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TRANSIENT LUNAR PHENOMENA: REGULARITY and REALITY Arlin P
The Astrophysical Journal, 697:1–15, 2009 May 20 doi:10.1088/0004-637X/697/1/1 C 2009. The American Astronomical Society. All rights reserved. Printed in the U.S.A. TRANSIENT LUNAR PHENOMENA: REGULARITY AND REALITY Arlin P. S. Crotts Department of Astronomy, Columbia University, Columbia Astrophysics Laboratory, 550 West 120th Street, New York, NY 10027, USA Received 2007 June 27; accepted 2009 February 20; published 2009 April 30 ABSTRACT Transient lunar phenomena (TLPs) have been reported for centuries, but their nature is largely unsettled, and even their existence as a coherent phenomenon is controversial. Nonetheless, TLP data show regularities in the observations; a key question is whether this structure is imposed by processes tied to the lunar surface, or by terrestrial atmospheric or human observer effects. I interrogate an extensive catalog of TLPs to gauge how human factors determine the distribution of TLP reports. The sample is grouped according to variables which should produce differing results if determining factors involve humans, and not reflecting phenomena tied to the lunar surface. Features dependent on human factors can then be excluded. Regardless of how the sample is split, the results are similar: ∼50% of reports originate from near Aristarchus, ∼16% from Plato, ∼6% from recent, major impacts (Copernicus, Kepler, Tycho, and Aristarchus), plus several at Grimaldi. Mare Crisium produces a robust signal in some cases (however, Crisium is too large for a “feature” as defined). TLP count consistency for these features indicates that ∼80% of these may be real. Some commonly reported sites disappear from the robust averages, including Alphonsus, Ross D, and Gassendi. -
Why NASA Consistently Fails at Congress
W&M ScholarWorks Undergraduate Honors Theses Theses, Dissertations, & Master Projects 6-2013 The Wrong Right Stuff: Why NASA Consistently Fails at Congress Andrew Follett College of William and Mary Follow this and additional works at: https://scholarworks.wm.edu/honorstheses Part of the Political Science Commons Recommended Citation Follett, Andrew, "The Wrong Right Stuff: Why NASA Consistently Fails at Congress" (2013). Undergraduate Honors Theses. Paper 584. https://scholarworks.wm.edu/honorstheses/584 This Honors Thesis is brought to you for free and open access by the Theses, Dissertations, & Master Projects at W&M ScholarWorks. It has been accepted for inclusion in Undergraduate Honors Theses by an authorized administrator of W&M ScholarWorks. For more information, please contact [email protected]. The Wrong Right Stuff: Why NASA Consistently Fails at Congress A thesis submitted in partial fulfillment of the requirement for the degree of Bachelors of Arts in Government from The College of William and Mary by Andrew Follett Accepted for . John Gilmour, Director . Sophia Hart . Rowan Lockwood Williamsburg, VA May 3, 2013 1 Table of Contents: Acknowledgements 3 Part 1: Introduction and Background 4 Pre Soviet Collapse: Early American Failures in Space 13 Pre Soviet Collapse: The Successful Mercury, Gemini, and Apollo Programs 17 Pre Soviet Collapse: The Quasi-Successful Shuttle Program 22 Part 2: The Thin Years, Repeated Failure in NASA in the Post-Soviet Era 27 The Failure of the Space Exploration Initiative 28 The Failed Vision for Space Exploration 30 The Success of Unmanned Space Flight 32 Part 3: Why NASA Fails 37 Part 4: Putting this to the Test 87 Part 5: Changing the Method. -
CAMOC Museums of Cities Review
01 / 2017 www.camoc.icom.museum MUSEUMS OF CITIES REVIEW ISSN 2520-2472 The Lisbon that Could Have Been A new temporary exhibition at the Museum of Lisbon ANTÓNIO MIRANDA / RAQUEL HENRIQUES DA SILVA* The Eduardo VII park, view to the Tagus river. © www.all-free.photos.com “The Lisbon that could have been” is the newest and “Fragments of Colour - The Tiles Collection of temporary exhibition of the Museum of Lisbon, on the Museum of Lisbon”, the city museum keeps on show at the Black Pavilion gallery from January 27 pursuing research and exhibition projects that reveal the up to June 18. Following exhibitions like “Fishermen museum’s collections in innovative ways. wives – Memories