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Farley KA, Stack KM, Shuster DL, Horgan BHN, Hurowitz JA, Tarnas JD, Simon JI, Sun VZ, Scheller EL, Moore KR, McLennan SM, Vasconcelos PM, Wiens RC, Treiman AH, Mayhew LE, Beyssac O, Kizovski TV, Tosca NJ, Williford KH, Crumpler LS, Beegle LW, Bell JF, Ehlmann BL, Liu Y, Maki JN, Schmidt ME, Allwood AC, Amundsen HEF, Bhartia R, Bosak T, Brown AJ, Clark BC, Cousin A, Forni O, Gabriel TSJ, Goreva Y, Gupta S, Hamran SE, Herd CDK, Hickman-Lewis K, Johnson JR, Kah LC, Kelemen PB, Kinch KB, Mandon L, Mangold N, Quantin-Nataf C, Rice MS, Russell PS, Sharma S, Siljeström S, Steele A, Sullivan R, Wadhwa M, Weiss BP, Williams AJ, Wogsland BV, Willis PA, Acosta-Maeda TA, Beck P, Benzerara K, Bernard S, Burton AS, Cardarelli EL, Chide B, Clavé E, Cloutis EA, Cohen BA, Czaja AD, Debaille V, Dehouck E, Fairén AG, Flannery DT, Fleron SZ, Fouchet T, Frydenvang J, Garczynski BJ, Gibbons EF, Hausrath EM, Hayes AG, Henneke J, Jørgensen JL, Kelly EM, Lasue J, Le Mouélic S, Madariaga JM, Maurice S, Merusi M, Meslin PY, Milkovich SM, Million CC, Moeller RC, Núñez JI, Ollila AM, Paar G, Paige DA, Pedersen DAK, Pilleri P, Pilorget C, Pinet PC, Rice JW, Royer C, Sautter V, Schulte M, Sephton MA, Sharma SK, Sholes SF, Spanovich N, St Clair M, Tate CD, Uckert K, VanBommel SJ, Yanchilina AG, Zorzano MP. Aqueously altered igneous rocks sampled on the floor of Jezero crater, Mars. Science 2022; 377:eabo2196. [PMID: 36007009 DOI: 10.1126/science.abo2196] [Citation(s) in RCA: 11] [Impact Index Per Article: 5.5] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 01/08/2023]
Abstract
The Perseverance rover landed in Jezero crater, Mars, to investigate ancient lake and river deposits. We report observations of the crater floor, below the crater's sedimentary delta, finding the floor consists of igneous rocks altered by water. The lowest exposed unit, informally named Séítah, is a coarsely crystalline olivine-rich rock, which accumulated at the base of a magma body. Fe-Mg carbonates along grain boundaries indicate reactions with CO2-rich water, under water-poor conditions. Overlying Séítah is a unit informally named Máaz, which we interpret as lava flows or the chemical complement to Séítah in a layered igneous body. Voids in these rocks contain sulfates and perchlorates, likely introduced by later near-surface brine evaporation. Core samples of these rocks were stored aboard Perseverance for potential return to Earth.
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Affiliation(s)
- K A Farley
- Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA 91125, USA
| | - K M Stack
- Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA
| | - D L Shuster
- Department of Earth and Planetary Science, University of California, Berkeley, Berkeley, CA 94720, USA
| | - B H N Horgan
- Department of Earth, Atmospheric, and Planetary Sciences, Purdue University, West Lafayette, IN 47907, USA
| | - J A Hurowitz
- Department of Geosciences, Stony Brook University, Stony Brook, NY 11794, USA
| | - J D Tarnas
- Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA
| | - J I Simon
- Center for Isotope Cosmochemistry and Geochronology, Astromaterials Research and Exploration Science Division, NASA Johnson Space Center, Houston, TX 77058, USA
| | - V Z Sun
- Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA
| | - E L Scheller
- Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA 91125, USA
| | - K R Moore
- 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, USA
| | - P M Vasconcelos
- School of Earth and Environmental Sciences, University of Queensland, Brisbane, QLD 4072, Australia
| | - R C Wiens
- Planetary Exploration Team, Los Alamos National Laboratory, Los Alamos, NM 87545, USA
| | - A H Treiman
- Lunar and Planetary Institute, Universities Space Research Association, Houston, TX 77058, USA
| | - L E Mayhew
- Department of Geological Sciences, University of Colorado, Boulder, Boulder, CO 80309, USA
| | - O Beyssac
- Institut de Minéralogie, de Physique des Matériaux et de Cosmochimie, Centre National de la Recherche Scientifique, Sorbonne Université, Muséum National d'Histoire Naturelle, 75005 Paris, France
| | - T V Kizovski
- Department of Earth Sciences, Brock University, St. Catharines, ON L2S 3A1, Canada
| | - N J Tosca
- Department of Earth Sciences, University of Cambridge, Cambridge CB2 3EQ, UK
| | - K H Williford
- Blue Marble Space Institute of Science, Seattle, WA 98104, USA
| | - L S Crumpler
- New Mexico Museum of Natural History and Science, Albuquerque, NM 8710, USA
| | - L W Beegle
- Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA
| | - J F Bell
- School of Earth and Space Exploration, Arizona State University, Tempe, AZ 85287, USA
| | - B L Ehlmann
- Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA 91125, USA
| | - Y Liu
- Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA
| | - J N Maki
- Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA
| | - M E Schmidt
- Department of Earth Sciences, Brock University, St. Catharines, ON L2S 3A1, Canada
| | - A C Allwood
- Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA
| | - H E F Amundsen
- Center for Space Sensors and Systems, University of Oslo, 2007 Kjeller, Norway
| | - R Bhartia
- Photon Systems Inc., Covina, CA 91725, USA
| | - T Bosak
- Department of Earth, Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, MA 02139, USA
| | - A J Brown
- Plancius Research, Severna Park, MD 21146, USA
| | - B C Clark
- Space Science Institute, Boulder, CO 80301, USA
| | - A Cousin
- Institut de Recherche en Astrophysique et Planétologie, Université de Toulouse 3 Paul Sabatier, Centre National de la Recherche Scientifique, Centre National d'Etude Spatiale, 31400 Toulouse, France
| | - O Forni
- Institut de Recherche en Astrophysique et Planétologie, Université de Toulouse 3 Paul Sabatier, Centre National de la Recherche Scientifique, Centre National d'Etude Spatiale, 31400 Toulouse, France
| | - T S J Gabriel
- Astrogeology Science Center, US Geological Survey, Flagstaff, AZ 86001, USA
| | - Y Goreva
- Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA
| | - S Gupta
- Department of Earth Sciences and Engineering, Imperial College London, London SW7 2AZ, UK
| | - S-E Hamran
- Center for Space Sensors and Systems, University of Oslo, 2007 Kjeller, Norway
| | - C D K Herd
- Department of Earth and Atmospheric Sciences, University of Alberta, Edmonton, AB T6G 2E3, Canada
| | - K Hickman-Lewis
- Department of Earth Sciences, The Natural History Museum, London SW7 5BD, UK.,Dipartimento di Scienze Biologiche, Geologiche e Ambientali, Università di Bologna, 40126 Bologna, Italy
| | - J R Johnson
- Johns Hopkins University Applied Physics Laboratory, Laurel, MD 20723, USA
| | - L C Kah
- Department of Earth and Planetary Sciences, University of Tennessee, Knoxville, TN 37996, USA
| | - P B Kelemen
- Department of Earth and Environmental Sciences, Lamont Doherty Earth Observatory of Columbia University, Palisades, NY 10964, USA
| | - K B Kinch
- Niels Bohr Institute, University of Copenhagen, 1350 Copenhagen, Denmark
| | - L Mandon
- Laboratoire d'Etudes Spatiales et d'Instrumentation en Astrophysique, Observatoire de Paris, Centre National de la Recherche Scientifique, Sorbonne Université, Université Paris Diderot, 92195 Meudon, France
| | - N Mangold
- Laboratoire de Planétologie et Géosciences, Centre National de la Recherche Scientifique, Nantes Université, Université Angers, 44000 Nantes, France
| | - C Quantin-Nataf
- Laboratoire de Géologie de Lyon: Terre, Université de Lyon, Université Claude Bernard Lyon1, Ecole Normale Supérieure de Lyon, Université Jean Monnet Saint Etienne, Centre National de la Recherche Scientifique, 69622 Villeurbanne, France
| | - M S Rice
- Department of Geology, Western Washington University, Bellingham, WA 98225 USA
| | - P S Russell
- Department of Earth, Planetary, and Space Sciences, University of California, Los Angeles, Los Angeles, CA 90095, USA
| | - S Sharma
- Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA
| | - S Siljeström
- Department of Methodology, Textiles and Medical Technology, Research Institutes of Sweden, 11486 Stockholm, Sweden
| | - A Steele
- Earth and Planetary Laboratory, Carnegie Science, Washington, DC 20015, USA
| | - R Sullivan
- Cornell Center for Astrophysics and Planetary Science, Cornell University, Ithaca, NY 14853, USA
| | - M Wadhwa
- School of Earth and Space Exploration, Arizona State University, Tempe, AZ 85287, USA
| | - B P Weiss
- Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA.,Department of Earth, Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, MA 02139, USA
| | - A J Williams
- Department of Geological Sciences, University of Florida, Gainesville, FL 32611, USA
| | - B V Wogsland
- Department of Earth and Planetary Sciences, University of Tennessee, Knoxville, TN 37996, USA
| | - P A Willis
- Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA
| | - T A Acosta-Maeda
- Hawai'i Institute of Geophysics and Planetology, University of Hawai'i at Mānoa, Honolulu, HI 96822, USA
| | - P Beck
- Institut de Planétologie et Astrophysique de Grenoble, Centre National de la Recherche Scientifique, Université Grenoble Alpes, 38000 Grenoble, France
| | - K Benzerara
- Institut de Minéralogie, de Physique des Matériaux et de Cosmochimie, Centre National de la Recherche Scientifique, Sorbonne Université, Muséum National d'Histoire Naturelle, 75005 Paris, France
| | - S Bernard
- Institut de Minéralogie, de Physique des Matériaux et de Cosmochimie, Centre National de la Recherche Scientifique, Sorbonne Université, Muséum National d'Histoire Naturelle, 75005 Paris, France
| | - A S Burton
- NASA Johnson Space Center, Houston, TX 77058, USA
| | - E L Cardarelli
- Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA
| | - B Chide
- Planetary Exploration Team, Los Alamos National Laboratory, Los Alamos, NM 87545, USA
| | - E Clavé
- Centre Lasers Intenses et Applications, Centre National de la Recherche Scientifique, Commissariat à l'Energie Atomique, Université de Bordeaux, 33400 Bordeaux, France
| | - E A Cloutis
- Centre for Terrestrial and Planetary Exploration, University of Winnipeg, Winnipeg, MB R3B 2E9, Canada
| | - B A Cohen
- NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA
| | - A D Czaja
- Department of Geology, University of Cincinnati, Cincinnati, OH 45221, USA
| | - V Debaille
- Laboratoire G-Time, Université Libre de Bruxelles, 1050 Brussels, Belgium
| | - E Dehouck
- Laboratoire de Géologie de Lyon: Terre, Université de Lyon, Université Claude Bernard Lyon1, Ecole Normale Supérieure de Lyon, Université Jean Monnet Saint Etienne, Centre National de la Recherche Scientifique, 69622 Villeurbanne, France
| | - A G Fairén
- Centro de Astrobiología, Consejo Superior de Investigaciones Científicas-Instituto Nacional de Técnica Aeroespacial, 28850 Madrid, Spain.,Department of Astronomy, Cornell University, Ithaca, NY 14853, USA
| | - D T Flannery
- School of Earth and Atmospheric Sciences, Queensland University of Technology, Brisbane, QLD 4001, Australia
| | - S Z Fleron
