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STI Program Bibliography
Scientific and Technical Information Program Affordable Heavy Lift Capability: 2000-2004 This custom bibliography from the NASA Scientific and Technical Information Program lists a sampling of records found in the NASA Aeronautics and Space Database. The scope of this topic includes technologies to allow robust, affordable access of cargo, particularly to low-Earth orbit. This area of focus is one of the enabling technologies as defined by NASA’s Report of the President’s Commission on Implementation of United States Space Exploration Policy, published in June 2004. Best if viewed with the latest version of Adobe Acrobat Reader Affordable Heavy Lift Capability: 2000-2004 A Custom Bibliography From the NASA Scientific and Technical Information Program October 2004 Affordable Heavy Lift Capability: 2000-2004 This custom bibliography from the NASA Scientific and Technical Information Program lists a sampling of records found in the NASA Aeronautics and Space Database. The scope of this topic includes technologies to allow robust, affordable access of cargo, particularly to low-Earth orbit. This area of focus is one of the enabling technologies as defined by NASA’s Report of the President’s Commission on Implementation of United States Space Exploration Policy, published in June 2004. OCTOBER 2004 20040095274 EAC trains its first international astronaut class Bolender, Hans, Author; Bessone, Loredana, Author; Schoen, Andreas, Author; Stevenin, Herve, Author; ESA bulletin. Bulletin ASE. European Space Agency; Nov 2002; ISSN 0376-4265; Volume 112, 50-5; In English; Copyright; Avail: Other Sources After several years of planning and preparation, ESA’s ISS training programme has become operational. Between 26 August and 6 September, the European Astronaut Centre (EAC) near Cologne gave the first ESA advanced training course for an international ISS astronaut class. -
Appendix I Lunar and Martian Nomenclature
APPENDIX I LUNAR AND MARTIAN NOMENCLATURE LUNAR AND MARTIAN NOMENCLATURE A large number of names of craters and other features on the Moon and Mars, were accepted by the IAU General Assemblies X (Moscow, 1958), XI (Berkeley, 1961), XII (Hamburg, 1964), XIV (Brighton, 1970), and XV (Sydney, 1973). The names were suggested by the appropriate IAU Commissions (16 and 17). In particular the Lunar names accepted at the XIVth and XVth General Assemblies were recommended by the 'Working Group on Lunar Nomenclature' under the Chairmanship of Dr D. H. Menzel. The Martian names were suggested by the 'Working Group on Martian Nomenclature' under the Chairmanship of Dr G. de Vaucouleurs. At the XVth General Assembly a new 'Working Group on Planetary System Nomenclature' was formed (Chairman: Dr P. M. Millman) comprising various Task Groups, one for each particular subject. For further references see: [AU Trans. X, 259-263, 1960; XIB, 236-238, 1962; Xlffi, 203-204, 1966; xnffi, 99-105, 1968; XIVB, 63, 129, 139, 1971; Space Sci. Rev. 12, 136-186, 1971. Because at the recent General Assemblies some small changes, or corrections, were made, the complete list of Lunar and Martian Topographic Features is published here. Table 1 Lunar Craters Abbe 58S,174E Balboa 19N,83W Abbot 6N,55E Baldet 54S, 151W Abel 34S,85E Balmer 20S,70E Abul Wafa 2N,ll7E Banachiewicz 5N,80E Adams 32S,69E Banting 26N,16E Aitken 17S,173E Barbier 248, 158E AI-Biruni 18N,93E Barnard 30S,86E Alden 24S, lllE Barringer 29S,151W Aldrin I.4N,22.1E Bartels 24N,90W Alekhin 68S,131W Becquerei -
Crustal and Time-Varying Magnetic Fields at the Insight Landing Site on Mars
