The Kuehlthau Family Foundation

Total Page:16

File Type:pdf, Size:1020Kb

The Kuehlthau Family Foundation July 9 — October 1, 2017 Lead Sponsor: The Kuehlthau Family Foundation Awards Sponsors: Anonymous Alice Chang Huntsville Museum of Art Docents Susan and Robert Kuehlthau Kelly and Randy Schrimsher Anne and Ed Uher Additional Supporters: Alabama State Council on the Arts Altherr Howard Design Huntsville Museum of Art Guild Copyright © 2017 Huntsville Museum of Art All rights reserved ISBN 1-885820-48-8 Catalogue Design, Illustration & Production: Betty Altherr Howard New Market, AL Photography: The Individual Artists Jeff White Huntsville, AL Printing: Colonial Printing Huntsville, AL Huntsville Museum of Art 300 Church Street Southwest Huntsville, AL 35801 USA 256.535.4350 www.hsvmuseum.org The Red Clay Survey is organized by Peter J. Baldaia, Director of Curatorial Affairs, and David J. Reyes, Curator of Exhibitions and Collections of the Huntsville Museum of Art, to highlight outstanding regional contemporary art. Contents Foreword & Acknowledgments 4 Museum Purchase Awards 5 Juror’s Comments 8 Juror’s Awards 10 The Exhibition 17 Exhibition Checklist 61 Foreword & Acknowledgments by Peter J. Baldaia Director of Curatorial Affairs of the Huntsville Museum of Art The Huntsville Museum of Art is very pleased Purves — for their hard work on behalf of to present the 2017 edition of The Red Clay this endeavor. Thanks also go to graphic Survey exhibition of contemporary Southern designer Betty Altherr Howard for providing art. Since its inception in 1988, this recurring a handsomely designed exhibition competition has provided a showcase for announcement and catalogue, and for her current art in our region through a critical meticulous supervision of all aspects of their selection of work from eleven Southern production. states. This year’s Survey features 81 works by 54 artists, juried by distinguished artist Public and private support provides the and educator Gerry Bergstein. As always, foundation for this exhibition. We are honored the exhibition took shape through a to recognize The Kuehlthau Family Foundation comprehensive two-fold process. The first as the lead sponsor of The Red Clay Survey. stage online review of images reduced an We are also grateful to The Alabama State initial field of nearly 1,500 submissions to Council on the Arts, Altherr Howard Design, 105 works by 72 artists. The second stage, and The Huntsville Museum of Art Guild, on-site review of actual works determined for providing additional project support. final inclusions and cash awards. For the Special thanks go to the following generous exhibition juror, the responsibility of sifting underwriters of artist awards: The Huntsville through such an abundance of material Museum Docents — Museum Purchase Awards; to formulate the exhibition is formidable. Susan and Robert Kuehlthau — Juror’s Choice Bergstein rose to the occasion with a diverse Award; Kelly and Randy Schrimsher — and well-considered selection of works that Alabama Artist Award; Anonymous Donor — celebrate maturity of vision, mastery of Merit Awards; Alice Chang — Merit Award and materials, and the unique artistic voice, People’s Choice Award; and Anne and Ed Uher serving the exhibition well. — Merit Awards. For the Museum, the logistics of organizing Finally, we extend our appreciation to each and managing a multi-faceted project of this artist represented in the 2017 Red Clay scale requires great team effort. Many thanks Survey, for providing impressive evidence go to the entire staff — with special thanks to of the unique strength and enduring vitality Curator of Exhibitions and Collections, David of contemporary Southern art. Reyes, and Curatorial Assistant, Katherine 4 Museum Purchase Award Sponsored by the Huntsville Museum of Art Docents Fragmented Transmogrification, 2016, saggar fired clay Robert Detamore born in 1947, Americus, Georgia lives in Barnesville, Georgia 2008 Group Exhibition, Art House Gallery, Atlanta, GA SCAD Foundation Faculty Group Exhibition, Savannah 1976 BVA Georgia State University, Atlanta, GA College of Art & Design, Savannah, GA 1978 MFA University of Georgia, Athens, GA Honors & Awards 2009 — Present, Assistant Professor of Art, Visual Arts, Gordon State College, Barnesville, GA 2015 First Place, Second Place, Third Place and Honorable Mention, Georgia National