Shallow Crustal Composition of Mercury As Revealed by Spectral Properties and Geological Units of Two Impact Craters
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Washington Division of Geology and Earth Resources Open File Report
l 122 EARTHQUAKES AND SEISMOLOGY - LEGAL ASPECTS OPEN FILE REPORT 92-2 EARTHQUAKES AND Ludwin, R. S.; Malone, S. D.; Crosson, R. EARTHQUAKES AND SEISMOLOGY - LEGAL S.; Qamar, A. I., 1991, Washington SEISMOLOGY - 1946 EVENT ASPECTS eanhquak:es, 1985. Clague, J. J., 1989, Research on eanh- Ludwin, R. S.; Qamar, A. I., 1991, Reeval Perkins, J. B.; Moy, Kenneth, 1989, Llabil quak:e-induced ground failures in south uation of the 19th century Washington ity of local government for earthquake western British Columbia [abstract). and Oregon eanhquake catalog using hazards and losses-A guide to the law Evans, S. G., 1989, The 1946 Mount Colo original accounts-The moderate sized and its impacts in the States of Califor nel Foster rock avalanches and auoci earthquake of May l, 1882 [abstract). nia, Alaska, Utah, and Washington; ated displacement wave, Vancouver Is Final repon. Maley, Richard, 1986, Strong motion accel land, British Columbia. erograph stations in Oregon and Wash Hasegawa, H. S.; Rogers, G. C., 1978, EARTHQUAKES AND ington (April 1986). Appendix C Quantification of the magnitude 7.3, SEISMOLOGY - NETWORKS Malone, S. D., 1991, The HAWK seismic British Columbia earthquake of June 23, AND CATALOGS data acquisition and analysis system 1946. [abstract). Berg, J. W., Jr.; Baker, C. D., 1963, Oregon Hodgson, E. A., 1946, British Columbia eanhquak:es, 1841 through 1958 [ab Milne, W. G., 1953, Seismological investi earthquake, June 23, 1946. gations in British Columbia (abstract). stract). Hodgson, J. H.; Milne, W. G., 1951, Direc Chan, W.W., 1988, Network and array anal Munro, P. S.; Halliday, R. J.; Shannon, W. -
Copyrighted Material
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 -
Mercury's Low-Reflectance Material: Constraints from Hollows
Mercury’s low-reflectance material: Constraints from hollows Rebecca Thomas, Brian Hynek, David Rothery, Susan Conway To cite this version: Rebecca Thomas, Brian Hynek, David Rothery, Susan Conway. Mercury’s low-reflectance material: Constraints from hollows. Icarus, Elsevier, 2016, 277, pp.455-465. 10.1016/j.icarus.2016.05.036. hal-02271739 HAL Id: hal-02271739 https://hal.archives-ouvertes.fr/hal-02271739 Submitted on 27 Aug 2019 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. Accepted Manuscript Mercury’s Low-Reflectance Material: Constraints from Hollows Rebecca J. Thomas , Brian M. Hynek , David A. Rothery , Susan J. Conway PII: S0019-1035(16)30246-9 DOI: 10.1016/j.icarus.2016.05.036 Reference: YICAR 12084 To appear in: Icarus Received date: 23 February 2016 Revised date: 9 May 2016 Accepted date: 24 May 2016 Please cite this article as: Rebecca J. Thomas , Brian M. Hynek , David A. Rothery , Susan J. Conway , Mercury’s Low-Reflectance Material: Constraints from Hollows, Icarus (2016), doi: 10.1016/j.icarus.2016.05.036 This is a PDF file of an unedited manuscript that has been accepted for publication. As a service to our customers we are providing this early version of the manuscript. -
The Parliament of Poets: an Epic Poem
The Parliament of Poets “Like a story around a campfire.” —From the Audience “A great epic poem of startling originality and universal significance, in every way partaking of the nature of world literature.” —Dr. Hans-George Ruprecht, CKCU Literary News, Carleton University, Ottawa, Canada “A remarkable poem by a uniquely inspired poet, taking us out of time into a new and unspoken consciousness...” —Kevin McGrath, Lowell House, South Asian Studies, Harvard University “Mr. Glaysher has written an epic poem of major importance... Truly a major accomplishment and contribution to American Letters... A landmark achievement.” —ML Liebler, Department of English, Wayne State University, Detroit, Michigan “Glaysher is really an epic poet and this is an epic poem! Glaysher has written a masterpiece...” —James Sale (UK), The Society of Classical Poets “And a fine