Analysis of the Influence of Lunar Cycle on the Frequency of Spontaneous Deliveries: a Single-Centre Retrospective Study
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Warren and Taylor-2014-In Tog-The Moon-'Author's Personal Copy'.Pdf
This article was originally published in Treatise on Geochemistry, Second Edition published by Elsevier, and the attached copy is provided by Elsevier for the author's benefit and for the benefit of the author's institution, for non- commercial research and educational use including without limitation use in instruction at your institution, sending it to specific colleagues who you know, and providing a copy to your institution’s administrator. All other uses, reproduction and distribution, including without limitation commercial reprints, selling or licensing copies or access, or posting on open internet sites, your personal or institution’s website or repository, are prohibited. For exceptions, permission may be sought for such use through Elsevier's permissions site at: http://www.elsevier.com/locate/permissionusematerial Warren P.H., and Taylor G.J. (2014) The Moon. In: Holland H.D. and Turekian K.K. (eds.) Treatise on Geochemistry, Second Edition, vol. 2, pp. 213-250. Oxford: Elsevier. © 2014 Elsevier Ltd. All rights reserved. Author's personal copy 2.9 The Moon PH Warren, University of California, Los Angeles, CA, USA GJ Taylor, University of Hawai‘i, Honolulu, HI, USA ã 2014 Elsevier Ltd. All rights reserved. This article is a revision of the previous edition article by P. H. Warren, volume 1, pp. 559–599, © 2003, Elsevier Ltd. 2.9.1 Introduction: The Lunar Context 213 2.9.2 The Lunar Geochemical Database 214 2.9.2.1 Artificially Acquired Samples 214 2.9.2.2 Lunar Meteorites 214 2.9.2.3 Remote-Sensing Data 215 2.9.3 Mare Volcanism -
The Association Between the Lunar Cycle and Patterns
THE ASSOCIATION BETWEEN THE LUNAR CYCLE AND PATTERNS OF PATIENT PRESENTATION TO THE EMERGENCY DEPARTMENT. Grant Dudley Futcher Student number: 7709742 A research report submitted to the Faculty of Health Sciences, University of the Witwatersrand, in partial fulfilment of the requirements for the degree of Master of Science in Medicine in Emergency Medicine. Johannesburg, 2015 i DECLARATION I, Grant Dudley Futcher, declare that this research report is my own work. It is being submitted for the degree of Master of Science in Medicine (Emergency Medicine) in the University of the Witwatersrand, Johannesburg. It has not been submitted before for any degree or examination at this or any other University. Signed on 25th day of August 2015 ii DEDICATION This work is dedicated to my children, Charis, Luke and Jarryd, who have patiently endured their father’s choice of medical discipline. iii PUBLICATIONS ARISING FROM THIS STUDY Nil iv ABSTRACT Aim: To determine any association between the lunar synodic or anomalistic months and the nature and volume of emergency department patient consultations and hospital admissions from the emergency department (ED). Design: A retrospective, descriptive study. Setting: All South African EDs of a private hospital group. Patients: All patients consulted from 01 January 2005 to 31 December 2010. Methods: Data was extracted from monthly records and statistically evaluated, controlling for calendric variables. Lunar variables were modelled with volumes of differing priority of hospital admissions and consultation categories including; trauma, medical, paediatric, work injuries, obstetrics and gynaecology, intentional self harm, sexual assault, dog bites and total ED consultations. Main Results: No significant differences were found in all anomalistic and most synodic models with the consultation categories. -
Secondary Resonances Due to the Solar Radiation Pressure in the Vicinity of the Global Navigation Satellites Regions
