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NITROGEN on MARS: INSIGHTS from CURIOSITY. J. C. Stern1 , B. Sutter2, W. A. Jackson3, Rafael Na- Varro-González4, Christopher P
Lunar and Planetary Science XLVIII (2017) 2726.pdf 1 2 3 NITROGEN ON MARS: INSIGHTS FROM CURIOSITY. J. C. Stern , B. Sutter , W. A. Jackson , Rafael Na- varro-González4, Christopher P. McKay5, Douglas W. Ming6, P. Douglas Archer2, D. P. Glavin1, A. G. Fairen7,8 and Paul R. Mahaffy1. 1NASA GSFC, Code 699, Greenbelt, MD 20771, [email protected], 2Jacobs, NASA Johnson Space Center, Houston, TX 77058, 3Texas Tech University, Lubbock, TX 79409, 4Universidad Nacional Autónoma de México, México, D.F. 04510, Mexico, 5NASA Ames Research Center, Moffett Field, CA 94035, 6NASA Johnson Space Center, Houston TX 77058, 7Centro de Astrobiologia, Madrid, Spain, 8Cornell University, Ithaca, NY 14853 Introduction: Recent detection of nitrate on Mars [1] indicates that nitrogen fixation processes occurred in early martian history. Data collected by the Sample Analysis at Mars (SAM) instrument on the Curiosity Rover can be integrated with Mars analog work in order to better understand the fixation and mobility of nitrogen on Mars, and thus its availability to putative biology. In particular, the relationship between nitrate and other soluble salts may help reveal the timing of nitrogen fixation and post-depositional behavior of nitrate on Mars. In addition, in situ measurements of nitrogen abundance and isotopic composition may be used to model atmospheric conditions on early Mars. Methods: The data presented are from analyses of solid Martian drilled and scooped samples by the Sam- ple Analysis at Mars (SAM) instrument suite on the Mars Science Laboratory (MSL) Curiosity Rover. SAM performs evolved gas analysis (EGA), in which a 3 Figure 1. -
Non-Collider Searches for Stable Massive Particles
Non-collider searches for stable massive particles S. Burdina, M. Fairbairnb, P. Mermodc,, D. Milsteadd, J. Pinfolde, T. Sloanf, W. Taylorg aDepartment of Physics, University of Liverpool, Liverpool L69 7ZE, UK bDepartment of Physics, King's College London, London WC2R 2LS, UK cParticle Physics department, University of Geneva, 1211 Geneva 4, Switzerland dDepartment of Physics, Stockholm University, 106 91 Stockholm, Sweden ePhysics Department, University of Alberta, Edmonton, Alberta, Canada T6G 0V1 fDepartment of Physics, Lancaster University, Lancaster LA1 4YB, UK gDepartment of Physics and Astronomy, York University, Toronto, ON, Canada M3J 1P3 Abstract The theoretical motivation for exotic stable massive particles (SMPs) and the results of SMP searches at non-collider facilities are reviewed. SMPs are defined such that they would be suffi- ciently long-lived so as to still exist in the cosmos either as Big Bang relics or secondary collision products, and sufficiently massive such that they are typically beyond the reach of any conceiv- able accelerator-based experiment. The discovery of SMPs would address a number of important questions in modern physics, such as the origin and composition of dark matter and the unifi- cation of the fundamental forces. This review outlines the scenarios predicting SMPs and the techniques used at non-collider experiments to look for SMPs in cosmic rays and bound in mat- ter. The limits so far obtained on the fluxes and matter densities of SMPs which possess various detection-relevant properties such as electric and magnetic charge are given. Contents 1 Introduction 4 2 Theory and cosmology of various kinds of SMPs 4 2.1 New particle states (elementary or composite) . -
Perchlorate and Chlorate Biogeochemistry in Ice-Covered Lakes of the Mcmurdo Dry Valleys, Antarctica
Available online at www.sciencedirect.com Geochimica et Cosmochimica Acta 98 (2012) 19–30 www.elsevier.com/locate/gca Perchlorate and chlorate biogeochemistry in ice-covered lakes of the McMurdo Dry Valleys, Antarctica W. Andrew Jackson a,⇑, Alfonso F. Davila b,c, Nubia Estrada a, W. Berry Lyons d, John D. Coates e, John C. Priscu f a Department of Civil and Environmental Engineering, Texas Tech University, Lubbock, TX 79409, USA b NASA Ames Research Center, Moffett Field, CA 95136, USA c SETI Institute, 189 Bernardo Ave., Suite 100, Mountain View, CA 94043-5203, USA d Byrd Polar Research Center, The Ohio State University, Columbus, OH 43210, USA e Department of Plant and Microbial Biology, University of California, Berkeley, CA 94720, USA f Department of Land Resources & Environmental