A Possible Second Large Subglacial Impact Crater in Northwest Greenland
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Analogue Sites for Mars Missions: MSL and Beyond
Program and Abstract Volume LPI Contribution No. 1612 Analogue Sites for Mars Missions: MSL and Beyond March 5–6, 2011 • The Woodlands, Texas Sponsors National Aeronautics and Space Administration Lunar and Planetary Institute Conveners Mary Voytek, NASA Headquarters Michael Meyer, NASA Headquarters Victoria Hipkin, Canadian Space Agency Richard Leveille, Canadian Space Agency Shawn Domagal-Goldman, NASA Headquarters Lunar and Planetary Institute 3600 Bay Area Boulevard Houston TX 77058-1113 LPI Contribution No. 1612 Compiled in 2011 by Meeting and Publication Services Lunar and Planetary Institute USRA Houston 3600 Bay Area Boulevard, Houston TX 77058-1113 The Lunar and Planetary Institute is operated by the Universities Space Research Association under a cooperative agreement with the Science Mission Directorate of the National Aeronautics and Space Administration. Any opinions, findings, and conclusions or recommendations expressed in this volume are those of the author(s) and do not necessarily reflect the views of the National Aeronautics and Space Administration. Material in this volume may be copied without restraint for library, abstract service, education, or personal research purposes; however, republication of any paper or portion thereof requires the written permission of the authors as well as the appropriate acknowledgment of this publication. Abstracts in this volume may be cited as Author A. B. (2011) Title of abstract. In Analogue Sites for Mars Missions: MSL and Beyond, p. XX. LPI Contribution No. 1612, Lunar and Planetary Institute, Houston. ISSN No. 0161-5297 Preface This volume contains abstracts that have been accepted for presentation at the workshop on Analogue Sites for Mars Missions: MSL and Beyond, March 5–6, 2011, The Woodlands, Texas. -
Program and Abstracts of 2017 Congress / Programme Et Résumés
1 Sponsors | Commanditaires Gold Sponsors | Commanditaires d’or Silver Sponsors | Commanditaires d’argent Other Sponsors | Les autres Commanditaires 2 Contents Sponsors | Commanditaires .......................................................................................................................... 2 Welcome from the Premier of Ontario .......................................................................................................... 5 Bienvenue du premier ministre de l'Ontario .................................................................................................. 6 Welcome from the Mayor of Toronto ............................................................................................................ 7 Mot de bienvenue du maire de Toronto ........................................................................................................ 8 Welcome from the Minister of Fisheries, Oceans and the Canadian Coast Guard ...................................... 9 Mot de bienvenue de ministre des Pêches, des Océans et de la Garde côtière canadienne .................... 10 Welcome from the Minister of Environment and Climate Change .............................................................. 11 Mot de bienvenue du Ministre d’Environnement et Changement climatique Canada ................................ 12 Welcome from the President of the Canadian Meteorological and Oceanographic Society ...................... 13 Mot de bienvenue du président de la Société canadienne de météorologie et d’océanographie ............. -
Appendix I Lunar and Martian Nomenclature