- Department of Geosciences and Natural Resource Management, University of Copenhagen, 1350 Copenhagen, Denmark
| | - T Fouchet
- Laboratoire d'Etudes Spatiales et d'Instrumentation en Astrophysique, Observatoire de Paris, Centre National de la Recherche Scientifique, Sorbonne Université, Université Paris Diderot, 92195 Meudon, France
| | - J Frydenvang
- Globe Institute, University of Copenhagen, 1350 Copenhagen, Denmark
| | - B J Garczynski
- Department of Earth, Atmospheric, and Planetary Sciences, Purdue University, West Lafayette, IN 47907, USA
| | - E F Gibbons
- Department of Earth and Planetary Sciences, McGill University, Montreal, QC H3A 0E8, Canada
| | - E M Hausrath
- Department of Geoscience, University of Nevada, Las Vegas, Las Vegas, NV 89154, USA
| | - A G Hayes
- Department of Astronomy, Cornell University, Ithaca, NY 14853, USA
| | - J Henneke
- National Space Institute, Technical University of Denmark, 2800 Kongens Lyngby, Denmark
| | - J L Jørgensen
- National Space Institute, Technical University of Denmark, 2800 Kongens Lyngby, Denmark
| | - E M Kelly
- Hawai'i Institute of Geophysics and Planetology, University of Hawai'i at Mānoa, Honolulu, HI 96822, USA
| | - J Lasue
- Institut de Recherche en Astrophysique et Planétologie, Université de Toulouse 3 Paul Sabatier, Centre National de la Recherche Scientifique, Centre National d'Etude Spatiale, 31400 Toulouse, France
| | - S Le Mouélic
- Laboratoire de Planétologie et Géosciences, Centre National de la Recherche Scientifique, Nantes Université, Université Angers, 44000 Nantes, France
| | - J M Madariaga
- Department of Analytical Chemistry, University of the Basque Country, 48940 Leioa, Spain
| | - S Maurice
- Institut de Recherche en Astrophysique et Planétologie, Université de Toulouse 3 Paul Sabatier, Centre National de la Recherche Scientifique, Centre National d'Etude Spatiale, 31400 Toulouse, France
| | - M Merusi
- Niels Bohr Institute, University of Copenhagen, 1350 Copenhagen, Denmark
| | - P-Y Meslin
- Institut de Recherche en Astrophysique et Planétologie, Université de Toulouse 3 Paul Sabatier, Centre National de la Recherche Scientifique, Centre National d'Etude Spatiale, 31400 Toulouse, France
| | - S M Milkovich
- Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA
| | | | - R C Moeller
- Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA
| | - J I Núñez
- Johns Hopkins University Applied Physics Laboratory, Laurel, MD 20723, USA
| | - A M Ollila
- Los Alamos National Laboratory, Los Alamos, NM 87545 USA
| | - G Paar
- Institute for Information and Communication Technologies, Joanneum Research, 8010 Graz, Austria
| | - D A Paige
- Department of Earth, Planetary, and Space Sciences, University of California, Los Angeles, Los Angeles, CA 90095, USA
| | - D A K Pedersen
- National Space Institute, Technical University of Denmark, 2800 Kongens Lyngby, Denmark
| | - P Pilleri
- Institut de Recherche en Astrophysique et Planétologie, Université de Toulouse 3 Paul Sabatier, Centre National de la Recherche Scientifique, Centre National d'Etude Spatiale, 31400 Toulouse, France
| | - C Pilorget
- Institut d'Astrophysique Spatiale, Université Paris-Saclay, 91405 Orsay, France.,Institut Universitaire de France, Paris, France
| | - P C Pinet
- Institut de Recherche en Astrophysique et Planétologie, Université de Toulouse 3 Paul Sabatier, Centre National de la Recherche Scientifique, Centre National d'Etude Spatiale, 31400 Toulouse, France
| | - J W Rice
- School of Earth and Space Exploration, Arizona State University, Tempe, AZ 85287, USA
| | - C Royer
- Institut de Minéralogie, de Physique des Matériaux et de Cosmochimie, Centre National de la Recherche Scientifique, Sorbonne Université, Muséum National d'Histoire Naturelle, 75005 Paris, France
| | - V Sautter
- Institut de Minéralogie, de Physique des Matériaux et de Cosmochimie, Centre National de la Recherche Scientifique, Sorbonne Université, Muséum National d'Histoire Naturelle, 75005 Paris, France
| | - M Schulte
- Mars Exploration Program, Planetary Science Division, NASA Headquarters, Washington, DC 20546, USA
| | - M A Sephton
- Department of Earth Sciences and Engineering, Imperial College London, London SW7 2AZ, UK
| | - S K Sharma
- Hawai'i Institute of Geophysics and Planetology, University of Hawai'i at Mānoa, Honolulu, HI 96822, USA
| | - S F Sholes
- Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA
| | - N Spanovich
- Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA
| | - M St Clair
- Million Concepts, Louisville, KY 40204, USA
| | - C D Tate
- Department of Astronomy, Cornell University, Ithaca, NY 14853, USA
| | - K Uckert
- Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA
| | - S J VanBommel
- McDonnell Center for the Space Sciences and Department of Earth and Planetary Sciences, Washington University in St. Louis, St. Louis, MO 63130, USA
| | | | - M-P Zorzano
- Department of Astronomy, Cornell University, Ithaca, NY 14853, USA
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2
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Bell JF, Maki JN, Mehall GL, Ravine MA, Caplinger MA, Bailey ZJ, Brylow S, Schaffner JA, Kinch KM, Madsen MB, Winhold A, Hayes AG, Corlies P, Tate C, Barrington M, Cisneros E, Jensen E, Paris K, Crawford K, Rojas C, Mehall L, Joseph J, Proton JB, Cluff N, Deen RG, Betts B, Cloutis E, Coates AJ, Colaprete A, Edgett KS, Ehlmann BL, Fagents S, Grotzinger JP, Hardgrove C, Herkenhoff KE, Horgan B, Jaumann R, Johnson JR, Lemmon M, Paar G, Caballo-Perucha M, Gupta S, Traxler C, Preusker F, Rice MS, Robinson MS, Schmitz N, Sullivan R, Wolff MJ. The Mars 2020 Perseverance Rover Mast Camera Zoom (Mastcam-Z) Multispectral, Stereoscopic Imaging Investigation. Space Sci Rev 2021; 217:24. [PMID: 33612866 PMCID: PMC7883548 DOI: 10.1007/s11214-020-00755-x] [Citation(s) in RCA: 5] [Impact Index Per Article: 1.7] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Grants] [Track Full Text] [Subscribe] [Scholar Register] [Received: 05/22/2020] [Accepted: 09/25/2020] [Indexed: 05/16/2023]
Abstract
Mastcam-Z is a multispectral, stereoscopic imaging investigation on the Mars 2020 mission's Perseverance rover. Mastcam-Z consists of a pair of focusable, 4:1 zoomable cameras that provide broadband red/green/blue and narrowband 400-1000 nm color imaging with fields of view from 25.6° × 19.2° (26 mm focal length at 283 μrad/pixel) to 6.2° × 4.6° (110 mm focal length at 67.4 μrad/pixel). The cameras can resolve (≥ 5 pixels) ∼0.7 mm features at 2 m and ∼3.3 cm features at 100 m distance. Mastcam-Z shares significant heritage with the Mastcam instruments on the Mars Science Laboratory Curiosity rover. Each Mastcam-Z camera consists of zoom, focus, and filter wheel mechanisms and a 1648 × 1214 pixel charge-coupled device detector and electronics. The two Mastcam-Z cameras are mounted with a 24.4 cm stereo baseline and 2.3° total toe-in on a camera plate ∼2 m above the surface on the rover's Remote Sensing Mast, which provides azimuth and elevation actuation. A separate digital electronics assembly inside the rover provides power, data processing and storage, and the interface to the rover computer. Primary and secondary Mastcam-Z calibration targets mounted on the rover top deck enable tactical reflectance calibration. Mastcam-Z multispectral, stereo, and panoramic images will be used to provide detailed morphology, topography, and geologic context along the rover's traverse; constrain mineralogic, photometric, and physical properties of surface materials; monitor and characterize atmospheric and astronomical phenomena; and document the rover's sample extraction and caching locations. Mastcam-Z images will also provide key engineering information to support sample selection and other rover driving and tool/instrument operations decisions.
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Affiliation(s)
| | | | | | - M. A. Ravine
- Malin Space Science Systems, Inc., San Diego, CA USA
| | | | | | - S. Brylow
- Malin Space Science Systems, Inc., San Diego, CA USA
| | | | | | | | | | | | | | - C. Tate
- Cornell Univ., Ithaca, NY USA
| | | | | | - E. Jensen
- Malin Space Science Systems, Inc., San Diego, CA USA
| | - K. Paris
- Arizona State Univ., Tempe, AZ USA
| | | | - C. Rojas
- Arizona State Univ., Tempe, AZ USA
| | | | | | | | - N. Cluff
- Arizona State Univ., Tempe, AZ USA
| | | | - B. Betts
- The Planetary Society, Pasadena, CA USA
| | | | - A. J. Coates
- Mullard Space Science Laboratory, Univ. College, London, UK
| | - A. Colaprete
- NASA/Ames Research Center, Moffett Field, CA USA
| | - K. S. Edgett
- Malin Space Science Systems, Inc., San Diego, CA USA
| | - B. L. Ehlmann
- JPL/Caltech, Pasadena, CA USA
- Caltech, Pasadena, CA USA
| | | | | | | | | | | | - R. Jaumann
- Inst. of Geological Sciences, Free University Berlin, Berlin, Germany
| | | | - M. Lemmon
- Space Science Inst., Boulder, CO USA
| | - G. Paar
- Joanneum Research, Graz, Austria
| | | | | | | | - F. Preusker
- DLR/German Aerospace Center, Berlin, Germany
| | - M. S. Rice
- Western Washington Univ., Bellingham, WA USA
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3
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Lopes RMC, Malaska MJ, Schoenfeld AM, Solomonidou A, Birch SPD, Florence M, Hayes AG, Williams DA, Radebaugh J, Verlander T, Turtle EP, Le Gall A, Wall S. A Global Geomorphologic Map of Saturn's Moon Titan. Nat Astron 2020; 4:228-233. [PMID: 32500095 PMCID: PMC7271969 DOI: 10.1038/s41550-019-0917-6] [Citation(s) in RCA: 5] [Impact Index Per Article: 1.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Figures] [Subscribe] [Scholar Register] [Received: 01/03/2019] [Accepted: 09/13/2019] [Indexed: 06/11/2023]
Abstract
Titan has an active methane-based hydrologic cycle1 that has shaped a complex geologic landscape2, making its surface one of most geologically diverse in the solar system. Despite the different materials, temperatures, and gravity fields between Earth and Titan, many surface features are similar between the two worlds and can be interpreted as products of the same geologic processes3. However, Titan's thick and hazy atmosphere has hindered the identification of geologic features at visible wavelengths and the study of surface composition4. Here we identify and map the major geologic units on Titan's surface using radar and infrared data from the Cassini orbiter spacecraft. Correlations between datasets enabled us to produce a global map even where data sets were incomplete. The spatial and superposition relations between major geologic units reveals the likely temporal evolution of the landscape and gives insight into the interacting processes driving its evolution. We extract the relative dating of the various geological units by observing their spatial superposition in order to get information on the temporal evolution of the landscape. Dunes and lakes are relatively young, while hummocky/mountainous terrains are the oldest on Titan. Our results also show that Titan's surface is dominated by sedimentary/depositional processes with significant latitudinal variation, with dunes at the equator, plains at mid-latitudes and labyrinth terrains and lakes at the poles.
