2013 October 2
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Asteroid Retrieval Mission
Where you can put your asteroid Nathan Strange, Damon Landau, and ARRM team NASA/JPL-CalTech © 2014 California Institute of Technology. Government sponsorship acknowledged. Distant Retrograde Orbits Works for Earth, Moon, Mars, Phobos, Deimos etc… very stable orbits Other Lunar Storage Orbit Options • Lagrange Points – Earth-Moon L1/L2 • Unstable; this instability enables many interesting low-energy transfers but vehicles require active station keeping to stay in vicinity of L1/L2 – Earth-Moon L4/L5 • Some orbits in this region is may be stable, but are difficult for MPCV to reach • Lunar Weakly Captured Orbits – These are the transition from high lunar orbits to Lagrange point orbits – They are a new and less well understood class of orbits that could be long term stable and could be easier for the MPCV to reach than DROs – More study is needed to determine if these are good options • Intermittent Capture – Weakly captured Earth orbit, escapes and is then recaptured a year later • Earth Orbit with Lunar Gravity Assists – Many options with Earth-Moon gravity assist tours Backflip Orbits • A backflip orbit is two flybys half a rev apart • Could be done with the Moon, Earth or Mars. Backflip orbit • Lunar backflips are nice plane because they could be used to “catch and release” asteroids • Earth backflips are nice orbits in which to construct things out of asteroids before sending them on to places like Earth- Earth or Moon orbit plane Mars cyclers 4 Example Mars Cyclers Two-Synodic-Period Cycler Three-Synodic-Period Cycler Possibly Ballistic Chen, et al., “Powered Earth-Mars Cycler with Three Synodic-Period Repeat Time,” Journal of Spacecraft and Rockets, Sept.-Oct. -
Lori Garver, NASA Deputy Administrator SOFIA Joining Forces Event Joint Base Andrews September 22, 2011
Lori Garver, NASA Deputy Administrator SOFIA Joining Forces Event Joint Base Andrews September 22, 2011 Good afternoon. My name is Lori Garver, Deputy Administrator at NASA. I want to thank our German Aerospace Center partners and Joint Base Andrews for organizing this event and especially for making it possible for students and the children of military families to see this unique flying observatory up close. And let me just take a moment to commend First Lady Michelle Obama and Jill Biden for devoting their time and energy in encouraging all Americans to do more in support of the wives, husbands, sons, daughters and other family members of our men and women in uniform who are defending our freedom around the world. 1 I want to also welcome any and all Members of Congress who are here today. And a special hello to Mary Blessing, an astronomy teacher at Herndon High School -- one of only six American teachers selected to work with scientists aboard SOFIA and to share that experience with their students. I know you are all eager to tour this magnificent aircraft, so I am only going to speak briefly then turn it over to my colleagues, Paul Hertz, NASA’s Chief Scientist in our Science Mission Directorate; and Leland Melvin, our Associate Administrator for Education and a former astronaut. Paul and Leland will speak more about the amazing scientific and educational value of SOFIA, but let me just tell you that this project is a key component of NASA’s science objectives. 2 It will help us zoom in close on some of the most fundamental questions of the universe: Where did we come from? How was our solar system formed? And what else is out there? It is fitting that SOFIA means “wisdom” in Greek. -
Asteroid Retrieval Feasibility Study
Asteroid Retrieval Feasibility Study 2 April 2012 Prepared for the: Keck Institute for Space Studies California Institute of Technology Jet Propulsion Laboratory Pasadena, California 1 2 Authors and Study Participants NAME Organization E-Mail Signature John Brophy Co-Leader / NASA JPL / Caltech [email protected] Fred Culick Co-Leader / Caltech [email protected] Co -Leader / The Planetary Louis Friedman [email protected] Society Carlton Allen NASA JSC [email protected] David Baughman Naval Postgraduate School [email protected] NASA ARC/Carnegie Mellon Julie Bellerose [email protected] University Bruce Betts The Planetary Society [email protected] Mike Brown Caltech [email protected] Michael