APPENDIX I LUNAR AND MARTIAN NOMENCLATURE LUNAR AND MARTIAN NOMENCLATURE A large number of names of craters and other features on the Moon and Mars, were accepted by the IAU General Assemblies X (Moscow, 1958), XI (Berkeley, 1961), XII (Hamburg, 1964), XIV (Brighton, 1970), and XV (Sydney, 1973). The names were suggested by the appropriate IAU Commissions (16 and 17). In particular the Lunar names accepted at the XIVth and XVth General Assemblies were recommended by the 'Working Group on Lunar Nomenclature' under the Chairmanship of Dr D. H. Menzel. The Martian names were suggested by the 'Working Group on Martian Nomenclature' under the Chairmanship of Dr G. de Vaucouleurs. At the XVth General Assembly a new 'Working Group on Planetary System Nomenclature' was formed (Chairman: Dr P. M. Millman) comprising various Task Groups, one for each particular subject. For further references see: [AU Trans. X, 259-263, 1960; XIB, 236-238, 1962; Xlffi, 203-204, 1966; xnffi, 99-105, 1968; XIVB, 63, 129, 139, 1971; Space Sci. Rev. 12, 136-186, 1971. Because at the recent General Assemblies some small changes, or corrections, were made, the complete list of Lunar and Martian Topographic Features is published here. Table 1 Lunar Craters Abbe 58S,174E Balboa 19N,83W Abbot 6N,55E Baldet 54S, 151W Abel 34S,85E Balmer 20S,70E Abul Wafa 2N,ll7E Banachiewicz 5N,80E Adams 32S,69E Banting 26N,16E Aitken 17S,173E Barbier 248, 158E AI-Biruni 18N,93E Barnard 30S,86E Alden 24S, lllE Barringer 29S,151W Aldrin I.4N,22.1E Bartels 24N,90W Alekhin 68S,131W Becquerei -
Lunar Impact Basins Revealed by Gravity Recovery and Interior
Lunar impact basins revealed by Gravity Recovery and Interior Laboratory measurements Gregory Neumann, Maria Zuber, Mark Wieczorek, James Head, David Baker, Sean Solomon, David Smith, Frank Lemoine, Erwan Mazarico, Terence Sabaka, et al. To cite this version: Gregory Neumann, Maria Zuber, Mark Wieczorek, James Head, David Baker, et al.. Lunar im- pact basins revealed by Gravity Recovery and Interior Laboratory measurements. Science Advances , American Association for the Advancement of Science (AAAS), 2015, 1 (9), pp.e1500852. 10.1126/sci- adv.1500852. hal-02458613 HAL Id: hal-02458613 https://hal.archives-ouvertes.fr/hal-02458613 Submitted on 26 Jun 2020 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. RESEARCH ARTICLE PLANETARY SCIENCE 2015 © The Authors, some rights reserved; exclusive licensee American Association for the Advancement of Science. Distributed Lunar impact basins revealed by Gravity under a Creative Commons Attribution NonCommercial License 4.0 (CC BY-NC). Recovery and Interior Laboratory measurements 10.1126/sciadv.1500852 Gregory A. Neumann,1* Maria T. Zuber,2 Mark A. Wieczorek,3 James W. Head,4 David M. H. Baker,4 Sean C. Solomon,5,6 David E. Smith,2 Frank G. -
GRAIL Gravity Observations of the Transition from Complex Crater to Peak-Ring Basin on the Moon: Implications for Crustal Structure and Impact Basin Formation
Icarus 292 (2017) 54–73 Contents lists available at ScienceDirect Icarus journal homepage: www.elsevier.com/locate/icarus GRAIL gravity observations of the transition from complex crater to peak-ring basin on the Moon: Implications for crustal structure and impact basin formation ∗ David M.H. Baker a,b, , James W. Head a, Roger J. Phillips c, Gregory A. Neumann b, Carver J. Bierson d, David E. Smith e, Maria T. Zuber e a Department of Geological Sciences, Brown University, Providence, RI 02912, USA b NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA c Department of Earth and Planetary Sciences and McDonnell Center for the Space Sciences, Washington University, St. Louis, MO 63130, USA d Department of Earth and Planetary Sciences, University of California, Santa Cruz, CA 95064, USA e Department of Earth, Atmospheric and Planetary Sciences, MIT, Cambridge, MA 02139, USA a r t i c l e i n f o a b s t r a c t Article history: High-resolution gravity data from the Gravity Recovery and Interior Laboratory (GRAIL) mission provide Received 14 September 2016 the opportunity to analyze the detailed gravity and crustal structure of impact features in the morpho- Revised 1 March 2017 logical transition from complex craters to peak-ring basins on the Moon. We calculate average radial Accepted 21 March 2017 profiles of free-air anomalies and Bouguer anomalies for peak-ring basins, protobasins, and the largest Available online 22 March 2017 complex craters. Complex craters and protobasins have free-air anomalies that are positively correlated with surface topography, unlike the prominent lunar mascons (positive free-air anomalies in areas of low elevation) associated with large basins. -
