receptors play an important role in allergen-induced mediator release and antigen presentation by mast cells, basophils, and monocyte/macrophages in atopic disorders. The expression of FcepsilonRI by tissue eosinophils in atopic asthma after allergen challenge has not been established. For this reason we attempted to identify mRNA and protein product + FcepsilonRIalpha eosinophils in cytospins made from bronchoalveolar lavage (BAL) from atopic asthmatics (n = 9) and nonatopic normal subjects (n = 4) 24 h after segmental challenge with allergen or diluent. Messenger RNA for FcepsilonRIalpha was determined using in situ hybridization and FcepsilonRIalpha protein expression by immunocytochemistry using a mouse monoclonal antibody 22E7. Colocalization of FcepsilonRIalpha receptors to eosinophils was performed using chromotrope 2R. When compared with a control challenge, segmental challenge with Dermatophagoides pteronyssinus induced significant BAL eosinophilia (p = 0.007). The total number of BAL FcepsilonRIalpha mRNA and protein-positive cells also increased in asthmatics, median values 2 (0.7-7.2) and 11.5 (0.6-65.0) x 10(6) cells (p = 0.02) and 0 (0-0.3 x 10(6)) and 3.1 x 10(6) (0.45 - 162.5 x 10(6)) cells (p = 0.007), respectively, for mRNA and protein. Net increases in FcepsilonRIalpha+ cells correlated with the net increases in BAL eosinophils (r = 0.98, p = 0.0001 for mRNA and r = 0.72, p = 0.02 for protein). Colocalization studies with chromotrope 2R revealed that only 4% of FcepsilonRIalpha+ cells were eosinophils after control challenge and, in contrast, 85 to 95% of FcepsilonRIalpha+ cells were eosinophils after allergen. There were no differences in the numbers of FcepsilonRIalpha+ cells or eosinophils in normal control subjects. Our results demonstrated that local endobronchial allergen provocation in atopic asthmatics results in increased synthesis and expression of FcepsilonRIalpha predominantly on BAL eosinophils.
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Affiliation(s)
- K Rajakulasingam
- Upper Respiratory Medicine and Allergy and Clinical Immunology, Imperial College School of Medicine at the National Heart and Lung Institute, Dovehouse Street, London, United Kingdom
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Grant JA, Sarwark JF. Image of the month. 13-year-old girl with very mild and infrequent back pain. Pediatr Neurosurg 1998; 28:96. [PMID: 9712270 DOI: 10.1159/000028629] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [MESH Headings] [Track Full Text] [Journal Information] [Submit a Manuscript] [Subscribe] [Scholar Register] [Indexed: 11/19/2022]
Affiliation(s)
- J A Grant
- Children's Memorial Hospital, Chicago, IL 60614, USA
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