of the City”, “The Light of Lisbon” This exhibition uncovers how Lisbon was being thought over and planned for by mainly Portuguese architects and * Exhibition Curators: AM is a researcher at the Museum of Lisbon, and RHS is an Art Historian at Universidade Nova de Lisboa. urbanists, through the lens of projects that were CONTENTS 01 The Lisbon that Could Have Been 23 Urban Life, City Museums, and Children 04 The Chair’s Note 26 Antwerp à la carte 06 Migrations and Spontaneous Museums in Italy 29 The Power of Darkness-The night as a cultural landscape 09 Presenting Immigrant Culture at the National 33 City Circles Athens Museum of Ethnology, Japan 36 5th International Conference: Creative Cities 12 National Museum of Taiwan History and Immigrants 54 Special Dossier: Athens Workshop 14 CAMOC Annual Conference Call, Mexico 2017 57 Exhibition Alert 20 Towards the Hrant Dink Site of Memory 58 Conference Alert 1 CITY MUSEUMS Let us listen to the curators. -
PLANETARIAN Journal of the International Planetarium Society Vol
PLANETARIAN Journal of the International Planetarium Society Vol. 26, No.3, September 1997 Articles 5 Projections from Gallatin .................................................... Gary Likert 10 How Thinking Goes Wrong ....................................... Michael Shermer 17 Astronomy Link - A Beginning ........................................ Jim Manning 21 14th International Planetarium Conference ................................ IPS'98 Features 26 Opening the Dome .............................................................. Jon U. Bell 29 Planetarium Memories .........., .................................. Kenneth E. Perkins 31 Planetechnica: Shoestring Wire Management ......... Richard McColman 34 Forum ................................................................................. Steve Tidey 39 Book Reviews .................................................................. April S. Whitt 45 Mobile News Network ...................................................... Sue Reynolds 47 ',X/hat's New ...................................................................... Jim Manning 51 Gibbous Gazette ......................................................... Christine Shupla 53 Regional Roundup ............................................................ Lars Broman 58 President's Message ....................................................... Thomas Kraupe 62 Jane's Corner .................................................................... Jane Hastings " l1,c ZKPJ ;'\' jalltastic ... It IJrojec/x Ih e 11/ 0 0 1/ phases wilh (l -
Water on the Moon, III. Volatiles & Activity
Water on The Moon, III. Volatiles & Activity Arlin Crotts (Columbia University) For centuries some scientists have argued that there is activity on the Moon (or water, as recounted in Parts I & II), while others have thought the Moon is simply a dead, inactive world. [1] The question comes in several forms: is there a detectable atmosphere? Does the surface of the Moon change? What causes interior seismic activity? From a more modern viewpoint, we now know that as much carbon monoxide as water was excavated during the LCROSS impact, as detailed in Part I, and a comparable amount of other volatiles were found. At one time the Moon outgassed prodigious amounts of water and hydrogen in volcanic fire fountains, but released similar amounts of volatile sulfur (or SO2), and presumably large amounts of carbon dioxide or monoxide, if theory is to be believed. So water on the Moon is associated with other gases. Astronomers have agreed for centuries that there is no firm evidence for “weather” on the Moon visible from Earth, and little evidence of thick atmosphere. [2] How would one detect the Moon’s atmosphere from Earth? An obvious means is atmospheric refraction. As you watch the Sun set, its image is displaced by Earth’s atmospheric refraction at the horizon from the position it would have if there were no atmosphere, by roughly 0.6 degree (a bit more than the Sun’s angular diameter). On the Moon, any atmosphere would cause an analogous effect for a star passing behind the Moon during an occultation (multiplied by two since the light travels both into and out of the lunar atmosphere). -
Facts & Statistics About the Project
