A MESSENGER LOOK at BASIN ANTIPODES on MERCURY. David T. Blewett1, Brett W. Denevi2, Mark S. Robinson2, Carolyn M. Ernst1, Michael E
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Index Abulfeda crater chain (Moon), 97 Aphrodite Terra (Venus), 142, 143, 144, 145, 146 Acheron Fossae (Mars), 165 Apohele asteroids, 353–354 Achilles asteroids, 351 Apollinaris Patera (Mars), 168 achondrite meteorites, 360 Apollo asteroids, 346, 353, 354, 361, 371 Acidalia Planitia (Mars), 164 Apollo program, 86, 96, 97, 101, 102, 108–109, 110, 361 Adams, John Couch, 298 Apollo 8, 96 Adonis, 371 Apollo 11, 94, 110 Adrastea, 238, 241 Apollo 12, 96, 110 Aegaeon, 263 Apollo 14, 93, 110 Africa, 63, 73, 143 Apollo 15, 100, 103, 104, 110 Akatsuki spacecraft (see Venus Climate Orbiter) Apollo 16, 59, 96, 102, 103, 110 Akna Montes (Venus), 142 Apollo 17, 95, 99, 100, 102, 103, 110 Alabama, 62 Apollodorus crater (Mercury), 127 Alba Patera (Mars), 167 Apollo Lunar Surface Experiments Package (ALSEP), 110 Aldrin, Edwin (Buzz), 94 Apophis, 354, 355 Alexandria, 69 Appalachian mountains (Earth), 74, 270 Alfvén, Hannes, 35 Aqua, 56 Alfvén waves, 35–36, 43, 49 Arabia Terra (Mars), 177, 191, 200 Algeria, 358 arachnoids (see Venus) ALH 84001, 201, 204–205 Archimedes crater (Moon), 93, 106 Allan Hills, 109, 201 Arctic, 62, 67, 84, 186, 229 Allende meteorite, 359, 360 Arden Corona (Miranda), 291 Allen Telescope Array, 409 Arecibo Observatory, 114, 144, 341, 379, 380, 408, 409 Alpha Regio (Venus), 144, 148, 149 Ares Vallis (Mars), 179, 180, 199 Alphonsus crater (Moon), 99, 102 Argentina, 408 Alps (Moon), 93 Argyre Basin (Mars), 161, 162, 163, 166, 186 Amalthea, 236–237, 238, 239, 241 Ariadaeus Rille (Moon), 100, 102 Amazonis Planitia (Mars), 161 COPYRIGHTED -
Book of Abstracts: Studying Old Master Paintings
BOOK OF ABSTRACTS STUDYING OLD MASTER PAINTINGS TECHNOLOGY AND PRACTICE THE NATIONAL GALLERY TECHNICAL BULLETIN 30TH ANNIVERSARY CONFERENCE 1618 September 2009, Sainsbury Wing Theatre, National Gallery, London Supported by The Elizabeth Cayzer Charitable Trust STUDYING OLD MASTER PAINTINGS TECHNOLOGY AND PRACTICE THE NATIONAL GALLERY TECHNICAL BULLETIN 30TH ANNIVERSARY CONFERENCE BOOK OF ABSTRACTS 1618 September 2009 Sainsbury Wing Theatre, National Gallery, London The Proceedings of this Conference will be published by Archetype Publications, London in 2010 Contents Presentations Page Presentations (cont’d) Page The Paliotto by Guido da Siena from the Pinacoteca Nazionale of Siena 3 The rediscovery of sublimated arsenic sulphide pigments in painting 25 Marco Ciatti, Roberto Bellucci, Cecilia Frosinini, Linda Lucarelli, Luciano Sostegni, and polychromy: Applications of Raman microspectroscopy Camilla Fracassi, Carlo Lalli Günter Grundmann, Natalia Ivleva, Mark Richter, Heike Stege, Christoph Haisch Painting on parchment and panels: An exploration of Pacino di 5 The use of blue and green verditer in green colours in seventeenthcentury 27 Bonaguida’s technique Netherlandish painting practice Carole Namowicz, Catherine M. Schmidt, Christine Sciacca, Yvonne Szafran, Annelies van Loon, Lidwein Speleers Karen Trentelman, Nancy Turner Alterations in paintings: From noninvasive insitu assessment to 29 Technical similarities between mural painting and panel painting in 7 laboratory research the works of Giovanni da Milano: The Rinuccini -
Shallow Crustal Composition of Mercury As Revealed by Spectral Properties and Geological Units of Two Impact Craters