Sciences, Montana State University, Bozeman, MT 59717, USA Received 15 February 2012; accepted in revised form 5 September 2012; available online 19 September 2012 Abstract À À We measured chlorate (ClO3 ) and perchlorate (ClO4 ) concentrations in ice covered lakes of the McMurdo Dry Valleys À À (MDVs) of Antarctica, to evaluate their role in the ecology and geochemical evolution of the lakes. ClO3 and ClO4 are À À present throughout the MDV Lakes, streams, and other surface water bodies. ClO3 and ClO4 originate in the atmosphere and are transported to the lakes by surface inflow of glacier melt that has been differentially impacted by interaction with soils À À and aeolian matter. Concentrations of ClO3 and ClO4 in the lakes and between lakes vary based on both total evaporative concentration, as well as biological activity within each lake. -
NO ONE KNOWS ABOUT US by Bridget Canning. a Creative Writing
NO ONE KNOWS ABOUT US By Bridget Canning. A Creative Writing Thesis submitted to the School of Graduate Studies in partial fulfillment of the requirements for the degree of Masters of Arts in English (Creative Writing) Department of English, Memorial University of Newfoundland Abstract: No One Knows about Us is a collection of twelve contemporary short stories. As the title suggests, the characters in each story deal with secrets: relationships, longings, grudges, addictions, and trickery. For them, these secrets are simultaneously overwhelming and futile; their importance within their small worlds reflect a deeper feeling of insignificance in the greater scheme of life in a small city in a northern province hemmed on to the side of a continent. Here are a range of characters and situations set in St. John’s, Newfoundland and Labrador. The stories are mapped out in different areas of the city and move chronologically over a year, starting in fall and ending in late summer. They work together to create a small sample of life in modern-day St. John’s – one that is informed by the influences of history, economy, and weather. i Acknowledgements: This thesis would not have been accomplished without the help of the English department faculty at Memorial such as Robert Finley, Robert Chafe, and especially my thesis advisor, Lisa Moore. Thanks to the Graduate Society for their financial support. Thanks to Jonathan Weir, Deirdre Snook, and the members of the Naked Parade Writing Collective for their guidance and encouragement. ii Contents: 1. Seen, p. 1 2. With Glowing Hearts, p. 19 3. -
In Pdf Format
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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. -
The Mcmurdo Dry Valleys of Antarctica As an Analog for Past and Present Martian Surface Processes
51st Lunar and Planetary Science Conference (2020) 1777.pdf THE MCMURDO DRY VALLEYS OF ANTARCTICA AS AN ANALOG FOR PAST AND PRESENT MARTIAN SURFACE PROCESSES. M. R. Salvatore1, J. S. Levy2, J. W. Head3, and J. L. Dickson4, 1Department of Astronomy and Planetary Science, Northern Arizona University, [email protected], 2Dept. of Geology, Colgate University, 3Dept. of Earth, Environmental, and Planetary Sciences, Brown University, 4Division of Geological and Planetary Sciences, Caltech. Introduction: The McMurdo Dry Valleys (MDV) of observed on Mars. We also highlight where additional Antarctica have been considered a valuable martian work in the MDV is necessary to address outstanding analog since the Viking era of Mars exploration [1]. Over questions in martian science. the past two decades, our understanding of martian Cold and Icy Early Mars?: The apparent environmental and geologic evolution has significantly disagreement between observed fluvial and lacustrine improved thanks to the plethora of orbital and landed landforms and the inability for global climate models to missions. New observations have raised many new produce mean annual temperatures greater than 0º C enigmatic questions about how cold and dry geological suggest that the martian surface was possibly never systems evolve, which has revitalized the MDV as an clement from a terrestrial perspective. Instead of a long- important terrestrial analog for Mars, from its earliest lived and continuously active hydrological system on recorded geologic history [2] to the present [3]. early Mars, is it possible that hydrological activity was Global martian climate models struggle to produce more episodic through punctuated climatic excursions on consistently warm and wet conditions at the martian an otherwise cold and icy early Mars? The fluvial and surface early in its history, even with the aid of additional lacustrine systems of the MDV are one possible analog greenhouse gases to offset the distance between Mars and where localized climatic optima drive local hydrological the faint young Sun [4]. -
