Technetium and Rhenium in Volcanic Soils by Icpms
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Evidence for Thermal-Stress-Induced Rockfalls on Mars Impact Crater Slopes
Icarus 342 (2020) 113503 Contents lists available at ScienceDirect Icarus journal homepage: www.elsevier.com/locate/icarus Evidence for thermal-stress-induced rockfalls on Mars impact crater slopes P.-A. Tesson a,b,*, S.J. Conway b, N. Mangold b, J. Ciazela a, S.R. Lewis c, D. M�ege a a Space Research Centre, Polish Academy of Science, Wrocław, Poland b Laboratoire de Plan�etologie et G�eodynamique UMR 6112, CNRS, Nantes, France c School of Physical Sciences, The Open University, Walton Hall, Milton Keynes MK7 6AA, UK ARTICLE INFO ABSTRACT Keywords: Here we study rocks falling from exposed outcrops of bedrock, which have left tracks on the slope over which Mars, surface they have bounced and/or rolled, in fresh impact craters (1–10 km in diameter) on Mars. The presence of these Thermal stress tracks shows that these rocks have fallen relatively recently because aeolian processes are known to infill Ices topographic lows over time. Mapping of rockfall tracks indicate trends in frequency with orientation, which in Solar radiation � � turn depend on the latitudinal position of the crater. Craters in the equatorial belt (between 15 N and 15 S) Weathering exhibit higher frequencies of rockfall on their north-south oriented slopes compared to their east-west ones. � Craters >15 N/S have notably higher frequencies on their equator-facing slopes as opposed to the other ori entations. We computed solar radiation on the surface of crater slopes to compare insolation patterns with the spatial distribution of rockfalls, and found statistically significant correlations between maximum diurnal inso lation and rockfall frequency. -
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. -
The Mineralogy and Sedimentary History of the Glen Torridon Region, Gale Crater, Mars
52nd Lunar and Planetary Science Conference 2021 (LPI Contrib. No. 2548) 1519.pdf THE MINERALOGY AND SEDIMENTARY HISTORY OF THE GLEN TORRIDON REGION, GALE CRATER, MARS. M. T. Thorpe1*, T. F. Bristow2, E. B. Rampe1, J. P. Grotzinger3, V. K. Fox3, K. A. Bennett4, A. B. Bryk5 A. S. Yen6, A. R. VasavaDa6, D. T Vaniman7, V. Tu1, A. H. Treiman8, S. M. Morrison9, D. W. Ming1, R. V. Morris1, A.C. McAdam10, C.A. Malespin11, P. R. Mahaffy10, R. M. Hazen9, S. Gupta11, R. T. Downs12, G. W. Downs12, D. J. DesMarais2, P. I. Craig7, S. J. Chipera7, N. Castle8, D. F. Blake2, anD C. N. Achilles10, 1NASA JSC, Houston ([email protected]), TX, 2NASA Ames Research Center, 3Caltech, 4USGS, 5Univ. California, Berkeley, 6JPL/Caltech, 7PSI, 8LPI, 9Carnegie Institute, 10NASA GSFC, 11Imperial College, 12Univ. Arizona. Introduction: Gale crater was selecteD as member, two Different drill samples from both Glen Curiosity’s lanDing site largely because, from orbit, Etive (GE anD GE2) and Mary Anning (MA and MA3) phyllosilicate-rich strata were identifieD on the slopes of localities as well as Groken (GR) from the Knockfarril Mt. Sharp [1,2]. This phyllosilicate unit was later Hill member, the Glasgow (GG) target from the FIU, dubbed the Glen Torridon (GT) region, and the rover and Hutton (HU) from directly below the contact of the has been traversing this region since early January 2019. FIU anD Greenheugh pediment. Drill powder from each On Earth, phyllosilicates in the rock recorD preserve a sample was DelivereD to the CheMin X-ray history of aqueous conditions, overprinted with diffractometer (XRD). -