Planetary and Space Science 119 (2015) 250–263 Contents lists available at ScienceDirect Planetary and Space Science journal homepage: www.elsevier.com/locate/pss Shallow crustal composition of Mercury as revealed by spectral properties and geological units of two impact craters Piero D’Incecco a,n, Jörn Helbert a, Mario D’Amore a, Alessandro Maturilli a, James W. Head b, Rachel L. Klima c, Noam R. Izenberg c, William E. McClintock d, Harald Hiesinger e, Sabrina Ferrari a a Institute of Planetary Research, German Aerospace Center, Rutherfordstrasse 2, D-12489 Berlin, Germany b Department of Geological Sciences, Brown University, Providence, RI 02912, USA c The Johns Hopkins University Applied Physics Laboratory, Laurel, MD 20723, USA d Laboratory for Atmospheric and Space Physics, University of Colorado, Boulder, CO 80303, USA e Westfälische Wilhelms-Universität Münster, Institut für Planetologie, Wilhelm-Klemm Str. 10, D-48149 Münster, Germany article info abstract Article history: We have performed a combined geological and spectral analysis of two impact craters on Mercury: the Received 5 March 2015 15 km diameter Waters crater (106°W; 9°S) and the 62.3 km diameter Kuiper crater (30°W; 11°S). Using Received in revised form the Mercury Dual Imaging System (MDIS) Narrow Angle Camera (NAC) dataset we defined and mapped 9 October 2015 several units for each crater and for an external reference area far from any impact related deposits. For Accepted 12 October 2015 each of these units we extracted all spectra from the MESSENGER Atmosphere and Surface Composition Available online 24 October 2015 Spectrometer (MASCS) Visible-InfraRed Spectrograph (VIRS) applying a first order photometric correc- Keywords: tion. -
P U B L I C a T I E S
P U B L I C A T I E S 1 JANUARI – 31 DECEMBER 2001 2 3 INHOUDSOPGAVE Centrale diensten..............................................................................................................5 Coördinatoren...................................................................................................................8 Faculteit Letteren en Wijsbegeerte..................................................................................9 - Emeriti.........................................................................................................................9 - Vakgroepen...............................................................................................................10 Faculteit Rechtsgeleerdheid...........................................................................................87 - Vakgroepen...............................................................................................................87 Faculteit Wetenschappen.............................................................................................151 - Vakgroepen.............................................................................................................151 Faculteit Geneeskunde en Gezondheidswetenschappen............................................268 - Vakgroepen.............................................................................................................268 Faculteit Toegepaste Wetenschappen.........................................................................398 - Vakgroepen.............................................................................................................398 -
Picturing France