Busch UCLA [email protected] John Casani NASA JPL [email protected] Marcello Coradini ESA [email protected] John Dankanich NASA GRC [email protected] Paul Dimotakis Caltech [email protected] Harvard -Smithsonian Center for Martin Elvis [email protected] Astrophysics Ian Garrick-Bethel UCSC [email protected] Bob Gershman NASA JPL [email protected] Florida Institute for Human and Tom Jones [email protected] Machine Cognition Damon Landau NASA JPL [email protected] Chris Lewicki Arkyd Astronautics [email protected] John Lewis University of Arizona [email protected] Pedro Llanos USC [email protected] Mark Lupisella NASA GSFC [email protected] Dan Mazanek NASA LaRC [email protected] Prakhar Mehrotra Caltech [email protected] -
Photo Release -- Commercial Space Industry Works with NASA and Creates Tech Jobs in Silicon Valley
Photo Release -- Commercial Space Industry Works With NASA and Creates Tech Jobs in Silicon Valley NASA Deputy Administrator Lori Garver Looks to Commercial Space Industry to Support Agency Objectives, Visits Space Systems/Loral in Palo Alto, Calif. PALO ALTO, Calif., Aug. 1, 2011 (GLOBE NEWSWIRE) -- Space Systems/Loral (SS/L) today announced that Lori Garver, Deputy Administrator of NASA, and John Celli, President of Space Systems/Loral, met on July 29 to discuss commercial space industry capabilities and continuing job creation. Ms. Garver toured SS/L's state-of-the-art manufacturing facility in Palo Alto, Calif., where satellites for direct-to-home television (DTH), consumer broadband, and satellite radio are regularly designed, built and launched into space in two to three years from start to finish. A photo accompanying this release is available at http://www.globenewswire.com/newsroom/prs/?pkgid=10073 NASA continues to partner with companies such as Space Systems/Loral to help strengthen U.S. leadership in space while at the same time stimulating job growth in careers related to science, technology, engineering and math (STEM). Space Systems/Loral, the world's leading provider of commercial satellites, is currently working with NASA Ames to provide the propulsion system for the Lunar Atmosphere Dust Environment Explorer (LADEE) spacecraft. The propulsion system is based on a space-proven SS/L design that has been reconfigured to take a small spacecraft to the moon. When launched, NASA's LADEE spacecraft will study the moon's thin atmosphere and dust above the lunar surface. The propulsion system and structure that is being built by SS/L is a variant of the mission critical system Pete Worden, NASA Ames Center Director; Lori used over many years on SS/L's geostationary satellites. -
Administration of Barack H. Obama, 2009 Remarks at a White House
Administration of Barack H. Obama, 2009 Remarks at a White House Event Celebrating Scientific Exploration October 7, 2009 The President. Hello, everybody. Hi, guys. Well, it is good to see you, all of you. Good evening. I want to welcome all the students and teachers and amateur astronomers to the White House tonight. I won't speak long, because we've got a bunch of telescopes and great exhibits to get our hands on. But before we begin, let me first acknowledge a few other stars who are out tonight. First of all, John Holdren, my science adviser, an actual physicist, is here and eager to look through one of these telescopes. Our NASA Administrator, Charles Bolden, who's spent some time orbiting the Earth himself, and his deputy, Lori Garver, are here. Where's Charles and Lori? There're in the back there. Give them a round of applause. We've got some specialists from NASA, the Smithsonian, and the American Museum of Natural History in New York here with us as well. And we've got some of the heroes who have flown closer to the stars than anybody else. Buzz Aldrin, a man who actually walked on the Moon; where's Buzz? Right there. Sally Ride, the first American woman in space, is here. Mae Jemison, the first African American woman in space, give her a big round of applause. And John Grunsfeld is here, the man they call the "Hubble Repairman," not to be mistaken with the Maytag repairman—[laughter]—for all the upgrades that he's made up there to the telescope that allows us to see farther than anyone ever imagined. -
Revamping Federal Climate Science Recommendations for the Next President of the United States