Fair, Perry, GA Recent Exhibitions 2013 First Place Ceramics and Artist’s Award, Georgia National Fair, Perry, GA 2016 Academy/Academia Exhibition, Marietta/Cobb Museum of Art, Marietta, GA Museum & University Collections 2012 Two Person Ceramic Sculpture Exhibition, Lamar Arts, Barnesville, GA Albany Museum of Art, Albany, GA 2010 Delta National Small Print Exhibition, Arkansas State Baltimore Museum of Art, Baltimore, MD University, Jonesboro, AR Brooklyn Museum of Art, Brooklyn, NY 2009 32nd Bradley International Print and Drawing Exhibition, Greenville County Museum of Art, Greenville, SC Bradley University, Peoria, IL High Museum of Art, Atlanta, GA 50th Anniversary Atlanta College of Art Faculty Exhibition, Hunterdon Art Center, Clinton, NJ Woodruff Arts Center, Atlanta, GA Macon Museum of Arts and Science, Macon, GA 5 Museum Purchase Award Sponsored by the Huntsville Museum of Art Docents Wolf River Harbor Nocturne, 2016, oil on linen panel Marc Rouillard born in 1959, St. Louis, Missouri lives in Memphis, Tennessee 1981 AFA Graphic Communications, St. Louis Community College — Florissant Valley, St. Louis, MO 1983 BFA Advertising Design, Memphis College of Art, Number: Presents Art of the South 2015, Memphis Memphis,TN College of Art, Memphis, TN (also 2014) 2011 MFA Studio Art, Memphis College of Art, Memphis, TN River Arts Fest Invitational Show, Askew Nixon Ferguson Architects, Memphis, TN 2000 — Present, Instructor, Memphis College of Art, Memphis, TN Sideshow, LM Gallery 363, Memphis, TN Recent Exhibitions 57th Annual Delta Exhibition, Arkansas Arts Center, Little Rock, AR 2016 Idle Speed Only, Jay Etkin Gallery, Memphis, TN 2014 Biennial Alumni Exhibition 2014, Memphis College of Art, Watercolor USA, Springfield Art Museum, Springfield, MO Memphis, TN 2015 Commonplace, Memphis College of Art, Memphis, TN Horn Island 30 Selects, Gallery Ten Ninety-One, Horn Island Influences, Walter Anderson Museum of Art, Memphis, TN Ocean Springs, MS 2013 TEXT-URE, Jay Etkin Gallery, Santa Fe, NM MCA Inaugural Faculty Biennial, Memphis College of Art, Works on Paper, New Concept Gallery, Santa Fe, NM Memphis, TN 6 Museum Purchase Award Sponsored by the Huntsville Museum Association Cultivated, 2015, mixed media Ted Whisenhunt born in 1973, Birmingham, Alabama lives in Young Harris, Georgia 1995 BFA Sculpture, Birmingham-Southern College, 2007 The Red Clay Survey: 2007 Exhibition of Contemporary Birmingham, AL Southern Art, Huntsville Museum of Art, Huntsville, AL 1998 MFA Florida State University, Tallahassee, FL Honors & Awards 2009 — Present, Associate Professor of Art/Art Department Chair, Young Harris College, Young Harris, GA 2008 Grantee: Smithsonian Institute Traveling Exhibtion “New Harmonies”, Alabama Humanities Recent Exhibitions Foundation/Alabama State Council for the Arts, Montgomery, AL 2016 Cultivated (solo Eexhibition), The Rymer Gallery, 2007 Visiting Artist Grant, Hale County, AL Nashville, TN; Georgia State University, Atlanta, GA 2014 Alabama Sculpture Invitational, The Evelyn Burrow Museum & University Collections Museum, Hanceville, AL 2009 Two Person Invitational, Alabama Artist Gallery, Fayette Art Museum, Fayette, AL Montgomery, AL Judson College, Marion, AL 7 Juror’s Comments I very much enjoyed engaging with the terrific work The diversity of the work was quite striking. Many submitted to this year’s Red Clay Survey. My overall disciplines were represented as well as many approaches impression was that it was smart without being academic, to technique, form, and content. Such diversity is very imaginative, vibrant in expression, and liberated in its healthy and desirable. Work ranged from vehement to unselfconscious exercise of freedom. The painful difficulty almost silent, from manic to melancholic, from tightly came in the process of eliminating work and granting controlled to explosive — this list could go on for quite awards. There was much more wonderful work than a while. What counts is not the choice of what to available space could accommodate. I viewed each piece investigate, but the depth of the investigation. In a show several times, first online and then in person. I let my such as this, the distance between works can add to the impressions evolve slowly. I was not a judge in the sense depth of the viewing experience. Conversations between of reaching evaluations according to a rulebook, for such different