Astronomy in the Space Age - Erik Tandberg
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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 Space Race
The Space Race Aims: To arrange the key events of the “Space Race” in chronological order. To decide which country won the Space Race. Space – the Final Frontier “Space” is everything Atmosphere that exists outside of our planet’s atmosphere. The atmosphere is the layer of Earth gas which surrounds our planet. Without it, none of us would be able to breathe! Space The sun is a star which is orbited (circled) by a system of planets. Earth is the third planet from the sun. There are nine planets in our solar system. How many of the other eight can you name? Neptune Saturn Mars Venus SUN Pluto Uranus Jupiter EARTH Mercury What has this got to do with the COLD WAR? Another element of the Cold War was the race to control the final frontier – outer space! Why do you think this would be so important? The Space Race was considered important because it showed the world which country had the best science, technology, and economic system. It would prove which country was the greatest of the superpowers, the USSR or the USA, and which political system was the best – communism or capitalism. https://www.youtube.com/watch?v=xvaEvCNZymo The Space Race – key events Discuss the following slides in your groups. For each slide, try to agree on: • which of the three options is correct • whether this was an achievement of the Soviet Union (USSR) or the Americans (USA). When did humans first send a satellite into orbit around the Earth? 1940s, 1950s or 1960s? Sputnik 1 was launched in October 1957. -
Assessment of Spectral Properties of Apollo 12 Landing Site Yann Chemin1, Ian Crawford2, Peter Grindrod2, and Louise Alexander2
Assessment of spectral properties of Apollo 12 landing site Yann Chemin1, Ian Crawford2, Peter Grindrod2, and Louise Alexander2 1Student, Birkbeck Colllege, University of London 2Birkbeck Colllege, University of London Corresponding author: Yann Chemin1 Email address: [email protected] ABSTRACT The geology and mineralogy of the Apollo 12 landing site has been the subject of recent studies that this research attempts to complement from a remote sensing point of view using the Moon Mineralogy Mapper (M3) sensor data, onboard the Chandrayaan-1 lunar orbiter. It is a higher spatial-spectral resolution sensor than the Clementine UVVis sensor and gives the opportunity to study the lunar surface with a comparatively more detailed spectral resolution. We used ISIS and GRASS GIS to study the M3 data. The M3 signatures are showing a monotonic featureless increment, with very low reflectance, suggesting a mature regolith. The regolith maturity is splitting the landing site in a younger Northwest and older Southeast. The mineral identification using the lunar sample spectra from within the Relab database found some similarity to a basaltic rock/glass mix. The spectrum features of clinopyroxene have been found in the Copernican rays and at the landing site. Lateral mixing increases FeO content away from the central part of the ray. The presence of clinopyroxene in the pigeonite basalt in the stratigraphy of the landing site brings forth some complexity in differentiating the Copernican ray’s clinopyroxene from the local source, as the spectra are twins but for their vertical shift in reflectance, reducing away from the central part of the ray. Spatial variations in mineralogy were not found mostly because of the pixel size compared to the landing site area. -
Workshop on Moon in Transition: Apollo 14, Kreep, and Evolved Lunar Rocks
WORKSHOP ON MOON IN TRANSITION: APOLLO 14, KREEP, AND EVOLVED LUNAR ROCKS (NASA-CR-I"'-- N90-I_02o rRAN31TION: APJLLN l_p KRFEP, ANu _VOLVFD LUNAR ROCKS (Lunar and Pl_net3ry !nst.) I_7 p C_CL O3B Unclas G3/91 0253133 LPI Technical Report Number 89-03 UNAR AND PLANETARY INSTITUTE 3303 NASA ROAD 1 HOUSTON, TEXAS 77058-4399 7 WORKSHOP ON MOON IN TRANSITION: APOLLO 14, KREEP, AND EVOLVED LUNAR ROCKS Edited by G. J. Taylor and P. H. Warren Sponsored by Lunar and Planetary Institute NASA Johnson Space Center November 14-16, 1988 Houston, Texas Lunar and Planetary Institute 330 ?_NASA Road 1 Houston, Texas 77058-4399 LPI Technical Report Number 89-03 Compiled in 1989 by the LUNAR AND PLANETARY INSTITUTE The Institute is operated by Universities Space Research Association under Contract NASW-4066 with the National Aeronautics and Space Administration. Material in this document may be copied without restraint for Library, abstract service, educational, or personal research purposes; however, republication of any portion requires the written permission of the authors as well as appropriate acknowledgment of this publication. This report may be cited as: Taylor G. J. and Warren PI H., eds. (1989) Workshop on Moon in Transition: Apo{l_ 14 KREEP, and Evolved Lunar Rocks. [PI Tech. Rpt. 89-03. Lunar and Planetary Institute, Houston. 156 pp. Papers in this report may be cited as: Author A. A. (1989) Title of paper. In W_nkshop on Moon in Transition: Ap_llo 14, KREEP, and Evolved Lunar Rocks (G. J. Taylor and P. H. Warren, eds.), pp. xx-yy. LPI Tech. Rpt. -