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Affiliation(s)
- R M C Lopes
- Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA 91109, USA
| | - M J Malaska
- Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA 91109, USA
| | - A M Schoenfeld
- UCLA Department of Earth, Planetary, and Space Sciences595 Charles E Young Dr, E Los Angeles, CA, 90095, USA
| | | | - S P D Birch
- Department of Astronomy, Cornell University, 14853 Ithaca NY, USA
| | - M Florence
- Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA 91109, USA
| | - A G Hayes
- Department of Astronomy, Cornell University, 14853 Ithaca NY, USA
| | | | - J Radebaugh
- Department of Geological Sciences, Brigham Young University, Provo, UT 84602, USA
| | - T Verlander
- University of Oklahoma, School of Civil Engineering and Environmental Science, Norman, Oklahoma, USA
| | - E P Turtle
- JHU Applied Physics Lab, Laurel, MD 20723, USA
| | - A Le Gall
- LATMOS/IPSL, UVSQ Université Paris-Saclay, UPMC Univ. Paris 06, CNRS, Guyancourt, France
| | - S Wall
- Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA 91109, USA
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4
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Hayes AG, Grotzinger JP, Edgar LA, Squyres SW, Watters WA, Sohl-Dickstein J. Reconstruction of eolian bed forms and paleocurrents from cross-bedded strata at Victoria Crater, Meridiani Planum, Mars. ACTA ACUST UNITED AC 2011. [DOI: 10.1029/2010je003688] [Citation(s) in RCA: 30] [Impact Index Per Article: 2.3] [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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Turtle EP, Perry JE, Hayes AG, Lorenz RD, Barnes JW, McEwen AS, West RA, Del Genio AD, Barbara JM, Lunine JI, Schaller EL, Ray TL, Lopes RMC, Stofan ER. Rapid and Extensive Surface Changes Near Titan’s Equator: Evidence of April Showers. Science 2011; 331:1414-7. [DOI: 10.1126/science.1201063] [Citation(s) in RCA: 167] [Impact Index Per Article: 12.8] [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)
- E. P. Turtle
- Johns Hopkins University Applied Physics Laboratory, Laurel, MD 20723, USA
| | - J. E. Perry
- Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ 85721, USA
| | - A. G. Hayes
- Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA 91125, USA
| | - R. D. Lorenz
- Johns Hopkins University Applied Physics Laboratory, Laurel, MD 20723, USA
| | - J. W. Barnes
- Department of Physics, University of Idaho, Moscow, ID 83844, USA
| | - A. S. McEwen
- Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ 85721, USA
| | - R. A. West
- Jet Propulsion Laboratory, Pasadena, CA 91109, USA
| | - A. D. Del Genio
- NASA Goddard Institute for Space Studies, New York, NY 10025, USA
| | - J. M. Barbara
- NASA Goddard Institute for Space Studies, New York, NY 10025, USA
| | - J. I. Lunine
- Dipartimento di Fisica, Università degli Studi di Roma “Tor Vergata,” 00133 Rome, Italy
| | - E. L. Schaller
- Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ 85721, USA
| | - T. L. Ray
- Jet Propulsion Laboratory, Pasadena, CA 91109, USA
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6
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Hayes AG, Wolf AS, Aharonson O, Zebker H, Lorenz R, Kirk RL, Paillou P, Lunine J, Wye L, Callahan P, Wall S, Elachi C. Bathymetry and absorptivity of Titan's Ontario Lacus. ACTA ACUST UNITED AC 2010. [DOI: 10.1029/2009je003557] [Citation(s) in RCA: 48] [Impact Index Per Article: 3.4] [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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7
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Bell JF, Squyres SW, Arvidson RE, Arneson HM, Bass D, Calvin W, Farrand WH, Goetz W, Golombek M, Greeley R, Grotzinger J, 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, Morris RV, Dobrea EZN, Parker TJ, Proton J, Rice JW, Seelos F, Soderblom JM, Soderblom LA, Sohl-Dickstein JN, Sullivan RJ, Weitz CM, Wolff MJ. Pancam multispectral imaging results from the Opportunity Rover at Meridiani Planum. Science 2004; 306:1703-9. [PMID: 15576603 DOI: 10.1126/science.1105245] [Citation(s) in RCA: 115] [Impact Index Per Article: 5.8] [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 (Pancam) images from Meridiani Planum reveal a low-albedo, generally flat, and relatively rock-free surface. Within and around impact craters and fractures, laminated outcrop rocks with higher albedo are observed. Fine-grained materials include dark sand, bright ferric iron-rich dust, angular rock clasts, and millimeter-size spheroidal granules that are eroding out of the laminated rocks. Spectra of sand, clasts, and one dark plains rock are consistent with mafic silicates such as pyroxene and olivine. Spectra of both the spherules and the laminated outcrop materials indicate the presence of crystalline ferric oxides or oxyhydroxides. Atmospheric observations show a steady decline in dust opacity during the mission. Astronomical observations captured solar transits by Phobos and Deimos and time-lapse observations of sunsets.
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Affiliation(s)
- J F Bell
- Department of Astronomy, Cornell University, Ithaca NY 14853, USA.
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8
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Herkenhoff KE, Squyres SW, Arvidson R, Bass DS, Bell JF, Bertelsen P, Ehlmann BL, Farrand W, Gaddis L, Greeley R, Grotzinger J, Hayes AG, Hviid SF, Johnson JR, Jolliff B, Kinch KM, Knoll AH, Madsen MB, Maki JN, McLennan SM, McSween HY, Ming DW, Rice JW, Richter L, Sims M, Smith PH, Soderblom LA, Spanovich N, Sullivan R, Thompson S, Wdowiak T, Weitz C, Whelley P. Evidence from Opportunity's Microscopic Imager for water on Meridiani Planum. Science 2004; 306:1727-30. [PMID: 15576607 DOI: 10.1126/science.1105286] [Citation(s) in RCA: 118] [Impact Index Per Article: 5.9] [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: 11/02/2022]
Abstract
The Microscopic Imager on the Opportunity rover analyzed textures of soils and rocks at Meridiani Planum at a scale of 31 micrometers per pixel. The uppermost millimeter of some soils is weakly cemented, whereas other soils show little evidence of cohesion. Rock outcrops are laminated on a millimeter scale; image mosaics of cross-stratification suggest that some sediments were deposited by flowing water. Vugs in some outcrop faces are probably molds formed by dissolution of relatively soluble minerals during diagenesis. Microscopic images support the hypothesis that hematite-rich spherules observed in outcrops and soils also formed diagenetically as concretions.
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Affiliation(s)
- K E Herkenhoff
- U.S. Geological Survey Astrogeology Team, Flagstaff, AZ 86001, USA.
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9
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Christensen PR, Wyatt MB, Glotch TD, Rogers AD, Anwar S, Arvidson RE, Bandfield JL, Blaney DL, Budney C, Calvin WM, Fallacaro A, Fergason RL, Gorelick N, Graff TG, Hamilton VE, Hayes AG, Johnson JR, Knudson AT, McSween HY, Mehall GL, Mehall LK, Moersch JE, Morris RV, Smith MD, Squyres SW, Ruff SW, Wolff MJ. Mineralogy at Meridiani Planum from the Mini-TES Experiment on the Opportunity Rover. Science 2004; 306:1733-9. [PMID: 15576609 DOI: 10.1126/science.1104909] [Citation(s) in RCA: 114] [Impact Index Per Article: 5.7] [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 Miniature Thermal Emission Spectrometer (Mini-TES) on Opportunity investigated the mineral abundances and compositions of outcrops, rocks, and soils at Meridiani Planum. Coarse crystalline hematite and olivine-rich basaltic sands were observed as predicted from orbital TES spectroscopy. Outcrops of aqueous origin are composed of 15 to 35% by volume magnesium and calcium sulfates [a high-silica component modeled as a combination of glass, feldspar, and sheet silicates (approximately 20 to 30%)], and hematite; only minor jarosite is identified in Mini-TES spectra. Mini-TES spectra show only a hematite signature in the millimeter-sized spherules. Basaltic materials have more plagioclase than pyroxene, contain olivine, and are similar in inferred mineral composition to basalt mapped from orbit. Bounce rock is dominated by clinopyroxene and is close in inferred mineral composition to the basaltic martian meteorites. Bright wind streak material matches global dust. Waterlain rocks covered by unaltered basaltic sands suggest a change from an aqueous environment to one dominated by physical weathering.
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Affiliation(s)
- P R Christensen
- Department of Geological Sciences, Arizona State University, Tempe, AZ 85287, USA.