A Review of Sample Analysis at Mars-Evolved Gas Analysis Laboratory Analog Work Supporting the Presence of Perchlorates and Chlorates in Gale Crater, Mars
minerals Review A Review of Sample Analysis at Mars-Evolved Gas Analysis Laboratory Analog Work Supporting the Presence of Perchlorates and Chlorates in Gale Crater, Mars Joanna Clark 1,* , Brad Sutter 2, P. Douglas Archer Jr. 2, Douglas Ming 3, Elizabeth Rampe 3, Amy McAdam 4, Rafael Navarro-González 5,† , Jennifer Eigenbrode 4 , Daniel Glavin 4 , Maria-Paz Zorzano 6,7 , Javier Martin-Torres 7,8, Richard Morris 3, Valerie Tu 2, S. J. Ralston 2 and Paul Mahaffy 4 1 GeoControls Systems Inc—Jacobs JETS Contract at NASA Johnson Space Center, Houston, TX 77058, USA 2 Jacobs JETS Contract at NASA Johnson Space Center, Houston, TX 77058, USA; [email protected] (B.S.); [email protected] (P.D.A.J.); [email protected] (V.T.); [email protected] (S.J.R.) 3 NASA Johnson Space Center, Houston, TX 77058, USA; [email protected] (D.M.); [email protected] (E.R.); [email protected] (R.M.) 4 NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA; [email protected] (A.M.); [email protected] (J.E.); [email protected] (D.G.); [email protected] (P.M.) 5 Institito de Ciencias Nucleares, Universidad Nacional Autonoma de Mexico, Mexico City 04510, Mexico; [email protected] 6 Centro de Astrobiología (INTA-CSIC), Torrejon de Ardoz, 28850 Madrid, Spain; [email protected] 7 Department of Planetary Sciences, School of Geosciences, University of Aberdeen, Aberdeen AB24 3FX, UK; [email protected] 8 Instituto Andaluz de Ciencias de la Tierra (CSIC-UGR), Armilla, 18100 Granada, Spain Citation: Clark, J.; Sutter, B.; Archer, * Correspondence: [email protected] P.D., Jr.; Ming, D.; Rampe, E.; † Deceased 28 January 2021. -
Pplanetary Materials Research At
N. L. CHABOT ET AL . Planetary Materials Research at APL Nancy L. Chabot, Catherine M. Corrigan, Charles A. Hibbitts, and Jeffrey B. Plescia lanetary materials research offers a unique approach to understanding our solar system, one that enables numerous studies and provides insights that are not pos- sible from remote observations alone. APL scientists are actively involved in many aspects of planetary materials research, from the study of Martian meteorites, to field work on hot springs and craters on Earth, to examining compositional analogs for asteroids. Planetary materials research at APL also involves understanding the icy moons of the outer solar system using analog materials, conducting experiments to mimic the conditions of planetary evolution, and testing instruments for future space missions. The diversity of these research projects clearly illustrates the abundant and valuable scientific contributions that the study of planetary materials can make to Pspace science. INTRODUCTION In most space science and astronomy fields, one is When people think of planetary materials, they com- limited to remote observations, either from telescopes monly think of samples returned by space missions. Plan- or spacecraft, to gather data about celestial objects and etary materials available for study do include samples unravel their origins. However, for studying our solar returned by space missions, such as samples of the Moon system, we are less limited. We have samples of plan- returned by the Apollo and Luna missions, comet dust etary materials from multiple bodies in our solar system. collected by the Stardust mission, and implanted solar We can inspect these samples, examine them in detail wind ions collected by the Genesis mission. -