The New American Space Age: a Progress Report on Human Spaceflight the New American Space Age: a Progress Report on Human Spaceflight the International Space
The New American Space Age: A PROGRESS REPORT ON HUMAN SpaCEFLIGHT The New American Space Age: A Progress Report on Human Spaceflight The International Space Station: the largest international scientific and engineering achievement in human history. The New American Space Age: A Progress Report on Human Spaceflight Lately, it seems the public cannot get enough of space! The recent hit movie “Gravity” not only won 7 Academy Awards – it was a runaway box office success, no doubt inspiring young future scientists, engineers and mathematicians just as “2001: A Space Odyssey” did more than 40 years ago. “Cosmos,” a PBS series on the origins of the universe from the 1980s, has been updated to include the latest discoveries – and funded by a major television network in primetime. And let’s not forget the terrific online videos of science experiments from former International Space Station Commander Chris Hadfield that were viewed by millions of people online. Clearly, the American public is eager to carry the torch of space exploration again. Thankfully, NASA and the space industry are building a host of new vehicles that will do just that. American industry is hard at work developing new commercial transportation services to suborbital altitudes and even low Earth orbit. NASA and the space industry are also building vehicles to take astronauts beyond low Earth orbit for the first time since the Apollo program. Meanwhile, in the U.S. National Lab on the space station, unprecedented research in zero-g is paving the way for Earth breakthroughs in genetics, gerontology, new vaccines and much more. -
Lunar and Planetary Science XXXII (2001) 1815.Pdf
Lunar and Planetary Science XXXII (2001) 1815.pdf NEW AGE DETERMINATIONS OF LUNAR MARE BASALTS IN MARE COGNITUM, MARE NUBIUM, OCEANUS PROCELLARUM, AND OTHER NEARSIDE MARE H. Hiesinger1, J. W. Head III1, U. Wolf2, G. Neukum2 1 Department of Geological Sciences, Brown University, Providence, RI 02912, [email protected] 2 DLR-Inst. of Planetary Exploration, Rutherfordstr. 2, 12489 Berlin/Germany Introduction see a second small peak in volcanic activity at ~2-2.2 Lunar mare basalts cover about 17% of the lunar b.y. surface [1]. A significant portion of lunar mare basalts are exposed within Oceanus Procellarum for which Oceanus Procellarum, Mare Cognitum, Mare Nubium absolute radiometric age data are still lacking. Here we (Binned Ages of Mare Basalts) present age data that are based on remote sensing 20 techniques, that is, crater counts. We performed new crater size-frequency distribution measurements for spectrally homogeneous basalt units in Mare Cogni- 15 tum, Mare Nubium, and Oceanus Procellarum. The investigated area was previously mapped by Whitford- Stark and Head [2] who, based on morphology and 10 spectral characteristics, defined 21 distinctive basalt Frequency types in this part of the lunar nearside. Based on a high-resolution Clementine color ratio composite (e.g., 5 750-400/750+400 ratio as red, 750/990 ratio as green, and 400/750 ratio as blue), we remapped the distribu- 0 tion of distinctive basalts and found that their map well 1.1 1.5 2 2.5 3 3.5 4 discriminates the major basalt types. However, based Age [b.y.; bins of 100 m.y.] on the new high-resolution color data several of their units can be further subdivided into spectrally different Fig. -
Apollo Over the Moon: a View from Orbit (Nasa Sp-362)
chl APOLLO OVER THE MOON: A VIEW FROM ORBIT (NASA SP-362) Chapter 1 - Introduction Harold Masursky, Farouk El-Baz, Frederick J. Doyle, and Leon J. Kosofsky [For a high resolution picture- click here] Objectives [1] Photography of the lunar surface was considered an important goal of the Apollo program by the National Aeronautics and Space Administration. The important objectives of Apollo photography were (1) to gather data pertaining to the topography and specific landmarks along the approach paths to the early Apollo landing sites; (2) to obtain high-resolution photographs of the landing sites and surrounding areas to plan lunar surface exploration, and to provide a basis for extrapolating the concentrated observations at the landing sites