ALPHABETICAL LISTING of THURSDAY EVENING POSTER LOCATIONS ** Poster Location Numbers Correspond to Numbers Shown on Boards

Total Page:16

File Type:pdf, Size:1020Kb

ALPHABETICAL LISTING of THURSDAY EVENING POSTER LOCATIONS ** Poster Location Numbers Correspond to Numbers Shown on Boards ALPHABETICAL LISTING OF THURSDAY EVENING POSTER LOCATIONS ** Poster location numbers correspond to numbers shown on boards. ** POSTER LOCATION AUTHORS TITLE/ABSTRACT NUMBER NUMBER Abe M. Yada T. Fujimura A. Okada T. Asteroid Itokawa Sample Curation and Distribution Ishibashi Y. Shirai K. Uesugi M. Karouji Y. for Initial Analyses and International AO held in the 70 Yakame S. Nakamura T. Noguchi T. Planetary Material Sample Curation Facility of Okazaki R. Mukai T. Fujimoto M. JAXA [#1708] Yoshikawa M. Kawaguchi J. Abedin M. N. Bradley A. T. Hibberd J. Planetary Surfaces and Atmosphere Refaat T. F. Ismail S. Sharma S. K. Characterization Using Combined Raman, 599 Misra A. K. Garcia C. S. Mau J. Fluorescence, and Lidar Instrument from Rovers and Sandford S. P. Landers [#1219] Abell P. A. Barbee B. W. Mink R. G. The Near-Earth Object Human Space Flight Adamo D. R. Alberding C. M. Mazanek D. D. Accessible Targets Study (NHATS) List of Near- 65 Johnson L. N. Yeomans D. K. Chodas P. W. Earth Asteroids: Identifying Potential Targets for Chamberlin A. B. Benner L. A. M. Future Exploration [#2842] Drake B. G. Friedensen V. P. Abou-Aly S. Mader M. M. McCullough E. Signficance of Science-Tactical Liaison Role in 286 Preston L. J. Moores J. Tornebene L. L. Mission Control for the Krash Lunar Analogue Osinski G. R. ILSR Team Sample Return Mission [#2310] Effects of Kapton Sample Cell Windows on the Achilles C. N. Ming D. W. Morris R. V. Detection Limit of Smectite: Implications for 511 Blake D. F. CheMin on the Mars Science Laboratory Mission [#2786] Micro-Raman Mapping of Mineral Phases in the 394 Acosta T. E. Scott E. R. D. Sharma S. K. Strongly Shocked Taiban Ordinary Chondrite [#2725] The Dissolution Rate of Whitlockite and Implications 419 Adcock C. T. Hausrath E. M. for the Habitability of Early Mars [#2446] Er and Yb Isotope Fractionation in Planetary 319 Albalat E. Telouk P. Albarede F. Material [#1129] Mars 2012: Opposition and Educational 529 Albin E. F. Opportunities at Fernbank Science Center [#2045] Toward Lower Organic Environments in Allton J. H. Allen C. C. Burkett P. J. 552 Astromaterial Sample Curation for Diverse Calaway M. J. Oehler D. Z. Collections [#2439] Al-Samir M. van Berk W. Kneissl T. A Model Scenario for Kieserite-Dominated 310 van Gasselt S. Gross C. Wendt L. Jaumann R. Evaporites in Juventae Chasma, Mars [#2453] Alwmark C. Holm S. Meier M. M. M. A Study of Shocked Quartz in Distal Ries Ejecta from 133 Hofmann B. A. Eastern Switzerland [#1827] Presolar Graphite from the Murchison Meteorite: 332 Amari S. Zinner E. Gallino R. Puzzles Related to Its Origins [#1031] Amini R. B. Beegle L. Castillo-Rogez J. C. Electric Propulsion Induced Secondary Mass 636 Giapis K. Snyder J. S. Spectroscopy (EPI-SMS) [#2781] Portable Geochronology with LDRIMS: Learning to Anderson F. S. Nowicki K. Hamilton V. 614 Date Meteorites like Zagami with the Boulder Creek Whitaker T. J. Granite [#2844] Correlations Between Multispectral