Picturing France Classroom Guide VISUAL ARTS PHOTOGRAPHY ORIENTATION ART APPRECIATION STUDIO Traveling around France SOCIAL STUDIES Seeing Time and Pl ace Introduction to Color CULTURE / HISTORY PARIS GEOGRAPHY PaintingStyles GOVERNMENT / CIVICS Paris by Night Private Inve stigation LITERATURELANGUAGE / CRITICISM ARTS Casual and Formal Composition Modernizing Paris SPEAKING / WRITING Department Stores FRENCH LANGUAGE Haute Couture FONTAINEBLEAU Focus and Mo vement Painters, Politics, an d Parks MUSIC / DANCENATURAL / DRAMA SCIENCE I y Fontainebleau MATH Into the Forest ATreebyAnyOther Nam e Photograph or Painting, M. Pa scal? ÎLE-DE-FRANCE A Fore st Outing Think L ike a Salon Juror Form Your Own Ava nt-Garde The Flo ating Studio AUVERGNE/ On the River FRANCHE-COMTÉ Stream of Con sciousness Cheese! Mountains of Fra nce Volcanoes in France? NORMANDY “I Cannot Pain tan Angel” Writing en Plein Air Culture Clash Do-It-Yourself Pointillist Painting BRITTANY Comparing Two Studie s Wish You W ere Here Synthétisme Creating a Moo d Celtic Culture PROVENCE Dressing the Part Regional Still Life Color and Emo tion Expressive Marks Color Collectio n Japanese Prin ts Legend o f the Château Noir The Mistral REVIEW Winds Worldwide Poster Puzzle Travelby Clue Picturing France Classroom Guide NATIONAL GALLERY OF ART, WASHINGTON page ii This Classroom Guide is a component of the Picturing France teaching packet. © 2008 Board of Trustees of the National Gallery of Art, Washington Prepared by the Division of Education, with contributions by Robyn Asleson, Elsa Bénard, Carla Brenner, Sarah Diallo, Rachel Goldberg, Leo Kasun, Amy Lewis, Donna Mann, Marjorie McMahon, Lisa Meyerowitz, Barbara Moore, Rachel Richards, Jennifer Riddell, and Paige Simpson. -
Geologic Map of the Victoria Quadrangle (H02), Mercury
H01 - Borealis Geologic Map of the Victoria Quadrangle (H02), Mercury 60° Geologic Units Borea 65° Smooth plains material 1 1 2 3 4 1,5 sp H05 - Hokusai H04 - Raditladi H03 - Shakespeare H02 - Victoria Smooth and sparsely cratered planar surfaces confined to pools found within crater materials. Galluzzi V. , Guzzetta L. , Ferranti L. , Di Achille G. , Rothery D. A. , Palumbo P. 30° Apollonia Liguria Caduceata Aurora Smooth plains material–northern spn Smooth and sparsely cratered planar surfaces confined to the high-northern latitudes. 1 INAF, Istituto di Astrofisica e Planetologia Spaziali, Rome, Italy; 22.5° Intermediate plains material 2 H10 - Derain H09 - Eminescu H08 - Tolstoj H07 - Beethoven H06 - Kuiper imp DiSTAR, Università degli Studi di Napoli "Federico II", Naples, Italy; 0° Pieria Solitudo Criophori Phoethontas Solitudo Lycaonis Tricrena Smooth undulating to planar surfaces, more densely cratered than the smooth plains. 3 INAF, Osservatorio Astronomico di Teramo, Teramo, Italy; -22.5° Intercrater plains material 4 72° 144° 216° 288° icp 2 Department of Physical Sciences, The Open University, Milton Keynes, UK; ° Rough or gently rolling, densely cratered surfaces, encompassing also distal crater materials. 70 60 H14 - Debussy H13 - Neruda H12 - Michelangelo H11 - Discovery ° 5 3 270° 300° 330° 0° 30° spn Dipartimento di Scienze e Tecnologie, Università degli Studi di Napoli "Parthenope", Naples, Italy. Cyllene Solitudo Persephones Solitudo Promethei Solitudo Hermae -30° Trismegisti -65° 90° 270° Crater Materials icp H15 - Bach Australia Crater material–well preserved cfs -60° c3 180° Fresh craters with a sharp rim, textured ejecta blanket and pristine or sparsely cratered floor. 2 1:3,000,000 ° c2 80° 350 Crater material–degraded c2 spn M c3 Degraded craters with a subdued rim and a moderately cratered smooth to hummocky floor. -
Updates on Geologic Mapping of Kuiper (H06) Quadrangle
