Geologic Mapping of Vinogradov Crater on Mars: Ancient Phyllosilicates to Alluvial Fans
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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. -
11 Fall Unamagazine
FALL 2011 • VOLUME 19 • No. 3 FOR ALUMNI AND FRIENDS OF THE UNIVERSITY OF NORTH ALABAMA Cover Story 10 ..... Thanks a Million, Harvey Robbins Features 3 ..... The Transition 14 ..... From Zero to Infinity 16 ..... Something Special 20 ..... The Sounds of the Pride 28 ..... Southern Laughs 30 ..... Academic Affairs Awards 33 ..... Excellence in Teaching Award 34 ..... China 38 ..... Words on the Breeze Departments 2 ..... President’s Message 6 ..... Around the Campus 45 ..... Class Notes 47 ..... In Memory FALL 2011 • VOLUME 19 • No. 3 for alumni and friends of the University of North Alabama president’s message ADMINISTRATION William G. Cale, Jr. President William G. Cale, Jr. The annual everyone to attend one of these. You may Vice President for Academic Affairs/Provost Handy festival contact Dr. Alan Medders (Vice President John Thornell is drawing large for Advancement, [email protected]) Vice President for Business and Financial Affairs crowds to the many or Mr. Mark Linder (Director of Athletics, Steve Smith venues where music [email protected]) for information or to Vice President for Student Affairs is being played. At arrange a meeting for your group. David Shields this time of year Sometimes we measure success by Vice President for University Advancement William G. Cale, Jr. it is impossible the things we can see, like a new building. Alan Medders to go anywhere More often, though, success happens one Vice Provost for International Affairs in town and not hear music. The festival student at a time as we provide more and Chunsheng Zhang is also a reminder that we are less than better educational opportunities. -
Widespread Crater-Related Pitted Materials on Mars: Further Evidence for the Role of Target Volatiles During the Impact Process ⇑ Livio L
Icarus 220 (2012) 348–368 Contents lists available at SciVerse ScienceDirect Icarus journal homepage: www.elsevier.com/locate/icarus Widespread crater-related pitted materials on Mars: Further evidence for the role of target volatiles during the impact process ⇑ Livio L. Tornabene a, , Gordon R. Osinski a, Alfred S. McEwen b, Joseph M. Boyce c, Veronica J. Bray b, Christy M. Caudill b, John A. Grant d, Christopher W. Hamilton e, Sarah Mattson b, Peter J. Mouginis-Mark c a University of Western Ontario, Centre for Planetary Science and Exploration, Earth Sciences, London, ON, Canada N6A 5B7 b University of Arizona, Lunar and Planetary Lab, Tucson, AZ 85721-0092, USA c University of Hawai’i, Hawai’i Institute of Geophysics and Planetology, Ma¯noa, HI 96822, USA d Smithsonian Institution, Center for Earth and Planetary Studies, Washington, DC 20013-7012, USA e NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA article info abstract Article history: Recently acquired high-resolution images of martian impact craters provide further evidence for the Received 28 August 2011 interaction between subsurface volatiles and the impact cratering process. A densely pitted crater-related Revised 29 April 2012 unit has been identified in images of 204 craters from the Mars Reconnaissance Orbiter. This sample of Accepted 9 May 2012 craters are nearly equally distributed between the two hemispheres, spanning from 53°Sto62°N latitude. Available online 24 May 2012 They range in diameter from 1 to 150 km, and are found at elevations between À5.5 to +5.2 km relative to the martian datum. The pits are polygonal to quasi-circular depressions that often occur in dense clus- Keywords: ters and range in size from 10 m to as large as 3 km. -
Martian Subsurface Properties and Crater Formation Processes Inferred from Fresh Impact Crater Geometries
Martian Subsurface Properties and Crater Formation Processes Inferred From Fresh Impact Crater Geometries The Harvard community has made this article openly available. Please share how this access benefits you. Your story matters Citation Stewart, Sarah T., and Gregory J. Valiant. 