GETTY SHIPING IMAGES/LIU Revamping Federal Climate Science Recommendations for the Next President of the United States By John Podesta, Bidisha Bhattacharyya, and Bianca Majumder December 2020 WWW.AMERICANPROGRESS.ORG Contents 1 Introduction and Summary 4 Recommendations to restore scientific integrity across the government 9 Recommendations for rebuilding the federal climate science workforce 13 Recommendations to coordinate climate science in the White House and across the federal government 19 Recommendations to define interagency climate science research and data priorities 31 Recommendations for prioritizing adaptation and resilience 34 Recommendations to promote international coordination on climate science 40 Conclusion 41 About the authors 41 Acknowledgments 44 Appendix: References and further reading 46 Endnotes Introduction and summary The United States has been the global leader in climate science for decades. Unfortunately, progress has slowed—and in some cases, even moved backward— over the past four years, with the Trump administration dismantling core elements of the federal climate science apparatus. As the country and the planet head toward an increasingly unstable climate, the U.S. government needs to get back to the business of being the preeminent source of trusted applied science that supports climate change mitigation and adaptation decision-making of governments and civilian stakeholders. The science is clear: To avoid the worst impacts of climate change, the United States and the world must take aggressive action to decarbonize all sectors of the global economy, protect the Earth’s natural systems, and limit warming to 1.5 degrees Celsius above preindustrial levels. This means achieving net-zero greenhouse gas emissions globally by no later than 2050 and ensuring an equitable and just transition to a clean energy economy. -
GRAIL Reveals Secrets of the Lunar Interior
GRAIL Reveals Secrets of the Lunar Interior — Dr. Patrick J. McGovern, Lunar and Planetary Institute A mini-flotilla of spacecraft sent to the Moon in the past few years by several nations has revealed much about the characteristics of the lunar surface via techniques such as imaging, spectroscopy, and laser ranging. While the achievements of these missions have been impressive, only GRAIL has seen deeply enough to reveal inner secrets that the Moon holds. LRecent Lunar Missions Country Name Launch Date Status ESA Small Missions for Advanced September 27, 2003 Ended with lunar surface impact on Research in Technology-1 (SMART-1) September 3, 2006 USA Acceleration, Reconnection, February 27, 2007 Extension of the THEMIS mission; ended Turbulence and Electrodynamics of in 2012 the Moon’s Interaction with the Sun (ARTEMIS) Japan SELENE (Kaguya) September 14, 2007 Ended with lunar surface impact on June 10, 2009 PChina Chang’e-1 October 24, 2007 Taken out of orbit on March 1, 2009 India Chandrayaan-1 October 22, 2008 Two-year mission; ended after 315 days due to malfunction and loss of contact USA Lunar Reconnaissance Orbiter (LRO) June 18, 2009 Completed one-year primary mission; now in five-year extended mission USA Lunar Crater Observation and June 18, 2009 Ended with lunar surface impact on Sensing Satellite (LCROSS) October 9, 2009 China Chang’e-2 October 1, 2010 Primary mission lasted for six months; extended mission completed flyby of asteroid 4179 Toutatis in December 2012 USA Gravity Recovery and Interior September 10, 2011 Ended with lunar surface impact on I Laboratory (GRAIL) December 17, 2012 To probe deeper, NASA launched the Gravity Recovery and Interior Laboratory (GRAIL) mission: twin spacecraft (named “Ebb” and “Flow” by elementary school students from Montana) flying in formation over the lunar surface, tracking each other to within a sensitivity of 50 nanometers per second, or one- twenty-thousandth of the velocity that a snail moves [1], according to GRAIL Principal Investigator Maria Zuber of the Massachusetts Institute of Technology. -
John F. Kennedy and the Race to the Moon Palgrave Studies in the History of Science and Technology