DOI: 10.13009/EUCASS2019-420 8TH EUROPEAN CONFERENCE FOR AERONAUTICS AND SPACE SCIENCES (EUCASS) Secondary resonances due to the solar radiation pressure in the vicinity of the global navigation satellites regions Eduard Kuznetsov, Vladislav Gusev and Ivan Malyutin Ural Federal University Lenina Avenue, 51, Yekaterinburg, Russia 620000, [email protected] Abstract The secondary resonances due to solar radiation pressure are investigated in the vicinity of orbits of the global navigation systems GLONASS (main resonance is 8:17), GPS (main resonance is 1:2), BeiDou (main resonance is 7:13), and Galileo (main resonance is 10:17). The secondary resonances were considered for both the main resonances and the sub-resonances i- and e-types. The secondary resonances locations were estimated analytically and were improved by numerically. The secondary resonance zones were found for both low (0.02, 0.2, and 1 m2/kg) and high (10 m2/kg and more) area- to-mass ratios. The secondary resonances have a significant effect on the dynamical evolution of objects with area-to-mass ratio 10 m2/kg and more. This result is very important when describing the long-term orbital evolution of space debris. 1. Introduction Valk et al. [1] found a relevant class of secondary resonances on both sides of the well-known pendulum-like pattern of geostationary objects. They have considered the secondary resonances due to solar radiation pressure with a resonant argument Ψ = 푘Φ ± 휆⨀. Here Φ is a resonant argument of a main resonance 1:1 and 휆⨀ is the ecliptic longitude of the Sun. The secondary resonances were detected for objects with high area-to-mass ratio γ = 10 m2/kg and more. -
37131054409156D.Pdf
YEZAD A Romance of the Unknown By GEORGE BABCOCK PUBLISHED BY CO-OPERATIVE PUBLISHING CO., INC. BRIDGEPORT, CONN. NEW YORK, N. Y. Copyright, November, 1922, by GEORGE BABCOCK All rights reserved To MY S1sTER, EVA STANTON (BABCOCK) BROWNING., this story 1s affectionately inscribed. GEORGE BABCOCK. Brooklyn, N. Y. November, 19ff. CHARACTERS l JOHN BACON, Aviator. 2 JuLIA BACON, His Wife. 3 PAUL BACON, Son. 4 ELLEN BACON, Daughter. 5 AnoLPH VON PosEN, Inventor, in love. 6 SALLY T1MPOLE, the Cook, also in love. 7 JASPER PERKINS } 8 SILAS CUMMINGS The old quaint cronies. 9 NANCY PRINDLE 10 DOCTOR PETER KLOUSE. 11 HESTER DOUGLASS} 12 F IN LEY D OU GLASS Grandchildren of the Doctor. 13 SAM WILLIS, the dreadful liar. 14 WILLIAM THADDEUS TITUS, Champion of several trades. 15 WILLIAM GRENNELL, the Village Blacksmith. 16 MINNA BACON } 17 B RENDA B ACON Children of Paul and Hester. 18 RoBERT DouGLAss, Son of Finley and Ellen. 19 CHARLOTTE Dun LEY, a Maiden of Mars. 20 CHRISTOPHER SPENCER, Astronomer of Mars. 21 FELIX CLAUDIO, the Devil's Son. 22 DocToR NATHAN ELIZABRAT of Mars. 23 MARCOMET, a Guard of the Great White \Vay. 24 JOHN BACON'S DUALITY. Note:-A Glossary of coined and unusual words and their mean ing, used by the author in Yezad, will be found on pages 449 to 463. CONTENTS CHAPTER PAGE I THE PRICE OF PROGRESS 1 II THE GHOST • 20 III NEW NEIGHBORS 33 IV DOCTOR KLOUSE 45 V HEREDITY VS. KLOUSE PHILOSOPHY 52 VI A DREADFUL LIAR • 57 VII AMONG THE ABORIGINES 71 VIII AN ODD EXPERIMENT . -
Origin and Evolution of the Moon's Procellarum KREEP
Decadal Survey 2023 White Paper: Origin and Evolution of the Procellarum KREEP Terrane Origin and Evolution of the Moon’s Procellarum KREEP Terrane A White Paper submitted to the 2023 Planetary Science Decadal Survey, July 15, 2020 Authorship Brad Jolliff, Washington University in St. Louis, [email protected] Mark Robinson, Arizona State University, [email protected] Srinidhi Ravi, Arizona State University, [email protected] Co-signatories on the last page The Procellarum KREEP Terrane on the Moon’s nearside is a unique province that produced volcanism over an extended period of the Moon’s history. Thermal evolution of the lunar mantle in this region may have been driven by a high concentration of radiogenic heat-producing elements. This region is key to unlocking the thermal evolution of the Moon and may have implications for our understanding of extensive volcanism on other inner Solar System bodies such as Mercury and Mars. Major volcanic features of this terrane could be explored by a long-distance rover in a New Frontiers class mission to answer questions about how this planetary asymmetry formed, why volcanism was so voluminous in this region, and how it persisted for nearly 4 billion years. Introduction. The Moon displays a fundamental asymmetry that has been evident since the first images of the farside revealed an ancient, mountainous, heavily cratered feldspathic highlands but very little of the low-lying, dark basaltic plains that are prominent on the nearside, especially the western regions that incorporate Oceanus Procellarum, Imbrium, and several other nearside impact basins. Apollo orbital remote sensing revealed the first glimpses of compositional variations that corresponded to the hemispheric asymmetry, but only in narrow, near-equatorial orbital swaths. -
