November 2020 Nasa Presidential Transition Binder
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Hayabusa2 and the Formation of the Solar System PPS02-25
PPS02-25 JpGU-AGU Joint Meeting 2017 Hayabusa2 and the formation of the Solar System *Sei-ichiro WATANABE1,2, Hayabusa2 Science Team2 1. Division of Earth and Planetary Sciences, Graduate School of Science, Nagoya University, 2. JAXA/ISAS Explorations of small solar system bodies bring us direct and unique information about the formation and evolution of the Solar system. Asteroids may preserve accretion processes of planetesimals or pebbles, a sequence of destructive events induced by the gas-driven migration of giant planets, and hydrothermal processes on the parent bodies. After successful small-body missions like Rosetta to comet 67P/Churyumov-Gerasimenko, Dawn to Vesta and Ceres, and New Horizons to Pluto, two spacecraft Hayabusa2 and OSIRIS-REx are now traveling to dark primitive asteroids.The Hayabusa2 spacecraft journeys to a C-type near-earth asteroid (162173) Ryugu (1999 JU3) to conduct detailed remote sensing observations and return samples from the surface. The Haybusa2 spacecraft developed by Japan Aerospace Exploration Agency (JAXA) was successfully launched on 3 Dec. 2014 by the H-IIA Launch Vehicle and performed an Earth swing-by on 3 Dec. 2015 to set it on a course toward its target. The spacecraft will reach Ryugu in the summer of 2018, observe the asteroid for 18 months, and sample surface materials from up to three different locations. The samples will be delivered to the Earth in Nov.-Dec. 2020. Ground-based observations have obtained a variety of optical reflectance spectra for Ryugu. Some reported the 0.7 μm absorption feature and steep slope in the short wavelength region, suggesting hydrated minerals. -
NASA) Memoranda and Reports Concerning the Decommissioning of the International Space Station (ISS), 2010-2016
Description of document: Unpublished National Aeronautics and Space Administration (NASA) memoranda and reports concerning the decommissioning of the International Space Station (ISS), 2010-2016 Requested date: 28-July-2016 Released date: 05-April-2017 Posted date: 21-May-2018 Source of document: NASA Headquarters 300 E Street, SW Room 5Q16 Washington, DC 20546 Fax: (202) 358-4332 Email: [email protected] The governmentattic.org web site (“the site”) is noncommercial and free to the public. The site and materials made available on the site, such as this file, are for reference only. The governmentattic.org web site and its principals have made every effort to make this information as complete and as accurate as possible, however, there may be mistakes and omissions, both typographical and in content. The governmentattic.org web site and its principals shall have neither liability nor responsibility to any person or entity with respect to any loss or damage caused, or alleged to have been caused, directly or indirectly, by the information provided on the governmentattic.org web site or in this file. The public records published on the site were obtained from government agencies using proper legal channels. Each document is identified as to the source. Any concerns about the contents of the site should be directed to the agency originating the document in question. GovernmentAttic.org is not responsible for the contents of documents published on the website. National Aeronautics and Space Administration Lyndon B. Johnson Space Center 2101 NASA Parkway Houston, Texas 77058-3696 April 5, 2017 Replytoattn.of AD91 l/JSC FOIA Office REF: 16-JSC-F-00829 - Final Release Thank you for your Freedom oflnformation Act (FOIA) request dated and received in the NASA Headquarters FOIA Office on July 28, 2016. -
Research Article Subsurface Thermal Modeling of Oxia Planum, Landing Site of Exomars 2022
Hindawi Advances in Astronomy Volume 2021, Article ID 9924571, 10 pages https://doi.org/10.1155/2021/9924571 Research Article Subsurface Thermal Modeling of Oxia Planum, Landing Site of ExoMars 2022 M. Formisano ,1 M. C. De Sanctis ,1 C. Federico,1 G. Magni,1 F. Altieri ,1 E. Ammannito ,2 S. De Angelis ,1 M. Ferrari ,1 and A. Frigeri 1 1INAF-IAPS, Via del Fosso del Cavaliere 100, Rome, Italy 2Italian Space Agency (ASI), Rome, Italy Correspondence should be addressed to M. Formisano; [email protected] Received 8 March 2021; Revised 18 May 2021; Accepted 25 June 2021; Published 2 September 2021 Academic Editor: Eriita Jones Copyright © 2021 M. Formisano et al. &is is an open access article distributed under the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited. Numerical simulations are required to thermophysically characterize Oxia Planum, the landing site of the mission ExoMars 2022. A drilling system is installed on the ExoMars rover, and it will be able to analyze down to 2 meters in the subsurface of Mars. &e spectrometer Ma_MISS (Mars Multispectral Imager for Subsurface, Coradini and Da Pieve, 2001) will investigate the lateral wall of the borehole generated by the drill, providing hyperspectral images. It is not fully clear if water ice can be found in the subsurface at Oxia Planum. However, Ma_MISS has the capability to characterize and map the presence of possible ices, in particular water ice. We performed simulations of the subsurface temperatures by varying the thermal inertia, and we quantified the effects of self-heating. -