ARTICLES https://doi.org/10.1038/s41561-020-0537-x Crustal and time-varying magnetic fields at the InSight landing site on Mars Catherine L. Johnson 1,2 ✉ , Anna Mittelholz1, Benoit Langlais3, Christopher T. Russell4, Véronique Ansan 3, Don Banfield 5, Peter J. Chi 4, Matthew O. Fillingim 6, Francois Forget 7, Heidi Fuqua Haviland 8, Matthew Golombek9, Steve Joy 4, Philippe Lognonné 10, Xinping Liu4, Chloé Michaut 11, Lu Pan 12, Cathy Quantin-Nataf12, Aymeric Spiga 7,13, Sabine Stanley14,15, Shea N. Thorne 1, Mark A. Wieczorek 16, Yanan Yu4, Suzanne E. Smrekar9 and William B. Banerdt 9 Magnetic fields provide a window into a planet’s interior structure and evolution, including its atmospheric and space environ- ments. Satellites at Mars have measured crustal magnetic fields indicating an ancient dynamo. These crustal fields interact with the solar wind to generate transient fields and electric currents in Mars’s upper atmosphere. Surface magnetic field data play a key role in understanding these effects and the dynamo. Here we report measurements of magnetic field strength and direction at the InSight (Interior Exploration using Seismic Investigations, Geodesy and Heat Transport) landing site on Mars. We find that the field is ten times stronger than predicted by satellite-based models. We infer magnetized rocks beneath the surface, within ~150 km of the landing site, consistent with a past dynamo with Earth-like strength. Geological mapping and InSight seismic data suggest that much or all of the magnetization sources are carried in basement rocks, which are at least 3.9 billion years old and are overlain by between 200 m and ~10 km of lava flows and modified ancient terrain. -
Aerobraking to Lower Apogee in Earth Orbit with the Small Payload Orbit Transfer (SPORT™) Microsatellite Vehicle
View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by DigitalCommons@USU SSC01-XI-8 Aerobraking to Lower Apogee in Earth Orbit with the Small Payload ORbit Transfer (SPORT™) Microsatellite Vehicle Paul Gloyer AeroAstro, Inc. 160 Adams Lane, Waveland, MS 39576 228-466-9863, [email protected] Tony Robinson AeroAstro, Inc. 520 Huntmar Park Drive, Herndon, VA 20170 703-709-2240 x133, [email protected] Adeena Mignogna AeroAstro, Inc. 520 Huntmar Park Drive, Herndon, VA 20170 703-709-2240 x126, [email protected] Yasser Ahmad Astronautic Technology Sdn. Bhd. 520 Huntmar Park Drive, Herndon, VA 20170 703-709-2240 x138, [email protected] Abstract. AeroAstro, Inc. and Astronautic Technology Sdn. Bhd. (a Malaysian space company) are commercially developing the Small Payload ORbit Transfer (SPORT) vehicle, which uses advanced earth aerobraking technology to achieve efficient orbit transfer from Geosynchronous-Transfer Orbit (GTO) to Low Earth Orbit (LEO). After being delivered to GTO by a large launch vehicle, such as Ariane, SPORT uses its onboard propulsion system to adjust its perigee altitude to about 150 km. At this altitude, the large deployable aerobrake produces enough drag to reduce the apogee altitude from 36,000+ km to about 1,000 km in approximately 300 orbits. Upon reaching the target apogee altitude, the propulsion system is used to raise the perigee to the desired altitude, thereby allowing SPORT to release its payload. Aerobraking technology enables orbit transfer in a cost-effective manner, reducing the overall mass of the spacecraft by drastically reducing the amount of propellant required to achieve the maneuver. -
Re-Usable Launch and Payload Delivery System MDDP 2012/3
Group 2 Re-usable Launch and Payload Delivery System MDDP 2012/3 Re-usable Launch and Payload Delivery System MDDP Group 2 James Dobberson Robert Taylor Matthew Chapman Timothy West Mukudzei Muchengeti William Wou Group 2 Re-usable Launch and Payload Delivery System MDDP 2012/3 1. Contents 1. Contents ..................................................................................................................................... i 2. Executive Summary .................................................................................................................. ii 3. Introduction .............................................................................................................................. 1 4. Down Selection and Integration Methodology ......................................................................... 2 5. Presentation of System Concept and Operations ...................................................................... 5 6. System Investment Plan ......................................................................................................... 20 7. Numerical Analysis and Statement of Feasibility .................................................................. 23 8. Conclusions and Future Work ................................................................................................ 29 9. Launch Philosophy ................................................................................................................. 31 10. Propulsion .............................................................................................................................. -