Formation Flying in the Sun-Earth/Moon Perturbed Restricted Three-Body Problem
DELFT UNIVERSITY OF TECHNOLOGY FACULTY OF AEROSPACE ENGINEERING MASTER’S THESIS Formation Flying in the Sun-Earth/Moon Perturbed Restricted Three-Body Problem IN PARTIAL FULFILLMENT OF THE REQUIREMENTS FOR THE DEGREE OF MASTER OF SCIENCE IN AEROSPACE ENGINEERING Committee: Author: Prof. Dr. Ir. P.N.A.M VISSER Ingvar OUT Dr. Ir. J.A.A. van den IJSSEL Ir. B.T.C. ZANDBERGEN April 18, 2017 Preface This report describes the results of a Master’s thesis on formation flying in the Sun-Earth/Moon perturbed restricted three-body problem, performed in partial fulfillment of a Master of Science degree in Aerospace Engineering at Delft University of Technology. Note that all simulations performed for the investigation of formation flying in the restricted three-body problem, are written entirely by the current author, with the exception of the Dormand-Prince numerical integrator, for which the TU Delft Astrodynamics Toolbox (TUDat) is used, comprising a set of C++ libraries written for a variety of astrodynamics applications. TUDat is developed and maintained by the astrodynamics and space missions research group at the faculty of Aerospace Engineering at Delft University of Technology. This Master’s thesis has been performed in collaboration with Dr. Ir. J. van den IJssel, whose guidance throughout the process of my thesis was key in shaping my research, and whom my sincerest gratitude goes out to for her feedback and support. iii Contents Preface iii Summary vii 1 Introduction 1 2 The Circular Restricted Three-Body Problem 3 2.1 Equations of motion . .3 2.2 Jacobi’s integral . -
(GRAIL) Mission Maria T. Zuber1*, David E. Smith1, M
Gravity Field of the Moon from the Gravity Recovery and Interior Laboratory (GRAIL) Mission Maria T. Zuber1*, David E. Smith1, Michael M. Watkins2, Sami W. Asmar2, Alexander S. Konopliv2, Frank G. Lemoine3, H. Jay Melosh4, Gregory A. Neumann3, Roger J. Phillips5, Sean C. Solomon6,7, Mark A. Wieczorek8, James G. Williams2, Sander J. Goossens9, Gerhard Kruizinga2, Erwan Mazarico1, Ryan S. Park2 and Dah-Ning Yuan2 Submitted to: Science 12 October 2012 Spacecraft-to-spacecraft tracking observations from the Gravity Recovery and Interior Laboratory (GRAIL) have been used to construct a gravitational field of the Moon to spherical harmonic degree and order 420. The GRAIL field reveals features not previously resolved, including tectonic structures, volcanic landforms, basin rings, crater central peaks, and numerous simple craters. From degrees 80 through 300, over 98% of the gravitational signature is associated with topography, which reflects the preservation of craters in highly fractured crust. The remaining 2% represents fine details of subsurface structure not previously resolved. Ghost craters in the maria are not abundant, consistent with underlying highland crust being significantly modified by dikes and intrusions. GRAIL elucidates the role of impact bombardment in homogenizing the distribution of shallow density anomalies on terrestrial planetary bodies. _____________ The Moon is a key to deciphering the evolutionary history of the terrestrial planets because it is the most accessible planetary body that preserves a surface record spanning most of solar system history. Reconstructing planetary evolution requires an understanding of the structure of the interior, which contains information on bulk composition, differentiation, and the nature of heat generation and heat loss that has influenced the style, extent, and duration of volcanism and tectonics. -
Phd Thesis, University of the Armed Forces Germany, 2003
