Planetary Penetrators: Their Origins, History and Future
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Geoscience and a Lunar Base
" t N_iSA Conference Pubhcatmn 3070 " i J Geoscience and a Lunar Base A Comprehensive Plan for Lunar Explora, tion unclas HI/VI 02907_4 at ,unar | !' / | .... ._-.;} / [ | -- --_,,,_-_ |,, |, • • |,_nrrr|l , .l -- - -- - ....... = F _: .......... s_ dd]T_- ! JL --_ - - _ '- "_r: °-__.......... / _r NASA Conference Publication 3070 Geoscience and a Lunar Base A Comprehensive Plan for Lunar Exploration Edited by G. Jeffrey Taylor Institute of Meteoritics University of New Mexico Albuquerque, New Mexico Paul D. Spudis U.S. Geological Survey Branch of Astrogeology Flagstaff, Arizona Proceedings of a workshop sponsored by the National Aeronautics and Space Administration, Washington, D.C., and held at the Lunar and Planetary Institute Houston, Texas August 25-26, 1988 IW_A National Aeronautics and Space Administration Office of Management Scientific and Technical Information Division 1990 PREFACE This report was produced at the request of Dr. Michael B. Duke, Director of the Solar System Exploration Division of the NASA Johnson Space Center. At a meeting of the Lunar and Planetary Sample Team (LAPST), Dr. Duke (at the time also Science Director of the Office of Exploration, NASA Headquarters) suggested that future lunar geoscience activities had not been planned systematically and that geoscience goals for the lunar base program were not articulated well. LAPST is a panel that advises NASA on lunar sample allocations and also serves as an advocate for lunar science within the planetary science community. LAPST took it upon itself to organize some formal geoscience planning for a lunar base by creating a document that outlines the types of missions and activities that are needed to understand the Moon and its geologic history. -
Planetary Surfaces
Chapter 4 PLANETARY SURFACES 4.1 The Absence of Bedrock A striking and obvious observation is that at full Moon, the lunar surface is bright from limb to limb, with only limited darkening toward the edges. Since this effect is not consistent with the intensity of light reflected from a smooth sphere, pre-Apollo observers concluded that the upper surface was porous on a centimeter scale and had the properties of dust. The thickness of the dust layer was a critical question for landing on the surface. The general view was that a layer a few meters thick of rubble and dust from the meteorite bombardment covered the surface. Alternative views called for kilometer thicknesses of fine dust, filling the maria. The unmanned missions, notably Surveyor, resolved questions about the nature and bearing strength of the surface. However, a somewhat surprising feature of the lunar surface was the completeness of the mantle or blanket of debris. Bedrock exposures are extremely rare, the occurrence in the wall of Hadley Rille (Fig. 6.6) being the only one which was observed closely during the Apollo missions. Fragments of rock excavated during meteorite impact are, of course, common, and provided both samples and evidence of co,mpetent rock layers at shallow levels in the mare basins. Freshly exposed surface material (e.g., bright rays from craters such as Tycho) darken with time due mainly to the production of glass during micro- meteorite impacts. Since some magnetic anomalies correlate with unusually bright regions, the solar wind bombardment (which is strongly deflected by the magnetic anomalies) may also be responsible for darkening the surface [I]. -
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 -
3.1 the Dambusters Revisited
The Dambusters Revisited J.L. HINKS, Halcrow Group Ltd. C. HEITEFUSS, Ruhr River Association M. CHRIMES, Institution of Civil Engineers SYNOPSIS. The British raid on the Möhne, Eder and Sorpe dams on the night of 16/17 May, 1943 caused the breaching of the 40m high Möhne and 48m high Eder dams and serious damage to the 69m high Sorpe dam. This paper considers the planning for the raid, model testing, the raid itself, the effects of the breaches and the subsequent rehabilitation of the dams. Whilst the subject is of considerable historical interest it also has significant contemporary relevance. Events following the breaching of the dams have been used for the calibration of dambreak studies and emphasise the vulnerability of road and railway bridges which is not always acknowledged in contemporary studies. INTRODUCTION In researching this paper the authors have been very struck by the human interest in the story of English, German and Ukrainian people, whether civilian or in uniform, who participated in some aspect of the raid or who lost their lives or homes. As befits a paper for the British Dam Society, this paper, however, concentrates on the technical questions that arise, leaving the human story to others. This paper was prompted by the BDS sponsored visit, in April 2009, to the Derwent Reservoir by 43 members of the Association of Friends of the Hubert-Engels Institute of Hydraulic Engineering and Applied Hydromechanics at Dresden University of Technology. There is a small museum at the dam run by Vic Hallam, an employee of Severn Trent Water. -
