Model Assessments for French: Stage II
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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. -
250.000 Judar -Skall Bort Fran B~,F!Fj/!Est Fran St:~T:S :Gjrlinredakti,Ir Chrisq.ER
·- COCPERATI ON WITH O'rHSR GOVER~'MK'iTS: :-ll!,UTPJU. ~L-.'l0P3:AJ;; (SWEDE~!) VOL.z (LAST PART) LETT,;RS F!!OM IVKR C. OLSEN, TRM/SMITTHG PRESS RELEASES & TRAN3J,ATIONS FROM S'o'3DEN ----- 3 lm<:UBt 1'3, 1'144 - iind'onc·· . ~. 'I THE FOREIGN SERVICE OF THE UNil'ED STATES OF AMERICA AMERICAN LEGATION 848/MET Stockholm, Sweden December 4, 1944 Mr. John w. Pehle Executive Director War Refugee Board Washington, D. c. Dear•Mr. Pehle: For the information of the Board, there are enclosed a few articles and translations from the local press. Sincerely yours, ~~ Ma~abet~For: rver c. Thomps~nOlsen Special Attach~ for War Refugee Board Enclosures - 4 . i •· --I ~· SOURCE: Dagens Nyheter, November 18, 1944 FOR POLAND'S CHILDREN. The collection which the Help Poland's Children Committee started during Poland Week in September and which is still going on has at present resulted in 154,000 crowns, apart from the great quantity of clothes and shoes. Great amounts have come from industries and shops in the country, Among the more noticeable contributions is the one from teachers and pupils at Vasaetaden's girls' school through a bazaar, The sum was 2,266 crowns, from the employees and workers in the ASEA factories in Ludvika, 2,675 crowns, from employees and workers at Telefon AB L,M. Ericsson 1,382 crowns, and from the staff at AB Clothing Factory in Nassjo 629 crowns. Through the committee 35,000 kg. of food have been sent to the evacuation camp at Pruezkow and other plaoes, and we hope to be able to send even more food and clothes to other camps where the population of Warsow has been brought. -
Executive Intelligence Review, Volume 17, Number 15, April 6, 1990
LAROUCHE So, You Wish to Leant All About BUT YOU'D BEDER EconoInics? KNOW WHAT H. Jr. HE HAS TO SAY by Lyndon LaRouche, A text on elementary mathematical economics, by the world's leading economist. Find out why EIR was right, when everyone else was wrong. The Power of Order from: Ben Franklin Booksellers, Inc. Reason: 1988 27 South King Street Leesburg, Va. 22075 An Autobiography by Lyndon H. LaRouche, Jr. $9.95 plus shipping ($1.50 for first book, $.50 for each additional book). Information on bulk rates and videotape Published by Executive Intelligence Review Order from Ben Franklin Booksellers, 27 South King St., Leesburg, VA 22075. available on request. $10 plus shipping ($1.50 for first copy, .50 for each ad,:::ional). Bulk rates available. THE POWER OF REASON 1iM.'" An exciting new videotape is now available on the life and work of Lyndon LaRouche, political leader and scientist, who is currently an American political prisoner, together with six of his leading associates. This tape includes clips of some of LaRouche's most important, historic speeches, on economics, history, culture, science, AIDS, and t e drug trade. , This tape will recruit your friends to the fight forr Western civilization! Order it today! $100.00 Checks or money orders should be sent to: P.O. Box 535, Leesburg, VA 22075 HumanPlease specify Rights whether Fund you wish Beta or VHS. Allow 4 weeks for delivery. Founder and Contributing Editor: From the Editor Lyndon H. LaRouche. Jr. Editor: Nora Hamerman Managing Editors: John Sigerson, Susan Welsh Assistant Managing Editor: Ronald Kokinda Editorial Board: Warren Hamerman. -
Pre-Mission Insights on the Interior of Mars Suzanne E