Bevan Jones, R., Thapar, A., Rice, F., Mars, B., Agha, S., Smith, D. J., Merry, S., Stallard, P., Thapar, A., Jones, I., & Simpson , S
Bevan Jones, R., Thapar, A., Rice, F., Mars, B., Agha, S., Smith, D. J., Merry, S., Stallard, P., Thapar, A., Jones, I., & Simpson , S. (2020). A Digital Intervention for Adolescent Depression ‘MoodHwb’: Mixed- Methods Feasibility Evaluation. JMIR Mental Health, 7(7), [e14536]. https://doi.org/10.2196/14536 Publisher's PDF, also known as Version of record License (if available): CC BY Link to published version (if available): 10.2196/14536 Link to publication record in Explore Bristol Research PDF-document This is the final published version of the article (version of record). It first appeared online via JMIR Publications at https://mental.jmir.org/2020/7/e14536/. Please refer to any applicable terms of use of the publisher. University of Bristol - Explore Bristol Research General rights This document is made available in accordance with publisher policies. Please cite only the published version using the reference above. Full terms of use are available: http://www.bristol.ac.uk/red/research-policy/pure/user-guides/ebr-terms/ JMIR MENTAL HEALTH Bevan Jones et al Original Paper A Digital Intervention for Adolescent Depression (MoodHwb): Mixed Methods Feasibility Evaluation Rhys Bevan Jones1,2,3, PhD, MRCPsych; Anita Thapar1,2, PhD, FRCPsych; Frances Rice1,2, PhD; Becky Mars4, PhD; Sharifah Shameem Agha1,2,3, PhD; Daniel Smith5, MD, FRCPsych; Sally Merry6, MD, FRANZP; Paul Stallard7, PhD; Ajay K Thapar1,2, MD, PhD, MRCGP; Ian Jones1,2, PhD, MRCPsych; Sharon A Simpson8, PhD 1Division of Psychological Medicine and Clinical Neurosciences, -
Iv. Books, Articles and Essays, Dissertations
IV. BOOKS, ARTICLES AND ESSAYS, DISSERTATIONS N., I.: Dostoevski and George Sand: Two Opponents of the Anthill. In: Dostoevski and the Human Condition After a Century. A. Ugrinsky, F. Lambasa and V. K. Ozolins, eds. New York: Greenwood Press, 1986: 199-210. N., I.: A Nigilistka and a Communarde: Two Voices of the Nineteenth-Century Russian Intelligentka. In: Woman As Mediatrix: Essays on Nineteenth- Century European Women Writers. Edited by. A. H. Goldberger. New York: Greenwood Press, 1987: 145-158. (Contributions in Women's Studies, 73) [S. V. Kovalevskaia, A. V. Korvin-Krukovskaia and Dostoevskii] N., I.: The Serenity of Influence: The Literary Relationship of George Sand and Dostoevsky. In: George Sand: Collected Essays. J. Glasgow, ed. Troy, New York: Whitston, 1985: 110-25. Naafs, J.: Tussen goed en kwaad. In: Sociologische gids 47, 1 (2000): 54-56. [“Between good and evil” as illustrated in Dostoevskii] Nabokov, V. V.: Fedor Dostoevskii. In: Literaturnaia gazeta 36 (1990.09.05): 7. Nabokov, V. V.: Fedor Dostoevskii. In: Russkie emigranty o Dostoevskom. Sankt- Peterburg: Andreev i sinov'ia, 1994: 378-85. Nabokov, V. V.: F'odor Dosotevski: Iz lektsiite za rus. literature. In: Teatur 45, 8-9 (1992): 33-35. Nabokov, V. V.: Fyodor Dostoevski. In: Nabokov, V. V. Lectures on Russian literature. Ed. with an introduction by F. Bowers. NY: Harcourt Brace, Jovanovich, 1981: 97-135. Nabokov, V. V.: Lektsii po russkoi literature: Chekhov, Dostoevskii, Gogol’, Gor’kii, Tolstoi, Turgenev. Predisl. Iv. Tolstogo. Moskva: Nezavisimaia gazeta, 1996. 440p. Nabokov, V. V.: Nabokov on Dostoevsky. In: New York Times Magazine (1981.08.23): 35+ [excerpt from Lectures on Russian Literature] Nad"iarnykh, N. -