major work it is.” —Arthur McMaster, Contributing Editor, Poets’ Quarterly; Department of English, Converse College, Spartanburg, South Carolina “This Great Poem promises to be the defining Epic of the Age and will be certain to endure for many Centuries. Frederick Glaysher uses his great Poetic and Literary Skills in an artistic way that is unique for our Era and the Years to come. I strongly recommend this book to all those who enjoy the finest Poetry. A profound spiritual message for humanity.” —Alan Jacobs, Poet Writer Author, Amazon UK Review, London “Very readable and intriguingly enjoyable. A masterpiece that will stand the test of time.” —Poetry Cornwall, No. 36, England, UK “Bravo to the Poet for this toilsome but brilliant endeavour.” —Umme Salma, Transnational Literature, Flinders University, Adelaide, Australia “Am in awe of its brilliance.. -
Space Weathering on Mercury
Advances in Space Research 33 (2004) 2152–2155 www.elsevier.com/locate/asr Space weathering on Mercury S. Sasaki *, E. Kurahashi Department of Earth and Planetary Science, The University of Tokyo, Tokyo 113 0033, Japan Received 16 January 2003; received in revised form 15 April 2003; accepted 16 April 2003 Abstract Space weathering is a process where formation of nanophase iron particles causes darkening of overall reflectance, spectral reddening, and weakening of absorption bands on atmosphereless bodies such as the moon and asteroids. Using pulse laser irra- diation, formation of nanophase iron particles by micrometeorite impact heating is simulated. Although Mercurian surface is poor in iron and rich in anorthite, microscopic process of nanophase iron particle formation can take place on Mercury. On the other hand, growth of nanophase iron particles through Ostwald ripening or repetitive dust impacts would moderate the weathering degree. Future MESSENGER and BepiColombo mission will unveil space weathering on Mercury through multispectral imaging observations. Ó 2003 COSPAR. Published by Elsevier Ltd. All rights reserved. 1. Introduction irradiation should change the optical properties of the uppermost regolith surface of atmosphereless bodies. Space weathering is a proposed process to explain Although Hapke et al. (1975) proposed that formation spectral mismatch between lunar soils and rocks, and of iron particles with sizes from a few to tens nanome- between asteroids (S-type) and ordinary chondrites. ters should be responsible for the optical property Most of lunar surface and asteroidal surface exhibit changes, impact-induced formation of glassy materials darkening of overall reflectance, spectral reddening had been considered as a primary cause for space (darkening of UV–Vis relative to IR), and weakening of weathering. -
Case Fil Copy
NASA TECHNICAL NASA TM X-3511 MEMORANDUM CO >< CASE FIL COPY REPORTS OF PLANETARY GEOLOGY PROGRAM, 1976-1977 Compiled by Raymond Arvidson and Russell Wahmann Office of Space Science NASA Headquarters NATIONAL AERONAUTICS AND SPACE ADMINISTRATION • WASHINGTON, D. C. • MAY 1977 1. Report No. 2. Government Accession No. 3. Recipient's Catalog No. TMX3511 4. Title and Subtitle 5. Report Date May 1977 6. Performing Organization Code REPORTS OF PLANETARY GEOLOGY PROGRAM, 1976-1977 SL 7. Author(s) 8. Performing Organization Report No. Compiled by Raymond Arvidson and Russell Wahmann 10. Work Unit No. 9. Performing Organization Name and Address Office of Space Science 11. Contract or Grant No. Lunar and Planetary Programs Planetary Geology Program 13. Type of Report and Period Covered 12. Sponsoring Agency Name and Address Technical Memorandum National Aeronautics and Space Administration 14. Sponsoring Agency Code Washington, D.C. 20546 15. Supplementary Notes 16. Abstract A compilation of abstracts of reports which summarizes work conducted by Principal Investigators. Full reports of these abstracts were presented to the annual meeting of Planetary Geology Principal Investigators and their associates at Washington University, St. Louis, Missouri, May 23-26, 1977. 17. Key Words (Suggested by Author(s)) 18. Distribution Statement Planetary geology Solar system evolution Unclassified—Unlimited Planetary geological mapping Instrument development 19. Security Qassif. (of this report) 20. Security Classif. (of this page) 21. No. of Pages 22. Price* Unclassified Unclassified 294 $9.25 * For sale by the National Technical Information Service, Springfield, Virginia 22161 FOREWORD This is a compilation of abstracts of reports from Principal Investigators of NASA's Office of Space Science, Division of Lunar and Planetary Programs Planetary Geology Program. -
