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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. -
Impact Melt Emplacement on Mercury
Western University Scholarship@Western Electronic Thesis and Dissertation Repository 7-24-2018 2:00 PM Impact Melt Emplacement on Mercury Jeffrey Daniels The University of Western Ontario Supervisor Neish, Catherine D. The University of Western Ontario Graduate Program in Geology A thesis submitted in partial fulfillment of the equirr ements for the degree in Master of Science © Jeffrey Daniels 2018 Follow this and additional works at: https://ir.lib.uwo.ca/etd Part of the Geology Commons, Physical Processes Commons, and the The Sun and the Solar System Commons Recommended Citation Daniels, Jeffrey, "Impact Melt Emplacement on Mercury" (2018). Electronic Thesis and Dissertation Repository. 5657. https://ir.lib.uwo.ca/etd/5657 This Dissertation/Thesis is brought to you for free and open access by Scholarship@Western. It has been accepted for inclusion in Electronic Thesis and Dissertation Repository by an authorized administrator of Scholarship@Western. For more information, please contact [email protected]. Abstract Impact cratering is an abrupt, spectacular process that occurs on any world with a solid surface. On Earth, these craters are easily eroded or destroyed through endogenic processes. The Moon and Mercury, however, lack a significant atmosphere, meaning craters on these worlds remain intact longer, geologically. In this thesis, remote-sensing techniques were used to investigate impact melt emplacement about Mercury’s fresh, complex craters. For complex lunar craters, impact melt is preferentially ejected from the lowest rim elevation, implying topographic control. On Venus, impact melt is preferentially ejected downrange from the impact site, implying impactor-direction control. Mercury, despite its heavily-cratered surface, trends more like Venus than like the Moon. -
Cfa in the News ~ Week Ending 3 January 2010
Wolbach Library: CfA in the News ~ Week ending 3 January 2010 1. New social science research from G. Sonnert and co-researchers described, Science Letter, p40, Tuesday, January 5, 2010 2. 2009 in science and medicine, ROGER SCHLUETER, Belleville News Democrat (IL), Sunday, January 3, 2010 3. 'Science, celestial bodies have always inspired humankind', Staff Correspondent, Hindu (India), Tuesday, December 29, 2009 4. Why is Carpenter defending scientists?, The Morning Call, Morning Call (Allentown, PA), FIRST ed, pA25, Sunday, December 27, 2009 5. CORRECTIONS, OPINION BY RYAN FINLEY, ARIZONA DAILY STAR, Arizona Daily Star (AZ), FINAL ed, pA2, Saturday, December 19, 2009 6. We see a 'Super-Earth', TOM BEAL; TOM BEAL, ARIZONA DAILY STAR, Arizona Daily Star, (AZ), FINAL ed, pA1, Thursday, December 17, 2009 Record - 1 DIALOG(R) New social science research from G. Sonnert and co-researchers described, Science Letter, p40, Tuesday, January 5, 2010 TEXT: "In this paper we report on testing the 'rolen model' and 'opportunity-structure' hypotheses about the parents whom scientists mentioned as career influencers. According to the role-model hypothesis, the gender match between scientist and influencer is paramount (for example, women scientists would disproportionately often mention their mothers as career influencers)," scientists writing in the journal Social Studies of Science report (see also ). "According to the opportunity-structure hypothesis, the parent's educational level predicts his/her probability of being mentioned as a career influencer (that ism parents with higher educational levels would be more likely to be named). The examination of a sample of American scientists who had received prestigious postdoctoral fellowships resulted in rejecting the role-model hypothesis and corroborating the opportunity-structure hypothesis. -
Montana Kaimin, April 28, 2010 Students of the Niu Versity of Montana, Missoula