visions can be as exciting as a single vision. I a book does not exist in the multifaceted world of hope that my selections will spark resonances between contemporary art. Instead I ended up including work that individual artworks and lead viewers to compare and touched my heart, mind, and spirit more deeply with contrast the different visions of these artists with the each repeated viewing. Some works were ambitiously often contradictory complexity of their own visions of virtuosic and others quite subtle and understated. Some the world. seemed to grow while others diminished. Of course, had there been even more time I might have reached different Gerry Bergstein conclusions. Such are the vagaries of experiencing art. Cambridge, Massachusetts 8 Gerry Bergstein born in 1945, New York, New York lives in Cambridge, Massachusetts 1969 BFA Painting, School of
Recommended publications
  • Curiosity's Candidate Field Site in Gale Crater, Mars
    Curiosity’s Candidate Field Site in Gale Crater, Mars K. S. Edgett – 27 September 2010 Simulated view from Curiosity rover in landing ellipse looking toward the field area in Gale; made using MRO CTX stereopair images; no vertical exaggeration. The mound is ~15 km away 4th MSL Landing Site Workshop, 27–29 September 2010 in this view. Note that one would see Gale’s SW wall in the distant background if this were Edgett, 1 actually taken by the Mastcams on Mars. Gale Presents Perhaps the Thickest and Most Diverse Exposed Stratigraphic Section on Mars • Gale’s Mound appears to present the thickest and most diverse exposed stratigraphic section on Mars that we can hope access in this decade. • Mound has ~5 km of stratified rock. (That’s 3 miles!) • There is no evidence that volcanism ever occurred in Gale. • Mound materials were deposited as sediment. • Diverse materials are present. • Diverse events are recorded. – Episodes of sedimentation and lithification and diagenesis. – Episodes of erosion, transport, and re-deposition of mound materials. 4th MSL Landing Site Workshop, 27–29 September 2010 Edgett, 2 Gale is at ~5°S on the “north-south dichotomy boundary” in the Aeolis and Nepenthes Mensae Region base map made by MSSS for National Geographic (February 2001); from MOC wide angle images and MOLA topography 4th MSL Landing Site Workshop, 27–29 September 2010 Edgett, 3 Proposed MSL Field Site In Gale Crater Landing ellipse - very low elevation (–4.5 km) - shown here as 25 x 20 km - alluvium from crater walls - drive to mound Anderson & Bell
    [Show full text]
  • Supervolcanoes Within an Ancient Volcanic Province in Arabia Terra, Mars 2 3 4 Joseph
    EMBARGOED BY NATURE 1 1 Supervolcanoes within an ancient volcanic province in Arabia Terra, Mars 2 3 4 Joseph. R. Michalski 1,2 5 1Planetary Science Institute, Tucson, Arizona 85719, [email protected] 6 2Dept. of Earth Sciences, Natural History Museum, London, United Kingdom 7 8 Jacob E. Bleacher3 9 3NASA Goddard Space Flight Center, Greenbelt, MD, USA. 10 11 12 Summary: 13 14 Several irregularly shaped craters located within Arabia Terra, Mars represent a 15 new type of highland volcanic construct and together constitute a previously 16 unrecognized martian igneous province. Similar to terrestrial supervolcanoes, these 17 low-relief paterae display a range of geomorphic features related to structural 18 collapse, effusive volcanism, and explosive eruptions. Extruded lavas contributed to 19 the formation of enigmatic highland ridged plains in Arabia Terra. Outgassed sulfur 20 and erupted fine-grained pyroclastics from these calderas likely fed the formation of 21 altered, layered sedimentary rocks and fretted terrain found throughout the 22 equatorial region. Discovery of a new type of volcanic construct in the Arabia 23 volcanic province fundamentally changes the picture of ancient volcanism and 24 climate evolution on Mars. Other eroded topographic basins in the ancient Martian 25 highlands that have been dismissed as degraded impact craters should be 26 reconsidered as possible volcanic constructs formed in an early phase of 27 widespread, disseminated magmatism on Mars. 28 29 30 EMBARGOED BY NATURE 2 31 The source of fine-grained, layered deposits1,2 detected throughout the equatorial 32 region of Mars3 remains unresolved, though the deposits are clearly linked to global 33 sedimentary processes, climate change, and habitability of the surface4.