Earth and Space Science. a Guide for Secondary Teachers. INSTITUTION Pennsylvania State Dept
DOCUMENT RESUME ED 094 956 SE 016 611 AUTHOR Bolles, William H.; And Others TITLE Earth and Space Science. A Guide for Secondary Teachers. INSTITUTION Pennsylvania State Dept. of Education, Harrisburg. Bureau of Curriculum Services. PUB DATE 73 NOTE 200p. EDRS PRICE MF-$O.75 HC-$9.00 PLUS POSTAGE DESCRIPTORS Aerospace Education; *Astronomy; *Curriculum Guides; *Earth Science; Geology; Laboratory Experiments; Oceanology; Science Activities; Science Education; *Secondary School Science IDENTIFIERS Pennsylvania ABSTRACT Designed for use in Pennsylvania secondary school science classes, this guide is intended to provide fundamental information in each of the various disciplines of the earth sciences. Some of the material contained in the guide is intended as background material for teachers. Five units are presented: The Earth, The Oceans, The Space Environment, The Atmosphere, and The Exploration of Space. The course is organized so that students proceed from the familiar, everyday world to the atmosphere and the space environment. Teaching geology in the fall takes advantage of weather conditions which permit field study. The purpose of the Earth and Space Science course is to encourage student behaviors which will be indicative of a broad understanding of man1s physical environment of earth and space as well as an awareness of the consequences which could result from changes which man may effect.(PEB) BEST COPY AVAILABLE U S DEPARTMENT OF HEALTH. EDUCATION & WELFARE NATIONAL INSTITUTE OF 6 Fe elz+C EDUCATION Try,' DOCUMENT FIRSBEEN REPRO -
Sessions Calendar
Associated Societies GSA has a long tradition of collaborating with a wide range of partners in pursuit of our mutual goals to advance the geosciences, enhance the professional growth of society members, and promote the geosciences in the service of humanity. GSA works with other organizations on many programs and services. AASP - The American Association American Geophysical American Institute American Quaternary American Rock Association for the Palynological Society of Petroleum Union (AGU) of Professional Association Mechanics Association Sciences of Limnology and Geologists (AAPG) Geologists (AIPG) (AMQUA) (ARMA) Oceanography (ASLO) American Water Asociación Geológica Association for Association of Association of Earth Association of Association of Geoscientists Resources Association Argentina (AGA) Women Geoscientists American State Science Editors Environmental & Engineering for International (AWRA) (AWG) Geologists (AASG) (AESE) Geologists (AEG) Development (AGID) Blueprint Earth (BE) The Clay Minerals Colorado Scientifi c Council on Undergraduate Cushman Foundation Environmental & European Association Society (CMS) Society (CSS) Research Geosciences (CF) Engineering Geophysical of Geoscientists & Division (CUR) Society (EEGS) Engineers (EAGE) European Geosciences Geochemical Society Geologica Belgica Geological Association Geological Society of Geological Society of Geological Society of Union (EGU) (GS) (GB) of Canada (GAC) Africa (GSAF) Australia (GSAus) China (GSC) Geological Society of Geological Society of Geologische Geoscience -
Introduction to Astronomy from Darkness to Blazing Glory