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10
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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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11
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Herkenhoff KE, Squyres SW, Arvidson R, Bass DS, Bell JF, Bertelsen P, Cabrol NA, Gaddis L, Hayes AG, Hviid SF, Johnson JR, Kinch KM, Madsen MB, Maki JN, McLennan SM, McSween HY, Rice JW, Sims M, Smith PH, Soderblom LA, Spanovich N, Sullivan R, Wang A. Textures of the Soils and Rocks at Gusev Crater from Spirit's Microscopic Imager. Science 2004. [DOI: 10.1126/science.3050824] [Citation(s) in RCA: 113] [Impact Index Per Article: 5.7] [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)
- K. E. Herkenhoff
- U.S. Geological Survey Astrogeology Team, Flagstaff, AZ 86001, USA
- Department of Astronomy, Space Sciences Building, Cornell University, Ithaca, NY 14853, USA
- Department of Earth and Space Sciences, Washington University, St. Louis, MO 63130, USA
- Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA
- Center for Planetary Science, Danish Space Research Institute and Niels Bohr Institute for Astronomy, Physics, and Geophysics, University of Copenhagen, Denmark
| | - S. W. Squyres
- U.S. Geological Survey Astrogeology Team, Flagstaff, AZ 86001, USA
- Department of Astronomy, Space Sciences Building, Cornell University, Ithaca, NY 14853, USA
- Department of Earth and Space Sciences, Washington University, St. Louis, MO 63130, USA
- Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA
- Center for Planetary Science, Danish Space Research Institute and Niels Bohr Institute for Astronomy, Physics, and Geophysics, University of Copenhagen, Denmark
| | - R. Arvidson
- U.S. Geological Survey Astrogeology Team, Flagstaff, AZ 86001, USA
- Department of Astronomy, Space Sciences Building, Cornell University, Ithaca, NY 14853, USA
- Department of Earth and Space Sciences, Washington University, St. Louis, MO 63130, USA
- Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA
- Center for Planetary Science, Danish Space Research Institute and Niels Bohr Institute for Astronomy, Physics, and Geophysics, University of Copenhagen, Denmark
| | - D. S. Bass
- U.S. Geological Survey Astrogeology Team, Flagstaff, AZ 86001, USA
- Department of Astronomy, Space Sciences Building, Cornell University, Ithaca, NY 14853, USA
- Department of Earth and Space Sciences, Washington University, St. Louis, MO 63130, USA
- Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA
- Center for Planetary Science, Danish Space Research Institute and Niels Bohr Institute for Astronomy, Physics, and Geophysics, University of Copenhagen, Denmark
| | - J. F. Bell
- U.S. Geological Survey Astrogeology Team, Flagstaff, AZ 86001, USA
- Department of Astronomy, Space Sciences Building, Cornell University, Ithaca, NY 14853, USA
- Department of Earth and Space Sciences, Washington University, St. Louis, MO 63130, USA
- Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA
- Center for Planetary Science, Danish Space Research Institute and Niels Bohr Institute for Astronomy, Physics, and Geophysics, University of Copenhagen, Denmark
| | - P. Bertelsen
- U.S. Geological Survey Astrogeology Team, Flagstaff, AZ 86001, USA
- Department of Astronomy, Space Sciences Building, Cornell University, Ithaca, NY 14853, USA
- Department of Earth and Space Sciences, Washington University, St. Louis, MO 63130, USA
- Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA
- Center for Planetary Science, Danish Space Research Institute and Niels Bohr Institute for Astronomy, Physics, and Geophysics, University of Copenhagen, Denmark
| | - N. A. Cabrol
- U.S. Geological Survey Astrogeology Team, Flagstaff, AZ 86001, USA
- Department of Astronomy, Space Sciences Building, Cornell University, Ithaca, NY 14853, USA
- Department of Earth and Space Sciences, Washington University, St. Louis, MO 63130, USA
- Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA
- Center for Planetary Science, Danish Space Research Institute and Niels Bohr Institute for Astronomy, Physics, and Geophysics, University of Copenhagen, Denmark
| | - L. Gaddis
- U.S. Geological Survey Astrogeology Team, Flagstaff, AZ 86001, USA
- Department of Astronomy, Space Sciences Building, Cornell University, Ithaca, NY 14853, USA
- Department of Earth and Space Sciences, Washington University, St. Louis, MO 63130, USA
- Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA
- Center for Planetary Science, Danish Space Research Institute and Niels Bohr Institute for Astronomy, Physics, and Geophysics, University of Copenhagen, Denmark
| | - A. G. Hayes
- U.S. Geological Survey Astrogeology Team, Flagstaff, AZ 86001, USA
- Department of Astronomy, Space Sciences Building, Cornell University, Ithaca, NY 14853, USA
- Department of Earth and Space Sciences, Washington University, St. Louis, MO 63130, USA
- Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA
- Center for Planetary Science, Danish Space Research Institute and Niels Bohr Institute for Astronomy, Physics, and Geophysics, University of Copenhagen, Denmark
| | - S. F. Hviid
- U.S. Geological Survey Astrogeology Team, Flagstaff, AZ 86001, USA
- Department of Astronomy, Space Sciences Building, Cornell University, Ithaca, NY 14853, USA
- Department of Earth and Space Sciences, Washington University, St. Louis, MO 63130, USA
- Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA
- Center for Planetary Science, Danish Space Research Institute and Niels Bohr Institute for Astronomy, Physics, and Geophysics, University of Copenhagen, Denmark
| | - J. R. Johnson
- U.S. Geological Survey Astrogeology Team, Flagstaff, AZ 86001, USA
- Department of Astronomy, Space Sciences Building, Cornell University, Ithaca, NY 14853, USA
- Department of Earth and Space Sciences, Washington University, St. Louis, MO 63130, USA
- Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA
- Center for Planetary Science, Danish Space Research Institute and Niels Bohr Institute for Astronomy, Physics, and Geophysics, University of Copenhagen, Denmark
| | - K. M. Kinch
- U.S. Geological Survey Astrogeology Team, Flagstaff, AZ 86001, USA
- Department of Astronomy, Space Sciences Building, Cornell University, Ithaca, NY 14853, USA
- Department of Earth and Space Sciences, Washington University, St. Louis, MO 63130, USA
- Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA
- Center for Planetary Science, Danish Space Research Institute and Niels Bohr Institute for Astronomy, Physics, and Geophysics, University of Copenhagen, Denmark
| | - M. B. Madsen
- U.S. Geological Survey Astrogeology Team, Flagstaff, AZ 86001, USA
- Department of Astronomy, Space Sciences Building, Cornell University, Ithaca, NY 14853, USA
- Department of Earth and Space Sciences, Washington University, St. Louis, MO 63130, USA
- Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA
- Center for Planetary Science, Danish Space Research Institute and Niels Bohr Institute for Astronomy, Physics, and Geophysics, University of Copenhagen, Denmark
| | - J. N. Maki
- U.S. Geological Survey Astrogeology Team, Flagstaff, AZ 86001, USA
- Department of Astronomy, Space Sciences Building, Cornell University, Ithaca, NY 14853, USA
- Department of Earth and Space Sciences, Washington University, St. Louis, MO 63130, USA
- Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA
- Center for Planetary Science, Danish Space Research Institute and Niels Bohr Institute for Astronomy, Physics, and Geophysics, University of Copenhagen, Denmark
| | - S. M. McLennan
- U.S. Geological Survey Astrogeology Team, Flagstaff, AZ 86001, USA
- Department of Astronomy, Space Sciences Building, Cornell University, Ithaca, NY 14853, USA
- Department of Earth and Space Sciences, Washington University, St. Louis, MO 63130, USA
- Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA
- Center for Planetary Science, Danish Space Research Institute and Niels Bohr Institute for Astronomy, Physics, and Geophysics, University of Copenhagen, Denmark
| | - H. Y. McSween
- U.S. Geological Survey Astrogeology Team, Flagstaff, AZ 86001, USA
- Department of Astronomy, Space Sciences Building, Cornell University, Ithaca, NY 14853, USA
- Department of Earth and Space Sciences, Washington University, St. Louis, MO 63130, USA
- Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA
- Center for Planetary Science, Danish Space Research Institute and Niels Bohr Institute for Astronomy, Physics, and Geophysics, University of Copenhagen, Denmark
| | - J. W. Rice
- U.S. Geological Survey Astrogeology Team, Flagstaff, AZ 86001, USA
- Department of Astronomy, Space Sciences Building, Cornell University, Ithaca, NY 14853, USA
- Department of Earth and Space Sciences, Washington University, St. Louis, MO 63130, USA
- Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA
- Center for Planetary Science, Danish Space Research Institute and Niels Bohr Institute for Astronomy, Physics, and Geophysics, University of Copenhagen, Denmark
| | - M. Sims
- U.S. Geological Survey Astrogeology Team, Flagstaff, AZ 86001, USA
- Department of Astronomy, Space Sciences Building, Cornell University, Ithaca, NY 14853, USA
- Department of Earth and Space Sciences, Washington University, St. Louis, MO 63130, USA
- Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA
- Center for Planetary Science, Danish Space Research Institute and Niels Bohr Institute for Astronomy, Physics, and Geophysics, University of Copenhagen, Denmark
| | - P. H. Smith
- U.S. Geological Survey Astrogeology Team, Flagstaff, AZ 86001, USA
- Department of Astronomy, Space Sciences Building, Cornell University, Ithaca, NY 14853, USA
- Department of Earth and Space Sciences, Washington University, St. Louis, MO 63130, USA
- Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA
- Center for Planetary Science, Danish Space Research Institute and Niels Bohr Institute for Astronomy, Physics, and Geophysics, University of Copenhagen, Denmark
| | - L. A. Soderblom
- U.S. Geological Survey Astrogeology Team, Flagstaff, AZ 86001, USA
- Department of Astronomy, Space Sciences Building, Cornell University, Ithaca, NY 14853, USA
- Department of Earth and Space Sciences, Washington University, St. Louis, MO 63130, USA
- Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA
- Center for Planetary Science, Danish Space Research Institute and Niels Bohr Institute for Astronomy, Physics, and Geophysics, University of Copenhagen, Denmark
| | - N. Spanovich
- U.S. Geological Survey Astrogeology Team, Flagstaff, AZ 86001, USA
- Department of Astronomy, Space Sciences Building, Cornell University, Ithaca, NY 14853, USA
- Department of Earth and Space Sciences, Washington University, St. Louis, MO 63130, USA
- Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA
- Center for Planetary Science, Danish Space Research Institute and Niels Bohr Institute for Astronomy, Physics, and Geophysics, University of Copenhagen, Denmark
| | - R. Sullivan
- U.S. Geological Survey Astrogeology Team, Flagstaff, AZ 86001, USA
- Department of Astronomy, Space Sciences Building, Cornell University, Ithaca, NY 14853, USA
- Department of Earth and Space Sciences, Washington University, St. Louis, MO 63130, USA
- Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA
- Center for Planetary Science, Danish Space Research Institute and Niels Bohr Institute for Astronomy, Physics, and Geophysics, University of Copenhagen, Denmark
| | - A. Wang
- U.S. Geological Survey Astrogeology Team, Flagstaff, AZ 86001, USA
- Department of Astronomy, Space Sciences Building, Cornell University, Ithaca, NY 14853, USA
- Department of Earth and Space Sciences, Washington University, St. Louis, MO 63130, USA
- Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA
- Center for Planetary Science, Danish Space Research Institute and Niels Bohr Institute for Astronomy, Physics, and Geophysics, University of Copenhagen, Denmark
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12
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Herkenhoff KE, Squyres SW, Arvidson R, Bass DS, Bell JF, Bertelsen P, Cabrol NA, Gaddis L, Hayes AG, Hviid SF, Johnson JR, Kinch KM, Madsen MB, Maki JN, McLennan SM, McSween HY, Rice JW, Sims M, Smith PH, Soderblom LA, Spanovich N, Sullivan R, Wang A. Textures of the soils and rocks at Gusev Crater from Spirit's Microscopic Imager. Science 2004; 305:824-6. [PMID: 15297663 DOI: 10.1126/science.1100015] [Citation(s) in RCA: 4] [Impact Index Per Article: 0.2] [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 Microscopic Imager on the Spirit rover analyzed the textures of the soil and rocks at Gusev crater on Mars at a resolution of 100 micrometers. Weakly bound agglomerates of dust are present in the soil near the Columbia Memorial Station. Some of the brushed or abraded rock surfaces show igneous textures and evidence for alteration rinds, coatings, and veins consistent with secondary mineralization. The rock textures are consistent with a volcanic origin and subsequent alteration and/or weathering by impact events, wind, and possibly water.
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Affiliation(s)
- K E Herkenhoff
- U.S. Geological Survey Astrogeology Team, Flagstaff, AZ 86001, USA.