Mars Science Laboratory Landing
PRESS KIT/JULY 2012 Mars Science Laboratory Landing Media Contacts Dwayne Brown NASA’s Mars 202-358-1726 Steve Cole Program 202-358-0918 Headquarters [email protected] Washington [email protected] Guy Webster Mars Science Laboratory 818-354-5011 D.C. Agle Mission 818-393-9011 Jet Propulsion Laboratory [email protected] Pasadena, Calif. [email protected] Science Payload Investigations Alpha Particle X-ray Spectrometer: Ruth Ann Chicoine, Canadian Space Agency, Saint-Hubert, Québec, Canada; 450-926-4451; [email protected] Chemistry and Camera: James Rickman, Los Alamos National Laboratory, Los Alamos, N.M.; 505-665-9203; [email protected] Chemistry and Mineralogy: Rachel Hoover, NASA Ames Research Center, Moffett Field, Calif.; 650-604-0643; [email protected] Dynamic Albedo of Neutrons: Igor Mitrofanov, Space Research Institute, Moscow, Russia; 011-7-495-333-3489; [email protected] Mars Descent Imager, Mars Hand Lens Imager, Mast Camera: Michael Ravine, Malin Space Science Systems, San Diego; 858-552-2650 extension 591; [email protected] Radiation Assessment Detector: Donald Hassler, Southwest Research Institute; Boulder, Colo.; 303-546-0683; [email protected] Rover Environmental Monitoring Station: Luis Cuesta, Centro de Astrobiología, Madrid, Spain; 011-34-620-265557; [email protected] Sample Analysis at Mars: Nancy Neal Jones, NASA Goddard Space Flight Center, Greenbelt, Md.; 301-286-0039; [email protected] Engineering Investigation MSL Entry, Descent and Landing Instrument Suite: Kathy Barnstorff, NASA Langley Research Center, Hampton, Va.; 757-864-9886; [email protected] Contents Media Services Information. -
The Impact Origin and Evolution of Chryse Planitia on Mars Revealed by Buried Craters
ARTICLE https://doi.org/10.1038/s41467-019-12162-0 OPEN The impact origin and evolution of Chryse Planitia on Mars revealed by buried craters Lu Pan 1, Cathy Quantin-Nataf1, Sylvain Breton1 & Chloé Michaut 1 Large impacts are one of the most important processes shaping a planet’s surface. On Mars, the early formation of the Martian crust and the lack of large impact basins (only four unambiguously identified: Hellas, Argyre, Utopia, and Isidis) indicates that a large part of ’ 1234567890():,; early records of Mars impact history is missing. Here we show, in Chryse Planitia, the scarcity of buried impact craters in a near-circular area could be explained by a pre-existing topographic depression with more intense resurfacing. Spatially correlated with positive Bouguer anomaly, this near-circular region with a diameter of ~1090 km likely originated from an impact. This proposed large impact basin must have been quickly relaxed or buried after its formation more than 4.0 billion years ago and heavily modified by subsequent resurfacing events. We anticipate our study to open a new window to unravelling the buried records of early Martian bombardment record. 1 Université de Lyon, Université Claude Bernard Lyon 1, ENS de Lyon, CNRS, UMR 5276 Laboratoire de Géologie de Lyon -Terre, Planètes, Environnement, 69622 Villeurbanne, France. Correspondence and requests for materials should be addressed to L.P. (email: [email protected]) NATURE COMMUNICATIONS | (2019) 10:4257 | https://doi.org/10.1038/s41467-019-12162-0 | www.nature.com/naturecommunications 1 ARTICLE NATURE COMMUNICATIONS | https://doi.org/10.1038/s41467-019-12162-0 arge basin-forming impacts significantly modified planetary could be the original Chryse impact basin, which subsequently surfaces and crusts, especially in the first billion years of underwent heavy degradation. -