1 Hubble’s 15th Anniversary – Facts about the ESA project Introduction 24 April 2005 marked the 15th anniversary of the launch of the NASA/ESA Hubble Space Telescope. As an observatory in space, Hubble is a major project that has made an enormous impact both in terms of scientific output and in its immediate public appeal. Hubble has exploited its unique scientific capabilities in regions where no other instruments can compete. The telescope consistently delivers super-sharp images and clean, uncontaminated spectra over the entire near-infrared to ultraviolet regions of the electromagnetic spectrum. This has opened up new scientific territory and has resulted in many paradigm-breaking discoveries. Exquisite quality images have enabled astronomers to gain entirely new insights into the workings of a huge range of different astronomical objects. Hubble has provided a visual overview of the underlying astrophysical processes taking place in these objects, ranging from planets in our Solar System to galaxies in the young Universe. The renowned British astronomer Malcolm Longair writes in the preface to ESA’s anniversary book: ”The Hubble Space Telescope has undoubtedly had a greater public impact than any other space astronomy mission ever. The images included in this beautiful volume are quite staggering in the detail they reveal about the Universe we live in and have already become part of our common scientific and cultural heritage.” The project Many people agree that the long-term well-being and cultural development of European citizens depends on research and technological development. Information about science and scientists is a vital component of the scientific process, but the competition for attention in today’s mass-media market is fierce. -
Zoe in Wonderland by Brenda Woods
A Choose to Read Ohio Toolkit Zoe in Wonderland By Brenda Woods Use this toolkit to About the Book plan book discussions, library Coretta Scott King Honor winner Brenda Woods programs, or introduces introverted, daydream-prone Zoe, classroom who’s afraid her real life will never be as activities. exciting as her imaginary one. Meet Ohio native, Zoe Reindeer considers herself “just Zoe”— California-based, never measuring up to her too-perfect older award-winning sister or her smarty-pants little brother. Truthfully, author Brenda though, she’d rather just blend in with the Woods. plants at the family business, Doc Reindeer’s Exotic Plant Wonderland. She does have one Select from a range friend, Q, and he’s the best one ever—but he’s of discussion moving away, leaving Zoe to fend for herself, questions and and she doesn’t know what she’ll do without him. That is until a tall astronomer from extension activities Madagascar comes to the nursery looking for a to deepen the Baobab tree. His visit starts a ball rolling that experience of makes Zoe long for real adventures, not just reading imaginary ones—and shows her that perhaps Zoe in Wonderland. her first real adventure is finally beginning. Book jacket image and book description courtesy of Penguin Random House. Used with permission. Discover informative books, videos, websites, Book Details and other resources to explore topics Zoe in Wonderland by Brenda Woods and themes in Nancy Paulsen Books (Penguin Random House), 2016. ISBN 9780399170973. 196 pages. depth. Ages 8+. Leveled Reading: AR Points 5.0. -
Space and Planetary Environment Criteria Guidelines for Use in Space Vehicle Development, 1 9 8 2 Revision Volume 1
NASA Technicd Memorandum 8 2 4 7 8 Space and Planetary Environment Criteria Guidelines for Use in Space Vehicle Development, 1 9 8 2 Revision Volume 1 Robert E. Smith ar~dGeorge S. West, Compilers George C. Marshall Space Flight Center Marshall Space Flight Center, Alabama National Aeronautics and Space Administration Sclentlfice and Technical lealormation 'Branch TABLE OF CONTENTS Page viii SECTIOP; 1. THE SUN ............................................ .......... 1.1 Introduction ....................... .. ............. ....a* 1.2 Brief Qualitative Description ............................. 1.3 Physical Properties .................................... .. 1.4 Solar Emanations - Descriptive .......................... 1.4.1 The Nature of the Sun's Output .................. 