Daily Shipping Newsletter 2004 – 038
DAILY SHIPPING NEWSLETTER 2004 – 038 Number 038 ****DAILY SHIPPING NEWSLETTER****Friday 16-04-2004 THIS NEWSLETTER IS BROUGHT TO YOU BY : VLIERODAM WIRE ROPES Ltd. wire ropes, chains, hooks, shackles, webbing slings, lifting beams, crane blocks, turnbuckles etc. Binnenbaan 36 3161VB RHOON The Netherlands Telephone: (+31)105018000 (+31) 105015440 (a.o.h.) Fax : (+31)105013843 Internet & E-mail www.vlierodam.nl [email protected] Jan de Nul´s CHRISTOFORO COLOMBO Photo: Peter Andriessen © PSi-Daily Shipping News Page 1 4/15/2004 DAILY SHIPPING NEWSLETTER 2004 – 038 EVENTS, INCIDENTS & OPERATIONS Bow Mariner survivors testify SURVIVING crewmembers of the ill-fated Bow Mariner are finally telling their stories, but it may be some time before we hear them. Granted immunity from US prosecution, the four crewmen from the Singapore-flagged chemical tanker that exploded and sank on 28 February off Virginia are giving evidence to a federal grand jury, a testimony that is held secret. Two of the six surviving crew had already given their evidence to Coast Guard investigators and the first of the remaining four testified on Friday. Rating Ramon Ronquillo spent 90 minutes with the grand jury before leaving the closed- door proceedings. The other three are scheduled to testify Wednesday in Norfolk, Virginia. While the four have been granted immunity in the US – a demand from their lawyers before they would talk – Singapore has not granted immunity. The Bow Mariner was carrying 11,570 tonnes of ethanol as well diesel fuel and fuel oil when it exploded and sank on its way from New York to Houston. -
Stratigraphy and Topography of Mcmurdo Crater Area, Planum
Mars Polar Science 2000 4101.pdf STRATIGRAPHY AND TOPOGRAPHY OF MCMURDO CRATER AREA, PLANUM AUSTRALE MARS: IMPLICATIONS FOR RESURFACING HISTORY AND POROUS CHARACTER OF THE SOUTH POLAR LAYERED DEPOSITS. K. L. Tanaka1, P. H. Schultz2, and K. E. Herkenhoff1, 1U.S. Geo- logical Survey, 2255 N. Gemini Dr., Flagstaff, AZ 86001, [email protected], 2Department of Geological Sciences, Brown University, Providence, RI, [email protected]. Introduction: McMurdo Crater (84.5¡S, 0¡W) is ondaries are unevenly distributed, apparently due to the largest extant impact (~23 km diameter) that has local burial and perhaps erosion [1,2]. On Planum scarred the south polar layered deposits (SPLD) of Australe, a smooth mantle of variable albedo (unit Planum Australe, Mars. It occurs along the margin of Apm in Fig. 3) appears to bury the secondaries. This the SLPD and formed a broad field of secondary craters unit; mapped as SPLD (unit Apl) in previous mapping across the planum. These secondaries as well as other [3], might form the uppermost SPLD below the resid- associated features serve as both (1) key stratigraphic ual ice cap (unit Api) as well as deposits on broad, flat markers that provide a basis for resolving stages in the terraces southeast of McMurdo. resurfacing history of the SPLD, and (2) important Peripheral to Planum Australe, the stratigraphy is indicators of the SPLD substrate character. less clear because of apparent eolian mantling. Hilly McMurdo Crater: Table 1 shows crater mor- terrain may be made up of degraded ancient highland phology parameters measured from Viking images material (unit HNu), whereas as undulating, locally (421B77-80) and 18 MOLA profiles currently available high-standing material may be an outlier of SPLD across the crater . -
Ross Island Trail System Mcmurdo Station & Scott Base, Antarctica