EPSC Abstracts Vol. 12, EPSC2018-721-1, 2018 European Planetary Science Congress 2018 EEuropeaPn PlanetarSy Science CCongress c Author(s) 2018 Updates on geologic mapping of Kuiper (H06) quadrangle Lorenza Giacomini (1), Valentina Galluzzi (1), Cristian Carli (1), Matteo Massironi (2), Luigi Ferranti (3) and Pasquale Palumbo (4,1). (1) INAF, Istituto di Astrofisica e Planetologia Spaziali (IAPS), Rome, Italy ([email protected]); (2) Dipartimento di Geoscienze, Università degli Studi di Padova, Padua, Italy; (3) DISTAR, Università degli Studi di Napoli Federico II, Naples, Italy; (4) Dipartimento di Scienze & Tecnologie, Università degli Studi di Napoli ‘Parthenope’, Naples, Italy. 1. Introduction -C3 craters. They represent fresh craters with sharp rim and extended bright and rayed ejecta; Kuiper quadrangle is located at the equatorial zone of -C2 craters. Moderate degraded craters whose rim is Mercury and encompasses the area between eroded but clearly detectable. Extensive ejecta longitudes 288°E – 360°E and latitudes 22.5°N – blankets are still present; 22.5°S. The quadrangle was previously mapped for -C1 craters. Very degraded craters with an almost its most part by [2] that, using Mariner10 data, completely obliterated rim. Ejecta are very limited or produced a final 1:5M scale map of the area. In this absent. work we present the preliminary results of a more Different plain units were also identified and classified as: detailed geological map (1:3M scale) of the Kuiper - Intercrater plains. Densely cratered terrains, quadrangle that we compiled using the higher characterized by a rough surface texture. They resolution MESSENGER data. represent the more extended plains on the quadrangle; - Intermediate plains. -
Thomas Robert Watters
THOMAS ROBERT WATTERS Address: Center for Earth and Planetary Studies National Air and Space Museum Smithsonian Institution P. O. Box 37012, Washington, DC 20013-7012 Education: George Washington University, Ph.D., Geology (1981-1985). Bryn Mawr College, M.A., Geology (1977-1979). West Chester University, B.S. (magna cum laude), Earth Sciences (1973-1977). Experience: Senior Scientist, Center for Earth and Planetary Studies, National Air and Space Museum, Smithsonian Institution (1998-present). Chairman, Center for Earth and Planetary Studies, National Air and Space Museum, Smithsonian Institution (1989-1998). Research Geologist, Center for Earth and Planetary Studies, Smithsonian Institution, Planetary Geology and Tectonics, Structural Geology, Tectonophysics (1981-1989). Research Assistant, Department of Terrestrial Magnetism, Carnegie Institution of Washington, Chemical Analysis and Fission Track Studies of Meteorites (1980-1981). Research Fellowship, American Museum of Natural History, Electron Microprobe and Petrographic Study of Aubrites and Related Meteorites (1978-1980). Teaching Assistant, Bryn Mawr College (1977-1979), Physical and Historical Geology, Crystallography and Optical Crystallography. Undergraduate Assistant, West Chester University (1973-1977), Teaching Assistant in General and Advanced Astronomy, Physical and Historical Geology. Honors: William P. Phillips Memorial Scholarship (West Chester University); National Air and Space Museum Certificate of Award 1983, 1986, 1989, 1991, 1992, 2002, 2004; American Geophysical Union Editor's Citation for Excellence in Refereeing - Journal Geophysical Research-Planets, 1992; Smithsonian Exhibition Award - Earth Today: A Digital View of Our Dynamic Planet, 1999; Certificate of Appreciation, Geological Society of America, 2005, 2006; Elected to Fellowship in the Geological Society of America, 2007. The Johns Hopkins University Applied Physics Laboratory 2009 Publication Award - Outstanding Research Paper, “Return to Mercury: A Global Perspective on MESSENGER’s First Mercury Flyby (S.C. -