2006. Martian subsurface properties and crater formation processes inferred from fresh impact crater geometries. Meteoritics and Planetary Sciences 41: 1509-1537. Published Version http://meteoritics.org/ Citable link http://nrs.harvard.edu/urn-3:HUL.InstRepos:4727301 Terms of Use This article was downloaded from Harvard University’s DASH repository, and is made available under the terms and conditions applicable to Other Posted Material, as set forth at http:// nrs.harvard.edu/urn-3:HUL.InstRepos:dash.current.terms-of- use#LAA Meteoritics & Planetary Science 41, Nr 10, 1509–1537 (2006) Abstract available online at http://meteoritics.org Martian subsurface properties and crater formation processes inferred from fresh impact crater geometries Sarah T. STEWART* and Gregory J. VALIANT Department of Earth and Planetary Sciences, Harvard University, 20 Oxford Street, Cambridge, Massachusetts 02138, USA *Corresponding author. E-mail: [email protected] (Received 22 October 2005; revision accepted 30 June 2006) Abstract–The geometry of simple impact craters reflects the properties of the target materials, and the diverse range of fluidized morphologies observed in Martian ejecta blankets are controlled by the near-surface composition and the climate at the time of impact. Using the Mars Orbiter Laser Altimeter (MOLA) data set, quantitative information about the strength of the upper crust and the dynamics of Martian ejecta blankets may be derived from crater geometry measurements. -
First Year of Coordinated Science Observations by Mars Express and Exomars 2016 Trace Gas Orbiter
MANUSCRIPT PRE-PRINT Icarus Special Issue “From Mars Express to ExoMars” https://doi.org/10.1016/j.icarus.2020.113707 First year of coordinated science observations by Mars Express and ExoMars 2016 Trace Gas Orbiter A. Cardesín-Moinelo1, B. Geiger1, G. Lacombe2, B. Ristic3, M. Costa1, D. Titov4, H. Svedhem4, J. Marín-Yaseli1, D. Merritt1, P. Martin1, M.A. López-Valverde5, P. Wolkenberg6, B. Gondet7 and Mars Express and ExoMars 2016 Science Ground Segment teams 1 European Space Astronomy Centre, Madrid, Spain 2 Laboratoire Atmosphères, Milieux, Observations Spatiales, Guyancourt, France 3 Royal Belgian Institute for Space Aeronomy, Brussels, Belgium 4 European Space Research and Technology Centre, Noordwijk, The Netherlands 5 Instituto de Astrofísica de Andalucía, Granada, Spain 6 Istituto Nazionale Astrofisica, Roma, Italy 7 Institut d'Astrophysique Spatiale, Orsay, Paris, France Abstract Two spacecraft launched and operated by the European Space Agency are currently performing observations in Mars orbit. For more than 15 years Mars Express has been conducting global surveys of the surface, the atmosphere and the plasma environment of the Red Planet. The Trace Gas Orbiter, the first element of the ExoMars programme, began its science phase in 2018 focusing on investigations of the atmospheric composition with unprecedented sensitivity as well as surface and subsurface studies. The coordination of observation programmes of both spacecraft aims at cross calibration of the instruments and exploitation of new opportunities provided by the presence of two spacecraft whose science operations are performed by two closely collaborating teams at the European Space Astronomy Centre (ESAC). In this paper we describe the first combined observations executed by the Mars Express and Trace Gas Orbiter missions since the start of the TGO operational phase in April 2018 until June 2019. -
In Pdf Format
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Simulating Martian Regolith in the Laboratory
ARTICLE IN PRESS Planetary and Space Science 56 (2008) 2009–2025 www.elsevier.com/locate/pss Simulating Martian regolith in the laboratory Karsten Seiferlina,Ã, Pascale Ehrenfreundb, James Garryb, Kurt Gundersona,E.Hu¨tterc, Gu¨nter Karglc, Alessandro Maturillid, Jonathan Peter Merrisone aPhysikalisches Institut, Universita¨t Bern, Sidlerstrasse 5, 3012 Bern, Switzerland bAstrobiology Laboratory, Leiden Institute of Chemistry, P.O. Box 9502, 2300 RA Leiden, The Netherlands cInstitut fu¨r Weltraumforschung, Graz, O¨sterreichische Akademie der Wissenschaften, Austria dGerman Aerospace Centre (DLR), Institute for Planetary Research, Rutherfordstr. 2, 12489 Berlin-Adlershof, Germany eAarhus Mars Simulation Laboratory, Aarhus University, Denmark Received 6 December 2007; received in revised form 21 July 2008; accepted 21 September 2008 Available online 15 October 2008 Abstract Regolith and dust cover the surfaces of the Solar Systems solid bodies, and thus constitute the visible surface of these objects. The topmost layers also interact with space or the atmosphere in the case of Mars, Venus and Titan. Surface probes have been proposed, studied and flown to some of these worlds. Landers and some of the mechanisms they carry, e.g. sampling devices, drills and subsurface probes (‘‘moles’’) will interact with the porous surface layer. The absence of true extraterrestrial test materials in ample quantities restricts experiments to the use of soil or regolith analogue materials. Several standardized soil simulants have been developed and produced and are commonly used for a variety of laboratory experiments. In this paper we intend to give an overview of some of the most important soil simulants, and describe experiments (penetrometry, thermal conductivity, aeolian transport, goniometry, spectroscopy and exobiology) made in various European laboratory facilities. -