Imaging and Compositional Data from the Mars Exploration 495 Anderson R. B. Bell J. F. III Rovers and Implications for Mars Science Laboratory (MSL) Data Analysis [#2284] Enabling New Exploration Opportunities on 592 Anderson R. C. Nesnas I. A. Planetary Surfaces [#2907] Andrews D. J. Morse A. D. Barber S. J. Ptolemy: Operations at 21 Lutetia as part of the 53 Leese M. R. Morgan G. H. Sheridan S. Rosetta Mission and Future Implications [#2113] Wright I. P. Pillinger C. T. POSTER LOCATION AUTHORS TITLE/ABSTRACT NUMBER NUMBER Delayed Activation of Martian Core Dynamo 321 Arkani-Hamed J. [#1563] Elucidating the Formation of Archean-Proterozoic 136 Artemieva N. Simonson B. M. Boundary Spherule Layers [#1372] Artemieva N. Wuennemann K. Stoeffler D. Ries Suevite — Plume Ejecta, Melt Flow or 130 Reimold W. U. Something Else? [#1364] Thermal Emission Spectroscopy of Unpowdered 140 Ashley J. W. Christensen P. R. Meteorites [#2519] Impact Crater Morphologies as Indicators of 446 Atkins C. M. Barlow N. G. Volatiles in Northeastern Arabia Terra, Mars [#2122] Mars Curriculum for K–12 Science Education, 2nd Aubele J. C. Stanley J. Grochowski A. 528 Edition, Making Tracks on Mars Teacher Resource Jones K. Aragon J. and Activity Guide [#1266] Baecker B. Cordier C. Folco F. Trieloff M. Noble Gas Inventory of Micrometeorites from the 362 Cartwright J. A. Ott U. Transantarctic Mountains [#1824] Bailen M. S. Hare T. M. Akins S. W. Astropedia — A Data Portal for Planetary Science 249 Isbell C. [#2478] Karst Landforms in Northern Sinus Meridiani, Mars 519 Baioni D. Sgavetti M. Wezel F. C. [#1052] Trace Elements Reveal Complex Histories in 31 Balta J. B. Beck A. W. McSween H. Y. Jr. Diogenites [#1189] Evaluating Dune Delineation on Images from Mars 484 Bandeira L. Saraiva J. Pina P. Marques J. S. [#1988] Banerdt W. B. Smrekar S. Alkalai L. Hoffman T. Warwick R. Hurst K. Folkner W. Lognonné P. Spohn T. Asmar S. Banfield D. Boschi L. Christensen U. Dehant V. InSight: An Integrated Exploration of the Interior of 541 Giardini D. Goetz W. Golombek M. Grott M. Mars [#2838] Hudson T. Johnson C. Kargl G. Kobayashi N. Maki J. Mimoun D. Mocquet A. Morgan P. Panning M. Pike W. T. Tromp J. van Zoest T. Weber R. Wieczorek M. InSight Team The Long-Term Effects of Surface Frosts, Seasonal Atmospheric Water Variation and Ice Fraction- 450 Bapst J. Wood S. E. Dependent Thermal Conductivity on Martian Ground Ice [#2808] Ozone Production by Colliding Dust in the Martian 540 Baragiola R. A. Dukes C. A. Atmosphere [#2471] Modeling Electric Field Generation in Martian Dust 539 Barth E. L. Farrell W. M. Rafkin S. C. R. Devils [#2794] Barucci M. A. Michel P. Cheng A. MarcoPolo-R: Near Earth Asteroid Sample Return Böhnhardt H. Brucato J. R. Dotto E. 581 Mission Selected for ESA Assessment Study Phase Ehrenfreund P. Franchi I. A. Green S. F. [#1457] Lara L. -M. Marty B. Koschny D. Lunar Effects on Close Encounters of Near Earth 66 Bazso A. Asteroids [#1809] Debris-Covered Glacier Deposits in a Trio of Impact Craters in the Southern Mid-Latitudes of Mars: 438 Beach M. J. Head J. W. III Evidence for Ice Accumulation and Intercrater Flow in Connected Concentric Crater Fill [#1140] Becker K. J. Anderson J. A. Barrett J. M. 4 ISIS Support for Dawn Instruments [#2892] Sides S. C. Titus T. N. Trace Elements Reveal a Possible Link Between Jack 158 Bell E. A. Harrison T. M. Hills Detrital Zircons and the Late Heavy Bombardment [#2736] POSTER LOCATION AUTHORS TITLE/ABSTRACT NUMBER NUMBER Mastcam Multispectral Imaging on the Mars Science Bell J. F. III Malin M. C. Caplinger M. A. Laboratory Rover: Wavelength Coverage and 496 Ravine M. A. Godber A. S. Jungers M. C. Imaging Strategies at the Gale Crater Field Site Rice M. S. Anderson R. B. [#2541] Detection of a Radar Signature of the Uprange 131 Bell S. B. Schultz P. H. Plume in Fresh Oblique Lunar Craters [#2824] Benfield M. P. J. Hakkila J. Blevins E. R. Cronus and Oceanus — Two Undergraduate Titan 590 Turner M. W. Farrington P. A. Runyon C. J. Lake Lander Mission Concepts [#1660] Bennett K. A. Bell J. F. III McConnochie T. H. Extending CRISM Spectral Coverage in Gale Crater 497 Wolff M. J. Using THEMIS-VIS and HiRISE [#2761] Berard G. Applin D. Stromberg J. Sharma R. A Hypersaline Spring Analogue in Manitoba, Mann P. Grasby S. Bezys R. Horgan B. 311 Canada for Potential Ancient Spring Deposits on Londry K. Rice M. Last B. Last F. Mars [#1513] Badiou P. Goldsborough G. Bell J. F. III Bérczi Sz. Nagy Sz. Gyollai I. Józsa S. EBSD Studies of Ringwoodite Microcrystalline 391 Havancsák K. Dankházi Z. Varga G. Fabrics in the Shocked NWA 5011 L6 Chondritic Ratter K. Pál-Molnár E. Fintor K. Gucsik A. Meteorite [#1332] Testing of a Polar Nephelometer for Use in the Berlanga G. Richard D. T. Marshall J. 240 Creation of a Dust Database Supporting Lunar Davis S. Science Applications [#2464] Investigations of Transverse Aeolian Ridges on Mars 475 Berman D. C. Balme M. R. [#1598] Constraints on the Formation and Modification of 445 Berman D. C. Crown D. A. Joseph E. C. S. Lobate Debris Aprons Through Categorized Crater Counts [#1593] 580 Bernal J. A. Wegel D. C. Nuth J. A. III Harpoon-Based Sample Acquisition System [#1182] Possible Glacio-Fluvial Landforms in Southern Bernhardt H. Hiesinger H. Reiss D. 440 Argyre Planitia, Mars: Implications for Glacier Ivanov M. Erkeling G. Thickness and Depositional Settings [#1830] HiRISE Photoclinometry of Final MSL Landing Sites 499 Beyer R. A. Kirk R. L. [#2694] Study of Hydrous Sulfates from the Deccan Volcanic Bhattacharya S. Jain N. Parthasarathy G. 270 Province (DVP) of Kutch, India: Implications for Chauhan P. Ajai Aqueous Alteration Processes on Mars [#1468] Lunar Regolith Activity Inferred from Cosmogenic Binnie S. A. Nishiizumi K. Welten K. W. 227 Radionuclides 26Al and 36Cl in Core 60014/60013 Caffee M. W. [#1900] Lithified Aeolian Bedforms as Evidence for Ancient Birnie C. Fueten F. Stesky R. Cheel R. 518 Water Circulation in West Candor Chasma, Mars Rossi A. P. [#1292] New Microscopic Laser-Coupled Spectroscopy Blacksberg J. Maruyama Y. Choukroun M. Instrument Combining Raman, Libs, and 602 Charbon E. Rossman G. R. Fluorescence for Planetary Surface Mineralogy [#1510] Testing the Gefion Family as a Possible Parent Body 56 Blagen J. R. Gaffey M. J. Fieber-Beyer S. K. for the L-Chondrite Meteorites [#1643] Significance of Mission Control Science Blain S. Mader M. M. Tornabene L. L. 287 Documentarian in the KRASH Lunar Analogue Osinski G. R. ILSR team Mission [#2079] Blanchette-Guertin J.-F.
