Summer Conference on Lunar Exploration and Science (1965)
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LUNAR INTERACTIONS ABSTRACTS of PAPERS PRESENTED at the CONFERENCE on INTERACTIONS of the INTERPLANETARY PLASMA with the MODERN and ANCIENT MOON
LUNAR INTERACTIONS ABSTRACTS OF PAPERS PRESENTED AT THE CONFERENCE ON INTERACTIONS OF THE INTERPLANETARY PLASMA with the MODERN AND ANCIENT MOON ORGANIZED BY THE I. N 3 LUNAR SCIENCE INSTITUTE m I 3 AND THE I- 2 SPACE PHYSICS DEPARTMENT RICE UNIVERSITY sponsored by the NATIONAL AERONAUTICS m m AND 0 .. I-( OIW mrl SPACE ADMINISTRATION ZX CV OH IOI H WclU AND THE uux- V&H 0 NATIONAL SCIENCE FOUNDATION g,,,, wm. WWO@W u u ? ZZLOX€e HW5H vlOHU ffiMHrnfC 4 ffi H 2.~4~4a Edited by 3 dz ,.aV)ffiuJO ffiwcstn WPt.4" DAVID R. CRISWELL ,!a !a Pl r 4 W Pa4 %- rn ZW. and Or=4OcC+J fO Hi4 r WWF I rnU2.M ffiBZ* JOHN W. FREEMAN UUW4aJ I amor 0 alffiwffi E REPRODUCTION RESTRICTIONS OVERRIDDEN 2Z~OZ E 2 2 .: u Bmscientific ma Technical Information FaciLitX -eu $4 to) Copyright O 1974 by the Lunar Science Institute Conference held at George Williams College Lake Geneva Campus Williams Bay, Wisconsin 30 September - 4 October 1974 Compiled by and available from The Lunar Science Institute 3303 Nasa Road 1 Houston, Texas 77058 PREFACE The field of lunar science has essentially completed a period of exponential growth promoted by the national efforts of the 1960's to land on the moon. As normally happens in a diverse scientific community, the interpretations of specialized lunar data have reflected the precepts in the various specialized fields. Constant promotion of the broadest overviews between these diverse fields is appropriate to identify processes or phenomenon recog- nized in one avenue of investigation which may have great importance in explaining the data of other specialities. -
Tazewell County Warren County Westmoreland~CO~Tt~~'~Dfla
If you have issues viewing or accessing this file, please contact us at NCJRS.gov. Tazewell County Warren County Westmoreland~CO~tt~~'~dfla Bedford Bristol Buena Vista Charl~esville ~ake clnr(~ F:Org I Heights Covington Danville Emporia Fairfax Falls ~.~tur.~~l~).~ ~urg Galax Hampton HarrisonburgHopj~ll~l Lexingtor~ynchburgl~'~assa ~ anassas Martinsville Newport News Norfolk Norton PetersbutrgPoque~o~ .Portsmouth Radford Richmond Roano~l~~ Salem ~th Bostor~t~nto SuffoLk Virginia Beach Waynesboro Williamsburg Winchester ~a~:~ingham Ceuul~ Carroll County Charlotte County Cra~ Col~ty Roar~ County~cco~Lac= Albemarle County Alleghany County Amelia County#~rlb~ ~NJ~/Ly,~ll~iatt~ County Arlington CountyAugula County Bath i~nty BerJ~rd Cd~t B.I.... ~1 County Botetourt County Brunswick County Buchanal~C~ut~ ~~wrtty Caroline County Charles City C~nty Ch~erfield~bunty C~rrke Co~t CT~-~eperCounty Dickenson County Dinwiddie County~ ~~~ r-'luvanneCounty Frederick County C~ucester (~unty C~yson (j~nty Gre~=~ County Greensville County Halifax County Hanover County ~ .(D~I~ I~liry Cottnty Highland County Isle of *~.P-.o.~t~l~me~y C~ ~county King George County King William County~r .(~,t~ ~ (~'~ Loudoun County Louisa County M~ Mat~s Cot]1~l~~ qt... ~ Montgomery County New Kent County North~ur~d County N~y County Page County Pittsylvania CouniY--Powhatan]~.~unty Princ~eorg, oC'6-~ty Prince William County Rappahannock County Richmol~l 0~)1~1=I~Woo~ Gi0ochtandCounty Lunenburg County Mecklenburl~nty Nelson Count Northampton CountyOrange County Patrick CountyPdn¢~ -
Is the Brain-Mind Quantum? a Theoretical Proposal with Supporting Evidence