Pre-mission InSights on the Interior of Mars Suzanne E. Smrekar, Philippe Lognonné, Tilman Spohn, W. Bruce Banerdt, Doris Breuer, Ulrich Christensen, Véronique Dehant, Mélanie Drilleau, William Folkner, Nobuaki Fuji, et al. To cite this version: Suzanne E. Smrekar, Philippe Lognonné, Tilman Spohn, W. Bruce Banerdt, Doris Breuer, et al.. Pre-mission InSights on the Interior of Mars. Space Science Reviews, Springer Verlag, 2019, 215 (1), pp.1-72. 10.1007/s11214-018-0563-9. hal-01990798 HAL Id: hal-01990798 https://hal.archives-ouvertes.fr/hal-01990798 Submitted on 23 Jan 2019 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. Open Archive Toulouse Archive Ouverte (OATAO ) OATAO is an open access repository that collects the wor of some Toulouse researchers and ma es it freely available over the web where possible. This is an author's version published in: https://oatao.univ-toulouse.fr/21690 Official URL : https://doi.org/10.1007/s11214-018-0563-9 To cite this version : Smrekar, Suzanne E. and Lognonné, Philippe and Spohn, Tilman ,... [et al.]. Pre-mission InSights on the Interior of Mars. (2019) Space Science Reviews, 215 (1). -
Martian Sub-Surface Ionising Radiation: Abstract Introduction ∗ Biosignatures and Geology Conclusions References Tables Figures L
Biogeosciences Discuss., 4, 455–492, 2007 Biogeosciences www.biogeosciences-discuss.net/4/455/2007/ Discussions BGD © Author(s) 2007. This work is licensed 4, 455–492, 2007 under a Creative Commons License. Biogeosciences Discussions is the access reviewed discussion forum of Biogeosciences Martian radiation L. R. Dartnell et al Title Page Martian sub-surface ionising radiation: Abstract Introduction ∗ biosignatures and geology Conclusions References Tables Figures L. R. Dartnell1, L. Desorgher2, J. M. Ward3, and A. J. Coates4 1CoMPLEX (Centre for Mathematics & Physics in the Life Sciences and Experimental J I Biology), University College London, UK J I 2Physikalisches Institut, University of Bern, Switzerland 3Department of Biochemistry and Molecular Biology, University College London, UK Back Close 4Mullard Space Science Laboratory, University College London, UK Full Screen / Esc Received: 8 January 2007 – Accepted: 7 February 2007 – Published: 9 February 2007 Correspondence to: L. R. Dartnell ([email protected]) Printer-friendly Version Interactive Discussion EGU ∗Invited contribution by L. R. Dartnell, one of the Union Young Scientist Award winners 2006. 455 Abstract BGD The surface of Mars, unshielded by thick atmosphere or global magnetic field, is ex- posed to high levels of cosmic radiation. This ionizing radiation field is deleterious to 4, 455–492, 2007 the survival of dormant cells or spores and the persistence of molecular biomarkers in 5 the subsurface, and so its characterisation is of prime astrobiological interest. Previous Martian radiation research has attempted to address the question of biomarker persistence by inappro- priately using dose profiles weighted specifically for cellular survival. Here, we present L. R. Dartnell et al modelling results of the unmodified physically absorbed radiation dose as a function of depth through the Martian subsurface. -
Life on Mars 2019
LIFE ON MARS Toward a metamorphosis? How are institutions changing today? How are artists interpreting their role? Which are the practices that are inspiring the cultural sector nowadays based on new models of social inclusion, cultural and political participation? What programs are being enac- ted under cultural policy? What focused actions are artists and organizations taking? Are they representing a field in which top-down and bottom-up forces can work toge- ther? Life on Mars 2019 - "Toward a metamorphosis?" reflects on the paradigm-shift in the artistic practices, in the cultural policies, and on the theme of "cultural resistance”. The latter is here un- derstood as a transformational outlook designed to bring into being cultural bodies that rethink their artistic, social and political mission in favour of an inclusive society, drawing strength from diversity (no matter what the form) while experimenting with different approaches, policies and practices (artistic