Recommended publications
  • Copyrighted Material
    Index Abulfeda crater chain (Moon), 97 Aphrodite Terra (Venus), 142, 143, 144, 145, 146 Acheron Fossae (Mars), 165 Apohele asteroids, 353–354 Achilles asteroids, 351 Apollinaris Patera (Mars), 168 achondrite meteorites, 360 Apollo asteroids, 346, 353, 354, 361, 371 Acidalia Planitia (Mars), 164 Apollo program, 86, 96, 97, 101, 102, 108–109, 110, 361 Adams, John Couch, 298 Apollo 8, 96 Adonis, 371 Apollo 11, 94, 110 Adrastea, 238, 241 Apollo 12, 96, 110 Aegaeon, 263 Apollo 14, 93, 110 Africa, 63, 73, 143 Apollo 15, 100, 103, 104, 110 Akatsuki spacecraft (see Venus Climate Orbiter) Apollo 16, 59, 96, 102, 103, 110 Akna Montes (Venus), 142 Apollo 17, 95, 99, 100, 102, 103, 110 Alabama, 62 Apollodorus crater (Mercury), 127 Alba Patera (Mars), 167 Apollo Lunar Surface Experiments Package (ALSEP), 110 Aldrin, Edwin (Buzz), 94 Apophis, 354, 355 Alexandria, 69 Appalachian mountains (Earth), 74, 270 Alfvén, Hannes, 35 Aqua, 56 Alfvén waves, 35–36, 43, 49 Arabia Terra (Mars), 177, 191, 200 Algeria, 358 arachnoids (see Venus) ALH 84001, 201, 204–205 Archimedes crater (Moon), 93, 106 Allan Hills, 109, 201 Arctic, 62, 67, 84, 186, 229 Allende meteorite, 359, 360 Arden Corona (Miranda), 291 Allen Telescope Array, 409 Arecibo Observatory, 114, 144, 341, 379, 380, 408, 409 Alpha Regio (Venus), 144, 148, 149 Ares Vallis (Mars), 179, 180, 199 Alphonsus crater (Moon), 99, 102 Argentina, 408 Alps (Moon), 93 Argyre Basin (Mars), 161, 162, 163, 166, 186 Amalthea, 236–237, 238, 239, 241 Ariadaeus Rille (Moon), 100, 102 Amazonis Planitia (Mars), 161 COPYRIGHTED
    [Show full text]
  • Annual Report COOPERATIVE INSTITUTE for RESEARCH in ENVIRONMENTAL SCIENCES
    2015 Annual Report COOPERATIVE INSTITUTE FOR RESEARCH IN ENVIRONMENTAL SCIENCES COOPERATIVE INSTITUTE FOR RESEARCH IN ENVIRONMENTAL SCIENCES 2015 annual report University of Colorado Boulder UCB 216 Boulder, CO 80309-0216 COOPERATIVE INSTITUTE FOR RESEARCH IN ENVIRONMENTAL SCIENCES University of Colorado Boulder 216 UCB Boulder, CO 80309-0216 303-492-1143 [email protected] http://cires.colorado.edu CIRES Director Waleed Abdalati Annual Report Staff Katy Human, Director of Communications, Editor Susan Lynds and Karin Vergoth, Editing Robin L. Strelow, Designer Agreement No. NA12OAR4320137 Cover photo: Mt. Cook in the Southern Alps, West Coast of New Zealand’s South Island Birgit Hassler, CIRES/NOAA table of contents Executive summary & research highlights 2 project reports 82 From the Director 2 Air Quality in a Changing Climate 83 CIRES: Science in Service to Society 3 Climate Forcing, Feedbacks, and Analysis 86 This is CIRES 6 Earth System Dynamics, Variability, and Change 94 Organization 7 Management and Exploitation of Geophysical Data 105 Council of Fellows 8 Regional Sciences and Applications 115 Governance 9 Scientific Outreach and Education 117 Finance 10 Space Weather Understanding and Prediction 120 Active NOAA Awards 11 Stratospheric Processes and Trends 124 Systems and Prediction Models Development 129 People & Programs 14 CIRES Starts with People 14 Appendices 136 Fellows 15 Table of Contents 136 CIRES Centers 50 Publications by the Numbers 136 Center for Limnology 50 Publications 137 Center for Science and Technology
    [Show full text]
  • Interpretations of Gravity Anomalies at Olympus Mons, Mars: Intrusions, Impact Basins, and Troughs
    Lunar and Planetary Science XXXIII (2002) 2024.pdf INTERPRETATIONS OF GRAVITY ANOMALIES AT OLYMPUS MONS, MARS: INTRUSIONS, IMPACT BASINS, AND TROUGHS. P. J. McGovern, Lunar and Planetary Institute, Houston TX 77058-1113, USA, ([email protected]). Summary. New high-resolution gravity and topography We model the response of the lithosphere to topographic loads data from the Mars Global Surveyor (MGS) mission allow a re- via a thin spherical-shell flexure formulation [9, 12], obtain- ¡g examination of compensation and subsurface structure models ing a model Bouguer gravity anomaly ( bÑ ). The resid- ¡g ¡g ¡g bÓ bÑ in the vicinity of Olympus Mons. ual Bouguer anomaly bÖ (equal to - ) can be Introduction. Olympus Mons is a shield volcano of enor- mapped to topographic relief on a subsurface density interface, using a downward-continuation filter [11]. To account for the mous height (> 20 km) and lateral extent (600-800 km), lo- cated northwest of the Tharsis rise. A scarp with height up presence of a buried basin, we expand the topography of a hole Ö h h ¼ ¼ to 10 km defines the base of the edifice. Lobes of material with radius and depth into spherical harmonics iÐÑ up h with blocky to lineated morphology surround the edifice [1-2]. to degree and order 60. We treat iÐÑ as the initial surface re- Such deposits, known as the Olympus Mons aureole deposits lief, which is compensated by initial relief on the crust mantle =´ µh c Ñ c (hereinafter abbreviated as OMAD), are of greatest extent to boundary of magnitude iÐÑ . These interfaces the north and west of the edifice.