The Interference of Tetrachloromethane
The interference of tetrachloromethane in the measurement of benzene in air by Gas Chromatography - Photoionisation Detector (GC-PID) Cristina Romero-Trigueros1, Esther González 2, Marta Doval Miñarro3, Enrique González Ferradás2 5 1Dipartimento di Scienze Agro-Ambientali e Territoriali, University of Bari Aldo Moro, Via Amendola, 165/A, 70126, Bari, Italy 2Chemical Engineering Department, School of Chemistry, University of Murcia, 30071, Murcia, Spain 3Chemical and Environmental Engineering Department, Technical University of Cartagena, Paseo Alfonso XIII, 52, 30203 Cartagena, Murcia, Spain 10 Correspondence to: Esther González ([email protected]) Abstract. The European Union requires that benzene in air is continuously measured due to its toxicity and widespread presence in the population nuclei, mainly motivated by vehicle emissions. The reference measuring technique is gas chromatography (GC). Automatic chromatographs used in monitoring stations must verify the operating conditions 15 established in Standard EN 14662 part 3, which includes a type approval section with a number of tests that analysers must pass. Among these tests, the potential interference of a number of compounds is evaluated. The 2005 version of the mentioned standard requires the evaluation of the potential interference of tetrachloromethane (TCM). The 2015 version eliminates TCM as a potential interferent. Although most consumer uses of TCM have been banned, recent studies have measured significant concentrations of TCM in air. In this paper, the potential interference -
Exobiology in the Solar System & the Search for Life on Mars
SP-1231 SP-1231 October 1999 Exobiology in the Solar System & The Search for Life on Mars for The Search Exobiology in the Solar System & Exobiology in the Solar System & The Search for Life on Mars Report from the ESA Exobiology Team Study 1997-1998 Contact: ESA Publications Division c/o ESTEC, PO Box 299, 2200 AG Noordwijk, The Netherlands Tel. (31) 71 565 3400 - Fax (31) 71 565 5433 SP-1231 October 1999 EXOBIOLOGY IN THE SOLAR SYSTEM AND THE SEARCH FOR LIFE ON MARS Report from the ESA Exobiology Team Study 1997-1998 Cover Fossil coccoid bacteria, 1 µm in diameter, found in sediment 3.3-3.5 Gyr old from the Early Archean of South Africa. See pages 160-161. Background: a portion of the meandering canyons of the Nanedi Valles system viewed by Mars Global Surveyor. The valley is about 2.5 km wide; the scene covers 9.8 km by 27.9 km centred on 5.1°N/48.26°W. The valley floor at top right exhibits a 200 m-wide channel covered by dunes and debris. This channel suggests that the valley might have been carved by water flowing through the system over a long period, in a manner similar to rivers on Earth. (Malin Space Science Systems/NASA) SP-1231 ‘Exobiology in the Solar System and The Search for Life on Mars’, ISBN 92-9092-520-5 Scientific Coordinators: André Brack, Brian Fitton and François Raulin Edited by: Andrew Wilson ESA Publications Division Published by: ESA Publications Division ESTEC, Noordwijk, The Netherlands Price: 70 Dutch Guilders/ EUR32 Copyright: © 1999 European Space Agency Contents Foreword 7 I An Exobiological View of the -
Earth and Space Science. a Guide for Secondary Teachers. INSTITUTION Pennsylvania State Dept
DOCUMENT RESUME ED 094 956 SE 016 611 AUTHOR Bolles, William H.; And Others TITLE Earth and Space Science. A Guide for Secondary Teachers. INSTITUTION Pennsylvania State Dept. of Education, Harrisburg. Bureau of Curriculum Services. PUB DATE 73 NOTE 200p. EDRS PRICE MF-$O.75 HC-$9.00 PLUS POSTAGE DESCRIPTORS Aerospace Education; *Astronomy; *Curriculum Guides; *Earth Science; Geology; Laboratory Experiments; Oceanology; Science Activities; Science Education; *Secondary School Science IDENTIFIERS Pennsylvania ABSTRACT Designed for use in Pennsylvania secondary school science classes, this guide is intended to provide fundamental