University of Montana ScholarWorks at University of Montana Associated Students of the University of Montana Montana Kaimin, 1898-present (ASUM) 4-28-2010 Montana Kaimin, April 28, 2010 Students of The niU versity of Montana, Missoula Let us know how access to this document benefits ouy . Follow this and additional works at: https://scholarworks.umt.edu/studentnewspaper Recommended Citation Students of The nivU ersity of Montana, Missoula, "Montana Kaimin, April 28, 2010" (2010). Montana Kaimin, 1898-present. 5323. https://scholarworks.umt.edu/studentnewspaper/5323 This Newspaper is brought to you for free and open access by the Associated Students of the University of Montana (ASUM) at ScholarWorks at University of Montana. It has been accepted for inclusion in Montana Kaimin, 1898-present by an authorized administrator of ScholarWorks at University of Montana. For more information, please contact [email protected]. Page 5 Pages 7-11 Page 13 Foresters gather ASUM candidates Recalling the for a day answer questions Mount St. Helens of competition before election eruption after 30 years www.montanakaimin.com MKontana UM’s Independent Campus Newspaper Since 1898 aVolumeimin CXII Issue 96 Wednesday, April 28, 2010 Endangered species of the mind The past and future of the President’s Lecture Series Andrew Dusek position he thoroughly enjoys, Montana Kaimin and he completely invests himself With the carefully constructed in the coordination process, from cadences of an academic, Alexan- establishing initial contact to the der Nehamas spoke to the crowd lecturer’s last uttered phrase. that had gathered in the dark- The process begins more than ness before him on a late-March a year in advance. -
San Diego History Center Is One of the Largest and Oldest Historical Organizations on the West Coast
The Journal of San Diego Volume 61 Spring 2015 Number 2 • The Journal of San Diego History Diego San of Journal 2 • The Number 2015 Spring 61 Volume History Publication of The Journal of San Diego History is underwritten by major grants from the Robert D. L. Gardiner Foundation and the Quest for Truth Foundation, established by the late James G. Scripps. Additional support is provided by “The Journal of San Diego History Fund” of the San Diego Foundation and private donors. Founded in 1928 as the San Diego Historical Society, today’s San Diego History Center is one of the largest and oldest historical organizations on the West Coast. It houses vast regionally significant collections of objects, photographs, documents, films, oral histories, historic clothing, paintings, and other works of art. The San Diego History Center operates two major facilities in national historic landmark districts: The Research Library and History Museum in Balboa Park and the Serra Museum in Presidio Park. The San Diego History Center presents dynamic changing exhibitions that tell the diverse stories of San Diego’s past, present, and future, and it provides educational programs for K-12 schoolchildren as well as adults and families. www.sandiegohistory.org Front Cover: Colorized postcards from the 1915 Panama-California Exhibition. (Clockwise) California Tower, Botanical Building, Cabrillo Bridge, and Commerce and Industries Building. Back Cover: USO Headquarters at Horton Plaza, World War II, supported by the Wax Family of San Diego. Design and Layout: Allen Wynar Printing: Crest Offset Printing Editorial Assistants: Travis Degheri Cynthia van Stralen Joey Seymour Articles appearing in The Journal of San Diego History are abstracted and indexed in Historical Abstracts and America: History and Life. -
Radiocarbon, Volume 15, Number 2 (1973)