to nearby areas; and (3) to obtain photographs suitable for regional studies of the lunar geologic environment and the processes that act upon it. Through study of the photographs and all other arrays of information gathered by the Apollo and earlier lunar programs, we may develop an understanding of the evolution of the lunar crust. In this introductory chapter we describe how the Apollo photographic systems were selected and used; how the photographic mission plans were formulated and conducted; how part of the great mass of data is being analyzed and published; and, finally, we describe some of the scientific results. Historically most lunar atlases have used photointerpretive techniques to discuss the possible origins of the Moon's crust and its surface features. The ideas presented in this volume also rely on photointerpretation. However, many ideas are substantiated or expanded by information obtained from the huge arrays of supporting data gathered by Earth-based and orbital sensors, from experiments deployed on the lunar surface, and from studies made of the returned samples. -
Project Xpedition Is the Product of Purdue University‟S Aeronautical and Astronautical Engineering Department Senior Spacecraft Design Class in the Spring of 2009
92 Project Xpedition Purdue University AAE 450 Spacecraft Design Spring 2009 Contents 1 – FOREWORD ........................................................................................................................................... 5 2 – INTRODUCTION ................................................................................................................................... 7 2.1 – BACKGROUND .................................................................................................................................... 7 2.2 – WHAT‟S IN THIS REPORT? .................................................................................................................. 9 2.3 – ACKNOWLEDGEMENTS .....................................................................................................................10 2.4 – ACRONYM LIST .................................................................................................................................12 3 – PROJECT OVERVIEW ....................................................................................................................... 14 3.1 – DESIGN REQUIREMENTS ...................................................................................................................14 3.2 – INTERPRETATION OF DESIGN REQUIREMENTS ...................................................................................18 3.3 – DESIGN PROCESS ..............................................................................................................................19 3.4 – RISK -
STATEMENT of CHAIRMAN AJIT PAI Re: Mitigation of Orbital Debris in the New Space Age, IB Docket No
STATEMENT OF CHAIRMAN AJIT PAI Re: Mitigation of Orbital Debris in the New Space Age, IB Docket No. 18-313. Shortly after becoming FCC Chairman, I had the opportunity to meet Newton Minow, who was Chairman of the FCC during the Kennedy Administration. To me, the most interesting part of our conversation was his description of how the FCC helped spur the beginning of the U.S. commercial space industry. Chairman Minow famously believed that putting satellites into space was more important than putting a human being there. As he put it, “Communications satellites are more important than sending a man into space because they will launch ideas, and ideas will last longer than men and women.” Today, our nation’s commercial space sector is growing rapidly. And at the FCC, we have been working hard to help our industry seize the opportunities of the new space age. Because satellites have become smaller and we now have more agile, reusable launch vehicles, we can send large numbers of satellites into low- or mid-Earth orbit. These non-geostationary satellite orbit, or NGSO, constellations could be a game changer, benefiting Americans across the country and making high-speed Internet access a reality for more consumers—particularly those in remote and hard-to-serve areas. That’s why, under my leadership, the Commission has approved 14 applications and market access requests by 11 companies for NGSO systems. Our action in this area fits well with the FCC’s twin goals of closing the digital divide and promoting innovation. However, more satellites in space means a lot more traffic, especially in low-earth orbit. -
Shoot the Moon – 1967