    [Show full text]
  • No. 40. the System of Lunar Craters, Quadrant Ii Alice P
    NO. 40. THE SYSTEM OF LUNAR CRATERS, QUADRANT II by D. W. G. ARTHUR, ALICE P. AGNIERAY, RUTH A. HORVATH ,tl l C.A. WOOD AND C. R. CHAPMAN \_9 (_ /_) March 14, 1964 ABSTRACT The designation, diameter, position, central-peak information, and state of completeness arc listed for each discernible crater in the second lunar quadrant with a diameter exceeding 3.5 km. The catalog contains more than 2,000 items and is illustrated by a map in 11 sections. his Communication is the second part of The However, since we also have suppressed many Greek System of Lunar Craters, which is a catalog in letters used by these authorities, there was need for four parts of all craters recognizable with reasonable some care in the incorporation of new letters to certainty on photographs and having diameters avoid confusion. Accordingly, the Greek letters greater than 3.5 kilometers. Thus it is a continua- added by us are always different from those that tion of Comm. LPL No. 30 of September 1963. The have been suppressed. Observers who wish may use format is the same except for some minor changes the omitted symbols of Blagg and Miiller without to improve clarity and legibility. The information in fear of ambiguity. the text of Comm. LPL No. 30 therefore applies to The photographic coverage of the second quad- this Communication also. rant is by no means uniform in quality, and certain Some of the minor changes mentioned above phases are not well represented. Thus for small cra- have been introduced because of the particular ters in certain longitudes there are no good determi- nature of the second lunar quadrant, most of which nations of the diameters, and our values are little is covered by the dark areas Mare Imbrium and better than rough estimates.
    [Show full text]
  • Imagining Outer Space Also by Alexander C
    Imagining Outer Space Also by Alexander C. T. Geppert FLEETING CITIES Imperial Expositions in Fin-de-Siècle Europe Co-Edited EUROPEAN EGO-HISTORIES Historiography and the Self, 1970–2000 ORTE DES OKKULTEN ESPOSIZIONI IN EUROPA TRA OTTO E NOVECENTO Spazi, organizzazione, rappresentazioni ORTSGESPRÄCHE Raum und Kommunikation im 19. und 20. Jahrhundert NEW DANGEROUS LIAISONS Discourses on Europe and Love in the Twentieth Century WUNDER Poetik und Politik des Staunens im 20. Jahrhundert Imagining Outer Space European Astroculture in the Twentieth Century Edited by Alexander C. T. Geppert Emmy Noether Research Group Director Freie Universität Berlin Editorial matter, selection and introduction © Alexander C. T. Geppert 2012 Chapter 6 (by Michael J. Neufeld) © the Smithsonian Institution 2012 All remaining chapters © their respective authors 2012 All rights reserved. No reproduction, copy or transmission of this publication may be made without written permission. No portion of this publication may be reproduced, copied or transmitted save with written permission or in accordance with the provisions of the Copyright, Designs and Patents Act 1988, or under the terms of any licence permitting limited copying issued by the Copyright Licensing Agency, Saffron House, 6–10 Kirby Street, London EC1N 8TS. Any person who does any unauthorized act in relation to this publication may be liable to criminal prosecution and civil claims for damages. The authors have asserted their rights to be identified as the authors of this work in accordance with the Copyright, Designs and Patents Act 1988. First published 2012 by PALGRAVE MACMILLAN Palgrave Macmillan in the UK is an imprint of Macmillan Publishers Limited, registered in England, company number 785998, of Houndmills, Basingstoke, Hampshire RG21 6XS.