Radiocarbon, Volume 15, Number 2 (1973) Item Type Journal; text Publisher American Journal of Science Journal Radiocarbon Rights Copyright © The American Journal of Science Download date 05/10/2021 14:21:24 Item License http://rightsstatements.org/vocab/InC/1.0/ Version Final published version Link to Item http://hdl.handle.net/10150/655401 I Volume 1.5, Number 2 - 1973 RADIOCARBON Published by THE AMERICAN JOURNAL OF SCIENCE Editors RICHARD FOSTER FLINT-1. GORDON OLDEN, III IRVING, ROUSE - MINZE ,S'FUIVER Managing Editor RENEE S. KRA YALE UNIVERSITY 798 NEW HAVEN, CONNECTICUT w U3 V3 U RADIOCARBON Editors: RlcH.vcl( FosrI R FtINr-J. GORDON OlCI N, III-IRt'1Ne ROUST-MINZ6. Srmvr:R Managing Edilor: RtNF.r. S. Kltn Published by THE AMERICAN JOURNAL OF SCIENCE Editors: JOHN ROUCt:RS, JOHN 11. OSIROJT, AND PHILIP M. ORv'n.ti, Published tri-annually, in Winter, Spring, and Sltulmer, at Yale University, New Ilasen, Connecticut. Subscription rate 515.00 (for institutions), 530.00 (lot- individuals), available only in whole volumes. All correspondence and Iuanuscripis should be addressed to the Managing Editor, RADIOCARBON, Box 21(11, `ale Station, New Ilavcn, Conucclicut 06520. INSIRCCHONS 10 CONTRIBU TOILS \[auuseriltts of rediouufi0H papers should follow the recommendations ill Su.i;ges- (totts to .lullims, 501 ed.* All cola' (including the hibliographv unrst be lvpetvritten in doable dune. Nlanu.scripts [or vol. 16, to. I must he submitted in dttltlirnle by Juuc 1, 1973. Vol. 15, no.03 has ahradv been filled. I)esnil)liotts of samples, in date lists, should follow as closely as possible the style shown in this volume. -
And Other Essays
University of New Orleans ScholarWorks@UNO University of New Orleans Theses and Dissertations Dissertations and Theses Spring 5-17-2013 "Two Thousand Hours" and Other Essays Bradley P. Guillory University of New Orleans, [email protected] Follow this and additional works at: https://scholarworks.uno.edu/td Part of the Nonfiction Commons Recommended Citation Guillory, Bradley P., ""Two Thousand Hours" and Other Essays" (2013). University of New Orleans Theses and Dissertations. 1682. https://scholarworks.uno.edu/td/1682 This Thesis is protected by copyright and/or related rights. It has been brought to you by ScholarWorks@UNO with permission from the rights-holder(s). You are free to use this Thesis in any way that is permitted by the copyright and related rights legislation that applies to your use. For other uses you need to obtain permission from the rights- holder(s) directly, unless additional rights are indicated by a Creative Commons license in the record and/or on the work itself. This Thesis has been accepted for inclusion in University of New Orleans Theses and Dissertations by an authorized administrator of ScholarWorks@UNO. For more information, please contact [email protected]. University of New Orleans ScholarWorks@UNO University of New Orleans Theses and Dissertations Dissertations and Theses 5-17-2013 "Two Thousand Hours" and Other Essays Bradley P. Guillory Follow this and additional works at: http://scholarworks.uno.edu/td This Thesis is brought to you for free and open access by the Dissertations and Theses at ScholarWorks@UNO. It has been accepted for inclusion in University of New Orleans Theses and Dissertations by an authorized administrator of ScholarWorks@UNO. -
Cambridge University Press 978-1-107-15445-2 — Mercury Edited by Sean C
Cambridge University Press 978-1-107-15445-2 — Mercury Edited by Sean C. Solomon , Larry R. Nittler , Brian J. Anderson Index More Information INDEX 253 Mathilde, 196 BepiColombo, 46, 109, 134, 136, 138, 279, 314, 315, 366, 403, 463, 2P/Encke, 392 487, 488, 535, 544, 546, 547, 548–562, 563, 564, 565 4 Vesta, 195, 196, 350 BELA. See BepiColombo: BepiColombo Laser Altimeter 433 Eros, 195, 196, 339 BepiColombo Laser Altimeter, 554, 557, 558 gravity assists, 555 activation energy, 409, 412 gyroscope, 556 adiabat, 38 HGA. See BepiColombo: high-gain antenna adiabatic decompression melting, 38, 60, 168, 186 high-gain antenna, 556, 560 adiabatic gradient, 96 ISA. See BepiColombo: Italian Spring Accelerometer admittance, 64, 65, 74, 271 Italian Spring Accelerometer, 549, 554, 557, 558 aerodynamic fractionation, 507, 509 Magnetospheric Orbiter Sunshield and Interface, 