Ahotrod Forthesolar System
AAcover07-0809.qxd:.qxd 6/18/09 11:47 AM Page 1 7-8 AEROSPACE AMERICA July-August 2009 JULY-AUGUST 2009 Ahotrod forthesolar system ABL aims at final tests Business aircraft market falls hard APUBLICATIONOFTHEAMERICANINSTITUTEOFAERONAUTICSANDASTRONAUTICS toc.jul-aug2009.qxd:AA Template 6/19/09 12:00 PM Page 1 July-August 2009 DEPARTMENTS Page 8 EDITORIAL 3 A worthwhile effort all around. INTERNATIONAL BEAT 4 Page 20 Fuel efficiency improvements escalate. ASIA UPDATE 8 Joining the space race, carefully. WASHINGTON WATCH 12 Looking to new leaders. CONVERSATIONS 16 With Ken Hodgkins. VIEW FROM HERE 20 Page 26 Four test flights that boosted Apollo 11. INDUSTRY INSIGHTS 24 Navigation satellites fuel payload growth. AIRCRAFT UPDATE 26 Business aircraft market falls hard. HONORS & AWARDS 30 OUT OF THE PAST 50 CAREER OPPORTUNITIES 54 Page 32 FEATURES GOCE ADDS GRAVITY TO ESA’S AGENDA 32 ESA’s Gravity Field and Steady State Ocean Circulation Explorer satellite will provide new insights into one of Earth’s most fundamental forces. by J.R.Wilson A HOT ROD FOR THE SOLAR SYSTEM 38 An astronaut’s concept for a plasma rocket that could get to Mars in a month Page 38 is due for a space workout. by Frank Sietzen Jr. AIRBORNE LASER AIMS AT FINAL TESTS 44 After achieving breakthroughs once believed impossible, the Airborne Laser may soon be ready for practical use in combat. by J.R.Wilson BULLETIN Page 44 AIAA Meeting Schedule B2 AIAA Courses and Training Program B4 AIAA News B5 Meetings Programs B18 Calls for Papers B30 COVER ESA’s Gravity Field and Steady State Ocean Circulation Explorerer,now in orbit,will be taking measurements that will provide a whole new level of understanding abut gravity.To learn more ,turn to the story beginning on page 32. -
Seeds and Supplies 2021
FEDCO 2021 Seeds and Supplies Where Is erthing Ordering Instructions page 160 Order Forms pages 161-166 Complete Index inside back cover begin on page Welcome to Fedco’s rd ear Vegetable Seeds 5 “May you live in interesting times”… redux. Herb Seeds 79 How eerily prescient it was to invoke that adage a year Flower Seeds 86 ago—and then to experience it play out as both a curse and a blessing. Onion Sets & Plants 110 So much has shifted in a year. In our last catalog we Ginger, turmeric, sweet potato 111 brought you interviews with innovators in agriculture whose Potatoes 111 wisdom spoke to a more inclusive, regenerative and Farm Seed / Cover Crops 118 holistic future. Those visions, with all the excitement and challenge they bring, are rapidly taking hold and Soil Amendments 124 rooting in the disturbance of 2020. Pest Control 134 We see it all around us: my son’s cul-de-sac Tools 140 organized to grow food together. Neighborhoods Books 151 started seed banks. Signs sprang up in towns for Planting Guides & Lists: Give & Take tables for garden produce, to share what you can and take what you need. Winona La Duke, in Vegetable Chart 77 her (online) Common Ground Fair keynote, stressed the Botanical Index 78 building of local infrastructures. If we look outside the Herb Chart 79 strident newsfeed, we see new structures evolving from Flower Chart 86 common values. Seed Longevity Charts 92, 106 So in this year’s interviews we take a closer look at Organic Variety List 104 what’s unfolding.