Introduction to Astronomy From Darkness to Blazing Glory Homework DVD This is a spiral galaxy. There are billions of this type in the Universe. The cloudy areas are a mix of gas, dust and stars. The center has a black hole as well as millions upon millions of closely packed stars systems. Jeff Scott JAS EP SpiralGalaxy M81 1 This DVD contains : •Your semester’s homework assignments. •Your generic homework sheet. •The textbook glossary. •Website suggestions. Comet Tempel 1 A special thank you to NASA, NOAA and USGS for the images, photographs and diagrams. Earthrise photo taken by an Apollo Astronaut. On the Moon. JAS EP 2 This DVD provides instruction for student homework assignments. Each chapter has its own assignments. The teacher will assign due dates. You may use the generic homework page at the end of the DVD by printing out a copy. The picture on the right is of a nebula. It is a cloud in space made of dust and gas. These clouds can be enormous. Credit: NASA, H.Ford (JHU), G. Cone Nebula (NG2264) Illingsworth (USCC?LO), Mclampin (STScl), G.HARtwig (STScl), the ACS 3 Science Team and ESA Table Of Contents Reports Pg. 7 Chapter 1 Astronomy Basics Pg. 8 Chapter 2 Time Pg. 10 Chapter 3 Solar System Overview Pg. 13 Chapter 4 Our Sun Pg. 15 Chapter 5 Terrestrial Planets Pg. 17 Chapter 6 Outer and Exoplanets Pg. 29 Chapter 7 The Moons Pg. 37 Chapter 8 Rocks N’ Ice Pg. 43 Chapter 9 The Stars Pg. 49 Stephan’s Quintet Galaxy Grouping Chapter 10 Galaxies Pg. -
Mars Aerocapture/Aerobraking Aeroshell Configurations by Abraham Chavez
Mars Aerocapture/Aerobraking Aeroshell Configurations by Abraham Chavez This presentation provides a review of those studies and a starting point for considering Aerocapture/Aerobraking technology as a way to reduce mass and cost, to achieve the ambitious science returns currently desired What is Aerocapture: is first of all a very rapid process, requiring a heavy heat shield resulting in high g-forces, Descent into a relatively dense atmosphere is suffciently rapid that the deceleration causes severe heating requiring What is Aerobraking: is a very gradual process that has the advantage that small reductions in spacecraft velocity are achieved by drag of the solar arrays in the outer atmosphere, thus no additional mass for a heat shield is necessary. an aeroshell. Sasakawa International Center for Space Architecture, University of Houston College of Architecture Aerocapture vs Aerobraking Entry targeting burn Atmospheric entry Atmospheric Drag Aerocapture Reduces Orbit Period Periapsis Energy raise dissipation/ maneuver Autonomous Aerobraking (propulsive) guidance Target ~300 Passes Jettison Aeroshell Hyperbolic Through Upper orbit Approach Atmosphere Controlled exit Orbit Insertion Pros Cons Burn Uses very little fuel--significant mass Needs protective aeroshell savings for larger vehicles Pros Cons Establishes orbit quickly (single pass) One-shot maneuver; no turning back, Little spacecraft design impact Still need ~1/2 propulsive fuel load much like a lander Gradual adjustments; can pause Hundreds of passes = more chance of Has -
Digital Darwin: Editing the Loves of the Plants As a Case Study of the Theory and Practice of Digital Editions
Digital Darwin: Editing The Loves of the Plants as a Case Study of the Theory and Practice of Digital Editions by Alana Helen Rigby A thesis presented to the University of Waterloo in fulfillment of the thesis requirement for the degree of Master of Arts in English Waterloo, Ontario, Canada, 2016 © Alana Rigby 2016 Author’s Declaration I hereby declare that I am the sole author of this thesis. This is a true copy of the thesis, including any required final revisions, as accepted by my examiners. I understand that my thesis may be made electronically available to the public. ii Abstract Digital scholarly editing is an evolving field that allows for the rendering of complex print works that are rife with paratextual material. Erasmus Darwin’s The Loves of the Plants represents this kind of paratextually complex work: it is an eighteenth-century scientific poem of approximately 2000 lines, added to which are illustrations and extensive footnotes. Existing editions of the poem are 1) incomplete, presenting only a portion of the text, 2) lacking annotations, or 3) strip it of some of its paratextual elements, such as the footnotes or illustrations. This paper explores the use of digital editing methods to render Darwin’s most popular poem into the first-ever complete critical edition of part of Loves; using copy-text editing theory in the tradition of Greg and Bowers, an eclectic edition was created. A full transcription and annotations are included. Using the Text Encoding Initiative P5 Guidelines, a digital edition of the Front Materials, Canto I, and Interlude I was also created. -