IS THE BRAIN-MIND QUANTUM? A THEORETICAL PROPOSAL WITH SUPPORTING EVIDENCE Stuart Kauffmana and Dean Radinb a Emeritus Professor of Biochemistry and Biophysics, University of Pennsylvania, [email protected] b Chief Scientist, Institute of Noetic Sciences, Petaluma, CA; , Associated Distinguished Professor, California Institute of Integral Studies, San Francisco, CA, USA [email protected]. ORCID: 0000-0003-0041-322X Abstract If all aspects of the mind-brain relationship were adequately explained by classical physics, then there would be no need to propose alternative views. But faced with possibly unresolvable puzzles like qualia and free will, other approaches are required. We propose a non-substance dualism theory, following a suggestion by Heisenberg, whereby the world consists of both ontologically real Possibles that do not obey Aristotle’s law of the excluded middle, and ontologically real Actuals, that do obey the law of the excluded middle. Measurement converts Possibles into Actuals. This quantum-oriented approach solves numerous puzzles about the mind-brain relationship, but it also raises the intriguing possibility that some aspects of mind are nonlocal, and that mind plays an active role in the physical world. We suggest that the mind-brain relationship is partially quantum, and we present evidence supporting that proposition. Keywords: brain-mind, quantum biology, consciousness, quantum measurement 1. Introduction Of the three central mysteries in science, the Origin of the Universe, the Origin of Life, and the Origin of Consciousness, the last is the most challenging. As philosopher Jerry Fodor put it in 1992, “Nobody has the slightest idea how anything material could be conscious. Nobody even knows what it would be like to have the slightest idea about how anything could be conscious” [1]. -
Sky and Telescope
SkyandTelescope.com The Lunar 100 By Charles A. Wood Just about every telescope user is familiar with French comet hunter Charles Messier's catalog of fuzzy objects. Messier's 18th-century listing of 109 galaxies, clusters, and nebulae contains some of the largest, brightest, and most visually interesting deep-sky treasures visible from the Northern Hemisphere. Little wonder that observing all the M objects is regarded as a virtual rite of passage for amateur astronomers. But the night sky offers an object that is larger, brighter, and more visually captivating than anything on Messier's list: the Moon. Yet many backyard astronomers never go beyond the astro-tourist stage to acquire the knowledge and understanding necessary to really appreciate what they're looking at, and how magnificent and amazing it truly is. Perhaps this is because after they identify a few of the Moon's most conspicuous features, many amateurs don't know where Many Lunar 100 selections are plainly visible in this image of the full Moon, while others require to look next. a more detailed view, different illumination, or favorable libration. North is up. S&T: Gary The Lunar 100 list is an attempt to provide Moon lovers with Seronik something akin to what deep-sky observers enjoy with the Messier catalog: a selection of telescopic sights to ignite interest and enhance understanding. Presented here is a selection of the Moon's 100 most interesting regions, craters, basins, mountains, rilles, and domes. I challenge observers to find and observe them all and, more important, to consider what each feature tells us about lunar and Earth history. -
Revised 15555 Olivine-Normative Basalt 9614 Grams
Revised 15555 Olivine-normative Basalt 9614 grams Figure 1: Photo of S1 surface of 15555, illustrating large mirometeorite crater (zap pit) and vuggy nature of rock. NASA S71-43954. Scale is in cm. Introduction Lunar sample 15555 (called “Great Scott”, after the experimental studies related to the origin of lunar collector Dave Scott) is one of the largest samples basalts (e.g. Walker et al. 1977). returned from the moon and is representative of the basaltic samples found on the mare surface at Apollo 15555 has a large zap pit (~1 cm) on the S1 face, various 15. It contains olivine and pyroxene phenocrysts and penetrating fractures and a few percent vugs (figure is olivine normative in composition (Rhodes and 1). It has a