New Voyage to Rendezvous with a Small Asteroid Rotating with a Short Period
Hayabusa2 Extended Mission: New Voyage to Rendezvous with a Small Asteroid Rotating with a Short Period M. Hirabayashi1, Y. Mimasu2, N. Sakatani3, S. Watanabe4, Y. Tsuda2, T. Saiki2, S. Kikuchi2, T. Kouyama5, M. Yoshikawa2, S. Tanaka2, S. Nakazawa2, Y. Takei2, F. Terui2, H. Takeuchi2, A. Fujii2, T. Iwata2, K. Tsumura6, S. Matsuura7, Y. Shimaki2, S. Urakawa8, Y. Ishibashi9, S. Hasegawa2, M. Ishiguro10, D. Kuroda11, S. Okumura8, S. Sugita12, T. Okada2, S. Kameda3, S. Kamata13, A. Higuchi14, H. Senshu15, H. Noda16, K. Matsumoto16, R. Suetsugu17, T. Hirai15, K. Kitazato18, D. Farnocchia19, S.P. Naidu19, D.J. Tholen20, C.W. Hergenrother21, R.J. Whiteley22, N. A. Moskovitz23, P.A. Abell24, and the Hayabusa2 extended mission study group. 1Auburn University, Auburn, AL, USA ([email protected]) 2Japan Aerospace Exploration Agency, Kanagawa, Japan 3Rikkyo University, Tokyo, Japan 4Nagoya University, Aichi, Japan 5National Institute of Advanced Industrial Science and Technology, Tokyo, Japan 6Tokyo City University, Tokyo, Japan 7Kwansei Gakuin University, Hyogo, Japan 8Japan Spaceguard Association, Okayama, Japan 9Hosei University, Tokyo, Japan 10Seoul National University, Seoul, South Korea 11Kyoto University, Kyoto, Japan 12University of Tokyo, Tokyo, Japan 13Hokkaido University, Hokkaido, Japan 14University of Occupational and Environmental Health, Fukuoka, Japan 15Chiba Institute of Technology, Chiba, Japan 16National Astronomical Observatory of Japan, Iwate, Japan 17National Institute of Technology, Oshima College, Yamaguchi, Japan 18University of Aizu, Fukushima, Japan 19Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA 20University of Hawai’i, Manoa, HI, USA 21University of Arizona, Tucson, AZ, USA 22Asgard Research, Denver, CO, USA 23Lowell Observatory, Flagstaff, AZ, USA 24NASA Johnson Space Center, Houston, TX, USA 1 Highlights 1. -
National Aeronautics and Space Administration Planetary Science Subcommittee of the NASA Advisory Council
NAC Planetary Science Subcommittee, January 26-27, 2011 National Aeronautics and Space Administration Planetary Science Subcommittee of the NASA Advisory Council January 26-27, 2011 NASA Headquarters Washington, D.C. Meeting Minutes ____________________ ____________________ Jonathan Rall Ronald Greeley Executive Secretary Chair, Planetary Science Subcommittee 1 NAC Planetary Science Subcommittee, January 26-27, 2011 Table of Contents Welcome 3 NAC Science Committee Review of Analysis Groups 3 NLS II Update 3 Mars Exploration Program 4 Status of EJSM 5 Planetary Science Division Status 6 MESSENGER: Options for an EM 8 Q&A period with SMD AA 9 CAPTEM 10 LEAG 11 MEPAG 11 OPAG 12 VExAG 13 Discussion 14 NASA Chief Scientist Introduction 14 SBAG 15 SR&T 16 Draft report discussion 18 Technology Review Panel 19 Discussion and wrap-up 21 Appendix A- Agenda Appendix B- Membership Appendix C- Attendees Appendix D- List of Presentations Meeting report prepared by: Joan M. Zimmermann, Zantech IT 2 NAC Planetary Science Subcommittee, January 26-27, 2011 January 26, 2011 Welcome Dr. Ronald Greeley, Chair of the Planetary Science Subcommittee (PSS) opened the meeting. Members introduced themselves and agenda items were briefly reviewed. Dr. Greeley acknowledged members who would be cycling off the subcommittee by March 1, 2011; these were Drs. Cravens, Herzog, Johnson, and Slavin. Dr. James Green, Director of the Planetary Science Division (PSD) added his commentary, noting that this would be a critical meeting as Congress debates budget particulars that will undoubtedly impact the division. He added that he wished to ensure that PSD continue to perform top science tasks with guidance from PSS. -
Baikonur-International Space Station : International Approach to Lunar Exploration