and managerial) of collaboration and sustainable development. Life on Mars 2019 - "Toward a metamorphosis" is a moment of networking that aims to propose an exchange of equal footing between artists, institutions, researchers and cultural professionals, using participatory formats that offer opportunities of discussion and new relationships. Official language: English. Italian translation will be provided for the main panels. Learn more about the program and the speakers on www.life-on-mars.eu. TUESDAY 10TH SEPTEMBER ! OPENING _________________________________________ 13.30 -
CURRICULUM VITAE Dr
CURRICULUM VITAE Dr. Brian Michael Hynek Associate Professor in the Department of Geological Sciences and Research Associate at the Laboratory for Atmospheric and Space Physics Director, CU Center for Astrobiology 392 UCB, University of Colorado Boulder, CO 80309-0392 Email: [email protected] Educational Background Ph.D. in Earth and Planetary Sciences, Washington University, St. Louis, MO, 2003 Dissertation Title: The surface evolution of Mars with emphasis on hydrologic and volcanic processes (Roger Phillips, PhD advisor) M.A. in Earth and Planetary Sciences, Washington University, St. Louis, MO, 2001 B.A.s in Earth Science, Earth Science Education, and All Sciences Education, University of Northern Iowa, Cedar Falls, IA 1998 Academic Employment History 1998-1999 Teacher, Chemistry and Physics, John Jay High School, San Antonio, TX. 2001-2003 Part-Time Faculty, Astronomy, St. Louis Community College, St. Louis, MO, 2003-2005 Research Associate, Level I (Post-Doc), LASP, University of Colorado Boulder 2004-2007 Instructor, Astronomy Department, University of Colorado Boulder 2005-2007 Research Associate, Level II (Junior Researcher), LASP, University of Colorado Boulder 2007-2013 Assistant Professor, Department of Geological Sciences, University of Colorado Boulder 2013-present Associate Professor, Department of Geological Sciences, University of Colorado Boulder 2007-present Research Associate (Tenure Track), LASP, University of Colorado Boulder 2014 Visiting Research Scientist, Geophysical Institute, University of Alaska Fairbanks Profile Dr. Brian M. Hynek is an Associate Professor in the Department of Geological Sciences and Research Associate in the Laboratory for Atmospheric and Space Physics (LASP), both at the University of Colorado. He is also the Director of CU’s Center for Astrobiology. -
Exomars Lander Radioscience Lara, a Space Geodesy Experiment to Mars
EPSC Abstracts Vol. 11, EPSC2017-852, 2017 European Planetary Science Congress 2017 EEuropeaPn PlanetarSy Science CCongress c Author(s) 2017 ExoMars Lander Radioscience LaRa, a Space Geodesy Experiment to Mars. V. Dehant (1), S. Le Maistre (1), R.M. Baland (1), M. Yseboodt (1), M.J. Péters (1), Ö. Karatekin (1), A. Rivoldini (1), and T. Van Hoolst (1) (1) Royal Observatory of Belgium, Brussels, Belgium ([email protected]) Abstract These Doppler measurements will be used to obtain the orientation and rotation of Mars in space The LaRa (Lander Radioscience) experiment is (precession and nutations, polar motion, and length- designed to obtain coherent two-way Doppler of-day variations). The ultimate objectives are to measurements from the radio link between the obtain information on Mars’ interior and on the ExoMars lander and Earth over at least one Martian sublimation/condensation process of CO2. This is year. The instrument lifetime is larger than the one possible since one will be able to obtain the moment Earth year of nominal mission duration. The Doppler of inertia of the whole planet that includes the mantle measurements will be used to observe the orientation and the core, the moment of inertia of the core, as and rotation of Mars in space (precession, nutations, well as the seasonal mass transfer between the and length-of-day variations), as well as polar motion. atmosphere and ice caps. The ultimate objective is to obtain information / constraints on the Martian interior, and on the The LaRa experiment will be used jointly with the sublimation / condensation cycle of atmospheric CO2. -