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13
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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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14
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Bell JF, Squyres SW, Herkenhoff KE, Maki JN, Arneson HM, Brown D, Collins SA, Dingizian A, Elliot ST, Hagerott EC, Hayes AG, Johnson MJ, Johnson JR, Joseph J, Kinch K, Lemmon MT, Morris RV, Scherr L, Schwochert M, Shepard MK, Smith GH, Sohl-Dickstein JN, Sullivan RJ, Sullivan WT, Wadsworth M. Mars Exploration Rover Athena Panoramic Camera (Pancam) investigation. ACTA ACUST UNITED AC 2003. [DOI: 10.1029/2003je002070] [Citation(s) in RCA: 209] [Impact Index Per Article: 10.0] [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)
- J. F. Bell
- Department of Astronomy; Cornell University; Ithaca New York USA
| | - S. W. Squyres
- Department of Astronomy; Cornell University; Ithaca New York USA
| | | | - J. N. Maki
- Jet Propulsion Laboratory; California Institute of Technology; Pasadena California USA
| | - H. M. Arneson
- Department of Astronomy; Cornell University; Ithaca New York USA
| | - D. Brown
- Jet Propulsion Laboratory; California Institute of Technology; Pasadena California USA
| | - S. A. Collins
- Jet Propulsion Laboratory; California Institute of Technology; Pasadena California USA
| | - A. Dingizian
- Jet Propulsion Laboratory; California Institute of Technology; Pasadena California USA
| | - S. T. Elliot
- Jet Propulsion Laboratory; California Institute of Technology; Pasadena California USA
| | - E. C. Hagerott
- Jet Propulsion Laboratory; California Institute of Technology; Pasadena California USA
| | - A. G. Hayes
- Department of Astronomy; Cornell University; Ithaca New York USA
| | - M. J. Johnson
- Department of Astronomy; Cornell University; Ithaca New York USA
| | | | - J. Joseph
- Department of Astronomy; Cornell University; Ithaca New York USA
| | - K. Kinch
- Neils Bohr Institute; University of Copenhagen; Copenhagen Denmark
| | - M. T. Lemmon
- Department of Atmospheric Science; Texas A&M University; College Station Texas USA
| | | | - L. Scherr
- Jet Propulsion Laboratory; California Institute of Technology; Pasadena California USA
| | - M. Schwochert
- Jet Propulsion Laboratory; California Institute of Technology; Pasadena California USA
| | - M. K. Shepard
- Department of Geography and Geosciences; Bloomsburg University; Bloomsburg Pennsylvania USA
| | | | | | - R. J. Sullivan
- Department of Astronomy; Cornell University; Ithaca New York USA
| | - W. T. Sullivan
- Department of Astronomy; University of Washington; Seattle Washington USA
| | - M. Wadsworth
- Jet Propulsion Laboratory; California Institute of Technology; Pasadena California USA
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15
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Herkenhoff KE, Squyres SW, Bell JF, Maki JN, Arneson HM, Bertelsen P, Brown DI, Collins SA, Dingizian A, Elliott ST, Goetz W, Hagerott EC, Hayes AG, Johnson MJ, Kirk RL, McLennan S, Morris RV, Scherr LM, Schwochert MA, Shiraishi LR, Smith GH, Soderblom LA, Sohl-Dickstein JN, Wadsworth MV. Athena Microscopic Imager investigation. ACTA ACUST UNITED AC 2003. [DOI: 10.1029/2003je002076] [Citation(s) in RCA: 115] [Impact Index Per Article: 5.5] [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)
- K. E. Herkenhoff
- Astrogeology Team, U.S. Geological Survey; Flagstaff Arizona USA
| | - S. W. Squyres
- Department of Astronomy; Cornell University; Ithaca New York USA
| | - J. F. Bell
- Department of Astronomy; Cornell University; Ithaca New York USA
| | - J. N. Maki
- Jet Propulsion Laboratory; California Institute of Technology; Pasadena California USA
| | - H. M. Arneson
- Department of Astronomy; Cornell University; Ithaca New York USA
| | - P. Bertelsen
- Niels Bohr Institute for Astronomy, Physics and Geophysics; University of Copenhagen; Copenhagen Denmark
| | - D. I. Brown
- Jet Propulsion Laboratory; California Institute of Technology; Pasadena California USA
| | - S. A. Collins
- Jet Propulsion Laboratory; California Institute of Technology; Pasadena California USA
| | - A. Dingizian
- Jet Propulsion Laboratory; California Institute of Technology; Pasadena California USA
| | - S. T. Elliott
- Jet Propulsion Laboratory; California Institute of Technology; Pasadena California USA
| | - W. Goetz
- Niels Bohr Institute for Astronomy, Physics and Geophysics; University of Copenhagen; Copenhagen Denmark
| | - E. C. Hagerott
- Jet Propulsion Laboratory; California Institute of Technology; Pasadena California USA
| | - A. G. Hayes
- Department of Astronomy; Cornell University; Ithaca New York USA
| | - M. J. Johnson
- Department of Astronomy; Cornell University; Ithaca New York USA
| | - R. L. Kirk
- Astrogeology Team, U.S. Geological Survey; Flagstaff Arizona USA
| | - S. McLennan
- Department of Geosciences; State University of New York; Stony Brook New York USA
| | | | - L. M. Scherr
- Jet Propulsion Laboratory; California Institute of Technology; Pasadena California USA
| | - M. A. Schwochert
- Jet Propulsion Laboratory; California Institute of Technology; Pasadena California USA
| | - L. R. Shiraishi
- Jet Propulsion Laboratory; California Institute of Technology; Pasadena California USA
| | | | - L. A. Soderblom
- Astrogeology Team, U.S. Geological Survey; Flagstaff Arizona USA
| | | | - M. V. Wadsworth
- Jet Propulsion Laboratory; California Institute of Technology; Pasadena California USA
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16
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Dodrill CB, Arnett JL, Hayes AG, Garofalo EA, Greeley CA, Greiner MJ, Pierce MW. Cognitive abilities and adjustment with gabapentin: results of a multisite study. Epilepsy Res 1999; 35:109-21. [PMID: 10372564 DOI: 10.1016/s0920-1211(99)00006-6] [Citation(s) in RCA: 29] [Impact Index Per Article: 1.2] [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: 11/24/2022]
Abstract
The cognitive and quality of life effects of gabapentin are not yet well explored. While preliminary work in the area has provided positive findings, a large double-blinded study has been needed to explore this area more thoroughly. From 24 sites in North America, 201 adults were studied who had uncontrolled complex partial seizures with or without secondary generalization. Attempts were made to convert each patient from one or two marketed antiepileptic drugs (AEDs) taken in baseline to gabapentin monotherapy (600, 1200, or 2400 mg/day). Tests of cognitive abilities and adjustment were administered at the end of the 8-week baseline period and at the end of the 26-week double-blind treatment period. Analyses of baseline to treatment period changes were conducted for each dose group in comparison with a reference group of placebo-treated patients from another study. In the area of cognitive functioning, no changes in any of the gabapentin groups were found in comparison with the reference group. In the area of adjustment and mood, however, improvement with gabapentin administration was noted on several variables pertaining to emotional and interpersonal adjustment. These results are consistent with findings from previous studies.
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Affiliation(s)
- C B Dodrill
- Regional Epilepsy Center, Harborview Medical Center, Seattle, WA 98104-2499, USA.
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17
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Hayes AG, Nadkarni JB. Extensile posterior approach to the ankle. J Bone Joint Surg Br 1996; 78:468-70. [PMID: 8636188] [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] [Subscribe] [Scholar Register] [Indexed: 02/01/2023]
Abstract
Surgical exposure of the ankle is usually obtained by an anterior approach, especially for replacement arthroplasty. The transfibular approach has been popular for arthrodesis. We describe a new posterior approach to the ankle and posterior subtalar joint based on an extra-articular vertical calcaneal osteotomy behind the subtalar joint. The posterior flap so formed is hinged medially and offers wide exposure of the back of the ankle and posterior subtalar joint. This hinge allows safe and stable reduction of the osteotomised calcaneum, and the plane of dissection follows an 'internervous plane' behind the fibula. We have had good results after using this incision in 12 patients with osteoarthritis or rheumatoid arthritis and there have been no difficulties with wound healing.
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Affiliation(s)
- A G Hayes
- District General Hospital, Southport, England
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18
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Abstract
Surgical exposure of the ankle is usually obtained by an anterior approach, especially for replacement arthroplasty. The transfibular approach has been popular for arthrodesis. We describe a new posterior approach to the ankle and posterior subtalar joint based on an extra-articular vertical calcaneal osteotomy behind the subtalar joint. The posterior flap so formed is hinged medially and offers wide exposure of the back of the ankle and posterior subtalar joint. This hinge allows safe and stable reduction of the osteotomised calcaneum, and the plane of dissection follows an ‘internervous plane’ behind the fibula. We have had good results after using this incision in 12 patients with osteoarthritis or rheumatoid arthritis and there have been no difficulties with wound healing.
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Affiliation(s)
- A. G. Hayes
- District General Hospital, Town Lane, Kew, Southport, Merseyside PR8 6PN, UK
| | - J. B. Nadkarni
- District General Hospital, Town Lane, Kew, Southport, Merseyside PR8 6PN, UK
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19
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Hayes AG, Boudrieau RJ, Hungerford LL. Frequency and distribution of medial and lateral patellar luxation in dogs: 124 cases (1982-1992). J Am Vet Med Assoc 1994; 205:716-20. [PMID: 7989241] [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] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 01/28/2023]
Abstract
From the medical records of 124 dogs, patellar luxations were classified as congenital or acquired, medial or lateral, and unilateral or bilateral; were graded 1 to 4; and were subdivided according to size of dog. The 4 breed-size categories were based on guidelines from American Kennel Club standards for adult height and weight. Findings from these records were compared with the results from dogs with other orthopedic problems. A majority of dogs had congenital (91; 82%), as opposed to acquired (17; 15%) patellar luxations. Distribution of dogs with patellar luxations according to breed size included 54 (98%) with medial patellar luxations (MPL) and 1 (2%) with lateral patellar luxation (LPL) in small breeds, 17 (81%) with MPL and 4 (19%) with LPL in medium breeds, 35 (83%) with MPL and 7 (17%) with LPL in large breeds; and 4 (67%) with MPL and 2 (33%) with LPL in giant breeds. Medial patellar luxation was observed in 110 dogs and 14 dogs had LPL. Cases of MPL and LPL in the same stifle or of medial and lateral patellar luxation in contralateral stifles in the same dog were not observed. Surgical correction was performed primarily in dogs with grade-3 and grade-4 patellar luxations. Medial patellar luxations and LPL were detected in all breed categories. Small-breed dogs were admitted almost exclusively with MPL. Lateral patellar luxation was found uncommonly; however, it was observed more often in larger-breed dogs. Prevalence of MPL was greater, when compared with that for LPL, in every size/breed category.
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Affiliation(s)
- A G Hayes
- Department of Surgery, School of Veterinary Medicine, Tufts University, North Grafton, MA 01536
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20
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Naylor A, Judd DB, Scopes DI, Hayes AG, Birch PJ. 4-[(Alkylamino)methyl]furo[3,2-c]pyridines: a new series of selective kappa-receptor agonists. J Med Chem 1994; 37:2138-44. [PMID: 8035420 DOI: 10.1021/jm00040a004] [Citation(s) in RCA: 27] [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: 01/28/2023]
Abstract
The synthesis of 5-(arylacetyl)-4-[(alkylamino)methyl]furo[3,2-c] pyridines (16-23, 26, 27) and their activities as kappa-opioid receptor agonists are described. kappa-Agonist potency was particularly sensitive to the nature of the basic moiety. In particular, in the rabbit vas deferens (kappa-specific tissue), the 3-pyrrolidinol analogue 17 (IC50 = 2.7 nM) was found to be approximately 5-fold more potent than the corresponding pyrrolidine analogue 16 (IC50 = 15 nM). In the rat and hamster vasa deferentia (mu-specific and delta-specific tissues, respectively), 17 showed only weak antagonist activity (pKB > 5.5), underlining its selectivity for the kappa-opioid receptor. The major activity for 17 is resident in the 4S,3'S-isomer 26 (rabbit vas deferens IC50 = 1.1 nM). Compound 26 displays excellent antinociceptive activity, as determined in the mouse acetylcholine-induced abdominal constriction test (ED50 = 0.001 mg/kg, sc).
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Affiliation(s)
- A Naylor
- Department of Medicinal Chemistry, Glaxo Group Research Ltd., Ware, Hertfordshire, England
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21
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Abstract
Unilateral and bilateral injections of cis-2,4-methanoglutamate, a potent and selective NMDA agonist, were made into the striatum of rats. Unilateral injections elicited MK-801-sensitive dose-related increases in contralateral turning, beginning 10-15 min after injection. Bilateral injections elicited typical seizure-like behaviours commencing approximately 80 min postinjection. Forty-eight hours after unilateral injection, and presumably after lesion development, no spontaneous preference for turning was seen. Upon challenge with apomorphine (1 mg/kg SC), ipsilateral turning lasting approximately 60 min was seen. Correlates are drawn between this model and some of the features of Huntington's disease.