JOHN F. KENNEDY AND THE RACE TO THE MOON PALGRAVE STUDIES IN THE HISTORY OF SCIENCE AND TECHNOLOGY James Rodger Fleming (Colby College) and Roger D. Launius (National Air and Space Museum), Series Editors This series presents original, high-quality, and accessible works at the cutting edge of scholarship within the history of science and technology. Books in the series aim to disseminate new knowledge and new perspectives about the history of science and technology, enhance and extend education, foster public understanding, and enrich cultural life. Collectively, these books will break down conventional lines of demarcation by incorporating historical perspectives into issues of current and ongoing concern, offering international and global perspectives on a variety of issues, and bridging the gap between historians and practicing scientists. In this way they advance scholarly conversation within and across traditional disciplines but also to help define new areas of intellectual endeavor. Published by Palgrave Macmillan: Continental Defense in the Eisenhower Era: Nuclear Antiaircraft Arms and the Cold War By Christopher J. Bright Confronting the Climate: British Airs and the Making of Environmental Medicine By Vladimir Jankovic´ Globalizing Polar Science: Reconsidering the International Polar and Geophysical Years Edited by Roger D. Launius, James Rodger Fleming, and David H. DeVorkin Eugenics and the Nature-Nurture Debate in the Twentieth Century By Aaron Gillette John F. Kennedy and the Race to the Moon By John M. Logsdon John F. Kennedy and the Race to the Moon John M. Logsdon JOHN F. KENNEDY AND THE RACE TO THE MOON Copyright © John M. Logsdon, 2010. Softcover reprint of the hardcover 1st edition 2010 978-0-230-11010-6 All rights reserved. -
ISSUE 134, AUGUST 2013 2 Imperative: Venus Continued
Imperative: Venus — Virgil L. Sharpton, Lunar and Planetary Institute Venus and Earth began as twins. Their sizes and densities are nearly identical and they stand out as being considerably more massive than other terrestrial planetary bodies. Formed so close to Earth in the solar nebula, Venus likely has Earth-like proportions of volatiles, refractory elements, and heat-generating radionuclides. Yet the Venus that has been revealed through exploration missions to date is hellishly hot, devoid of oceans, lacking plate tectonics, and bathed in a thick, reactive atmosphere. A less Earth-like environment is hard to imagine. Venus, Earth, and Mars to scale. Which L of our planetary neighbors is most similar to Earth? Hint: It isn’t Mars. PWhy and when did Earth’s and Venus’ evolutionary paths diverge? This fundamental and unresolved question drives the need for vigorous new exploration of Venus. The answer is central to understanding Venus in the context of terrestrial planets and their evolutionary processes. In addition, however, and unlike virtually any other planetary body, Venus could hold important clues to understanding our own planet — how it has maintained a habitable environment for so long and how long it can continue to do so. Precisely because it began so like Earth, yet evolved to be so different, Venus is the planet most likely to cast new light on the conditions that determine whether or not a planet evolves habitable environments. NASA’s Kepler mission and other concurrent efforts to explore beyond our star system are likely to find Earth-sized planets around Sun-sized stars within a few years. -
Satellite Capture Mechanism in a Sun-Planet-Binary Four-Body System
Satellite capture mechanism in a sun-planet-binary four-body system Shengping Gong*, Miao Li † School of Aerospace Engineering, Tsinghua University, Beijing China, 100084 Abstract This paper studies the binary disruption problem and asteroid capture mechanism in a sun-planet-binary four-body system. Firstly, the binary disruption condition is studied and the result shows that the binary is always disrupted at the perigee of their orbit instantaneously. Secondly, an analytic expression to describe the energy exchange between the binary is derived based on the ‘instantaneous disruption’ hypothesis. The analytic result is validated through numerical integration. We obtain the energy exchange in encounters simultaneously by the analytic expression and numerical integration. The maximum deviation of this two results is always less than 25% and the mean deviation is about 8.69%. The analytic expression can give us an intuitive description of the energy exchange between the binary. It indicates that the energy change depends on the