Pre-Mission Insights on the Interior of Mars
Open Archive Toulouse Archive Ouverte (OATAO ) OATAO is an open access repository that collects the wor of some Toulouse researchers and ma es it freely available over the web where possible. This is an author's version published in: https://oatao.univ-toulouse.fr/21690 Official URL : https://doi.org/10.1007/s11214-018-0563-9 To cite this version : Smrekar, Suzanne E. and Lognonné, Philippe and Spohn, Tilman ,... [et al.]. Pre-mission InSights on the Interior of Mars. (2019) Space Science Reviews, 215 (1). 1-72. ISSN 0038-6308 Any correspondence concerning this service should be sent to the repository administrator: [email protected] Pre-mission InSights on the Interior of Mars 1 2 3 1 Suzanne E. Smrekar · Philippe Lognonné · Tilman Spohn · W. Bruce Banerdt · 3 · 4 · 5 · 2 · Doris Breuer Ulrich Christensen Véronique Dehant Mélanie Drilleau 1 2 6 7 William Folkner · Nobuaki Fuji · Raphael F. Garcia · Domenico Giardini · 1 · 3 · 8 · 9,10 · Matthew Golombek Matthias Grott Tamara Gudkova Catherine Johnson 7 11 9 11 Amir Khan · Benoit Langlais · Anna Mittelholz · Antoine Mocquet · 12 · 1 · 2 · 13 · Robert Myhill Mark Panning Clément Perrin Tom Pike 3 5 2 7 Ana-Catalina Plesa · Attilio Rivoldini · Henri Samuel · Simon C. Stähler · 7 · 5 · 11 · 14 · Martin van Driel Tim Van Hoolst Olivier Verhoeven Renee Weber 15 Mark Wieczorek Abstract The Interior exploration using Seismic Investigations, Geodesy, and Heat Trans- port (InSight) Mission will focus on Mars’ interior structure and evolution. The basic struc- ture of crust, mantle, and core form soon after accretion. Understanding the early differ- entiation process on Mars and how it relates to bulk composition is key to improving our understanding of this process on rocky bodies in our solar system, as well as in other solar B S.E. -
GROWTH and DESTRUCTION CYCLES and ERUPTION STYLES at THARSIS THOLUS, MARS. T. Platz1, PC Mcguire1,2, S. Münn3, B. Cailleau1
40th Lunar and Planetary Science Conference (2009) 1522.pdf GROWTH AND DESTRUCTION CYCLES AND ERUPTION STYLES AT THARSIS THOLUS, MARS. T. Platz1, P. C. McGuire1,2, S. Münn3, B. Cailleau1, A. Dumke1, G. Neukum1, J. N. Procter4, 1Freie Universität Ber- lin, Institute of Geosciences, Planetary Sciences and Remote Sensing, Malteserstr. 74-100, 12249 Berlin, Germany, [email protected], 2Washington University in St. Louis, McDonnell Center for the Space Sciences, Cam- pus Box 1169, One Brookings Drive, St. Louis, MO 63130-4899, 3 Leibniz Institute of Marine Sciences, IFM- GEOMAR, Wischhofstr. 1-3, 24148 Kiel, Germany, 4Massey University, Volcanic Risk Solutions, Institute of Natural Resources, Private Bag 11222, Palmerston North, New Zealand. Introduction: Tharsis Tholus is located in the mately 31.1×10³ km³, however, if a basal horizontal Tharsis region, approx. 800 km to the ENE of As- plane at 500 m is assumed, an edifice volume of craeus Mons. The edifice of Tharsis Tholus is unique >50×10³ km³ results. among Martian volcanoes as it is structurally divided Volcano-tectonic features: The edifice of Tharsis into sectors suggesting a complex volcano-tectonic Tholus shows the structures of at least four large de- evolution [1-3]. The objective of this study was 1) to formation events. The central and most prominent identify cycles of edifice growth and destruction and structure of the volcano is its central caldera. It is bor- causes of instability, 2) to estimate the mineralogical dered by a well-preserved system of concentric normal composition of rocks and loose deposits, 3) to provide faults. Peripheral ring faults generated individual a time frame of volcanic activity, and 4) to characterize blocks that moved downslope to varying degrees into eruptive styles at Tharsis Tholus. -