information in each of the various disciplines of the earth sciences. Some of the material contained in the guide is intended as background material for teachers. Five units are presented: The Earth, The Oceans, The Space Environment, The Atmosphere, and The Exploration of Space. The course is organized so that students proceed from the familiar, everyday world to the atmosphere and the space environment. Teaching geology in the fall takes advantage of weather conditions which permit field study. The purpose of the Earth and Space Science course is to encourage student behaviors which will be indicative of a broad understanding of man1s physical environment of earth and space as well as an awareness of the consequences which could result from changes which man may effect.(PEB) BEST COPY AVAILABLE U S DEPARTMENT OF HEALTH. EDUCATION & WELFARE NATIONAL INSTITUTE OF 6 Fe elz+C EDUCATION Try,' DOCUMENT FIRSBEEN REPRO -
Non-Linear Flow Modelling of a Martian Lobate Debris Apron
Journal of Glaciology Non-linear flow modelling of a Martian Lobate Debris Apron Louise Steffensen Schmidt1 , Christine Schøtt Hvidberg2, Jung Rack Kim3 4,5 Paper and Nanna Bjørnholt Karlsson 1 2 Cite this article: Schmidt LS, Hvidberg CS, Department of Earth Sciences, University of Iceland, Reykjavik, Iceland; Centre for Ice and Climate, Niels Bohr Kim JR, Karlsson NB (2019). Non-linear flow Institute, University of Copenhagen, Denmark; 3University of Seoul, Seoul, South Korea; 4Alfred-Wegener-Institut modelling of a Martian Lobate Debris Apron. Helmholtz-Zentrum für Polar-und Meeresforschung, Bremerhaven, Germany and 5Geological Survey of Denmark Journal of Glaciology 65(254), 889–899. https:// and Greenland, Copenhagen, Denmark doi.org/10.1017/jog.2019.54 Received: 5 September 2018 Abstract Revised: 23 July 2019 The Martian mid-latitudes contain numerous small water-ice deposits, collectively termed vis- Accepted: 24 July 2019 First published online: 30 September 2019 cous flow features (VFFs). The shape and topography of the deposits contain information on their past flow history and formation process. In order to access this information, it is imperative Keywords: to get information on their deformational properties. Here we use a high-resolution digital top- Extraterrestrial glaciology; glacier flow; ography map and ice-penetrating radar data in combination with an inverse method to constrain glacier mass balance; glacier modelling; ice temperature the deformational properties of a lobate debris apron, a class of VFF, in the southern hemisphere of Mars. We find that while the creep parameter and accumulation rates are not well constrained Author for correspondence: in absolute values, their ratio is robust. -
A Review and Strategy for Exploration
ASTROBIOLOGY Volume 19, Number 10, 2019 Review Articles Mary Ann Liebert, Inc. DOI: 10.1089/ast.2018.1960 Paleo-Rock-Hosted Life on Earth and the Search on Mars: A Review and Strategy for Exploration T.C. Onstott,1,* B.L. Ehlmann,2,3,* H. Sapers,2,3,4 M. Coleman,3,5 M. Ivarsson,6 J.J. Marlow,7 A. Neubeck,8 and P. Niles9 Abstract Here we review published studies on the abundance and diversity of terrestrial rock-hosted life, the environments it inhabits, the evolution of its metabolisms, and its fossil biomarkers to provide guidance in the search for life on Mars. Key findings are (1) much terrestrial deep subsurface metabolic activity relies on abiotic energy-yielding fluxes and in situ abiotic and biotic recycling of metabolic waste products rather than on buried organic products of photosynthesis; (2) subsurface microbial cell concentrations are highest at interfaces with pronounced chemical redox gradients or permeability variations and do not correlate with bulk host rock organic carbon; (3) metabolic pathways for chemolithoautotrophic microorganisms evolved earlier in Earth’s history than those of surface-dwelling phototrophic microorganisms; (4) the emergence of the former occurred at a time when Mars was habitable, whereas the emergence of the latter occurred at a time when the martian surface was not continually habitable; (5) the terrestrial rock record has biomarkers of subsurface life at least back hundreds of millions of years and likely to 3.45 Ga with several examples of excellent preservation in rock types that are quite different from those preserving the photosphere-supported biosphere. -