552, 553, 555, 560 Airy isostasy, 64 MDM. See BepiColombo: Mercury Dust Monitor Al. See aluminum Mercury Dust Monitor, 554, 560–561 Al exosphere. See aluminum exosphere Mercury flybys, 555 albedo, 192, 198 Mercury Gamma-ray and Neutron Spectrometer, 554, 558 compared with other bodies, 196 Mercury Imaging X-ray Spectrometer, 558 Alfvén Mach number, 430, 433, 442, 463 Mercury Magnetospheric Orbiter, 552, 553, 554, 555, 556, 557, aluminum, 36, 38, 147, 177, 178–184, 185, 186, 209, 559–561 210 Mercury Orbiter Radio Science Experiment, 554, 556–558 aluminum exosphere, 371, 399–400, 403, 423–424 Mercury Planetary Orbiter, 366, 549, 550, 551, 552, 553, 554, 555, ground-based observations, 423 556–559, 560, 562 andesite, 179, 182, 183 Mercury Plasma Particle Experiment, 554, 561 Andrade creep function, 100 Mercury Sodium Atmospheric Spectral Imager, 554, 561 Andrade rheological model, 100 Mercury Thermal Infrared Spectrometer, 366, 554, 557–558 anorthosite, 30, 210 Mercury Transfer Module, 552, 553, 555, 561–562 anticline, 70, 251 MERTIS. -
Arxiv:1707.07134V1 [Astro-Ph.GA] 22 Jul 2017 2 Radio-Selected AGN
Astronomy Astrophysics Review manuscript No. (will be inserted by the editor) Active Galactic Nuclei: what’s in a name? P. Padovani · D. M. Alexander · R. J. Assef · B. De Marco · P. Giommi · R. C. Hickox · G. T. Richards · V. Smolciˇ c´ · E. Hatziminaoglou · V. Mainieri · M. Salvato Received: June 12, 2017 / Accepted: July 21, 2017 Abstract Active Galactic Nuclei (AGN) are energetic as- sic differences between AGN, and primarily reflect varia- trophysical sources powered by accretion onto supermassive tions in a relatively small number of astrophysical parame- black holes in galaxies, and present unique observational ters as well the method by which each class of AGN is se- signatures that cover the full electromagnetic spectrum over lected. Taken together, observations in different electromag- more than twenty orders of magnitude in frequency. The netic bands as well as variations over time provide comple- rich phenomenology of AGN has resulted in a large number mentary windows on the physics of different sub-structures of different “flavours” in the literature that now comprise a in the AGN. In this review, we present an overview of AGN complex and confusing AGN “zoo”. It is increasingly clear multi-wavelength properties with the aim of painting their that these classifications are only partially related to intrin- “big picture” through observations in each electromagnetic band from radio to γ-rays as well as AGN variability. We P. Padovani · E. Hatziminaoglou · V. Mainieri address what we can learn from each observational method, European Southern Observatory, Karl-Schwarzschild-Str. 2, D-85748 the impact of selection effects, the physics behind the emis- Garching bei Munchen,¨ Germany sion at each wavelength, and the potential for future studies. -
Not Yet Imagined: a Study of Hubble Space Telescope Operations
NOT YET IMAGINED A STUDY OF HUBBLE SPACE TELESCOPE OPERATIONS CHRISTOPHER GAINOR NOT YET IMAGINED NOT YET IMAGINED A STUDY OF HUBBLE SPACE TELESCOPE OPERATIONS CHRISTOPHER GAINOR National Aeronautics and Space Administration Office of Communications NASA History Division Washington, DC 20546 NASA SP-2020-4237 Library of Congress Cataloging-in-Publication Data Names: Gainor, Christopher, author. | United States. NASA History Program Office, publisher. Title: Not Yet Imagined : A study of Hubble Space Telescope Operations / Christopher Gainor. Description: Washington, DC: National Aeronautics and Space Administration, Office of Communications, NASA History Division, [2020] | Series: NASA history series ; sp-2020-4237 | Includes bibliographical references and index. | Summary: “Dr. Christopher Gainor’s Not Yet Imagined documents the history of NASA’s Hubble Space Telescope (HST) from launch in 1990 through 2020. This is considered a follow-on book to Robert W. Smith’s The Space Telescope: A Study of