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 -
From Morpho-Stratigraphic to Geo(Spectro)-Stratigraphic Units: the PLANMAP Contribution
Planetary Geologic Mappers 2021 (LPI Contrib. No. 2610) 7045.pdf From morpho-stratigraphic to geo(spectro)-stratigraphic units: the PLANMAP contribution. Matteo Massironi1, Angelo Pio Rossi2, Jack Wright3, Francesca Zambon4, Claudia Poehler5, Lorenza Giacomini4, Cristian Carli4, Sabrina Ferrari6, Andrea Semenzato7, Erica Luzzi2, Riccardo Pozzobon6, Gloria Tognon6, David A. Rothery3, Carolyn Van der Bogert5, V. Galluzzi4, Francesca Altieri4 1Department of Geosciences, University of Padova, [email protected], 2Jacobs University Bremen, 3Open University, 4INAF-IAPS, 5Westfälische-Wilhelms Universität Münster 6CISAS, University of Padova 7Engineering Ingegneria Informatica S.p.A., Venezia Introduction: From the Apollo era onward, planetary ‘geologic’ mapping has been carried out using a photo-interpretative approach mainly on panchromatic and monochromatic images. This limits the definition of geological units to morpho-stratigraphic considerations so that units have been mainly defined by their stratigraphic position, surface textures and morphology, and attribution to general emplacement processes (a few related to magmatism, some broad sedimentary environments, some diverse impact domains, and all with uncertainties of interpretation). On the other hand, geological units on Earth are defined by several Figure 1: in-series interpretation from Giacomini et al. parameters besides the stratigraphic ones, such as rock EGU 2021-15052 textures, lithology, composition, and numerous environmental conditions of their origin (diverse Contextual interpretation: Geo(spectro)- magmatic, volcanic, metamorphic and sedimentary stratigraphic maps can be also produced directly from a environments). Hence, traditional morpho-stratigraphic contextual work on black and white images and RGB maps of planets and geological maps on the Earth are color compositions either using Principal Component still separated by an important conceptual and effective (PC) analysis (see Mercury examples in Semenzato et gap. -
Kaae, Leonard Kuuleinamoku, July 19, 2012 Leonard Kuuleinamoku Kaae, 84, of Honolulu, a Retired Hawaiian Tug & Barge Seaman and an Army Veteran, Died
Kaae, Leonard Kuuleinamoku, July 19, 2012 Leonard Kuuleinamoku Kaae, 84, of Honolulu, a retired Hawaiian Tug & Barge seaman and an Army veteran, died. He was born in Honolulu. He is survived by wife Ruth H. and sisters Ethel Hardley and Rose Giltner. Private services. [Honolulu Star-Advertiser 11 August 2012] Kaahanui, Agnes Lily Kahihiulaokalani, 77, of Honolulu, Hawaii, passed away June 14, 2012 at Kuakini Medical Center. Born July 10, 1934 in Honolulu, Hawaii. She was retired Maintenance Housekeeping Personel at Iolani Palace. She is survived by sons, Clifford Kalani (Marylyn) Kaahanui, Clyde Haumea Kaahanui, Cyrus Kamea Aloha Kaahanui, Hiromi (Jeanette) Fukuzawa; daughters, Katherine Ku’ulei Kaahanui, Kathleen Kuuipo (Arthur) Sing, Karen Kehaulani Kaahanui; 14 grandchildren; 10 great-grandchildren; sister, Rebecca Leimomi Naha. Visitation 10:00 a.m. Thursday (7/19) at Mililani Downtown Mortuary, Funeral Service 11:00 a.m., Burial 2:00 p.m. at Hawaiian Memorial Park Cemetery. Casual Attire. Flowers Welcome. [Honolulu Star-Advertiser 17 July 2012] Kaahanui, Agnes Lily Kahihiulaokalani, June 14, 2012 Agnes Lily Kahihiulaokalani Kaahanui, 77, of Honolulu, a retired Iolani Palace maintenance housekeeping worker, died in Kuakini Medical Center. She was born in Honolulu. She is survived by sons Clifford K., Clyde H. and Cyrus K. Kaahanui, and Hiromi Fukuzawa; daughters Katherine K. and Karen K. Kaahanui, and Kathleen K. Sing; sister Rebecca L. Naha; 14 grandchildren; and 10 great- grandchildren. Visitation: 10 a.m. Thursday at Mililani Downtown Mortuary. Services: 11 a.m. Burial: 2 p.m. at Hawaiian Memorial Park. Casual attire. Flowers welcome. [Honolulu Star- Advertiser 17 July 2012] Kaahanui, Carolyn Luana, July 21, 2012 Carolyn Luana Kaahanui, 59, of Kahului, a Makena Surf housekeeping department employee, died in Maui Memorial Medical Center. -