Morphology and Origin of Lunar Craters Von R
Morphology and origin of lunar craters Von R. S. Saunders, E. L. Haines, and J. E. Conel, Pasaderia" Summary: The general concensus among lunar geologists is th.at the majority of lunar craters, up to a few km in diameter, are of Impact origm. This conclusion is based on morphologie comparison with terrestrial meteorite craters, consideration of lunar regolrth formation by impact, direct observation of the morphology of smalI and microscopic craters on the lunar surface and experimental impact studtcs. Most Iarge craters are also interpreted to be ()f Impact origin. Although the morphology of unmodified craters changes somewhat with increasing size, these changes are completely gradational and there is no evidence to suggest that the predominant process of crater formation is different for large craters. However, selected craters of various sizes have been interpreted as volcanic. Understanding the origm of the multi-ring b asms presents greater difficulties. Theoretical treatments such as those of Bjork (1961) and Van Dorn (1969) seem to be the only approach. In such treatments it is nccessary to iriclude, in addition to hydrodynamic flow, large plastrc deformation arid br.it.tle failure of the target material, processes that are known to accompany Impact phenomena. Thus complete equations of state are required as well as a detailed microscopic (perhaps statistical) description of imperfections in rock mechanical properties. The required physical parameters arid the calculations are clearly formidable. Analysis of tracking data from Orbiter V has revealed positive graviational anomalies (mascons) over the circular maria (Mulle r und Sjogren, 1968). While a number of theories for the origin of the mascons has been proposed (see Kaula, 1969 for a summary), the nature of the anomalous masses remains in doubt as does the mechamsm whereby excess mass has been added to specific rcgtons, Resolution of these questions will tell us much about the thermal and struc tural history of the Moon. -
1 Introduction: Baltic Linguistics – State of the Art
Peter Arkadiev, Axel Holvoet and Björn Wiemer 1 Introduction: Baltic linguistics – State of the art This introductory chapter to the volume is meant to give an overview of the state of research in the description of extant Baltic languages. Of course, we cannot supply a fully comprehensive account of all aspects of these languages. We will mainly focus on synchronic linguistics. We have not let ourselves be guided by functionalists’ or formalists’ prominence, although the survey to some extent reflects those domains and frameworks for which we ourselves felt competent enough. Sometimes we decided to be more explicit on noteworthy research results if these have been published in one of the Baltic languages or another language the knowledge of which cannot be assumed to be very much widespread among Western linguists. In any case, we are eager to account for the study of Baltic lan guages in the light of theoretically interesting issues and methods. Before beginning our survey, we will give some basic introduction concern ing the general typological “outfit” of the contemporary Baltic languages and their genealogical affiliation. This includes short explanations about the main differ ences between Lithuanian, Latvian, and Latgalian and the internal dialectal fragmentation of East Baltic (Section 1). Sections 2 and 3 contain the main body of our task. Section 2 is subdivided according to rather traditional levels of struc tural description (from phonetics to the syntax of complex sentences). Derivation is given an extra subsection (2.4). Section 3 is devoted to semantics and pragma tics and also fragmented following generally accepted linguistic disciplines.