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Affiliation(s)
- M D Black
- Glaxo Institute of Applied Pharmacology, Department of Pharmacology, Cambridge, UK
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22
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Affiliation(s)
- A G Hayes
- Department of Pathology, University of Tennessee School of Medicine at Memphis
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23
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Naylor A, Judd DB, Lloyd JE, Scopes DI, Hayes AG, Birch PJ. A potent new class of kappa-receptor agonist: 4-substituted 1-(arylacetyl)-2-[(dialkylamino)methyl]piperazines. J Med Chem 1993; 36:2075-83. [PMID: 8393489 DOI: 10.1021/jm00067a004] [Citation(s) in RCA: 78] [Impact Index Per Article: 2.5] [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: 01/30/2023]
Abstract
The synthesis of 4-substituted 1-(arylacetyl)-2-[(alkylamino)methyl]piperazines (10-22, 26, 27, and 30-33) and their activities as kappa-opioid receptor agonists are described. This includes a range of 4-acyl and 4-carboalkoxy derivatives with the latter series showing the greatest kappa-agonist activity. In particular, methyl 4-[(3,4-dichlorophenyl)acetyl]-3-[(1-pyrrolidinyl) methyl]-1-piperazinecarboxylate (18) displays exceptional potency and selectivity. It showed the following activities in functional in vitro assays: rabbit vas deferens (kappa-specific tissue) IC50 = 0.041 nM, rat vas deferens (mu-specific tissue) IC50 > 10,000 nM, and hamster vas deferens (delta-specific tissue) IC50 > 10,000 nM. Compound 18 is also a highly potent antinociceptive agent, as determined in the mouse acetylcholine-induced abdominal constriction test: ED50 = 0.000 52 mg/kg, sc. The activity of 18 resides solely in its 3(R)-enantiomer. The kappa-agonist activity in both the 4-acyl and the 4-carbamate series is sensitive to the size of the 4-substituent. In addition, it would appear that an appreciable negative electrostatic potential in this region of the molecule is an important requirement for optimal potency.
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Affiliation(s)
- A Naylor
- Department of Medicinal Chemistry, Glaxo Group Research Ltd., Ware, Hertfordshire, England
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24
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25
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Abstract
We report an exceptional case of metastatic adenocarcinoma of the breast occurring within a benign intradermal nevus. An extensive review of the literature on metastatic breast carcinoma is included.
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Affiliation(s)
- A G Hayes
- Department of Pathology, University of Tennessee, Memphis
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26
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Affiliation(s)
- A G Hayes
- Department of Pathology, University of Tennessee, Memphis
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27
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Abstract
Extravascular escape of intravenously administered phenytoin can result in serious local soft tissue complications. Injury can range from simple phlebitis to chemical cellulitis or, in extreme cases, frank tissue necrosis that necessitates amputation. The histopathologic findings include extensive necrosis and sloughing of epidermis, widespread necrosis of dermis, subcutaneous tissue, muscles and nerves, and extensive thrombotic occlusion of vessel lumens. Results of elastic tissue stains reveal that the thrombosed vessels are exclusively veins and venules. Vascular fibrinoid necrosis, leukocytoclasis, and true inflammatory vasculitis are not features. This is the first detailed report of the histopathologic alterations associated with this therapeutic misadventure.
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Affiliation(s)
- A G Hayes
- Department of Pathology, University of Tennessee, Memphis
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Rogers H, Birch PJ, Harrison SM, Palmer E, Manchee GR, Judd DB, Naylor A, Scopes DI, Hayes AG. GR94839, a kappa-opioid agonist with limited access to the central nervous system, has antinociceptive activity. Br J Pharmacol 1992; 106:783-9. [PMID: 1327387 PMCID: PMC1907638 DOI: 10.1111/j.1476-5381.1992.tb14413.x] [Citation(s) in RCA: 26] [Impact Index Per Article: 0.8] [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: 12/26/2022] Open
Abstract
1. The pharmacological profile of GR94839, a kappa-opioid agonist with limited access to the central nervous system, has been investigated. Its antinociceptive activity has been compared with that of GR103545, a centrally-penetrating kappa-agonist and ICI204448, the previously described peripherally-selective kappa-agonist. 2. GR94839 was a potent agonist in the rabbit vas deferens in vitro assay for kappa-opioid receptors (IC50: 1.4 +/- 0.3 nM; n = 6), but had limited activity at mu- or delta-opioid receptors. 3. In the mouse abdominal constriction test, GR94839 was 238 fold more potent when given i.c.v. (ED50: 0.008 (0.004-0.029) mg kg-1; n = 18) than when s.c. (ED50: 1.9 (0.7-3.1) mg kg-1; n = 30). In comparison, GR103545 was equipotent when given i.c.v. or s.c. 4. After intravenous administration, the maximum plasma to brain concentration-ratio attained by GR94839 was 18 compared with 2 for GR85571, a structurally-related kappa-agonist that is centrally-penetrating. 5. GR94839 inhibited the 2nd phase of the rat formalin response at doses 7 fold lower than those required to inhibit the 1st phase (ED50 vs 1st phase: 10.2 (6.7-17.1) mg kg-1, s.c.; ED50 vs 2nd phase: 1.4 (1.0-1.8) mg kg-1, s.c.; n = 18). GR103545 was equipotent against the two phases. 6. Intraplantar administration of the opioid antagonists, norbinaltorphimine (100 micrograms) or naltrexone (1 microgram), reversed the antinociceptive effect of systemic GR94839 (3 mg kg-1, s.c.) against the 2nd phase of the formalin response and intraplantar injection of GR94839 (30-100 micrograms) selectively inhibited the 2nd phase.7. GR94839 and IC1204448 reversed the hyperalgesia in the zymosan-inflamed rat paw at doses (ED50 GR94839: 2.0 (1.1-3.2) mg kg-', s.c.; ED50 IC1204448: 1.2 (0.8-1.7) mg kg-', s.c.), lower than those required to raise the noxious pressure threshold in the non-inflamed paw (EDSO GR94839: 16.4 (8.6-46.7) mg kg', s.c.; ED50 IC1204448: 68.0 (22.1-32000) mg kg', s.c.). GR103545 raised the noxious presure threshold in the inflamed and non-inflamed paws at the same doses.8. GR94839 was sedative in the rat rotarod test (ED50: 35 (12-245) mg kg-', s.c.) at doses higher than those required to inhibit the 2nd phase of the formalin response or reverse hyperalgesia in the zymosan-inflamed rat paw. The doses were comparable to those that inhibited the 1st phase of the formalin response and raised the noxious pressure threshold in the non-inflamed paw.9. The results suggest that GR94839 is a selective kappa-agonist which has antinociceptive activity against inflammatory pain at doses that produce limited central effects. These antinociceptive effects are probably mediated at peripheral opioid receptors.
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Affiliation(s)
- H Rogers
- Department of Neuropharmacology, Glaxo Group Research Ltd., Ware, Herts
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29
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Abstract
Metastasis to the skin occurs rarely, regardless of the nature of the primary systemic neoplasm. Although carcinoma of the cervix is the fourth most common malignancy in women, cutaneous involvement originating from cervical cancer is particularly unusual, even in the terminal stages of disease. Only 22 cases, including this one, are clearly documented in the literature. The main sites of the cutaneous metastases in these cases were the abdominal wall or lower extremity. However, we describe a 41-year-old woman with cervical cancer who developed metastatic nodules on the upper back. The skin of the back is an uncommon location for metastasis from any malignant tumor, and when it occurs in women, it is generally associated with carcinoma of the breast or malignant melanoma. To the best of our knowledge, this is the first reported case of cervical carcinoma metastasis to this unlikely cutaneous site.
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Affiliation(s)
- A G Hayes
- Department of Pathology, University of Tennessee, Memphis 38146
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30
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Birch PJ, Harrison SM, Hayes AG, Rogers H, Tyers MB. The non-peptide NK1 receptor antagonist, (+/-)-CP-96,345, produces antinociceptive and anti-oedema effects in the rat. Br J Pharmacol 1992; 105:508-10. [PMID: 1320977 PMCID: PMC1908431 DOI: 10.1111/j.1476-5381.1992.tb09008.x] [Citation(s) in RCA: 99] [Impact Index Per Article: 3.1] [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: 12/26/2022] Open
Abstract
The non-peptide NK1 receptor antagonist, (+/-)-CP-96,345, has been evaluated for antinociceptive activity in two well-characterized inflammatory pain models in the rat. (+/-)-CP-96,345 abolished carrageenin-induced mechanical hyperalgesia, significantly reduced carrageenin-induced paw oedema and attenuated the second phase of the formalin response. The results suggest that NK1 receptor activation occurs during the induction of inflammatory pain states in the rat.
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Affiliation(s)
- P J Birch
- Department of Neuropharmacology, Glaxo Group Research Ltd., Ware, Herts
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31
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Judd DB, Brown DS, Lloyd JE, McElroy AB, Scopes DI, Birch PJ, Hayes AG, Sheehan MJ. Synthesis, antinociceptive activity, and opioid receptor profiles of substituted trans-3-(decahydro- and octahydro-4a-isoquinolinyl)phenols. J Med Chem 1992; 35:48-56. [PMID: 1310115 DOI: 10.1021/jm00079a005] [Citation(s) in RCA: 7] [Impact Index Per Article: 0.2] [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: 12/26/2022]
Abstract
A series of trans-3-(6- and 7-substituted-decahydro-4a-isoquinolinyl)phenols and trans-3-(octahydro-4a-isoquinolinyl)phenols have been synthesized as potential opioid analgesics. Using a combination of in vitro and in vivo test systems, the receptor profiles of selected compounds have been assessed and in some instances distinguish between mu- and kappa-receptor agonists. In general, introduction of a 6-exocyclic methylene group into the trans-3-(decahydro-4a-isoquinolinyl)phenol system enhanced both antinociceptive activity and kappa-opioid receptor selectivity. For each series, analogues bearing an N-cyclopropylmethyl substituent exhibited greater kappa-receptor selectivity while N-methyl derivatives showed greater mu-receptor selectivity. The 7-substituted compounds (3b) were significantly less potent antinociceptive agents than their 6-substituted counterparts (3a), the octahydroisoquinoline analogues exhibiting intermediate activity. The axial 8-methyl-6-exocyclic methylene isoquinoline (20) is the most potent compound in the mouse abdominal constriction assay (ED50 = 0.05 mg/kg sc), whereas the equatorial 8-methyl isomer (16) was significantly less potent (ED50 = 3.3 mg/kg sc).
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Affiliation(s)
- D B Judd
- Department of Medicinal Chemistry, Glaxo Group Research Ltd., Ware, Hertfordshire, United Kingdom
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32
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Birch PJ, Rogers H, Hayes AG, Hayward NJ, Tyers MB, Scopes DI, Naylor A, Judd DB. Neuroprotective actions of GR89696, a highly potent and selective kappa-opioid receptor agonist. Br J Pharmacol 1991; 103:1819-23. [PMID: 1657267 PMCID: PMC1907793 DOI: 10.1111/j.1476-5381.1991.tb09869.x] [Citation(s) in RCA: 79] [Impact Index Per Article: 2.4] [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: 12/28/2022] Open
Abstract
1. The effect of a novel, highly potent and selective kappa-opioid receptor agonist, GR89696, has been evaluated in two animal models of cerebral ischaemia: transient bilateral carotid artery occlusion in the Mongolian gerbil and permanent, unilateral middle cerebral artery occlusion in the mouse. 2. In the Mongolian gerbil model, administration of GR89696 (3 to 30 micrograms kg-1, s.c.), immediately before and at 4 h after insult, produced a dose-dependent reduction in the hippocampal CA1 neuronal cell loss resulting from a 7-min bilateral carotid occlusion. Similar effects were obtained with two other kappa-agonists, GR86014 (1 mgkg-1, s.c.) and GR91272 (1 mgkg-1, s.c.). The neuroprotective effect of GR89696 was completely blocked by prior administration of the opioid receptor antagonist, naltrexone, at 10 mgkg-1, s.c. Repeated post-treatment with GR89696 (100 micrograms kg-1, s.c.) or GR44821 (10 mgkg-1, s.c.) was also effective in protecting completely the hippocampal CA1 neurones from ischaemia-induced neurodegeneration. 3. In the permanent, unilateral middle cerebral artery occlusion model in the mouse, repeated administration of GR89696 at 300 micrograms kg-1, s.c. produced a 50% reduction in cerebrocortical infarct volume. In these experiments GR89696 was dosed 5 min, 4, 8, 12, 16, 20 and 24 h after occlusion on the first day and then three times daily for the next three days. GR89696 (300 micrograms kg-1) also produced a significant 35% reduction in infarct volume in this model when the initiation of dosing was delayed for 6 h after the insult. 4. The results indicate that the potent kappa-opioid receptor agonist, GR89696, is neuroprotective in both global and focal cerebral ischaemia models and suggest that, with this class of compound, there may be a considerable time window for pharmacological intervention.