The Development of Military Nuclear Strategy And
The Development of Military Nuclear Strategy and Anglo-American Relations, 1939 – 1958 Submitted by: Geoffrey Charles Mallett Skinner to the University of Exeter as a thesis for the degree of Doctor of Philosophy in History, July 2018 This thesis is available for Library use on the understanding that it is copyright material and that no quotation from the thesis may be published without proper acknowledgement. I certify that all material in this thesis which is not my own work has been identified and that no material has previously been submitted and approved for the award of a degree by this or any other University. (Signature) ……………………………………………………………………………… 1 Abstract There was no special governmental partnership between Britain and America during the Second World War in atomic affairs. A recalibration is required that updates and amends the existing historiography in this respect. The wartime atomic relations of those countries were cooperative at the level of science and resources, but rarely that of the state. As soon as it became apparent that fission weaponry would be the main basis of future military power, America decided to gain exclusive control over the weapon. Britain could not replicate American resources and no assistance was offered to it by its conventional ally. America then created its own, closed, nuclear system and well before the 1946 Atomic Energy Act, the event which is typically seen by historians as the explanation of the fracturing of wartime atomic relations. Immediately after 1945 there was insufficient systemic force to create change in the consistent American policy of atomic monopoly. As fusion bombs introduced a new magnitude of risk, and as the nuclear world expanded and deepened, the systemic pressures grew. -
Planning a Mission to the Lunar South Pole
Lunar Reconnaissance Orbiter: (Diviner) Audience Planning a Mission to Grades 9-10 the Lunar South Pole Time Recommended 1-2 hours AAAS STANDARDS Learning Objectives: • 12A/H1: Exhibit traits such as curiosity, honesty, open- • Learn about recent discoveries in lunar science. ness, and skepticism when making investigations, and value those traits in others. • Deduce information from various sources of scientific data. • 12E/H4: Insist that the key assumptions and reasoning in • Use critical thinking to compare and evaluate different datasets. any argument—whether one’s own or that of others—be • Participate in team-based decision-making. made explicit; analyze the arguments for flawed assump- • Use logical arguments and supporting information to justify decisions. tions, flawed reasoning, or both; and be critical of the claims if any flaws in the argument are found. • 4A/H3: Increasingly sophisticated technology is used Preparation: to learn about the universe. Visual, radio, and X-ray See teacher procedure for any details. telescopes collect information from across the entire spectrum of electromagnetic waves; computers handle Background Information: data and complicated computations to interpret them; space probes send back data and materials from The Moon’s surface thermal environment is among the most extreme of any remote parts of the solar system; and accelerators give planetary body in the solar system. With no atmosphere to store heat or filter subatomic particles energies that simulate conditions in the Sun’s radiation, midday temperatures on the Moon’s surface can reach the stars and in the early history of the universe before 127°C (hotter than boiling water) whereas at night they can fall as low as stars formed. -
Canadian Airmen Lost in Wwii by Date 1943