1.4.2 The Solar Cycle ................................... 1.4.3 Variation in the Sun's Output ................... .. 1.5 Solar Electromagnetic Radiation ........................... 1.5.1 Measurements of the Solar Constant ............... 1.5.2 Short-Term Fluctuations in the Solar Constant . .: . 1.5.3 The Solar Spectral Irradiance ..................... 1.6 Solar Plasma Emission .................................... 1.6.1 Properties of the Mean $olar Wind ................. 1.6.2 The Solar Wind and the Interplanetary Magnetic Field ............................................. 1.6.3 High-speed Streams ............................... 1.6.4 Coronal Transients ....................... .. .. .. ... 1.6.5 Spatial Variation of Solar Wind Properties ......... 1.6.6 Variation of the -
Metallic Species, Oxygen and Silicon in the Lunar Exosphere: Upper Limits and Prospects for LADEE Measurements Menelaos Sarantos,1,2,3 Rosemary M
JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 117, A03103, doi:10.1029/2011JA017044, 2012 Metallic species, oxygen and silicon in the lunar exosphere: Upper limits and prospects for LADEE measurements Menelaos Sarantos,1,2,3 Rosemary M. Killen,3,4 David A. Glenar,3,5,6 Mehdi Benna,7 and Timothy J. Stubbs3,7,8 Received 29 July 2011; revised 20 December 2011; accepted 22 December 2011; published 13 March 2012. [1] The only species that have been so far detected in the lunar exosphere are Na, K, Ar, and He. However, models for the production and loss of species derived from the lunar regolith through micrometeoroid impact vaporization, sputtering, and photon-stimulated desorption, predict that a host of other species should exist in the lunar exosphere. Assuming that loss processes are limited to ballistic escape, photoionization, and recycling to the surface, we have computed column abundances and compared them to published upper limits for the Moon. Only for Ca do modeled abundances clearly exceed the available measurements. This result suggests the relevance of some loss processes that were not included in the model, such as the possibility of gas-to-solid phase condensation during micrometeoroid impacts or the formation of stable metallic oxides. Our simulations and the recalculation of efficiencies for resonant light scattering show that models for other species studied are not well constrained by existing measurements. This fact underlines the need for improved remote and in situ measurements of the lunar exosphere such as those planned by the Lunar Atmosphere and Dust Environment Explorer (LADEE) spacecraft. Our simulations of the LADEE neutral mass spectrometer and visible/ultraviolet spectrometer indicate that LADEE measurements promise to provide definitive observations or set stringent upper limits for all regolith-driven exospheric species. -
Rine and the Apennine Mountains. INSTITUTION National Aeronautics and Space Administration, Washington, D.C
DOCUMENT RESUME ED 053 930 SE 012 016 AUTHOR Simmons, Gene TITLE On the Moon with Apollo 15,A Guidebook to Hadley Rine and the Apennine Mountains. INSTITUTION National Aeronautics and Space Administration, Washington, D.C. PUB DATE Jun 71 NOTE 52p. AVAILABLE FROM Superintendent of Documents, U.S. Government Printing Office, Washington, D.C. 20402 (3300-0384 $0.50) EDRS PRICE EDRS Price MF-$0.65 HC-$3.29 DESCRIPTORS *Aerospace Technology, Geology, Reading Materials, Resource Materials IDENTIFIERS *Lunar Studies, Moon ABSTRACT The booklet, published before the Apollo 15 mission, gives a timeline for the mission; describes and illustrates the physiography of the landing site; and describes and illustrates each lunar surface scientific experiment. Separate timelines are included for all traverses (the traverses are the Moon walks and, for Apollo 15, the Moon rides in the Rover) with descriptions of activities at each traverse stop. Each member of the crew and the backup crew is identified. Also included is a bibliography of lunar literature and glossary of terms used in lunar studies. Photographs and diagrams are utilized throughout. Content is descriptive and informative but with a minimum of technical detail. (Author/PR) , ON THE MOON WITH APOLLO 15 A Guidebook to Hadley Rille and the Apennine Mountains U.S. DEPARTMENT OFHEALTH, EDUCATION,& WELFARE OFFICE OF EDUCATION THIS DOCUMENT HAS SEENREPRO- DUCED EXACTLY AS RECEIVEDFROM THE PERSON OR ORGANIZATIONORIG INATING IT. POINTS OF VIEWOR OPIN IONS STATED DO NOTNECESSARILY REPRESENT OFFICIAL OFFICEOF EDU CATION POSITION OR POLICY isr) 1..r1 w fl R CO iiii0OP" O NATIONAL AERONAUTICS AND SPACE ADMINISTRATION June 1971 1 \n ON THE MOON WITH APOLLO 15 A uidebook to Hadley Rille and the Apennine Mountains by Gene Simmons Chief Scientist Manned Spacecraft Center NATIONAL AERONAUTICS AND SPACE ADMINISTRATION June 1971 2 For sale by the Superintendent of Documents, U.S. -