NASA, Science, Technology, and Politics, which recorded the development history of HST. Dr. Gainor’s book will be suitable for a general audience, while also being scholarly. Highly visible interactions among the general public, astronomers, engineers, govern- ment officials, and members of Congress about HST’s servicing missions by Space Shuttle crews is a central theme of this history book. Beyond the glare of public attention, the evolution of HST becoming a model of supranational cooperation amongst scientists is a second central theme. Third, the decision-making behind the changes in Hubble’s instrument packages on servicing missions is chronicled, along with HST’s contributions to our knowledge about our solar system, our galaxy, and our universe. -
Utah Copper Mine Generates Ing Address of P.O
2013 GSA Annual Meeting & Exposition Wrap-Up, p. 12 JANUARY 2014 | VOL.JANUARY 24, 2014 N O. 1 O. A PUBLICATION OF THE GEOLOGICAL SOCIETY OF AMERICA® MassIVE LANDSLIDE AT UTAH COPPER MINE GENERatES weaLTH OF geOPHYSICAL DATA JANuarY 2014 | VOlumE 24, NumbER 1 Featured Articles GSA TODAY (ISSN 1052-5173 USPS 0456-530) prints news and information for more than 25,000 GSA member readers and subscribing libraries, with 11 monthly issues (April/ May is a combined issue). GSA TODAY is published by The ScieNCE ARticle: Geological Society of America® Inc. (GSA) with offices at 3300 Penrose Place, Boulder, Colorado, USA, and a mail- 4 Massive landslide at Utah copper mine generates ing address of P.O. Box 9140, Boulder, CO 80301-9140, USA. wealth of geophysical data GSA provides this and other forums for the presentation of diverse opinions and positions by scientists worldwide, Kristine L. Pankow, Jeffrey R. Moore, J. Mark Hale, regardless of race, citizenship, gender, sexual orientation, Keith D. Koper, Tex Kubacki, Katherine M. Whidden, religion, or political viewpoint. Opinions presented in this and Michael K. McCarter publication do not reflect official positions of the Society. © 2014 The Geological Society of America Inc. All rights Cover photo: Massive landslide on 30 April 2013 in the Bingham reserved. Copyright not claimed on content prepared Canyon open-pit copper mine near Salt Lake City, Utah, USA. Image wholly by U.S. government employees within the scope of copyright Rio Tinto Kennecott Utah Copper; used with permission. their employment. Individual scientists are hereby granted See related article, p. -
Chapter Ten Venus and Mars
Q-CD vol. 2: Chaos and Creation, Ch. 10: Venus and Mars 255 CHAPTER TEN VENUS AND MARS From the brow of Zeus, sang the Greeks, sprang Pallas Athene -- fully armed and with a shout [1]. She was cometary Venus -- fiery-faced, owl-eyed, helmeted and horned, with a long gown and hair trailing behind. Meanwhile, in Mesopotamia the Akkadians were also chanting hymns to Venus, going here by the name of Inanna:[2] By night she sends out light like the Moon does. At noonday sends out light like the Sun does. The mistress of Evening whose largeness is until the limit of Heaven... The Holy light that fills the Heavens. Inanna who shines as far as the Sun. These words, along with the symbols of Inanna (Figure 31) part the curtains upon “a lady who needs no introduction to you,” as a master of ceremonies would say. Many scholars deny that it could happen; yet no astral event of the ancients was so well reported as the career of the glowing and devastating comet and proto-planet Venus [3]. For nearly a thousand years it raged through the heavens periodically, encountering first Earth, then Mars; then Jupiter; then Mars again. It periodically -- every half century -- threatened the Earth and sometimes repeated, less harshly, its first devastation of the planet. The age of Venusia lasted from about 1450 to 700 B.C. endured, that is, until the comet Venus lost its cometary appendages and became a hot, young planet circling the Sun for all the world like an ordinary planet is supposed to behave.