Biodiversity in Sub-Saharan Africa and Its Islands Conservation, Management and Sustainable Use
Biodiversity in Sub-Saharan Africa and its Islands Conservation, Management and Sustainable Use Occasional Papers of the IUCN Species Survival Commission No. 6 IUCN - The World Conservation Union IUCN Species Survival Commission Role of the SSC The Species Survival Commission (SSC) is IUCN's primary source of the 4. To provide advice, information, and expertise to the Secretariat of the scientific and technical information required for the maintenance of biologi- Convention on International Trade in Endangered Species of Wild Fauna cal diversity through the conservation of endangered and vulnerable species and Flora (CITES) and other international agreements affecting conser- of fauna and flora, whilst recommending and promoting measures for their vation of species or biological diversity. conservation, and for the management of other species of conservation con- cern. Its objective is to mobilize action to prevent the extinction of species, 5. To carry out specific tasks on behalf of the Union, including: sub-species and discrete populations of fauna and flora, thereby not only maintaining biological diversity but improving the status of endangered and • coordination of a programme of activities for the conservation of bio- vulnerable species. logical diversity within the framework of the IUCN Conservation Programme. Objectives of the SSC • promotion of the maintenance of biological diversity by monitoring 1. To participate in the further development, promotion and implementation the status of species and populations of conservation concern. of the World Conservation Strategy; to advise on the development of IUCN's Conservation Programme; to support the implementation of the • development and review of conservation action plans and priorities Programme' and to assist in the development, screening, and monitoring for species and their populations. -
Large Impact Crater Histories of Mars: the Effect of Different Model Crater Age Techniques ⇑ Stuart J
Icarus 225 (2013) 173–184 Contents lists available at SciVerse ScienceDirect Icarus journal homepage: www.elsevier.com/locate/icarus Large impact crater histories of Mars: The effect of different model crater age techniques ⇑ Stuart J. Robbins a, , Brian M. Hynek a,b, Robert J. Lillis c, William F. Bottke d a Laboratory for Atmospheric and Space Physics, 3665 Discovery Drive, University of Colorado, Boulder, CO 80309, United States b Department of Geological Sciences, 3665 Discovery Drive, University of Colorado, Boulder, CO 80309, United States c UC Berkeley Space Sciences Laboratory, 7 Gauss Way, Berkeley, CA 94720, United States d Southwest Research Institute and NASA Lunar Science Institute, 1050 Walnut Street, Suite 300, Boulder, CO 80302, United States article info abstract Article history: Impact events that produce large craters primarily occurred early in the Solar System’s history because Received 25 June 2012 the largest bolides were remnants from planet ary formation .Determi ning when large impacts occurred Revised 6 February 2013 on a planetary surface such as Mars can yield clues to the flux of material in the early inner Solar System Accepted 25 March 2013 which, in turn, can constrain other planet ary processes such as the timing and magnitude of resur facing Available online 3 April 2013 and the history of the martian core dynamo. We have used a large, global planetary databas ein conjunc- tion with geomorpholog icmapping to identify craters superposed on the rims of 78 larger craters with Keywords: diameters D P 150 km on Mars, 78% of which have not been previously dated in this manner. -
'1 Tanganyika