Video Transcript for Archival Research Catalog (ARC) Identifier 45011 Assignment: Shoot the Moon – 1967 Narrator: The assignment was specific: get photographs of the surface of the Moon that are good enough to determine whether or not it’s safe for a man to land there. But appearances can be deceiving, just as deceiving as trying to get a good picture of, well, a candy apple. Doesn’t seem to be too much of a problem, just set it up, light it, and snap the picture. Easy, quick, simple. But it can be tough. To begin with, the apple is some distance away, so you can’t get to it to just set it up, light it, and so on. To make things even more difficult, it isn’t even holding still; it’s moving around in circles. Now timing is important. You have to take your picture when the apple is nearest to you so you get the most detail and when the light that’s available is at the best angle for the photo. And even that’s not all. You are moving too, in circles. You’re both turning and circling about the apple. Now, about that assignment. As the technology of man in space was developing, it became more and more apparent that our knowledge of the Moon’s surface as a possible landing site was not sufficient. To land man safely on the Moon and get him safely off again, we had to know whether we could set up a precise enough trajectory to reach the Moon. -
Evolution of the Moon: the 1974 Model
Evolution of the Moon: The 1974 Model Harrison H. Schmitt Astronaut, Apollo 17* The geology of the decade of Apollo and Luna probably will become one of the fundamental turning points in the history of all science. For the first time, the scientists of the Earth have been presented with the opportunity to interpret their home planet through the direct investigations of another. Mankind can be proud and take heart in this fact. The interpretive evolution of the Moon can be divided now into seven major stages be- ginning sometime near the end of the formation of the solar system. These stages and their approximate durations in time are as follows: 1. The Beginning: 4.6 billion years ago 2. The Melted Shell: 4.6 to 4.4 billion years ago 3. The Cratered Highlands: 4.4 to 4.1 billion years ago 4. The Large Basins: 4.1 to 3.9 billion years ago 5. The Light-colored Plains: 3.9 to 3.8 billion years ago 6. The Basaltic Maria: 3.8 to 3.0 (?) billion years ago 7. The Quiet Crust: 3.0 (?) billion years ago to the present The Apollo and Luna explorations that permit us to study these stages of evolution each have contributed in progressive and significant ways. Through them we now can look with new insight-into the early differentiation of the Earth, the nature of the Earth's protocrust, the influence of the formation of large impact basins in that crust, the effects of early partial melting of the protomantle, and possibly the earliest stages of the breakup of the protocrust into continents and ocean basins. -
NASA in the Second Space
NASA in the Second Space Age: Exploration, Partnering, and Security The launch of Sputnik in 1957 and the dawn of the space age set off a frenetic competition between the Soviet Union and the United States. In the years that followed, both nations developed and orbited military satellites with increasingly sophisticated capabilities for intelligence col- lection, communications, and missile warning—capabilities largely in- tended to support strategic nuclear forces.1 For more than three decades the competition between these two superpowers was relatively stable, marked by notable periods of cooperation and engagement. Since the end of the Cold War, however, a gradual change has been under way, driven in part by advances in technology and the proliferation of space capabilities. This transformation has ushered in what the National Aero- nautics and Space Administration’s (NASA) Tom Cremins has termed the “second space age.”2 The second space age arguably began with the 1991 Gulf War. This conflict demonstrated, for the first time, the distinct advantages space- based capabilities can provide in conventional war fighting. The col- lapse of the Soviet Union also changed the geopolitical landscape and weakened the superpower duopoly in space. The 2011 National Security Space Strategy (NSSS) defines this new era by what has become known as the three Cs: congested, competitive, and contested.3 Space has be- come congested as more nations and private companies are launching and operating satellites for a variety of missions and increasingly com- petitive as they vie for economic and strategic advantage. According to the Space Foundation, global space activities generated some $330 bil- lion in economic activity in 2014, more than three-quarters of which came from commercial space products, services, infrastructure, and sup- port.4 A robust group of space startup companies has also emerged in recent years, injecting a fresh wave of innovation and competition in the space industry.