CRATER IMAGE METADATA EARTH IMAGES Country Or BMM Date Camera/ Lens Focal Image Image ID# LAT
CRATER IMAGE METADATA EARTH IMAGES Country or BMM Date Camera/ Lens Focal Image Image ID# LAT. LONG. Crater Name Geographic Acquired Instrument Length # Region E4: Kodak ISS006-E-16068 27.8S 16.4E Roter Kamm Namibia 12/28/2002 400 mm 1 DCS760C E4: Kodak ISS012-E-15881 51.5N 68.5W Manicouagan Canada 1/24/2006 50 mm 2 DCS760C E4: Kodak ISS014-E-11841 24.4N 24.4E Oasis Libya 1/13/2007 400 mm 3 DCS760C E4: Kodak ISS014-E-15775 35N 111W Barringer United States 3/1/2007 400 mm 4 DCS760C E4: Kodak ISS014-E-19496 29N 7.6W Ouarkziz Algeria 4/16/2007 800 mm 5 DCS760C E4: Kodak ISS015-E-17360 23.9S 132.3E Gosses Bluff Australia 7/13/2007 400 mm 6 DCS760C ISS018-E-14908 22.9N 10.4W Tenoumer Mauritania 12/20/2008 Nikon D2X 800 mm 7 ISS018-E-23713 20N 76.5E Lonar India 1/28/2009 Nikon D2X 800 mm 8 STS51I-33-56AA 27S 27.3E Vredefort South Africa 8/29/1985 Hasselblad 250 mm Clearwater STS61A-35-86 56.5N 74.7W Lakes Canada 11/1/1985 Hasselblad 250 mm (East & West) ISS028-E-14782 25.52S 120.53E Shoemaker Australia 7/6/2011 Nikon D2X 200 mm ISS034-E-29105 17.32S 128.25E Piccaninny Australia 1/15/2013 Nikon D2X 180 mm CRATER IMAGE METADATA MARS IMAGES BMM Geographic *Date or Camera/ Image Image ID# LAT. LONG. Crater Name Approx. YR Mission Name Region Instrument # Acquired PIA14290 5.4S 137.8E Gale Aeolis Mensae 2000's THEMIS IR Odyssey THEMIS IR Aeolis 14.5S 175.4E Gusev 2000's THEMIS IR Odyssey MOSAIC Quadrangle Mars Orbiter Colorized MOLA 42S 67E Hellas Basin Hellas Planitia 2000's Laser Altimeter Global Surveyor (MOLA) Viking Orbiter Margaritifer Visual -
Large Impact Basins on Mercury: Global Distribution, Characteristics, and Modification History from MESSENGER Orbital Data Caleb I
JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 117, E00L08, doi:10.1029/2012JE004154, 2012 Large impact basins on Mercury: Global distribution, characteristics, and modification history from MESSENGER orbital data Caleb I. Fassett,1 James W. Head,2 David M. H. Baker,2 Maria T. Zuber,3 David E. Smith,3,4 Gregory A. Neumann,4 Sean C. Solomon,5,6 Christian Klimczak,5 Robert G. Strom,7 Clark R. Chapman,8 Louise M. Prockter,9 Roger J. Phillips,8 Jürgen Oberst,10 and Frank Preusker10 Received 6 June 2012; revised 31 August 2012; accepted 5 September 2012; published 27 October 2012. [1] The formation of large impact basins (diameter D ≥ 300 km) was an important process in the early geological evolution of Mercury and influenced the planet’s topography, stratigraphy, and crustal structure. We catalog and characterize this basin population on Mercury from global observations by the MESSENGER spacecraft, and we use the new data to evaluate basins suggested on the basis of the Mariner 10 flybys. Forty-six certain or probable impact basins are recognized; a few additional basins that may have been degraded to the point of ambiguity are plausible on the basis of new data but are classified as uncertain. The spatial density of large basins (D ≥ 500 km) on Mercury is lower than that on the Moon. Morphological characteristics of basins on Mercury suggest that on average they are more degraded than lunar basins. These observations are consistent with more efficient modification, degradation, and obliteration of the largest basins on Mercury than on the Moon. This distinction may be a result of differences in the basin formation process (producing fewer rings), relaxation of topography after basin formation (subduing relief), or rates of volcanism (burying basin rings and interiors) during the period of heavy bombardment on Mercury from those on the Moon. -