    [Show full text]
  • 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.
    [Show full text]
  • 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.
    [Show full text]
  • 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.
    [Show full text]
  • Welcome Back: Fall 2014
    Keeping you in... The newsletter of the UA Department of Art and Art History! art.ua.edu Welcome Back: Fall 2014 WELCOME to our new office associates ANGIE BROWN (RIGHT) and MARTHA SEARS (BELOW), who have been with us for a few weeks this summer. Brown handles our budget and comes with lots of experi- ence in collections and bookkeeping. Sears established and managed a UA Students in Assistant Professor Pete campus ministry, Schulte’s class take an unusual approach to drawing from nature. and worked as a financial aid specialist at Savannah College of Art and Design. If you Two of our instructors and a current grad student have opened a have not met them yet, please visit Garland new art space in Northport. The Grocery – founded by VIRGINIA 103 and introduce yourself. ECKINGER (MFA 2014), CLAIRE LEWIS EVANS (MFA candidate) and ANNE HERBERT (MFA 2013 and full-time instructor) – opened its Welcome to APRIL JEHAN MORRIS (RIGHT), doors on Art Night, September 4. This artist-run studio, exhibit our new Medievalist, who teaches and performance space emanates creative vibes from 900 Main graduate and undergraduate courses in Avenue in Northport, Alabama. If you missed Art Night, visit them Medieval and Ancient art. Morris taught in person or check out their lovely and informative website, previously at Bowdoin College, Kenyon http://www.groceryartplace.com/. College and the University of North Texas. Her research focuses on the visual and material cultures of the Crusades Our New Website and on the roles of symbol, material and metaphor in Romanesque France. Thanks to the fabulous design team at e-Tech, our 21st-century Department of Art and Art History now has a website that reflects Congratulations to LUCY CURZON, who our mission, our accessibility and our expanding horizons.
    [Show full text]
  • Crater Geometry and Ejecta Thickness of the Martian Impact Crater Tooting
    Meteoritics & Planetary Science 42, Nr 9, 1615–1625 (2007) Abstract available online at http://meteoritics.org Crater geometry and ejecta thickness of the Martian impact crater Tooting Peter J. MOUGINIS-MARK and Harold GARBEIL Hawai‘i Institute of Geophysics and Planetology, University of Hawai‘i, Honolulu, Hawai‘i 96822, USA (Received 25 October 2006; revision accepted 04 March 2007) Abstract–We use Mars Orbiter Laser Altimeter (MOLA) topographic data and Thermal Emission Imaging System (THEMIS) visible (VIS) images to study the cavity and the ejecta blanket of a very fresh Martian impact crater ~29 km in diameter, with the provisional International Astronomical Union (IAU) name Tooting crater. This crater is very young, as demonstrated by the large depth/ diameter ratio (0.065), impact melt preserved on the walls and floor, an extensive secondary crater field, and only 13 superposed impact craters (all 54 to 234 meters in diameter) on the ~8120 km2 ejecta blanket. Because the pre-impact terrain was essentially flat, we can measure the volume of the crater cavity and ejecta deposits. Tooting crater has a rim height that has >500 m variation around the rim crest and a very large central peak (1052 m high and >9 km wide). Crater cavity volume (i.e., volume below the pre-impact terrain) is ~380 km3 and the volume of materials above the pre-impact terrain is ~425 km3. The ejecta thickness is often very thin (<20 m) throughout much of the ejecta blanket. There is a pronounced asymmetry in the ejecta blanket, suggestive of an oblique impact, which has resulted in up to ~100 m of additional ejecta thickness being deposited down-range compared to the up-range value at the same radial distance from the rim crest.