ICEUM4, 10-15 July 2000, ESTEC, Noordwijk, The Netherlands Baikonur-International Space Station : International Approach to Lunar Exploration Gulnara Omarova, National Aerospace Agency; Chinghis Omarov, ISU Summer Session '98 alumni On 20th November 1998 our aircraft made soft landing at the Baikonur airport. I was among onboard passengers - officials from Kazakhstan Space, press and diplomats. We all were invited to attend the launch of the International Space Station (ISS) first component (the Russian-made Zarya or Functional Cargo Module FGB) by Proton launch-vehicle at the Baikonur spaceport. Two hours before ISS first module launch we joined the official delegations from NASA, Russian Space Agency (RSA), ESA, Canadian Space Agency (CSA) and NASDA to see the modified facilities of both "Energiya" Corp. and Khrunichev's Proton assembly-and- test building. Mr. Yuri Koptev, Chief of RSA and Mr. Dan Goldin, NASA Administrator actively were drinking russian tea and talking about crucial issues of the International Space Station and the future of Space Exploration. In fact, Cold War is over and the world's top space powers accomplishments are stunning: • The first human flight in space in 1961; • Human space flight initiatives to ascertain if and how long a human could survive in space; • Project Gemini (flights during 1965-1966) to practice space operations, especially rendezvous and docking of spacecraft and extravehicular activity; • Project Apollo (flights during 1968-1972) to explore the Moon; • Space Shuttle's flights (1981 - present); • Satellite programs; • A permanently occupied space station "Mir" (during 1976-1999); • A permanently occupied International Space Station presently underway. We and a few people approached them to learn much more particulars of their talking and to ask them most interesting questions. -
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. -
An Overview of Hayabusa2 Mission and Asteroid 162173 Ryugu
Asteroid Science 2019 (LPI Contrib. No. 2189) 2086.pdf AN OVERVIEW OF HAYABUSA2 MISSION AND ASTEROID 162173 RYUGU. S. Watanabe1,2, M. Hira- bayashi3, N. Hirata4, N. Hirata5, M. Yoshikawa2, S. Tanaka2, S. Sugita6, K. Kitazato4, T. Okada2, N. Namiki7, S. Tachibana6,2, M. Arakawa5, H. Ikeda8, T. Morota6,1, K. Sugiura9,1, H. Kobayashi1, T. Saiki2, Y. Tsuda2, and Haya- busa2 Joint Science Team10, 1Nagoya University, Nagoya 464-8601, Japan ([email protected]), 2Institute of Space and Astronautical Science, JAXA, Japan, 3Auburn University, U.S.A., 4University of Aizu, Japan, 5Kobe University, Japan, 6University of Tokyo, Japan, 7National Astronomical Observatory of Japan, Japan, 8Research and Development Directorate, JAXA, Japan, 9Tokyo Institute of Technology, Japan, 10Hayabusa2 Project Summary: The Hayabusa2 mission reveals the na- Combined with the rotational motion of the asteroid, ture of a carbonaceous asteroid through a combination global surveys of Ryugu were conducted several times of remote-sensing observations, in situ surface meas- from ~20 km above the sub-Earth point (SEP), includ- urements by rovers and a lander, an active impact ex- ing global mapping from ONC-T (Fig. 1) and TIR, and periment, and analyses of samples returned to Earth. scan mapping from NIRS3 and LIDAR. Descent ob- Introduction: Asteroids are fossils of planetesi- servations covering the equatorial zone were performed mals, building blocks of planetary formation. In partic- from 3-7 km altitudes above SEP. Off-SEP observa- ular carbonaceous asteroids (or C-complex asteroids) tions of the polar regions were also conducted. Based are expected to have keys identifying the material mix- on these observations, we constructed two types of the ing in the early Solar System and deciphering the global shape models (using the Structure-from-Motion origin of water and organic materials on Earth [1]. -
The Artemis Accords: Employing Space Diplomacy to De-Escalate a National Security Threat and Promote Space Commercialization
American University National Security Law Brief Volume 11 Issue 2 Article 5 2021 The Artemis Accords: Employing Space Diplomacy to De-Escalate a National Security Threat and Promote Space Commercialization Elya A. Taichman Follow this and additional works at: https://digitalcommons.wcl.american.edu/nslb Part of the National Security Law Commons Recommended Citation Elya A. Taichman "The Artemis Accords: Employing Space Diplomacy to De-Escalate a National Security Threat and Promote Space Commercialization," American University National Security Law Brief, Vol. 11, No. 2 (2021). Available at: https://digitalcommons.wcl.american.edu/nslb/vol11/iss2/5 This Response or Comment is brought to you for free and open access by the Washington College of Law Journals & Law Reviews at Digital Commons @ American University Washington College of Law. It has been accepted for inclusion in American University National Security Law Brief by an authorized editor of Digital Commons @ American University Washington College of Law. For more information, please contact [email protected]. The Artemis Accords: Employing Space Diplomacy to De-Escalate a National Security Threat and Promote Space Commercialization Elya A. Taichman* “Those who came before us made certain that this country rode the first waves of the industrial revolutions, the first waves of modern invention, and the first wave of nuclear power, and this generation does not intend to founder in the backwash of the coming age of space. We mean to be a part of it—we mean to lead it. For the eyes of the world now look into space, to the Moon and to the planets beyond, and we have vowed that we shall not see it governed by a hostile flag of conquest, but by a banner of freedom and peace. -