Arxiv:2012.11628V3 [Astro-Ph.EP] 26 Jan 2021
manuscript submitted to JGR: Planets The Fundamental Connections Between the Solar System and Exoplanetary Science Stephen R. Kane1, Giada N. Arney2, Paul K. Byrne3, Paul A. Dalba1∗, Steven J. Desch4, Jonti Horner5, Noam R. Izenberg6, Kathleen E. Mandt6, Victoria S. Meadows7, Lynnae C. Quick8 1Department of Earth and Planetary Sciences, University of California, Riverside, CA 92521, USA 2Planetary Systems Laboratory, NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA 3Planetary Research Group, Department of Marine, Earth, and Atmospheric Sciences, North Carolina State University, Raleigh, NC 27695, USA 4School of Earth and Space Exploration, Arizona State University, Tempe, AZ 85287, USA 5Centre for Astrophysics, University of Southern Queensland, Toowoomba, QLD 4350, Australia 6Johns Hopkins University Applied Physics Laboratory, Laurel, MD 20723, USA 7Department of Astronomy, University of Washington, Seattle, WA 98195, USA 8Planetary Geology, Geophysics and Geochemistry Laboratory, NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA Key Points: • Exoplanetary science is rapidly expanding towards characterization of atmospheres and interiors. • Planetary science has similarly undergone rapid expansion of understanding plan- etary processes and evolution. • Effective studies of exoplanets require models and in-situ data derived from plan- etary science observations and exploration. arXiv:2012.11628v4 [astro-ph.EP] 8 Aug 2021 ∗NSF Astronomy and Astrophysics Postdoctoral Fellow Corresponding author: Stephen R. Kane, [email protected] {1{ manuscript submitted to JGR: Planets Abstract Over the past several decades, thousands of planets have been discovered outside of our Solar System. These planets exhibit enormous diversity, and their large numbers provide a statistical opportunity to place our Solar System within the broader context of planetary structure, atmospheres, architectures, formation, and evolution. -
March 21–25, 2016
FORTY-SEVENTH LUNAR AND PLANETARY SCIENCE CONFERENCE PROGRAM OF TECHNICAL SESSIONS MARCH 21–25, 2016 The Woodlands Waterway Marriott Hotel and Convention Center The Woodlands, Texas INSTITUTIONAL SUPPORT Universities Space Research Association Lunar and Planetary Institute National Aeronautics and Space Administration CONFERENCE CO-CHAIRS Stephen Mackwell, Lunar and Planetary Institute Eileen Stansbery, NASA Johnson Space Center PROGRAM COMMITTEE CHAIRS David Draper, NASA Johnson Space Center Walter Kiefer, Lunar and Planetary Institute PROGRAM COMMITTEE P. Doug Archer, NASA Johnson Space Center Nicolas LeCorvec, Lunar and Planetary Institute Katherine Bermingham, University of Maryland Yo Matsubara, Smithsonian Institute Janice Bishop, SETI and NASA Ames Research Center Francis McCubbin, NASA Johnson Space Center Jeremy Boyce, University of California, Los Angeles Andrew Needham, Carnegie Institution of Washington Lisa Danielson, NASA Johnson Space Center Lan-Anh Nguyen, NASA Johnson Space Center Deepak Dhingra, University of Idaho Paul Niles, NASA Johnson Space Center Stephen Elardo, Carnegie Institution of Washington Dorothy Oehler, NASA Johnson Space Center Marc Fries, NASA Johnson Space Center D. Alex Patthoff, Jet Propulsion Laboratory Cyrena Goodrich, Lunar and Planetary Institute Elizabeth Rampe, Aerodyne Industries, Jacobs JETS at John Gruener, NASA Johnson Space Center NASA Johnson Space Center Justin Hagerty, U.S. Geological Survey Carol Raymond, Jet Propulsion Laboratory Lindsay Hays, Jet Propulsion Laboratory Paul Schenk,