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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. -
Geologic Mapping of Vinogradov Crater on Mars: Ancient Phyllosilicates to Alluvial Fans
45th Lunar and Planetary Science Conference (2014) 2382.pdf GEOLOGIC MAPPING OF VINOGRADOV CRATER ON MARS: ANCIENT PHYLLOSILICATES TO ALLUVIAL FANS. S. A. Wilson1, J. A. Grant1, C. M. Weitz2 and R. P. Irwin1 1Center for Earth and Planetary Studies, National Air and Space Museum, Smithsonian Institution, 6th St. at Independence Ave. SW, Washington, DC, 20560 ([email protected]), 2Planetary Science Institute, 1700 E Fort Lowell, Suite 106, Tucson, AZ 85719. Introduction: Southern Margaritifer Terra on Mars preserves a long geologic history of water-related activity (Fig. 1). The northward-draining Uzboi– Ladon–Morava (ULM) outflow system dominates drainage in southwest Margaritifer Terra [1-4] and was incised during the Late Noachian to Hesperian [2]. Holden crater formed in the mid to Late Hesperian [5] and blocked the northern end of Uzboi, creating an enclosed basin that filled as a large paleolake [6]. The geology of Vinogradov crater and vicinity, located ~200 km west of Ladon basin and 250 km northwest of Holden crater (Fig. 1), is consistent with the long and diverse history of water in the region to the east [5]. Figure 2. Vinogradov crater is flanked by fan-bearing craters Roddy (D=85.8km; 21.7ºS, 320.6ºE), Gringauz (D=71.0km; 20.7ºS, 324.3ºE) and Luba (D=38.8km, 18.3ºS, 323ºE). Phyllosilicates are found in the depression (dashed line) between ejecta from Roddy and Gringauz (Fig. 3). MOLA 128 pixel/degree with 25 m contours over THEMIS daytime IR mosaic. Figure 1. Southern Margaritifer Terra indicating major place names. Stars show craters containing alluvial fans [7-8]. -
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. -
'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. -
Vladimircm TESE.Pdf
UNIVERSIDADE FEDERAL DO RIO GRANDE DO NORTE CENTRO DE CIÊNCIAS EXATAS E DA TERRA PROGRAMA DE PÓS-GRADUAÇÃO EM GEODINÂMICA E GEOFÍSICA TESE DE DOUTORADO Evolução Geodinâmica e Condicionamento Estrutural dos Terrenos Piancó-Alto Brígida e Alto Pajeú, Domínio da Zona Transversal, NE do Brasil. Autor: Vladimir Cruz de Medeiros Tese n0 09/PPGG ORIENTADOR: Prof. Dr. Emanuel Ferraz Jardim de Sá – PPGG/UFRN CO-ORIENTADORES Prof. Dr. Venerando Eustáquio Amaro – PPGG/UFRN Prof. Dr. Fernando César Alves da Silva – PPGG/UFRN Natal - RN, Setembro de 2004 UNIVERSIDADE FEDERAL DO RIO GRANDE DO NORTE CENTRO DE CIÊNCIAS EXATAS E DA TERRA PROGRAMA DE PÓS-GRADUAÇÃO EM GEODINÂMICA E GEOFÍSICA TESE DE DOUTORADO Evolução Geodinâmica e Condicionamento Estrutural dos Terrenos Piancó-Alto Brígida e Alto Pajeú, Domínio da Zona Transversal, NE do Brasil. Autor: Vladimir Cruz de Medeiros Tese de doutorado apresentada em 30 de Setembro de 2004, para obtenção do título de Doutor em Geodinâmica pelo Programa de Pós-Graduação em Geodinâmica e Geofísica da UFRN. Comissão Examinadora: PROF. Dr. Emanuel Ferraz Jardim de Sá (DG-PPGG-UFRN-Orientador) PROF. Dr. Venerando Eustáquio Amaro (DG-PPGG-UFRN-Co-Orientador) PROF. Dr. Walter Eugênio de Medeiros (DFTE-PPGG-UFRN) PROF. Dr. Elton Luiz Dantas (DG-UnB) Dr. Edilton José dos Santos (CPRM-Serviço Geológico do Brasil) Natal - RN, Setembro de 2004. - DEDICATÓRIA - Aos familiares Marília O. Cruz (in memorian). Silvino S. Medeiros (in memorian). Maria E. Medeiros (in memorian). Francisco das Chagas. Maria das Graças Souza. iii - AGRADECIMENTOS - A iniciativa de realizar e o desenvolvimento do presente trabalho contou com a colaboração e incentivo de várias pessoas e instituições, as quais queremos registrar os nossos agradecimentos. -
An Approach to the Brasiliano-Pan African Cycle and Orogenic Collage
155 by Benjamim Bley de Brito Neves1, Mário da Costa Campos Neto1, and Reinhardt Adolfo Fuck2 From Rodinia to Western Gondwana: An approach to the Brasiliano-Pan African Cycle and orogenic collage 1- Instituto de Geociências - Universidade de São Paulo. S. Paulo-SP. 2- Instítuto de Geociências - Universidade de Brasílía. Brasílía-DF. The basement of the South American platform displays east), Tocantins (Central-eastern, part of the Central- the lithostructural and tectonic records of three major western), Pampean (Central-southwestern) and Man- orogenic collages: Middle Paleoproterozoic (or tiqueira (East-southeast). Transamazonian), Late Mesoproterozoic/Early Neopro- terozoic and Late Neoproterozoic/Cambrian, the Brasil- Introduction iano-Pan African collage. The first two collages have their records in the basement of the Syn-Brasiliano cra- The history of the geologic evolution of the South American conti- tons and Brasiliano Fold Belts. nent from the Neoproterozoic to the early Cambrian is recording all The development of the Brasiliano-Pan African the steps of the development of a complete and wide tectonic cycle, collage started in Early Neoproterozoic times, with the in terms of J.T. Wilson. This means, from the fission/disarticulation of a former Late Mesoproterozoic Supercontinent (Rodinia) – up to first events of breakup of the Rodinia Supercontinent, the further fusion/agglutination of a newer supercontinent — West- and it has been characterized by diachrony since their ern Gondwana (Pannotia). early beginnings. The processes of break up and fission For the two major tectonic phenomena then developed (fission and subsequent fusion) it is necessary to remark, since now, the took place in different time intervals (ca.