subophitic, basaltic texture (figure 4) and Hubbard 1973, Ryder and Shuraytz 2001). The bulk there is little evidence for shock in the minerals. It has composition of 15555 is thought to represent that of a been found to be 3.3 b.y. old and has been exposed to primitive volcanic liquid and has been used for various cosmic rays for 80 m.y. Mineralogical Mode of 15555 Longhi et McGee et Heuer et Nord et al. 1972 al. 1977 al. 1972 al. 1973 Olivine 12.1 5-12 20 20 Pyroxene 52.4 52-65 40 40 Plagioclase 30.4 25-30 35 35 Opaques 2.7 5 Mesostasis 2.3 0.2-0.4 5 5 Silica 0.3-2 Lunar Sample Compendium C Meyer 2009 picritic CMeyer basalt 2006 olivine-normative 15385 15659 13 basalt 12 15555 15536 pigeonite basalt 15016 15535 15636 11 (quartz normative) MgO 15545 15647 15379 15065 10 15598 15256 15485 15058 15595 15557 15076 15499 9 15597 15495 15529 15476 15596 8 15388 15556 15085 15117 15682 7 15118 43 44 45 46 47 48 49 SiO2 Figure 2: Composition diagram for Apollo 15 basalts (best data available) showing two basic types. -
Short-Term Variability and Mass Loss in Be Stars I
A&A 588, A56 (2016) Astronomy DOI: 10.1051/0004-6361/201528026 & c ESO 2016 Astrophysics Short-term variability and mass loss in Be stars I. BRITE satellite photometry of η and μ Centauri D. Baade1, Th. Rivinius2, A. Pigulski3,A.C.Carciofi4, Ch. Martayan2,A.F.J.Moffat5,G.A.Wade6,W.W.Weiss7, J. Grunhut1, G. Handler8,R.Kuschnig9,7,A.Mehner2,H.Pablo5,A.Popowicz10,S.Rucinski11, and G. Whittaker11 1 European Organisation for Astronomical Research in the Southern Hemisphere (ESO), Karl-Schwarzschild-Str. 2, 85748 Garching, Germany e-mail: [email protected] 2 European Organisation for Astronomical Research in the Southern Hemisphere (ESO), Casilla 19001, Santiago 19, Chile 3 Astronomical Institute, Wrocław University, Kopernika 11, 51-622 Wrocław, Poland 4 Instituto de Astronomia, Geofísica e Ciências Atmosféricas, Universidade de São Paulo, Rua do Matão 1226, Cidade Universitária, 05508-900 São Paulo, SP, Brazil 5 Département de physique and Centre de Recherche en Astrophysique du Québec (CRAQ), Université de Montréal, CP 6128, Succ. Centre-Ville, Montréal, Québec, H3C 3J7, Canada 6 Department of Physics, Royal Military College of Canada, PO Box 17000, Stn Forces, Kingston, Ontario K7K 7B4, Canada 7 Institute of Astronomy, University of Vienna, Universitätsring 1, 1010 Vienna, Austria 8 Nicolaus Copernicus Astronomical Center, ul. Bartycka 18, 00-716 Warsaw, Poland 9 Department of Physics and Astronomy, University of British Columbia, Vancouver, BC V6T1Z1, Canada 10 Institute of Automatic Control, Silesian University of Technology, Gliwice, Poland 11 Department of Astronomy & Astrophysics, University of Toronto, 50 St. George St, Toronto, Ontario, M5S 3H4, Canada Received 21 December 2015 / Accepted 1 February 2016 ABSTRACT Context. -
DMAAC – February 1973
LUNAR TOPOGRAPHIC ORTHOPHOTOMAP (LTO) AND LUNAR ORTHOPHOTMAP (LO) SERIES (Published by DMATC) Lunar Topographic Orthophotmaps and Lunar Orthophotomaps Scale: 1:250,000 Projection: Transverse Mercator Sheet Size: 25.5”x 26.5” The Lunar Topographic Orthophotmaps and Lunar Orthophotomaps Series are the first comprehensive and continuous mapping to be accomplished from Apollo Mission 15-17 mapping photographs. This series is also the first major effort to apply recent advances in orthophotography to lunar mapping. Presently developed maps of this series were designed to support initial lunar scientific investigations primarily employing results of Apollo Mission 15-17 data. Individual maps of this series cover 4 degrees of lunar latitude and 5 degrees of lunar longitude consisting of 1/16 of the area of a 1:1,000,000 scale Lunar Astronautical Chart (LAC) (Section 4.2.1). Their apha-numeric identification (example – LTO38B1) consists of the designator LTO for topographic orthophoto editions or LO for orthophoto editions followed by the LAC number in which