United States V. Lara As a Story of Native Agency
Tulsa Law Review Volume 40 Issue 1 Tribal Sovereignty and United States v. Lara Fall 2004 United States v. Lara as a Story of Native Agency Bethany R. Berger Follow this and additional works at: https://digitalcommons.law.utulsa.edu/tlr Part of the Law Commons Recommended Citation Bethany R. Berger, United States v. Lara as a Story of Native Agency, 40 Tulsa L. Rev. 5 (2013). Available at: https://digitalcommons.law.utulsa.edu/tlr/vol40/iss1/2 This Native American Symposia Articles is brought to you for free and open access by TU Law Digital Commons. It has been accepted for inclusion in Tulsa Law Review by an authorized editor of TU Law Digital Commons. For more information, please contact [email protected]. Berger: United States v. Lara as a Story of Native Agency UNITED STATES V. LARA AS A STORY OF NATIVE AGENCY Bethany R. Berger* Like our ancestors, we must do battle for the rights of our tribes, for our survival as Indian nations and Indian people. Like they did, we must wage war on every front where our rights are threatened. American politics is one such battleground-a vast one, an important one, perhaps the most important one. If we retreat from that theater, can we survive the Armageddon that will then be upon us? America without conscience is Indian Apocalypse Now. Shall we throw in the towel, sit this one out, preach to the choir, rest in the belly of that Great Beast? No way.' Indian tribes are not falling apart in the face of the Supreme Court's virtual attack on tribal sovereignty and jurisdiction ....Rather, they are uniting to face the Court.2 The Supreme Court's decision in United States v. -
Geologic Mapping of Impact Craters and the Mahuea Tholus Construct: a Year Three Progress Report for the Mahuea Tholus (V-49) Quadrangle, Venus
Planetary Geologic Mappers Meeting 2018 (LPI Contrib. No. 2066) 7024.pdf GEOLOGIC MAPPING OF IMPACT CRATERS AND THE MAHUEA THOLUS CONSTRUCT: A YEAR THREE PROGRESS REPORT FOR THE MAHUEA THOLUS (V-49) QUADRANGLE, VENUS. N.P. Lang1 , M. Covley1, J. Beltran1, K. Rogers1, and B.J. Thomson2; 1Department of Geology, Mercyhurst University, Erie, PA 16546 ([email protected]), 2Department of Earth and Planetary Sciences, University of Tennessee – Knox- ville, Knoxville, TN 37996 ([email protected]). Introduction: The Mahuea Tholus quadrangle (V- edifice is ~100 km in diameter (with all flow materials, 49) extends from 25° to 50° S to 150° to 180° E and Mahuea is ~300 km in diameter), ~0.5 km in height encompasses >7×106 km2 of the Venusian surface. with a ~4 km diameter flattish top, and an erupted vol- Moving clockwise from due north, the Mahuea Tholus ume of ~103 km3. Mahuea is located within the center quadrangle is bounded by the Diana Chasma, Thetis of a topographic basin in Zhibek Planitia ~1400 km SE Regio, Artemis Chasma, Henie, Barrymore, Isabella, of the main axis of Diana-Dali Chasma-related rifting. and Stanton quadrangles; together with Stanton, Ma- The volcano resides at the eastern end of Annapurna huea Tholus is one of two remaining quadrangles to be Corona-related fractures (Naguchitsa Fossae) and over- geologically mapped in this part of Venus. Here we lies Annapurna-sourced flow material – material previ- report on our continued mapping of this quadrangle. ously interpreted as possible pyroclastic deposits Specifically, over the past year we have focused on sourced from Mahuea Tholus [3]; Annapurna-sourced mapping and cataloging impact craters located within flows were then subsequently deformed by NE- the quadrangle as well as larger-scale mapping of the trending wrinkle ridges, which was then followed by Mahuea Tholus construct; those efforts are described in formation of Mahuea Tholus.