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Affiliation(s)
- P J Birch
- Department of Neuropharmacology, Glaxo Group Research Ltd., Ware, Hertfordshire
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33
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Oakley NR, Hayes AG, Sheehan MJ. Effect of typical and atypical neuroleptics on the behavioural consequences of activation by muscimol of mesolimbic and nigro-striatal dopaminergic pathways in the rat. Psychopharmacology (Berl) 1991; 105:204-8. [PMID: 1686655 DOI: 10.1007/bf02244310] [Citation(s) in RCA: 24] [Impact Index Per Article: 0.7] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Journal Information] [Submit a Manuscript] [Subscribe] [Scholar Register] [Indexed: 12/28/2022]
Abstract
Direct injections of muscimol into the ventral tegmental area (VTA) or substantia nigra zona reticulata (SNR) have been used to selectively stimulate the mesolimbic and nigro-striatal dopamine pathways respectively. Such injections induced locomotor activity, rearing, sniffing and in some animals an intermittent grooming response. These responses were rapid in onset, dose-related and relatively short lasting (less than 40 min). Selective increases in dopamine turnover were seen in the nucleus accumbens and in the striatum following VTA and SNR injections of muscimol (100 ng) respectively. Haloperidol inhibited the behavioural consequences of VTA and SNR injections of muscimol with similar potency (ED50S 0.01-0.03 mg/kg IP), and fluphenazine did likewise (ED50S 0.05-0.16 mg/kg IP). However, thioridazine (ED50S VTA: 1.45-2.04 mg/kg IP, SNR 8.50-9.20 mg/kg IP) and in particular clozapine (ED50S VTA: 0.24-0.58 mg/kg IP, SNR: 6.10-9.70 mg/kg IP) were more potent at inhibiting the locomotor activity and sniffing responses due to VTA rather than SNR administered muscimol. Since dopamine D2 antagonists are believed to exert their anti-psychotic effects via an action on mesolimbic dopaminergic systems, and their ability to induce extrapyramidal side effects (EPS) is thought to be due to an action on nigro-striatal dopamine systems, these results suggest that the behavioural models described can be used to predict efficacy and side-effect liability of potential neuroleptic drugs.
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Affiliation(s)
- N R Oakley
- Neuropharmacology Department, Glaxo Group Research Ltd, Ware, Herts, UK
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34
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Hayes AG, Birch PJ, Hayward NJ, Sheehan MJ, Rogers H, Tyers MB, Judd DB, Scopes DI, Naylor A. A series of novel, highly potent and selective agonists for the kappa-opioid receptor. Br J Pharmacol 1990; 101:944-8. [PMID: 1964823 PMCID: PMC1917842 DOI: 10.1111/j.1476-5381.1990.tb14185.x] [Citation(s) in RCA: 32] [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: 12/29/2022] Open
Abstract
1. This paper describes the opioid receptor pharmacology and in vivo activity of several novel benzene-acetamidopiperidine and benzeneacetamidopiperazine analogues. 2. These compounds all showed potent, naloxone-reversible, full agonist activity in the field-stimulated rabbit vas deferens, indicating that they are kappa-opioid agonists; but showed very little activity in the rat or hamster vas deferens, indicating good selectivity with regard to mu- and delta-opioid receptors. 3. They were all potent antinociceptive agents, the most potent compound, GR 103545, having an ED50 value in the mouse abdominal constriction test of 0.25 micrograms kg-1 s.c. The compounds also produced sedation and diuresis, but had little effect on respiration rate or gastrointestinal motility. 4. It is concluded that the seven novel compounds described are all potent and selective agonists for the kappa-opioid receptor.
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Affiliation(s)
- A G Hayes
- Department of Neuropharmacology, Glaxo Group Research Ltd., Ware. Herts
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35
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Rogers H, Birch PJ, Hayes AG. Effects of hypoxia and hypoglycaemia on DC potentials recorded from the gerbil hippocampus in vitro. Naunyn Schmiedebergs Arch Pharmacol 1990; 342:547-53. [PMID: 2090952 DOI: 10.1007/bf00169044] [Citation(s) in RCA: 4] [Impact Index Per Article: 0.1] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 12/30/2022]
Abstract
The acute effects of hypoxia and/or hypoglycaemia on DC potentials recorded from CA1 pyramidal neurones of the gerbil hippocampal slice maintained in vitro were investigated. Depolarizing potential changes were recorded when the slice was superfused with the excitatory amino acid agonists: NMDA (N-methyl-D-aspartic acid; 3-30 microM), AMPA ((RS)alpha-amino-3-hydroxy-5-methyl-4-isoxazole-propionate; 1-30 microM), kainate (3-100 microM) and L-glutamate (1-10 mM). In response to a 20 min period of superfusion with an hypoxic artificial CSF solution at 30 degrees C, a transient depolarization occurred followed by a marked hyperpolarization. A further hyperpolarization occurred when superfusion of the slice with an oxygenated artificial CSF recommenced. Post-hypoxia, when the neurones had repolarized, the response to NMDA (10 microM) was less than the pre-hypoxic response. The extent of the depression of the NMDA response was found to depend on three variables: a) the duration of the period of hypoxia, b) the glucose concentration of the artificial CSF, and c) the temperature of the slice. As the duration of hypoxia was increased, the depression of the NMDA response was more marked. Reduction of the glucose concentration from 11 mM to 2 mM by partial substitution with sucrose (9 mM) made the tissues more sensitive to the effects of hypoxia, whereas reduction of the temperature from 30 degrees C to 20 degrees C made them less sensitive. The depression of the response to NMDA was observed over a range of concentrations of NMDA. The concentration response curve for AMPA was also flattened, however, the depolarizations in response to kainate or GABA were preserved.(ABSTRACT TRUNCATED AT 250 WORDS)
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Affiliation(s)
- H Rogers
- Department of Neuropharmacology, Glaxo Group Research, Ware, Herts., UK
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36
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Abstract
The present study was conducted to investigate the effects of various 5-hydroxytryptamine (5-HT) agonists and antagonists on motor behaviour in rats and marmosets. Various motor-based responses were assessed after central or peripheral administration of 5-HT agents to rats and marmosets. Drugs acting as agonists at the 5-HT1A receptor (8-OHDPAT, gepirone, BMY-7378, NAN-190, PAPP (LY165163) and flesinoxan) and 5-HT2/1C receptors (DOI) were found to reverse neuroleptic-induced catalepsy in the rat whereas 5-HT2/1C antagonists (mianserin, ritanserin and ICI-170,809) and the 5-HT1 antagonist ((+/-)pindolol) increased catalepsy. Agonists acting at 5-HT3 receptors (phenylbiguanide and 2-methyl-5-HT) had no effect on catalepsy. The putative 5-HT1A antagonist, (+/-) pindolol, attenuated the reversal of catalepsy by 8-OHDPAT. Although both 8-OHDPAT and BMY-7378 were tested, only the latter was found to reduce apomorphine-induced stereotypy. Bilateral or unilateral infusions of 8-OHDPAT, BMY-7378 or pindolol into the substantia nigra of non-lesioned rats had no effect on spontaneous locomotor or rotational activity, respectively. However, 8-OHDPAT and BMY-7378 were found to increase or decrease motor activity, after injection into the median or dorsal raphe nuclei, respectively. Finally, 8-OHDPAT and BMY-7378 were found to be inactive against MPTP-induced bradykinesia in the marmoset. It is concluded that both 5-HT1A and 5-HT2/1C receptors are involved in the anti-cataleptic effects of 5-HT agents. The 5-HT1A receptors are probably situated within the raphe, whereas the location of the 5-HT2/1C receptors remains undetermined.
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Affiliation(s)
- P J Elliott
- Department of Neuropharmacology, Glaxo Group Research Ltd, Ware, Herts, U.K
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Elliott PJ, Close SP, Walsh DM, Hayes AG, Marriott AS. Neuroleptic-induced catalepsy as a model of Parkinson's disease. I. Effect of dopaminergic agents. J Neural Transm Park Dis Dement Sect 1990; 2:79-89. [PMID: 1977409 DOI: 10.1007/bf02260896] [Citation(s) in RCA: 18] [Impact Index Per Article: 0.5] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 12/29/2022]
Abstract
Catalepsy was observed in the rat following intrastriatal injections of the dopamine antagonists sulpiride or fluphenazine and after subcutaneous administration of fluphenazine. The neuroleptic-induced catalepsy was reversed by the classical anti-parkinsonian agent L-DOPA and by agents that function through dopamine systems such as d- and methamphetamine and the direct D2 receptor agonist quinpirole. The D1 agonist SKF 38393, and the D1/D2 agonist apomorphine, were ineffective in this model. These results support limited use of the rat catalepsy model for the screening of potential anti-parkinsonian compounds and indicate that this procedure can provide valuable information concerning striatal dopamine function.
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Affiliation(s)
- P J Elliott
- Glaxo Group Research Ltd., Neuropharmacology Department, Ware, Hertfordshire, United Kingdom
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38
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Abstract
In the mouse vas deferens, naltrindole gave pKB values of 9.7, 8.3, and 7.5 at the delta-, mu-, and kappa-sites and in binding assays, pIC50 values of 9.6, 7.8 and 7.2 at the same sites. The affinity of naltrindole for the delta binding site was increased in the presence of sodium ions and 5'-guanylylimidophosphate. Naltrindole is, thus, a potent opioid antagonist with marked selectivity for the delta-opioid receptor.
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Affiliation(s)
- H Rogers
- Department of Neuropharmacology, Glaxo Group Research Ltd, Ware, Hertfordshire, UK
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39
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Abstract
A modified primate model of Parkinson's disease was developed to assess the effectiveness of various agents that act via dopamine, acetylcholine, serotonin or glutamate systems. Using a MPTP dosing regimen a reversible parkinsonian-like syndrome was produced in the marmoset. An obvious advantage of such a protocol is that it allows multiple drug studies to be undertaken in animals, without the need for prolonged anti-parkinsonian therapy to maintain their health. Results show that dopamine D2 agonists (bromocriptine, quinpirole, N,N-dipropyl,A,5,6-DTN, (+)3PPP and PHNO), anti-muscarinics (atropine, scopolamine and benztropine), in addition to L-DOPA and nomifensine, all reduced the bradykinesia induced by MPTP. The D1 agonist SKF-38393 and the partial dopamine agonist (-)3PPP were both ineffective. Finally, agents with potential therapeutic use in Parkinson's disease were also tested. However, a glutamate antagonist (MK801) and three serotonin antagonists (ritanserin, ketanserin and ICI 170,809) were all unable to alter the MPTP effects, at the doses used in our study.