they fall, followed by an A, B, C or D designator defining the pertinent LAC quadrant and a 1, 2, 3, or 4 designator defining the specific sub-quadrant actually covered. The following designation (250) identifies the sheets as being at 1:250,000 scale. The LTO editions display 100-meter contours, 50-meter supplemental contours and spot elevations in a red overprint to the base, which is lithographed in black and white. LO editions are identical except that all relief information is omitted and selenographic graticule is restricted to border ticks, presenting an umencumbered view of lunar features imaged by the photographic base. -
October 2006
OCTOBER 2 0 0 6 �������������� http://www.universetoday.com �������������� TAMMY PLOTNER WITH JEFF BARBOUR 283 SUNDAY, OCTOBER 1 In 1897, the world’s largest refractor (40”) debuted at the University of Chica- go’s Yerkes Observatory. Also today in 1958, NASA was established by an act of Congress. More? In 1962, the 300-foot radio telescope of the National Ra- dio Astronomy Observatory (NRAO) went live at Green Bank, West Virginia. It held place as the world’s second largest radio scope until it collapsed in 1988. Tonight let’s visit with an old lunar favorite. Easily seen in binoculars, the hexagonal walled plain of Albategnius ap- pears near the terminator about one-third the way north of the south limb. Look north of Albategnius for even larger and more ancient Hipparchus giving an almost “figure 8” view in binoculars. Between Hipparchus and Albategnius to the east are mid-sized craters Halley and Hind. Note the curious ALBATEGNIUS AND HIPPARCHUS ON THE relationship between impact crater Klein on Albategnius’ southwestern wall and TERMINATOR CREDIT: ROGER WARNER that of crater Horrocks on the northeastern wall of Hipparchus. Now let’s power up and “crater hop”... Just northwest of Hipparchus’ wall are the beginnings of the Sinus Medii area. Look for the deep imprint of Seeliger - named for a Dutch astronomer. Due north of Hipparchus is Rhaeticus, and here’s where things really get interesting. If the terminator has progressed far enough, you might spot tiny Blagg and Bruce to its west, the rough location of the Surveyor 4 and Surveyor 6 landing area. -
Open Hanagan Thesis Schreyer.Pdf
THE PENNSYLVANIA STATE UNIVERSITY SCHREYER HONORS COLLEGE DEPARTMENT OF EARTH AND MINERAL SCIENCES CHANGES IN CRATER MORPHOLOGY ASSOCIATED WITH VOLCANIC ACTIVITY AT TELICA VOLCANO, NICARAGUA: INSIGHT INTO SUMMIT CRATER FORMATION AND ERUPTION TRIGGERING CATHERINE E. HANAGAN SPRING 2019 A thesis submitted in partial fulfillment of the requirements for a baccalaureate degree in the Geosciences with honors in the Geosciences Reviewed and approved* by the following: Peter La Femina Associate Professor of Geosciences Thesis Supervisor Maureen Feineman Associate Research Professor and Associate Head for Undergraduate Programs Honors Adviser * Signatures are on file in the Schreyer Honors College. i ABSTRACT Telica is a persistently active basaltic-andesite stratovolcano in the Central American Volcanic Arc of Nicaragua. Poorly predicted sub-decadal, low explosivity (VEI 1-2) phreatic eruptions and background persistent activity with high-rates of seismic unrest and frequent degassing contribute to morphologic change in Telica’s active crater on a small spatiotemporal scale. These changes sustain a morphology similar to those of commonly recognized calderas or pit craters (Roche et al., 2001; Rymer et al., 1998), and have been related to sealing of the hydrothermal system prior to eruption (INETER Buletin Anual, 2013). We use photograph observations and Structure from Motion point cloud construction and comparison (Multiscale Model to Model Cloud Comparison, Lague et al., 2013; Westoby et al., 2012) from 1994 to 2017 to correlate changes in Telica’s crater with sustained summit crater formation and eruptive pre- cursors. Two previously proposed mechanisms for sealing at Telica are: 1) widespread hydrothermal mineralization throughout the magmatic-hydrothermal system (Geirsson et al., 2014; Rodgers et al., 2015; Roman et al., 2016); and/or 2) surficial blocking of the vent by landslides and rock fall (INETER Buletin Anual, 2013). -