Multiphase Low-Thrust Trajectory Optimization Using Evolutionary Neurocontrol Multiphase Low-Thrust Trajectory Optimization Using Evolutionary Neurocontrol Proefschrift ter verkrijging van de graad van doctor aan de Technische Universiteit Delft, op gezag van de Rector Magnificus prof.ir. K.C.A.M. Luyben; voorzitter van het College voor Promoties, in het openbaar te verdedigen op dinsdag 7 juni 2016 om 12:30 uur door Andreas OHNDORF Diplom-Ingenieur Luft- und Raumfahrttechnik (univ.), Universit¨atder Bundeswehr M¨unchen, Duitsland geboren te Finsterwalde, Duitsland Dit proefschrift is goedgekeurd door de promotor: Prof.dr. E. K. A. Gill Samenstelling promotiecommissie: Rector Magnificus, voorzitter Prof.dr. E. K. A. Gill, Technische Universiteit Delft Onafhankelijke leden: Prof.ir. B. A. C. Ambrosius, Technische Universiteit Delft Prof.dr.ir. M. Mulder, Technische Universiteit Delft Prof. D. Scheeres, University of Colorado, U.S.A. Prof. B. Dachwald, Aachen University of Applied Sciences (FH), Germany Prof. M. Vasile, University of Strathclyde, U.K. Prof. M. Lavagna, Politecnico di Milano, Italy Abstract To fulfill the objectives of deep space missions, such as in situ measurements at an outer planet's moon or investigations at main belt asteroids, spacecraft must be provided with sufficient energy to get to these distant objects. This energy be expressed with the so-called ∆V -budget, which is the sum of required velocity changes along a spacecraft's trajectory. As today's and future deep space missions are infeasible using chemical propulsion alone, their trajectories involve one or more close flybys at mass-rich celestial bodies to gain additional orbit energy. These maneuvers are called gravity assists and depend on the relative positions of the assisting body and the respective target. -
An Impact Origin of the Lunar Procellarum Kreep Terrane
51st Lunar and Planetary Science Conference (2020) 1318.pdf AN IMPACT ORIGIN OF THE LUNAR PROCELLARUM KREEP TERRANE. Matt J. Jones1 (mat- [email protected]), Alexander J. Evans1, Brandon C. Johnson2, Matthew B. Weller1, James T. Keane3, and Sonia M. Tikoo4, 1Department of Earth, Environmental and Planetary Sciences, Brown University, Providence, RI 02906, 2Department of Earth, Atmospheric, and Planetary Sciences, Purdue University, 3Division of Geological and Planetary Sciences, California Institute of Technology, 4School of Earth, Energy and Environmental Sciences, Stan- ford University. Introduction: The lunar South Pole–Aitken (SPA) shock-induced temperatures by the mantle solidus, as basin is the largest and oldest recognized impact basin the timescale of impact melt crystallization is short on the Moon [1]. Located on the farside hemisphere compared to the timescale of thermochemical convec- (Fig. 1), SPA is nearly antipodal to the nearside geo- tion [7, 13]. chemical province referred to as the Procellarum Initial Conditions. The silicate portion of the Moon KREEP Terrane (PKT) [2, 3]. (KREEP is a geochemical is hypothesized to have fractionally crystallized from a component named for its enrichment in incompatible el- lunar magma ocean (LMO); we initialized our simula- ements including Potassium (K), Rare Earth Elements tions with temperature and composition structures con- (REE), and Phosphorous (P) [4]). The PKT represents sistent with this hypothesis. Toward the end of solidifi- an as-of-yet unexplained compositional asymmetry on cation, a global layer of dense, low-viscosity, KREEP- the lunar surface, but the relative position of the two re- rich material is expected beneath the crust and above a gions may be indicative of the SPA impact playing a cumulate mantle [4, 14, 15]. -
The First Men in the Moon
i/-^ GLENN NEGIEV ARTHUR COWELL, STREET, 70, WESTBY LYTHA^A DUKE UNIVERSITY LIBRARY FRIENDS OF DUKE UNIVERSITY LIBRARY GIFT OF Glena Negley THE FIRST MEN IN THE MOON Digitized by tine Internet Arciiive in 2010 witii funding from Duke University Libraries littp://www.arcliive.org/details/firstmeninmooOOwell " I was progressing in great leaps and bounds Frontispiece. — The First Men in the Moon By H. G. Wells Author of "Tales of Space and Time," " Love and Mr. Lewisham," " and " Anticipations "Three thousand stadia from the earth to the moon. , . Marvel not, my comrade, if I appear talking to you on super-terrestrial and aerial topics. The long and the short of the matter is that I am running over the order of a Journey I have lately made." Lucian's Icaromenippus London George Newnes, Limited Southampton Street, Strand* 1901 CONTENTS PAGE I. MR. BEDFORD MEETS MR. CAVOR AT LYMPNE I II. THE B'IRST MAKING OF CAVORITE 28 III. THE BUILDING OF THE SPHERE 4T IV. INSIDE THE SPHERE 54 V. THE JOURNEY TO THE MOON 61 VI. THE LANDING ON THE MOON 70 VII. SUNRISE ON THE MOON 77 VIII. A LUNAR MORNING 85 IX. PROSPECTING BEGINS 92 X. LOST MEN IN THE MOON 107 XL THE MOONCALF PASTURES XII. THE SELENITE's FACE . 132 XIII. MR. CAVOR MAKES SOME SUGGESTIONS 140 XIV. EXPERIMENTS IN INTERCOURSE 152 XV. THE GIDDY BRIDGE 161 XVI. POINTS OF VIEW .... 178 XVII. THE FIGHT IN THE CAVE OF THE MOON BUTCHERS ..... 191 XVIII. IN THE SUNLIGHT 207 VI CONTENTS PAGE XIX. MR. BEDFORD ALONE ... -