CANADA'S AIR WAR 1945 updated 21/04/08 January 1945 424 Sqn. and 433 Sqn. begin to re-equip with Lancaster B.I & B.III aircraft (RCAF Sqns.). 443 Sqn. begins to re-equip with Spitfire XIV and XIVe aircraft (RCAF Sqns.). Helicopter Training School established in England on Sikorsky Hoverfly I helicopters. One of these aircraft is transferred to the RCAF. An additional 16 PLUTO fuel pipelines are laid under the English Channel to points in France (Oxford). Japanese airstrip at Sandakan, Borneo, is put out of action by Allied bombing. Built with forced labour by some 3,600 Indonesian civilians and 2,400 Australian and British PoWs captured at Singapore (of which only some 1,900 were still alive at this time). It is decided to abandon the airfield. Between January and March the prisoners are force marched in groups to a new location 160 miles away, but most cannot complete the journey due to disease and malnutrition, and are killed by their guards. Only 6 Australian servicemen are found alive from this group at the end of the war, having escaped from the column, and only 3 of these survived to testify against their guards. All the remaining enlisted RAF prisoners of 205 Sqn., captured at Singapore and Indonesia, died in these death marches (Jardine, wikipedia). On the Russian front Soviet and Allied air forces (French, Czechoslovakian, Polish, etc, units flying under Soviet command) on their front with Germany total over 16,000 fighters, bombers, dive bombers and ground attack aircraft (Passingham & Klepacki). During January #2 Flying Instructor School, Pearce, Alberta, closes (http://www.bombercrew.com/BCATP.htm). -
Download Complete Volume
JOURNAL OF THE TRANSACTIONS OF THE - VICTOR I A INSTITUTE. VOL. XXI. SECTION NI;> I FROM SEA. COAST AT A.Sl(A,LA ~ H JERUSAlEM TO THE J,JR~AN IIIC.0 JEHi CH O." t<0~110,n·... lsc"lt3''"'EII -I,,..,;;": C.S. Wlc.Sw,a.~t,n,,,ofl'l,illutin., N. l. Nwri,.wlil,: .l,V,W,,tn,u,, C. l . Crct,rcc,,,,,, J.,,,.,,,.i,,,,..., _ N. 1.:. }Vu.blit.n. Sun.J&/.,)1.,. F. V, £,,1.~1,,,,~. SECTION N'? 2. FRO M T H E. T A.B LE · LANO Of' S ,JUD.EA TOT Mt PLAINS Of'MOA.B ~. oFKtRAH. 8YJEB£L USOUM. TA.SL£ L,.ND or MOAB SECTION N~ 7 !='ROM cuLr o F sun MEAFtTO R eY THE M OUNTAINS o, s 1ttA.1 ro-:-wt: PLAT EAU or TH£ TIH. No rt,h, G. &rcy !Jra..,,,i, t;,e, (F>1.r-i,.t(C11) a.n.d, 5,·'hi.tt. w.:.th. ·m.,,m.flr-OU.4 d.y1<.r f! , • ..,,po.-w,g s,uubto,.,, n,,d.Li,,,... •w,,.-B,:,i,, / S . 8 L j 11flRl20NTALSCALr 11MIL[ S• I INCH. J)y l~o;1nniu,on of th i:J Oommittce (•f the /'o,T,i:sti.1w E :cpluMtivn Fund. JOURNAL OF THE TRANSACTIONS OF ~ht lictoria Jnstitut~, <'lR l!gilosopgital cSotiet~ of ~reat Jritain. EDITED BY THE HONORARY SECRETARY, CAPTAIN FRANCIS W. H. PETRIE, F.G.fS., &c. VOL. XXI. LONDON: (tBublisbell n11 tbe Institute). INDIA: W. THACKER & Co. UNITED STATES: G. T.PUTNAM'S SONS, N.Y_. -
Science Concept 5: Lunar Volcanism Provides a Window Into the Thermal and Compositional Evolution of the Moon
Science Concept 5: Lunar Volcanism Provides a Window into the Thermal and Compositional Evolution of the Moon Science Concept 5: Lunar volcanism provides a window into the thermal and compositional evolution of the Moon Science Goals: a. Determine the origin and variability of lunar basalts. b. Determine the age of the youngest and oldest mare basalts. c. Determine the compositional range and extent of lunar pyroclastic deposits. d. Determine the flux of lunar volcanism and its evolution through space and time. INTRODUCTION Features of Lunar Volcanism The most prominent volcanic features on the lunar surface are the low albedo mare regions, which cover approximately 17% of the lunar surface (Fig. 5.1). Mare regions are generally considered to be made up of flood basalts, which are the product of highly voluminous basaltic volcanism. On the Moon, such flood basalts typically fill topographically-low impact basins up to 2000 m below the global mean elevation (Wilhelms, 1987). The mare regions are asymmetrically distributed on the lunar surface and cover about 33% of the nearside and only ~3% of the far-side (Wilhelms, 1987). Other volcanic surface features include pyroclastic deposits, domes, and rilles. These features occur on a much smaller scale than the mare flood basalts, but are no less important in understanding lunar volcanism and the internal evolution of the Moon. Table 5.1 outlines different types of volcanic features and their interpreted formational processes. TABLE 5.1 Lunar Volcanic Features Volcanic Feature Interpreted Process -
Testing Hypotheses for the Origin of Steep Slope of Lunar Size-Frequency Distribution for Small Craters