The History Problem: the Politics of War
History / Sociology SAITO … CONTINUED FROM FRONT FLAP … HIRO SAITO “Hiro Saito offers a timely and well-researched analysis of East Asia’s never-ending cycle of blame and denial, distortion and obfuscation concerning the region’s shared history of violence and destruction during the first half of the twentieth SEVENTY YEARS is practiced as a collective endeavor by both century. In The History Problem Saito smartly introduces the have passed since the end perpetrators and victims, Saito argues, a res- central ‘us-versus-them’ issues and confronts readers with the of the Asia-Pacific War, yet Japan remains olution of the history problem—and eventual multiple layers that bind the East Asian countries involved embroiled in controversy with its neighbors reconciliation—will finally become possible. to show how these problems are mutually constituted across over the war’s commemoration. Among the THE HISTORY PROBLEM THE HISTORY The History Problem examines a vast borders and generations. He argues that the inextricable many points of contention between Japan, knots that constrain these problems could be less like a hang- corpus of historical material in both English China, and South Korea are interpretations man’s noose and more of a supportive web if there were the and Japanese, offering provocative findings political will to determine the virtues of peaceful coexistence. of the Tokyo War Crimes Trial, apologies and that challenge orthodox explanations. Written Anything less, he explains, follows an increasingly perilous compensation for foreign victims of Japanese in clear and accessible prose, this uniquely path forward on which nationalist impulses are encouraged aggression, prime ministerial visits to the interdisciplinary book will appeal to sociol- to derail cosmopolitan efforts at engagement. -
SPECIES REPORT Sierra Nevada Red Fox (Vulpes Vulpes Necator)
SPECIES REPORT Sierra Nevada Red Fox (Vulpes vulpes necator) U.S. FISH AND WILDLIFE SERVICE August 14, 2015 Table of Contents INTRODUCTION .......................................................................................................................... 4 ACRONYMS AND SUBSTITUTIONS USED ............................................................................. 4 SPECIES AND SUBSPECIES DESCRIPTION ............................................................................ 5 TAXONOMY AND GENETICS ................................................................................................... 6 Taxonomic History and Relationship to Other Fox Subspecies ........................................... 6 Genetics ...................................................................................................................................... 7 RANGE AND DISTRIBUTION .................................................................................................... 8 Historical Range ........................................................................................................................ 8 Map 1: SNRF Historical Range in California .................................................................... 9 Current Distribution ............................................................................................................... 10 Map 2: SNRF Sighting Areas............................................................................................. 12 Table 1: SNRF Sighting Areas .......................................................................................... -
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).