Hls-Ug-001 Human Landing System Lunar Thermal Analysis Guidebook
HLS-UG-001 BASELINE RELEASE National Aeronautics and EFFECTIVE DATE: JANUARY 04, 2021 Space Administration HUMAN LANDING SYSTEM LUNAR THERMAL ANALYSIS GUIDEBOOK Publicly Available: Release to Public Websites Requires Approval of Chief, Office of Primary Responsibility, and approval via the Scientific and Technical Information (STI) process, if applicable The electronic version is the official approved document. Verify this is the correct version before use. Human Landing System Lunar Thermal Analysis Guidebook January 2021 Revision: Baseline Release Document No: HLS-UG-01 Effective Date: January 04, 2021 Page: 1 of 147 Title: Human Landing System Lunar Thermal Analysis Guidebook REVISION AND HISTORY PAGE Revision Change Effective Description No. No. Date - HLS- Baseline Release (Reference HCB.07.01.2020) 01/04/2021 C0064 The electronic version is the official approved document. Verify this is the correct version before use. Human Landing System Lunar Thermal Analysis Guidebook January 2021 Revision: Baseline Release Document No: HLS-UG-01 Effective Date: January 04, 2021 Page: 2 of 147 Title: Human Landing System Lunar Thermal Analysis Guidebook TABLE OF CONTENTS SECTION PAGE 1.0 INTRODUCTION ................................................................................................. 10 PURPOSE ........................................................................................................... 10 SCOPE ................................................................................................................ 10 CHANGE -
Lunar and Planetary Bases, Habitats, and Colonies
Lunar and Planetary Bases, Habitats, and Colonies A Special Bibliography From the NASA Scientific and Technical Information Program Includes the design and construction of lunar and Mars bases, habitats, and settlements; construction materials and equipment; life support systems; base operations and logistics; thermal management and power systems; and robotic systems. January 2004 Lunar and Planetary Bases, Habitats, and Colonies A Special Bibliography from the NASA Scientific and Technical Information Program JANUARY 2004 20010057294 NASA Langley Research Center, Hampton, VA USA Radiation Transport Properties of Potential In Situ-Developed Regolith-Epoxy Materials for Martian Habitats Miller, J.; Heilbronn, L.; Singleterry, R. C., Jr.; Thibeault, S. A.; Wilson, J. W.; Zeitlin, C. J.; Microgravity Materials Science Conference 2000; March 2001; Volume 2; In English; CD-ROM contains the entire Conference Proceedings presented in PDF format; No Copyright; Abstract Only; Available from CASI only as part of the entire parent document We will evaluate the radiation transport properties of epoxy-martian regolith composites. Such composites, which would use both in situ materials and chemicals fabricated from elements found in the martian atmosphere, are candidates for use in habitats on Mars. The principal objective is to evaluate the transmission properties of these materials with respect to the protons and heavy charged particles in the galactic cosmic rays which bombard the martian surface. The secondary objective is to evaluate fabrication methods which could lead to technologies for in situ fabrication. The composites will be prepared by NASA Langley Research Center using simulated martian regolith. Initial evaluation of the radiation shielding properties will be made using transport models developed at NASA-LaRC and the results of these calculations will be used to select the composites with the most favorable radiation transmission properties.