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Affiliation(s)
- S P Close
- Department of Neuropharmacology, Glaxo Group Research Ltd., Ware, Hertfordshire, UK
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Birch PJ, Grossman CJ, Hayes AG. Antagonist profile of 6,7-dichloro-3-hydroxy-2-quinoxalinecarboxylate at excitatory amino acid receptors in the neonatal rat spinal cord. Eur J Pharmacol 1989; 163:127-31. [PMID: 2545458 DOI: 10.1016/0014-2999(89)90405-6] [Citation(s) in RCA: 17] [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: 01/01/2023]
Abstract
In the neonatal rat spinal cord, 6,7-dichloro-3-hydroxy-2- quinoxalinecarboxylate antagonised responses mediated at both N-methyl-D-aspartate (NMDA) and non-NMDA receptors. The antagonism of responses to NMDA was unsurmountable and mediated via an antagonist action at the allosterically-linked strychnine-insensitive glycine site. At non-NMDA receptors, 6,7-dichloro-3-hydroxy-2-quinoxalinecarboxylate appeared to act as a competitive antagonist at low concentrations and a non-competitive antagonist at higher concentrations. In contrast to published data, this antagonist did not distinguish between the responses mediated by DL-alpha-amino-3-hydroxy-5-methyl-4-isoxazole-propionate (AMPA) and kainate.
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Affiliation(s)
- P J Birch
- Department of Neuropharmacology, Glaxo Group Research Ltd., Ware, Herts., U.K
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Birch PJ, Grossman CJ, Hayes AG. 6,7-Dinitro-quinoxaline-2,3-dion and 6-nitro,7-cyano-quinoxaline-2,3-dion antagonise responses to NMDA in the rat spinal cord via an action at the strychnine-insensitive glycine receptor. Eur J Pharmacol 1988; 156:177-80. [PMID: 2905271 DOI: 10.1016/0014-2999(88)90163-x] [Citation(s) in RCA: 156] [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: 01/03/2023]
Abstract
6,7-Dinitro-quinoxaline-2,3-dion (DNQX) and 6-nitro,7-cyano-quinoxaline-2,3-dion (CNQX) produce an unsurmountable antagonism of responses to N-methyl-D-aspartate (NMDA) in the baby rat hemisected spinal cord. These effects of DNQX and CNQX can be prevented in a dose-dependent manner by co-superfusion with D-serine or glycine (in the presence of strychnine). The results suggest that the unsurmountable blockade of NMDA responses by DNQX and CNQX reflects an antagonist effect mediated at the allosterically linked strychnine-insensitive glycine receptor.
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Affiliation(s)
- P J Birch
- Department of Neuropharmacology, Glaxo Group Research Ltd., Ware, Hertfordshire, U.K
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42
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Abstract
The antagonism of the antinociceptive effects of various kappa-opioid agonists has been studied in the mouse abdominal constriction test. Naloxone produced a much smaller degree of antagonism of U50488H than it did of two other kappa-agonists, U69593 and tifluadom. The kappa-selective antagonist, norbinaltorphimine, also failed to shift the dose-response curve to U50488H in this test, despite producing considerable antagonism of the U50488H effect in the rotarod test and of U69593 in both experimental situations. These results are suggestive of a non-opioid component to the action of U50488H in the abdominal constriction test. At high concentrations, U50488H, but not U69593, also showed non-opioid effects in reducing contractile activity in the field-stimulated isolated guinea-pig ileum, as demonstrated by the profile of antagonism seen with beta-chlornaltrexamine and naloxone. These results suggest that U69593, rather than U50488H, may be the kappa-agonist of choice to use, particularly in in-vivo experiments.
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Affiliation(s)
- A G Hayes
- Department of Neuropharmacology, Glaxo Group Research Ltd., Ware, Hertfordshire, UK
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Abstract
Experiments were performed to test the hypothesis that the field-stimulated rat vas deferens preparation contains opioid receptors, other than of mu-type, which mediate part of the inhibitory effect of beta-endorphin. The Piebald Viral Glaxo strain of rats was used. The reported finding that delta-opioid receptors are present in Sprague-Dawley rat vas deferens, the effects of which are greatly enhanced in reduced calcium concentrations, could not be replicated in the rat strain used. Reducing the calcium concentration from 2.5 to 1.25 mM improved the response to opioid drugs: all full agonists were about 10 times more potent, the partial agonist normorphine became able to inhibit the twitch completely, and morphine (which behaves as a competitive antagonist in 2.5 mM Ca2+) appeared to behave as a partial agonist. The pA2 values for antagonism by naloxone in low calcium of the mu-selective peptide [D-Ala2,MePhe4,Gly(ol)5]enkephalin and other mu- or delta-selective agonists were consistent with an action at mu-receptors only. The value for beta-endorphin was slightly but significantly lower. A similar small discrepancy was found with two other competitive antagonists. The discrepancy remained in the presence of the peptidase inhibitors thiorphan, bestatin and bacitracin. Responses to both [D-Ala2,MePhe4,Gly(ol)5]enkephalin and beta-endorphin were attenuated by the irreversible antagonists beta-funaltrexamine and beta-chlornaltrexamine.(ABSTRACT TRUNCATED AT 250 WORDS)
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Affiliation(s)
- M J Sheehan
- Department of Neuropharmacology, Glaxo Group Research Ltd., Ware, Hertfordshire, U.K
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Abstract
Kynurenate produces an unsurmountable antagonism of the response to N-methyl-D-aspartate (NMDA) in the baby rat hemisected spinal cord. This effect is completely reversible and prevented by co-superfusion with D-serine or glycine in the presence of strychnine. In the presence of D-serine kynurenate acts as a weak competitive antagonist. The results suggest that one of the actions of kynurenate is to antagonise NMDA responses via an action at the strychnine-insensitive glycine receptor.
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Affiliation(s)
- P J Birch
- Department of Neuropharmacology, Glaxo Group Research, Ware, Herts., U.K
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Hayes AG, Birch PJ. Reversal by beta-funaltrexamine and 16-methyl cyprenorphine of the antinociceptive effects of opioid agonists in the mouse and guinea-pig. Neuropharmacology 1988; 27:813-6. [PMID: 3216959 DOI: 10.1016/0028-3908(88)90096-2] [Citation(s) in RCA: 6] [Impact Index Per Article: 0.2] [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: 01/04/2023]
Abstract
The present study compared the effects of two opioid antagonists, beta-funaltrexamine (beta-FNA) and 16-methyl cyprenorphine (RX8008M) on the antinociception produced by a range of opioid agonists in the abdominal constriction test in the mouse and the paw pressure test in the guinea-pig. Both antagonists produced large shifts in the dose-response curves to the mu-agonists, morphine and fentanyl, confirming their mu-antagonist activity. Neither antagonist produced any antagonism of the antinociceptive effects of the selective kappa-agonists U50488, U69593 and tifluadom, in the mouse. However, RX8008M produced small shifts in the dose-response curves to these agonists in the guinea-pig, which seems more likely to reflect mu-receptor activity of the agonists in the guinea-pig than lack of selectivity of the antagonists. Both beta-FNA and RX8008M produced some antagonism of bremazocine, ethyl-ketocyclazocine, proxorphan and butorphanol, indicating that these agonists have a prominent mu-receptor component to their antinociceptive actions.
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Affiliation(s)
- A G Hayes
- Department of Neuropharmacology, Glaxo Group Research Ltd, Ware, Hertfordshire, U.K
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Birch PJ, Grossman CJ, Hayes AG. Kynurenate and FG9041 have both competitive and non-competitive antagonist actions at excitatory amino acid receptors. Eur J Pharmacol 1988; 151:313-5. [PMID: 2901972 DOI: 10.1016/0014-2999(88)90814-x] [Citation(s) in RCA: 128] [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: 01/03/2023]
Abstract
The antagonist profile of kynurenate and FG9041 have been characterised in a modified preparation of the baby rat hemisected spinal cord. Both kynurenate and FG9041 were competitive antagonists of responses to kainate and AMPA, although neither antagonist was selective for kainate versus AMPA. In contrast, both antagonists produced an apparent unsurmountable antagonism of responses to NMDA, indicating a different mode of action at the NMDA receptor.
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Affiliation(s)
- P J Birch
- Department of Neuropharmacology, Glaxo Group Research Ltd., Ware, Herts., U.K
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47
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Abstract
The effect of the opioid antagonist, 16-methylcyprenorphine (RX8008M), on the antinociceptive action of the mu-selective agonist, morphine, and the kappa-selective agonist, U50488H, has been investigated in the mouse abdominal constriction test. RX8008M produced a dose-dependent antagonism of the antinociceptive effect of morphine, but did not antagonize the response to U50488H. RX8008M should prove a useful probe for the in-vivo characterization of the receptor selectivity of opioid drugs.
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Affiliation(s)
- P J Birch
- Department of Neuropharmacology, Glaxo Group Research Ltd., Ware, Herts, UK
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Abstract
A method of treatment of femoral shortening, which may follow medullary nailing of oblique or comminuted fractures of the shaft of the femur, is described. Three cases are reported in which this method was used. The method is simple and may be the only practical way of dealing with this difficult problem.
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Abstract
The pharmacological profile of the opioid antagonist norbinaltorphimine has been characterised in vitro and in vivo. In vitro, norbinaltorphimine reversibly antagonised the effects of kappa agonists with pA2 values of 10.2-10.4. Norbinaltorphimine was much less potent as an antagonist at mu and delta receptors, pA2 values were 7.4-7.6 and 7.6-7.8, respectively. In all cases Schild slopes were unity. In vivo, norbinaltorphimine was an effective antagonist only at high dose levels and was not very selective between mu and kappa. The results indicate that in vitro norbinaltorphimine is a potent selective kappa antagonist; however, this antagonist profile is not maintained in vivo.
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Affiliation(s)
- P J Birch
- Department of Neuropharmacology, Glaxo Group Research Ltd., Ware, Hertfordshire, U.K
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Hayes AG, Sheehan MJ, Tyers MB. Differential sensitivity of models of antinociception in the rat, mouse and guinea-pig to mu- and kappa-opioid receptor agonists. Br J Pharmacol 1987; 91:823-32. [PMID: 2822190 PMCID: PMC1853585 DOI: 10.1111/j.1476-5381.1987.tb11281.x] [Citation(s) in RCA: 81] [Impact Index Per Article: 2.2] [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: 01/02/2023] Open
Abstract
1 A range of opioid receptor agonists were tested for activity in five antinociceptive models: the acetylcholine-induced abdominal constriction, tail-flick and hot plate tests in the mouse and the paw pressure test in the rat and guinea-pig. 2 Agonists acting preferentially at the kappa-opioid receptor were significantly more potent in the guinea-pig than in the rat paw pressure test, whereas mu-receptor preferring agonists were equipotent in the two tests. The mouse abdominal constriction test was of equal sensitivity to the guinea-pig pressure test for both types of agonist. 3 The mouse tail-flick and hot plate tests were progressively less sensitive than the other three tests, particularly to kappa-receptor preferring agonists. 4 The efficacy of an agonist can also markedly affect its activity in antinociceptive tests. Thus, partial kappa-agonists were weak or inactive in the rat paw pressure test, and partial agonists at both mu- and kappa-opioid receptors were relatively weak in the tests in which heat was the noxious stimulus, particularly the mouse hot plate test. 5 The mouse abdominal constriction test is suggested as the most appropriate antinociceptive model for testing a broad range of opioid agonists, whilst the relative potency of a drug in the rat and guinea-pig paw pressure tests may indicate the degree to which it is selective for kappa-opioid receptors in vivo.
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Affiliation(s)
- A G Hayes
- Department of Neuropharmacology, Glaxo Group Research Ltd., Ware, Herts
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