hyperbolic shape of the binary orbit with respect to the planet, the masses of planet and the primary member of the binary, the binary phase at perigee. We can illustrate the capture/escape processes and give the capture/escape region of the binary clearly by numerical simulation. We analyse the influence of some critical *Associate professor, School of Aerospace Engineering; [email protected] † PhD candidate, School of Aerospace Engineering; [email protected] 1 factors to the capture region finally. Key words: binary; capture mechanism; disruption; analytic derivation; numerical results 1 Introduction In the last decade, hundreds of irregular satellites orbiting giant planets have been found in our solar system. -
Plenary Program
Pecora 21/ISRSE 38 Plenary Sessions Monday, October 7 08:30 am – 10:00 am Room – Harborside Ballroom Welcome/Opening Keynote Address and Pecora Awards Presentation Barbara Ryan, Pecora/ISRSE Conference Chair Dr. Gilberto Câmara, Secretariat Director, GEO - Group on Earth Observations Dr. Tim Petty, Assistant. Secretary for Water & Science at the Department of the Interior Dr. Sandra Cauffman, Acting Director, NASA Earth Science Division Welcome Barbara Ryan Barbara Ryan served as the Secretariat Director of the international Group on Earth Observations (GEO) until 2018 where she worked tirelessly to make Earth observation data more accessible and usable. GEO is an intergovernmental organization with over 100 member countries and over 100 participating partners working to integrate Earth observations comprehensively to understand how environmental factors impact human life and the environment. Under Ryan's leadership, millions of satellite images have been made available to the public at no charge allowing scientists, planners and policy makers to take a comprehensive approach to problems that transcend political boundaries including agriculture, biodiversity, climate change, disaster planning, energy and health. Ryan was previously the Director of the Space Program at the World Meteorological Organization (WMO) and Associate Director of Geography at the United States Geological Survey (USGS). She has also served as Chair of the Committee on Earth Observation Satellites (CEOS). 1 Opening Keynote Address A strategy for a results-oriented GEOSS Gilberto Câmara Dr. Gilberto Câmara is a Brazilian researcher in Geoinformatics, Spatial Analysis, Land Use Change, and Nature-Society Interactions, from Brazil's National Institute for Space Research (INPE). He is internationally recognized for promoting free access for geospatial data and for setting up an efficient satellite monitoring of the Brazilian Amazon rainforest. -
The Formation of the Martian Moons Rosenblatt P., Hyodo R
The Final Manuscript to Oxford Science Encyclopedia: The formation of the Martian moons Rosenblatt P., Hyodo R., Pignatale F., Trinh A., Charnoz S., Dunseath K.M., Dunseath-Terao M., & Genda H. Summary Almost all the planets of our solar system have moons. Each planetary system has however unique characteristics. The Martian system has not one single big moon like the Earth, not tens of moons of various sizes like for the giant planets, but two small moons: Phobos and Deimos. How did form such a system? This question is still being investigated on the basis of the Earth-based and space-borne observations of the Martian moons and of the more modern theories proposed to account for the formation of other moon systems. The most recent scenario of formation of the Martian moons relies on a giant impact occurring at early Mars history and having also formed the so-called hemispheric crustal dichotomy. This scenario accounts for the current orbits of both moons unlike the scenario of capture of small size asteroids. It also predicts a composition of disk material as a mixture of Mars and impactor materials that is in agreement with remote sensing observations of both moon surfaces, which suggests a composition different from Mars. The composition of the Martian moons is however unclear, given the ambiguity on the interpretation of the remote sensing observations. The study of the formation of the Martian moon system has improved our understanding of moon formation of terrestrial planets: The giant collision scenario can have various outcomes and not only a big moon as for the Earth.