    [Show full text]
  • Martian Crater Morphology
    ANALYSIS OF THE DEPTH-DIAMETER RELATIONSHIP OF MARTIAN CRATERS A Capstone Experience Thesis Presented by Jared Howenstine Completion Date: May 2006 Approved By: Professor M. Darby Dyar, Astronomy Professor Christopher Condit, Geology Professor Judith Young, Astronomy Abstract Title: Analysis of the Depth-Diameter Relationship of Martian Craters Author: Jared Howenstine, Astronomy Approved By: Judith Young, Astronomy Approved By: M. Darby Dyar, Astronomy Approved By: Christopher Condit, Geology CE Type: Departmental Honors Project Using a gridded version of maritan topography with the computer program Gridview, this project studied the depth-diameter relationship of martian impact craters. The work encompasses 361 profiles of impacts with diameters larger than 15 kilometers and is a continuation of work that was started at the Lunar and Planetary Institute in Houston, Texas under the guidance of Dr. Walter S. Keifer. Using the most ‘pristine,’ or deepest craters in the data a depth-diameter relationship was determined: d = 0.610D 0.327 , where d is the depth of the crater and D is the diameter of the crater, both in kilometers. This relationship can then be used to estimate the theoretical depth of any impact radius, and therefore can be used to estimate the pristine shape of the crater. With a depth-diameter ratio for a particular crater, the measured depth can then be compared to this theoretical value and an estimate of the amount of material within the crater, or fill, can then be calculated. The data includes 140 named impact craters, 3 basins, and 218 other impacts. The named data encompasses all named impact structures of greater than 100 kilometers in diameter.
    [Show full text]
  • Special Catalogue Milestones of Lunar Mapping and Photography Four Centuries of Selenography on the Occasion of the 50Th Anniversary of Apollo 11 Moon Landing
    Special Catalogue Milestones of Lunar Mapping and Photography Four Centuries of Selenography On the occasion of the 50th anniversary of Apollo 11 moon landing Please note: A specific item in this catalogue may be sold or is on hold if the provided link to our online inventory (by clicking on the blue-highlighted author name) doesn't work! Milestones of Science Books phone +49 (0) 177 – 2 41 0006 www.milestone-books.de [email protected] Member of ILAB and VDA Catalogue 07-2019 Copyright © 2019 Milestones of Science Books. All rights reserved Page 2 of 71 Authors in Chronological Order Author Year No. Author Year No. BIRT, William 1869 7 SCHEINER, Christoph 1614 72 PROCTOR, Richard 1873 66 WILKINS, John 1640 87 NASMYTH, James 1874 58, 59, 60, 61 SCHYRLEUS DE RHEITA, Anton 1645 77 NEISON, Edmund 1876 62, 63 HEVELIUS, Johannes 1647 29 LOHRMANN, Wilhelm 1878 42, 43, 44 RICCIOLI, Giambattista 1651 67 SCHMIDT, Johann 1878 75 GALILEI, Galileo 1653 22 WEINEK, Ladislaus 1885 84 KIRCHER, Athanasius 1660 31 PRINZ, Wilhelm 1894 65 CHERUBIN D'ORLEANS, Capuchin 1671 8 ELGER, Thomas Gwyn 1895 15 EIMMART, Georg Christoph 1696 14 FAUTH, Philipp 1895 17 KEILL, John 1718 30 KRIEGER, Johann 1898 33 BIANCHINI, Francesco 1728 6 LOEWY, Maurice 1899 39, 40 DOPPELMAYR, Johann Gabriel 1730 11 FRANZ, Julius Heinrich 1901 21 MAUPERTUIS, Pierre Louis 1741 50 PICKERING, William 1904 64 WOLFF, Christian von 1747 88 FAUTH, Philipp 1907 18 CLAIRAUT, Alexis-Claude 1765 9 GOODACRE, Walter 1910 23 MAYER, Johann Tobias 1770 51 KRIEGER, Johann 1912 34 SAVOY, Gaspare 1770 71 LE MORVAN, Charles 1914 37 EULER, Leonhard 1772 16 WEGENER, Alfred 1921 83 MAYER, Johann Tobias 1775 52 GOODACRE, Walter 1931 24 SCHRÖTER, Johann Hieronymus 1791 76 FAUTH, Philipp 1932 19 GRUITHUISEN, Franz von Paula 1825 25 WILKINS, Hugh Percy 1937 86 LOHRMANN, Wilhelm Gotthelf 1824 41 USSR ACADEMY 1959 1 BEER, Wilhelm 1834 4 ARTHUR, David 1960 3 BEER, Wilhelm 1837 5 HACKMAN, Robert 1960 27 MÄDLER, Johann Heinrich 1837 49 KUIPER Gerard P.