High-Resolution Topography of Mercury from Messenger Orbital Stereo Imaging – the Southern Hemisphere Quadrangles
The International Archives of the Photogrammetry, Remote Sensing and Spatial Information Sciences, Volume XLII-3, 2018 ISPRS TC III Mid-term Symposium “Developments, Technologies and Applications in Remote Sensing”, 7–10 May, Beijing, China HIGH-RESOLUTION TOPOGRAPHY OF MERCURY FROM MESSENGER ORBITAL STEREO IMAGING – THE SOUTHERN HEMISPHERE QUADRANGLES F. Preusker 1 *, J. Oberst 1,2, A. Stark 1, S. Burmeister 2 1 German Aerospace Center (DLR), Institute of Planet. Research, Berlin, Germany – (stephan.elgner, frank.preusker, alexander.stark, juergen.oberst)@dlr.de 2 Technical University Berlin, Institute for Geodesy and Geoinformation Sciences, Berlin, Germany – (steffi.burmeister, juergen.oberst)@tu-berlin.de Commission VI, WG VI/4 KEY WORDS: Mercury, MESSENGER, Digital Terrain Models ABSTRACT: We produce high-resolution (222 m/grid element) Digital Terrain Models (DTMs) for Mercury using stereo images from the MESSENGER orbital mission. We have developed a scheme to process large numbers, typically more than 6000, images by photogrammetric techniques, which include, multiple image matching, pyramid strategy, and bundle block adjustments. In this paper, we present models for map quadrangles of the southern hemisphere H11, H12, H13, and H14. 1. INTRODUCTION Mercury requires sophisticated models for calibrations of focal length and distortion of the camera. In particular, the WAC The MErcury Surface, Space ENviorment, GEochemistry, and camera and NAC camera were demonstrated to show a linear Ranging (MESSENGER) spacecraft entered orbit about increase in focal length by up to 0.10% over the typical range of Mercury in March 2011 to carry out a comprehensive temperatures (-20 to +20 °C) during operation, which causes a topographic mapping of the planet. -
Back Matter (PDF)
Index Page numbers in italic denote Figures. Page numbers in bold denote Tables. ‘a’a lava 15, 82, 86 Belgica Rupes 272, 275 Ahsabkab Vallis 80, 81, 82, 83 Beta Regio, Bouguer gravity anomaly Aino Planitia 11, 14, 78, 79, 83 332, 333 Akna Montes 12, 14 Bhumidevi Corona 78, 83–87 Alba Mons 31, 111 Birt crater 378, 381 Alba Patera, flank terraces 185, 197 Blossom Rupes fold-and-thrust belt 4, 274 Albalonga Catena 435, 436–437 age dating 294–309 amors 423 crater counting 296, 297–300, 301, 302 ‘Ancient Thebit’ 377, 378, 388–389 lobate scarps 291, 292, 294–295 anemone 98, 99, 100, 101 strike-slip kinematics 275–277, 278, 284 Angkor Vallis 4,5,6 Bouguer gravity anomaly, Venus 331–332, Annefrank asteroid 427, 428, 433 333, 335 anorthosite, lunar 19–20, 129 Bransfield Rift 339 Antarctic plate 111, 117 Bransfield Strait 173, 174, 175 Aphrodite Terra simple shear zone 174, 178 Bouguer gravity anomaly 332, 333, 335 Bransfield Trough 174, 175–176 shear zones 335–336 Breksta Linea 87, 88, 89, 90 Apollinaris Mons 26,30 Brumalia Tholus 434–437 apollos 423 Arabia, mantle plumes 337, 338, 339–340, 342 calderas Arabia Terra 30 elastic reservoir models 260 arachnoids, Venus 13, 15 strike-slip tectonics 173 Aramaiti Corona 78, 79–83 Deception Island 176, 178–182 Arsia Mons 111, 118, 228 Mars 28,33 Artemis Corona 10, 11 Caloris basin 4,5,6,7,9,59 Ascraeus Mons 111, 118, 119, 205 rough ejecta 5, 59, 60,62 age determination 206 canali, Venus 82 annular graben 198, 199, 205–206, 207 Canary Islands flank terraces 185, 187, 189, 190, 197, 198, 205 lithospheric flexure