CORE Metadata, citation and similar papers at core.ac.uk Provided by Springer - Publisher Connector Earth Planets Space, 55, 39–51, 2003 Testing hypotheses for the origin of steep slope of lunar size-frequency distribution for small craters Noriyuki Namiki1 and Chikatoshi Honda2 1Department of Earth and Planetary Sciences, Kyushu University, Hakozaki 6-10-1, Higashi-ku, Fukuoka 812-8581, Japan 2The Institute of Space and Astronautical Science, Yoshinodai 3-1-1, Sagamihara 229-8510, Japan (Received June 13, 2001; Revised June 24, 2002; Accepted January 6, 2003) The crater size-frequency distribution of lunar maria is characterized by the change in slope of the population between 0.3 and 4 km in crater diameter. The origin of the steep segment in the distribution is not well understood. Nonetheless, craters smaller than a few km in diameter are widely used to estimate the crater retention age for areas so small that the number of larger craters is statistically insufficient. Future missions to the moon, which will obtain high resolution images, will provide a new, large data set of small craters. Thus it is important to review current hypotheses for their distributions before future missions are launched. We examine previous and new arguments and data bearing on the admixture of endogenic and secondary craters, horizontal heterogeneity of the substratum, and the size-frequency distribution of the primary production function. The endogenic crater and heterogeneous substratum hypotheses are seen to have little evidence in their favor, and can be eliminated. The primary production hypothesis fails to explain a wide variation of the size-frequency distribution of Apollo panoramic photographs. -
Dr. Sergei Fedorovich Teselkin Lavochkin Association, Russian Federation, [email protected]
69th International Astronautical Congress 2018 Paper ID: 44581 oral IAF SPACE EXPLORATION SYMPOSIUM (A3) Solar System Exploration (5) Author: Dr. Sergei Fedorovich Teselkin Lavochkin Association, Russian Federation, [email protected] \TO VENUS TOGETHER": RUSSIAN-AMERICAN JOINT ENCORE OF VENUS RESEARCHES WITH ORBITER, LANDER AND ATMOSPHERIC PROBES IN THE PROJECT \VENUS-D" Abstract S. Lemeshevskii, Candidate of Economics, [email protected] O. Grafodatskiy, Doctor of Engineering Sci- ence,[email protected] Kh.Karchaev, Candidate of Economics, [email protected] S. Teselkin, Candi- date of PhysicsMathematics,[email protected] V. Vorontsov, Doctor of Engineering Science, [email protected] Lavochkin Association, Russia Mission "Venera-D" by Lavochkin Association implies a long-term study of Venus. International pay- load is to be installed on orbiter, lander and long-living station on Venus surface. The project is a basis for further large-scale international missions to Venus, previously carried out in 1960-80s and early 1990s by Soviet and American spacecraft. A large amount of data on structure, soil composition, atmosphere, cloud layers, wind speed on the surface were accumulated. Soviet Venus research program was completed in 1986 by landing of \VEGA" (Venus-Halley's comet), one of the most successful projects in Lavochkin history. Since 1994 (mapping with the NASA Magellan mission) Venus was studied by two spacecraft: \Venus Express" (ESA, 2005-2014) and \Akatsuki" (JAXA, launch - 2010, start of operation - 2015). The first steps of \Venera-D" appeared in the early 2000s with the idea to provide operations on the planet's surface for several hours and possibly days. With the latest developments, unification of design solutions and new technical tools used in-house Lavochkin experts consider the mission \VEGA" as a prototype for the next automatic interplanetary station destined to Venus. -
Icebreaker: a Lunar South Pole Exploring Robot Cmu-Ri-Tr-97-22
ICEBREAKER: A LUNAR SOUTH POLE EXPLORING ROBOT CMU-RI-TR-97-22 Matthew C. Deans Alex D. Foessel Gregory A. Fries Diana LaBelle N. Keith Lay Stewart Moorehead Ben Shamah Kimberly J. Shillcutt Professor: Dr. William Whittaker The Robotics Institute Carnegie Mellon University Pittsburgh PA 15213 Spring 1996-97 Executive Summary Icebreaker: A Lunar South Pole Exploring Robot Due to the low angles of sunlight at the lunar poles, craters and other depressions in the polar regions can contain areas which are in permanent darkness and are at cryogenic temperatures. Many scientists have theorized that these cold traps could contain large quantities of frozen volatiles such as water and carbon dioxide which have been deposited over billions of years by comets, meteors and solar wind. Recent bistatic radar data from the Clementine mission has yielded results consistent with water ice at the South Pole of the Moon however Earth based observations from the Arecibo Radar Observatory indicate that ice may not exist. Due to the controversy surrounding orbital and Earth based observations, the only way to definitively answer the question of whether ice exists on the Lunar South Pole is in situ analysis. The discovery of water ice and other volatiles on the Moon has many important benefits. First, this would provide a source of rocket fuel which could be used to power rockets to Earth, Mars or beyond, avoiding the high cost of Earth based launches. Secondly, water and carbon dioxide along with nitrogen from ammonia form the essential elements for life and could be used to help support human colonies on the Moon.