    [Show full text]
  • Worry Over Mistreating Clots Drove Push to Pause J&J Shot
    P2JW109000-6-A00100-17FFFF5178F ****** MONDAY,APRIL 19,2021~VOL. CCLXXVII NO.90 WSJ.com HHHH $4.00 Last week: DJIA 34200.67 À 400.07 1.2% NASDAQ 14052.34 À 1.1% STOXX 600 442.49 À 1.2% 10-YR. TREASURY À 27/32 , yield 1.571% OIL $63.13 À $3.81 EURO $1.1982 YEN 108.81 Bull Run What’s News In Stocks Widens, Business&Finance Signaling More stocks have been propelling the U.S. market higher lately,asignal that fur- Strength ther gains could be ahead, but howsmooth the climb might be remains up fordebate. A1 Technical indicators WeWork’s plan to list suggestmoregains, stock by merging with a but some question how blank-check company has echoes of its approach in smooth theywill be 2019,when the shared-office provider’s IPO imploded. A1 BY CAITLIN MCCABE Citigroup plans to scale up its services to wealthy GES Agreater number of stocks entrepreneurs and their IMA have been propelling the U.S. businesses in Asia as the market higher lately,asignal bank refocuses its opera- GETTY that—if historyisany indica- tions in the region. B1 SE/ tor—moregains could be ahead. What remains up forde- A Maryland hotel mag- bate, however, is how smooth natebehind an 11th-hour bid ANCE-PRES FR the climb will be. to acquireTribune Publish- Indicatorsthat point to a ing is working to find new ENCE stronger and moreresilient financing and partnership AG stock market have been hitting options after his partner ON/ LL rare milestones recently as the withdrew from the deal.
    [Show full text]
  • Volcanism on Mars
    Author's personal copy Chapter 41 Volcanism on Mars James R. Zimbelman Center for Earth and Planetary Studies, National Air and Space Museum, Smithsonian Institution, Washington, DC, USA William Brent Garry and Jacob Elvin Bleacher Sciences and Exploration Directorate, Code 600, NASA Goddard Space Flight Center, Greenbelt, MD, USA David A. Crown Planetary Science Institute, Tucson, AZ, USA Chapter Outline 1. Introduction 717 7. Volcanic Plains 724 2. Background 718 8. Medusae Fossae Formation 725 3. Large Central Volcanoes 720 9. Compositional Constraints 726 4. Paterae and Tholi 721 10. Volcanic History of Mars 727 5. Hellas Highland Volcanoes 722 11. Future Studies 728 6. Small Constructs 723 Further Reading 728 GLOSSARY shield volcano A broad volcanic construct consisting of a multitude of individual lava flows. Flank slopes are typically w5, or less AMAZONIAN The youngest geologic time period on Mars identi- than half as steep as the flanks on a typical composite volcano. fied through geologic mapping of superposition relations and the SNC meteorites A group of igneous meteorites that originated on areal density of impact craters. Mars, as indicated by a relatively young age for most of these caldera An irregular collapse feature formed over the evacuated meteorites, but most importantly because gases trapped within magma chamber within a volcano, which includes the potential glassy parts of the meteorite are identical to the atmosphere of for a significant role for explosive volcanism. Mars. The abbreviation is derived from the names of the three central volcano Edifice created by the emplacement of volcanic meteorites that define major subdivisions identified within the materials from a centralized source vent rather than from along a group: S, Shergotty; N, Nakhla; C, Chassigny.