Ross Island Trail System McMurdo Station & Scott Base, Antarctica Ross Island Trail System Recreational Routes CAL Seasonal Trail Please visit the McMurdo Intranet eFoot Plan site for further route information (route marked with trail signs) markers in mi (km): e.g. 1.22 (1.96) CRL Castle Rock Loop Trail & CRS Castle Rock Summit Trail (9.65 mi / 15.53 km) (0.1 mi / 0.17 km) IR Access Road (shared with vehicles) CRS This trip leads to the prominent landform called Castle Rock, named for its buttress-like shape. The Castle Rock routes are the most ambitious hikes, ski or runs in the McMurdo area. As you traverse across the snow and ice field, you see the prominent 0.11 (0.17) landform of Castle Rock ahead, spectacular views to the north, and the Transantarctic Mountains to the east. The route is also Castle Rock a large loop that extends to Castle Rock and ends at Scott Base. More adventurous hikers may want to attempt the Castle Rock Restricted Road Summit route. This route entails scrambling, exposed rock faces and the use of a fixed line as a handhold and should never be (no recreational travel) attempted without an experienced person in your group. The Castle Rock Summit is only open at certain periods due to safety CASTLE ROCK FALL CRL concerns. January 30, 1995 Check-in/Check-out 1 death (Building 182 Firehouse) HPR Hut Point Ridge Loop Trail 1.33 (2.13) (2.63 mi / 4.24 km) The Hut Point Ridge Loop Trail is one of the newest additions to recreation opportunities in the Ross Island area. -
Global Catastrophes in Earth History
GLOBAL CATASTROPHES IN EARTH HISTORY An Interdisciplinary Conference on Impacts, Volcanism, and Mass Mortality Snowbird, Utah October 20-23, 1988 N89-2 12E7 --?HEW- Sponsored by The Lunar and Planetary Institute and The National Academy of Sciences Abstracts Presented to the Topical Conference Global Catastrophes in Earth History: An Interdisciplinary Conference on Impacts, Volcanism, and Mass Mortality Snowbird, Utah October 20 - 23,1988 Sponsored by Lunar and Planetary Institute and The National Academy of Sciences LPI Contribution No. 673 Compiled in 1988 Lunar and Planetary Institute Material in this volume may be copied without restraint for library, abstract service, educational, or personal research purposes; however, republication of any paper or portion thereof requires the written permission of the authors as well as appropriate acknowledgment of this publication. PREFACE This volume contains abstracts that have been accepted for presentation at the topical conference Global Catastrophes in Earth History: An Interdisciplinary Conference on Impacts, Volcanism and Mass Mortality. The Organizing Committee consisted of Robert Ginsburg, Chairman, University of Miami; Kevin Burke, Lunar and Planetary Institute; Lee M. Hunt, National Research Council; Digby McLaren, University of Ottawa; Thomas Simkin, National Museum of Natural History; Starley L. Thompson, National Center for Atmospheric Research; Karl K. Turekian, Yale University; George W. Wetherill, Carnegie Institution of Washington. Logistics and administrative support were provided by the Projects Ofice at the Lunar and Planetary Institute. This abstract volume was prepared by the Publications Office staff at the Lunar and Planetary Institute. The Lunar and Planetary Institute is operated by the Universities Space Research Association under contract No. NASW-4066 with the National Aeronautics and Space Administration. -
Do Young Martian Ray Craters Have Ages Consistent with the Crater Count System?
Icarus 208 (2010) 621–635 Contents lists available at ScienceDirect Icarus journal homepage: www.elsevier.com/locate/icarus Do young martian ray craters have ages consistent with the crater count system? William K. Hartmann a,*, Cathy Quantin b, Stephanie C. Werner c, Olga Popova d a Planetary Science Institute, 1700 E. Ft. Lowell Rd., Suite 106, Tucson, AZ 85719-2395, United States b Laboratoire des Sciences de la Terre, Université Claude Bernard, Lyon1, 2, rue Raphaël Dubois, 69622 Villeurbanne Cedex, France c Physics of Geological Processes, University of Oslo, PO 1048 Blindern, 0316 Oslo, Norway d Institute for Dynamics of Geospheres, Russian Academy of Sciences, Leninsky Prospekt 38, Bldg. 1, 119334 Moscow, Russia article info abstract Article history: McEwen et al. (McEwen, A.S., Preblich, B.S., Turtle, E.P., Artemieva, N.A., Golombek, M.P., Hurst, M., Kirk, Received 9 September 2009 R.L., Burr, D.M., Christensen, P. [2005]. Icarus 176, 351–381) developed a useful test for the internal con- Revised 19 February 2010 sistency of crater-count chronometry systems. They argued that certain multi-kilometer, fresh-looking Accepted 24 March 2010 martian craters with prominent rays should be the youngest or near-youngest craters in their size range. Available online 21 April 2010 The ‘‘McEwen et al. test” is that the ages determined from crater densities of the smallest superimposed craters (typically diameter D 5–20 m) should thus be comparable to the expected formation intervals Keywords: of the host primary. McEwen et al. concluded from MOC data that crater chronometry failed this test by Crater chronology factors of 700–2000.