Vol. 37, No. 1 March 2008 Journal of the International Planetarium Society
Vol. 37, No. 1 March 2008 Journal of the International Planetarium Society Geoscience visualization in the dome…Page 6 Articles March 2008 Vol. 37 No. 1 6 A Do-it-Yourself Approach to Fulldome Visualization Tom Kwasnitschka Executive Editor 10 Astronomy’s All Around Us Sharon Shanks Steve Tidey Ward Beecher Planetarium 14 Preparing for IYA with the Astronomical Youngstown State University Society of the Pacific One University Plaza Jim Manning Youngstown, Ohio 44555 USA 16 Interactive Exhibition at Kyiv Planetarium, (1) 330-941-3619 Ukraine [email protected] Nataliya Kovalenko 18 The Changes of Meteorological Quantities Advertising Coordinator During Solar Eclipses Chuck Bueter Miloslav Machon 15893 Ashville Lane 21 Minutes of the IPS Council Meeting Granger, Indiana 46530 USA Lee Ann Henning (1) 574-271-3150 [email protected] www.ips-planetarium.org/planetarian/ratesheet.htm Columns 67 25 Years Ago. Thomas Wm. Hamilton Membership 66 Calendar of Events. .Loris Ramponi Individual: $50 one year; $90 two years 31 Digital Frontiers. Ed Lantz Institutional: $200 first year; $100 annual renewal 36 Educational Horizons . Steve Tidey Library Subscriptions: $36 one year 38 Forum. .Gary Lazich Direct membership requests and changes of 41 General Counsel . Christopher S. Reed address to the Treasurer/Membership Chairman 65 Gibbous Gazette. .James P. Hughes 5 In Front of the Console . .Sharon Shanks Back Issues of the Planetarian 43 International News. Lars Broman IPS Back Publications Repository maintained by the Treasurer/Membership Chair; 68 Last Light . April S. Whitt contact information is on next page 50 Mobile News. .Susan Reynolds Button 54 NASA Space Science News. -
Presence of Water on Exomoons Orbiting Free-Floating Planets
International Journal of Presence of water on exomoons orbiting Astrobiology free-floating planets: a case study cambridge.org/ Patricio Javier Ávila1, Tommaso Grassi2, Stefano Bovino1, Andrea Chiavassa3,4, Barbara Ercolano2, Sebastian Oscar Danielache5,6, Eugenio Simoncini6 Research Article 1Departamento de Astronomía, Facultad Ciencias Físicas y Matemáticas, Universidad de Concepción, Cite this article: Ávila PJ, Grassi T, Bovino 2 S, Chiavassa A, Ercolano B, Danielache Av. Esteban Iturra s/n Barrio Universitario, Casilla 160, Concepción, Chile; Ludwig Maximilian University SO, Simoncini E (2021) Presence of water of Munich, Scheinerstr. 1, D-81673 Munich, Germany; 3Universitè Côte d’Azur, Observatoire de la Côte on exomoons orbiting free-floating planets: d’Azur, CNRS, Laboratoire Lagrange, Bd de l’Observatoire, CS 34229, F-06304 Nice Cedex 4, France; a case study. International Journal of 4European Southern Observatory, Karl-Schwarzschild-Str. 2, D-85748 Garching bei München, Germany; Astrobiology 1–12. https://doi.org/10.1017/ 5 S1473550421000173 Department of Material and Life Sciences, Faculty of Science and Technology, Sophia University, 8 Chiy- oda, Tokyo, 102-8554, Japan; 6Earth and Life Science Institute, Tokyo Institute of Technology, Meguro, Received: 20 February 2021 Tokyo, 152-8551, Japan; Revised: 8 April 2021 Accepted: 9 May 2021 Abstract Key words: A free-floating planet is a planetary-mass object that orbits around a non-stellar massive object astrochemistry, atmospheres, planets and satellites. (e.g. a brown dwarf) or around the Galactic Center. The presence of exomoons orbiting free- floating planets has been theoretically predicted by several models. Under specific conditions, Author for correspondence: these moons are able to retain an atmosphere capable of ensuring the long-term thermal stability Patricio Javier Ávila, Email: of liquid water on their surface.