    [Show full text]
  • 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.
    [Show full text]
  • For Irn on Schooner
    '• ■ i.C; i-k'Jr: ■•rtb ' ' '•■,'■ / o ) i > /jriUrt »• ‘ • yf< . r f 11r<‘» ‘if'i'ff'!• i « I'l < t ■> j 1 v i * ' ’ ■ > ■ • '•i ' A VA AC B DAILY OmODLAflOM •for Ihii MoBtk<«f iu u w y , IMS ' ■— .... ' « ^ .......... 5> of > tbo 2 7Andlt 0 o f CtaoalotioBO. (CtaMUtod Adforllilag oa flMra U .) VOL. U L , NO. 118 . SOUTH BIAN,CHESTER, CONN., FRH)AY, FEBRUARY 1 0 ,1 9 8 8 . (8i:m EN RAGES) PRICE THREE CENt^ PRESm ENT-ELECT ROOSETVSliT VISITS BAHAMAS 18 REBELS KILLED i — ON DUTCH CRUISER a - FOR IRN ON SCHOONER Twenty-ire hjiired When HHTAlirS ENVOY M rio e e n On Stolen SAIUIDESDAY Japanese to Refuse E j ^ Men and Two W o n n Crnisor Refnse To Obey Who b d Started Ont To Ordera— Later Snrrender. Sr RonaU Unkay Will Request of League Look For Misflig Yorth, Brins Rqnrt On War Tokyo, Feb. 10.— (A P )—^An offi-^ maintaining that Japaneie-spon- A re ThemadTes Losfa Not Batavia, Java, Peb. 10.— (A P ) — dal statement that Japan wlU rei sored government in Manchuria, a EIgbteen men were killed and 25 In- ply with an emphatic "no" to a government spokesman said today Heard From For Over 40 juxod aboard the rebeDioua Dutch Debts To hreadent-HecL and that Chinese -u)verelgnty to League of Nations’ request for a Manchuria is ended forever, not­ cruiser de Zeven Provinden when a statement of Japan’s attitude to­ withstanding reports that toe b iB R — Yonth Sonfdd Ro* naval fighting plane dropped a London, Feb.
    [Show full text]
  • 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.
    [Show full text]
  • In Pdf Format
    lós 1877 Mik 88 ge N 18 e N i h 80° 80° 80° ll T 80° re ly a o ndae ma p k Pl m os U has ia n anum Boreu bal e C h o A al m re u c K e o re S O a B Bo l y m p i a U n d Planum Es co e ria a l H y n d s p e U 60° e 60° 60° r b o r e a e 60° l l o C MARS · Korolev a i PHOTOMAP d n a c S Lomono a sov i T a t n M 1:320 000 000 i t V s a Per V s n a s l i l epe a s l i t i t a s B o r e a R u 1 cm = 320 km lkin t i t a s B o r e a a A a A l v s l i F e c b a P u o ss i North a s North s Fo d V s a a F s i e i c a a t ssa l vi o l eo Fo i p l ko R e e r e a o an u s a p t il b s em Stokes M ic s T M T P l Kunowski U 40° on a a 40° 40° a n T 40° e n i O Va a t i a LY VI 19 ll ic KI 76 es a As N M curi N G– ra ras- s Planum Acidalia Colles ier 2 + te .
    [Show full text]
  • 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.
    [Show full text]