Envision – Front Cover
EnVision – Front Cover ESA M5 proposal - downloaded from ArXiV.org Proposal Name: EnVision Lead Proposer: Richard Ghail Core Team members Richard Ghail Jörn Helbert Radar Systems Engineering Thermal Infrared Mapping Civil and Environmental Engineering, Institute for Planetary Research, Imperial College London, United Kingdom DLR, Germany Lorenzo Bruzzone Thomas Widemann Subsurface Sounding Ultraviolet, Visible and Infrared Spectroscopy Remote Sensing Laboratory, LESIA, Observatoire de Paris, University of Trento, Italy France Philippa Mason Colin Wilson Surface Processes Atmospheric Science Earth Science and Engineering, Atmospheric Physics, Imperial College London, United Kingdom University of Oxford, United Kingdom Caroline Dumoulin Ann Carine Vandaele Interior Dynamics Spectroscopy and Solar Occultation Laboratoire de Planétologie et Géodynamique Belgian Institute for Space Aeronomy, de Nantes, Belgium France Pascal Rosenblatt Emmanuel Marcq Spin Dynamics Volcanic Gas Retrievals Royal Observatory of Belgium LATMOS, Université de Versailles Saint- Brussels, Belgium Quentin, France Robbie Herrick Louis-Jerome Burtz StereoSAR Outreach and Systems Engineering Geophysical Institute, ISAE-Supaero University of Alaska, Fairbanks, United States Toulouse, France EnVision Page 1 of 43 ESA M5 proposal - downloaded from ArXiV.org Executive Summary Why are the terrestrial planets so different? Venus should be the most Earth-like of all our planetary neighbours: its size, bulk composition and distance from the Sun are very similar to those of Earth. -
Crustal Magnetism, Tectonic Inheritance, and Continental Rifting in the Southeastern United States
Come to GSA in Vancouver, BC. We’ll be watching for you! Photo Tourism Vancouver / Suzanne Rushton APRIL/MAY | VOL. 24, 2014 4/5 NO. A PUBLICATION OF THE GEOLOGICAL SOCIETY OF AMERICA® Crustal magnetism, tectonic inheritance, and continental rifting in the southeastern United States APRIL/MAY 2014 | VOLUME 24, NUMBER 4/5 Featured Article GSA TODAY (ISSN 1052-5173 USPS 0456-530) prints news and information for more than 26,000 GSA member readers and subscribing libraries, with 11 monthly issues (April/ May is a combined issue). GSA TODAY is published by The SCIENCE: Geological Society of America® Inc. (GSA) with offices at 3300 Penrose Place, Boulder, Colorado, USA, and a mail- 4 Crustal magnetism, tectonic inheritance, and ing address of P.O. Box 9140, Boulder, CO 80301-9140, USA. continental rifting in the southeastern United States GSA provides this and other forums for the presentation of diverse opinions and positions by scientists worldwide, E.H. Parker Jr. regardless of race, citizenship, gender, sexual orientation, Cover: Seismic station deployed in the Coastal Plain of southeastern religion, or political viewpoint. Opinions presented in this publication do not reflect official positions of the Society. Georgia for the EarthScope SESAME flexible-array experiment. The 85-station SESAME array is designed to study crustal and mantle © 2014 The Geological Society of America Inc. All rights reserved. Copyright not claimed on content prepared structure across the Suwannee-Wiggins suture zone. See related wholly by U.S. government employees within the scope of article, p. 4–9. their employment. Individual scientists are hereby granted permission, without fees or request to GSA, to use a single figure, table, and/or brief paragraph of text in subsequent work and to make/print unlimited copies of items in GSA GSA News TODAY for noncommercial use in classrooms to further education and science.