    [Show full text]
  • March 21–25, 2016
    FORTY-SEVENTH LUNAR AND PLANETARY SCIENCE CONFERENCE PROGRAM OF TECHNICAL SESSIONS MARCH 21–25, 2016 The Woodlands Waterway Marriott Hotel and Convention Center The Woodlands, Texas INSTITUTIONAL SUPPORT Universities Space Research Association Lunar and Planetary Institute National Aeronautics and Space Administration CONFERENCE CO-CHAIRS Stephen Mackwell, Lunar and Planetary Institute Eileen Stansbery, NASA Johnson Space Center PROGRAM COMMITTEE CHAIRS David Draper, NASA Johnson Space Center Walter Kiefer, Lunar and Planetary Institute PROGRAM COMMITTEE P. Doug Archer, NASA Johnson Space Center Nicolas LeCorvec, Lunar and Planetary Institute Katherine Bermingham, University of Maryland Yo Matsubara, Smithsonian Institute Janice Bishop, SETI and NASA Ames Research Center Francis McCubbin, NASA Johnson Space Center Jeremy Boyce, University of California, Los Angeles Andrew Needham, Carnegie Institution of Washington Lisa Danielson, NASA Johnson Space Center Lan-Anh Nguyen, NASA Johnson Space Center Deepak Dhingra, University of Idaho Paul Niles, NASA Johnson Space Center Stephen Elardo, Carnegie Institution of Washington Dorothy Oehler, NASA Johnson Space Center Marc Fries, NASA Johnson Space Center D. Alex Patthoff, Jet Propulsion Laboratory Cyrena Goodrich, Lunar and Planetary Institute Elizabeth Rampe, Aerodyne Industries, Jacobs JETS at John Gruener, NASA Johnson Space Center NASA Johnson Space Center Justin Hagerty, U.S. Geological Survey Carol Raymond, Jet Propulsion Laboratory Lindsay Hays, Jet Propulsion Laboratory Paul Schenk,
    [Show full text]
  • The Alkaline Volcanic Rocks of Craters of the Moon National Monument, Idaho and the Columbia Hills of Gusev Crater, Mars Details
    The alkaline volcanic rocks of Craters of the Moon National Monument, Idaho and the Columbia Hills of Gusev Crater, Mars Details Meeting 2016 Fall Meeting Section Planetary Sciences Session Terrestrial Analogs for Planetary Processes: Oceans, Volcanoes, Impacts, and Dunes I Identifier P31E-01 Authors Haberle, C W*, Mars Space Flight Facility, Arizona State University, Tempe, AZ, United States Hughes, S S, Idaho State University, Idaho Falls, ID, United States Kobs-Nawotniak, S E, Department of Geosciences, Idaho State University, Idaho Falls, ID, United States Christensen, P R, Arizona State University, Tempe, AZ, United States Index Sediment transport [4558] Terms Atmospheres [5405] Titan [6281] Venus [6295] Abstract Idaho's Eastern Snake River Plain (ESRP) is host to extensive expressions of basaltic volcanism dominated by non evolved olivine tholeiites (NEOT) with localized occurrences of evolved lavas. Craters of the Moon National Monument (COTM) is a polygenetic lava field comprised of more than 60 lava flows emplaced during 8 eruptive periods spanning the last 15 kyrs. The most recent eruptive period (period A; 2500-2000 yr B.P.) produced flows with total alkali vs. silica classifications spanning basalt to trachyte. Coeval with the emplacement of the COTM period A volcanic pile was the emplacement of the Wapi and Kings Bowl NEOT 70 km SSE of COTM along the Great Rift. Previous investigations have determined a genetic link between these two compositionally distinct volcanic centers where COTM compositions can be generated from NEOT melts through complex ascent paths and variable degrees of fractionation and assimilation of lower-middle crustal materials. The Mars Exploration Rover, Spirit, conducted a robotic investigation of Gusev crater from 2004-2010.
    [Show full text]
  • Bio-Preservation Potential of Sediment in Eberswalde Crater, Mars
    Western Washington University Western CEDAR WWU Graduate School Collection WWU Graduate and Undergraduate Scholarship Fall 2020 Bio-preservation Potential of Sediment in Eberswalde crater, Mars Cory Hughes Western Washington University, [email protected] Follow this and additional works at: https://cedar.wwu.edu/wwuet Part of the Geology Commons Recommended Citation Hughes, Cory, "Bio-preservation Potential of Sediment in Eberswalde crater, Mars" (2020). WWU Graduate School Collection. 992. https://cedar.wwu.edu/wwuet/992 This Masters Thesis is brought to you for free and open access by the WWU Graduate and Undergraduate Scholarship at Western CEDAR. It has been accepted for inclusion in WWU Graduate School Collection by an authorized administrator of Western CEDAR. For more information, please contact [email protected]. Bio-preservation Potential of Sediment in Eberswalde crater, Mars By Cory M. Hughes Accepted in Partial Completion of the Requirements for the Degree Master of Science ADVISORY COMMITTEE Dr. Melissa Rice, Chair Dr. Charles Barnhart Dr. Brady Foreman Dr. Allison Pfeiffer GRADUATE SCHOOL David L. Patrick, Dean Master’s Thesis In presenting this thesis in partial fulfillment of the requirements for a master’s degree at Western Washington University, I grant to Western Washington University the non-exclusive royalty-free right to archive, reproduce, distribute, and display the thesis in any and all forms, including electronic format, via any digital library mechanisms maintained by WWU. I represent and warrant this is my original work, and does not infringe or violate any rights of others. I warrant that I have obtained written permissions from the owner of any third party copyrighted material included in these files.
    [Show full text]