'1 TANGANYIKA . EXHIB TION HANDBOOK V611 N2 H 004191 ~ - ,·~tt'.· . r:-. · . FLAX HEMP SISAL .. JUTE ALL DESCRIPTIONS Wi 82, ~1: VIS: Av· ONDON." ys, DUNDE::·--- --- -- -L -IV_E_R_ P_O_O_ L_ =-:-,..._ -r-... ~15 : 6, Euclid Crescent. 9. P · ,on C ourt, sa. Rue J ean- BELFAST : Cr Street. Jacques Rossea~~o Textile Building, I ~ YORK: BOLOGNA: L inenhall Street. s... •roadway. Via Oegli, Artieri No. a. CONTENTS PAGK OF TUB TERRITORY I ION' OF TilE TERRITORY: ion ••• 9 lte ••• II f-;~~crip.~.~n :-... ... 15 !Vegetation ••• ••• ••• 15 \nimals, Wild and Tame •.• 18 De Human Element ••• 19 ~owns and Communications 19 cts ••• ••• · 2l ,1 and Sanitation 31 ltunications : <ailways ••• 35 .:.oads 40 ~'osts and Telegraphs 40 l•lC ... · 4Z ~uages 47 51 l:tain.;.;~ng sB [lini_stration and Law 62 cation ••• ••• 6J .TURE:- eral ••• .... 69 ive Agricultural Industry 70 Plantation Industry 78 ::>NDITIONS 91 L OF EX·ENEMY PROPERTY 93 CoNDITIONS,,, 96 .TURAL ASSISTANCE ••• 97 AND CATTLE PRODUCTS ,,;, 99 y 107 AND MINERALS IIJ ( i.i I A• CONTENTS Geaeral ... ••• . ••• -· ••• Commen:ial Aooodatlous uul Fl.- ... Plantas' Aalciatl0111 and ~lemben ••• Castollll ••• - .;. :Ouiks Hotels and Shops ... ... ... APPENDIXES L Imports uul Exports II. Cenlus ••• III. Roada ..., JV. Admiaistratlve Districts and Sub-Districts v .. Details of Saleo ol ex-Enemy Property ... VI. :RaiDfRII _ ... vu. Game ••• · VUL Native Wooda IX. List of Book• Having Reference to the Territory X. Lisi of PubHcatloa~ Iasned la tbe Territocy XI. Weights uul Measures of tbe Territory ... XII. List ol Exh.iblton and Exhibits ... _ ... ·Map ol the Territory. Map Showing the Chief District. of the Principal Exporlll, ( iv) 2 HISTORY OF THE TERRITOR'\ of the conquering Arabs, it disappeared. -
The Prophecy That Is Shaping History
The Prophecy That Is Shaping History: New Research on Ezekiel’s Vision of the End Jon Mark Ruthven, PhD Ihab Griess, PhD Xulon Press 11350 Random Hills Drive #800 Fairfax, Virginia 22030 Copyright Jon Mark Ruthven © 2003 In memoriam Pamela Jessie Ruthven PhD, LCSW 26 March 1952 – 9 April 2001 Wife, mother, and faithful friend i Preface Great events in history often gather momentum and power long before they are recognized by the experts and commentators on world affairs. Easily one of the most neglected but powerfully galvanizing forces shaping history in the world today is the prophecy of Gog and Magog from the 38th and 39th chapters of the book of Ezekiel. This prophecy from the Jewish-Christian Bible has molded geo-politics, not only with- in the United States and the West but also, to an amazing degree, in the Muslim world as well. It seems that, millennia ago, Ezekiel’s vision actually named the nation which millions today believe plays the major role in this prophecy: the nation of Russia. Many modern scholars have dismissed Ezekiel’s Gog and Magog prophecy as a mystical apocalypse written to vindicate the ancient claims of a minor country’s deity. The very notion of such a prediction—that semi-mythical and unrelated nations that dwelt on the fringes of Israel’s geographical consciousness 2,500 years ago would, “in the latter days,” suddenly coalesce into a tidal wave of opposition to a newly regathered state of Jews—seems utterly incredible to a modern mentality. Such a scenario, the experts say, belongs only to the fundamentalist “pop religion” of The Late, Great Planet Earth and of TV evangelists. -
Peter Weiss. Andrei Platonov. Ragnvald Blix. Georg Henrik Von Wright. Adam Michnik
A quarterly scholarly journal and news magazine. March 2011. Vol IV:1 From the Centre for Baltic and East European Studies (CBEES) Södertörn University, Stockholm FEATURE. Steklov – Russian BALTIC temple of pure thought W O Rbalticworlds.com L D S COPING WITH TRANSITIONS PETER WEISS. ANDREI PLATONOV. RAGNVALD BLIX. GEORG HENRIK VON WRIGHT. ADAM MICHNIK. SLAVENKA DRAKULIĆ. Sixty pages BETRAYED GDR REVOLUTION? / EVERYDAY BELARUS / WAVE OF RELIGION IN ALBANIA / RUSSIAN FINANCIAL MARKETS 2short takes Memory and manipulation. Transliteration. Is anyone’s suffering more important than anyone else’s? Art and science – and then some “IF YOU WANT TO START a war, call me. Transliteration is both art and science CH I know all about how it's done”, says – and, in many cases, politics. Whether MÄ author Slavenka Drakulić with a touch царь should be written as tsar, tzar, ANNA of gallows humor during “Memory and czar, or csar may not be a particu- : H Manipulation: Religion as Politics in the larly sensitive political matter today, HOTO Balkans”, a symposium held in Lund, but the question of the transliteration P Sweden, on December 2, 2010. of the name of the current president This issue of the journal includes a of Belarus is exceedingly delicate. contribution from Drakulić (pp. 55–57) First, and perhaps most important: in which she claims that top-down gov- which name? Both the Belarusian ernance, which started the war, is also Аляксандр Лукашэнка, and the Rus- the path to reconciliation in the region. sian Александр Лукашенко are in use. Balkan experts attending the sympo- (And, while we’re at it, should that be sium agree that the war was directed Belarusian, or Belarussian, or Belaru- from the top, and that “top-down” is san, or Byelorussian, or Belorussian?) the key to understanding how the war BW does not want to take a stand on began in the region.