Kennedy's Quest: Leadership in Space
Kennedy’s Quest: Leadership in Space Overview Topic: “Space Race” Grade Level: 9-12 Subject Area: US History Time Required: One class period. Goals/Rationale: The decision by the Kennedy Administration to make a manned lunar landing the major goal of the US space program derived from political as well as scientific motivations. In this lesson plan, students do a close reading of four primary sources related to the US space program in 1961, analyzing how and why public statements made by the White House regarding space may have differed from private statements made within the Kennedy Administration. Essential Questions: How was the “Space Race” connected to the Cold War? How and why might the White House communicate differently in public and in private? How might the Administration garner support for their policy? Objectives Students will be able to: analyze primary sources, considering the purpose of the source, the audience, and the occasion. analyze the differences in the tone or content of the primary sources. explain the Kennedy Administration’s arguments for putting a human on the Moon by the end of the 1960s. Connections to Curriculum (Standards) National History Standards US History, Era 9: Postwar United States (1945 to early 1970s) Standard 2A: The student understands the international origins and domestic consequences of the Cold War. Historical Thinking Skills Standard 2: Historical Comprehension Reconstruct the literal meaning of a historical passage. Appreciate historical perspectives . Historical Thinking Skills Standard 4: Historical Research Capabilities Support interpretations with historical evidence. Massachusetts History and Social Science Curriculum Frameworks USII [T.5] 1. Using primary sources such as campaign literature and debates, news articles/analyses, editorials, and television coverage, analyze the important policies and events that took place during the presidencies of John F. -
Ames - 75 Years of World Leadership in Science and Technology on Aug
April 2014 - A Quarterly Publication Ames - 75 years of world leadership in science and technology On Aug. 4, 1939, the U.S. Senate passed a bill that included funding for a new National Advisory Committee for Aeronautics (NACA) research sta- tion, where advanced research facilities would be built to develop future flight technologies. Almost 20 years later, the NACA research laboratory became part of the National Aeronautics and Space Administration. Today, 75 years after its inception, NASA’s Ames Research Center at Moffett Field, Mountain View, Calif., continues its world leadership in science and technology. As part of our celebration to commemorate Ames and its glorious past, the Astrogram will publish a series of feature stories depicting past research projects and facilities. To all those who have been an integral part of our past and present, Happy 75th anniversary Ames! See historic Ames photos on page 6 Atmospheric science: NASA Ames’ early contribution to our home planet (part one) The prospect of war was the driv- ing force for Ames’ first research authorization, a study to protect airplanes from the hazards of icing while flying. In 1941, Ames researchers flew a Curtiss C-46 (left) as a flying de-icing research laboratory, to study atmospheric conditions. Wom- en are pictured in the photo, one in the cockpit and two standing with tools in hand. NACA photo BY RUTH DASSO MARLAIRE In 1941, Ames researchers flew a spaceflight program. He refused to Atmospheric research and air- Curtiss C-46 as a flying de-icing fund NASA at the 1960s level, but he borne science campaigns have been research laboratory to study atmo- did approve the start of NASA’s space strengths of NASA’s Ames Research spheric conditions, including liquid- shuttle program. -
The Eternal Fire of Vesta
2016 Ian McElroy All Rights Reserved THE ETERNAL FIRE OF VESTA Roman Cultural Identity and the Legitimacy of Augustus By Ian McElroy A thesis submitted to the Graduate School-New Brunswick Rutgers, The State University of New Jersey In partial fulfillment of the requirements For the degree of Master of Arts Graduate Program in Classics Written under the direction of Dr. Serena Connolly And approved by ___________________________________________ ___________________________________________ ___________________________________________ New Brunswick, New Jersey October 2016 ABSTRACT OF THE THESIS The Eternal Fire of Vesta: Roman Cultural Identity and the Legitimacy of Augustus By Ian McElroy Thesis Director: Dr. Serena Connolly Vesta and the Vestal Virgins represented the very core of Roman cultural identity, and Augustus positioned his public image beside them to augment his political legitimacy. Through analysis of material culture, historiography, and poetry that originated during the principate of Augustus, it becomes clear that each of these sources of evidence contributes to the public image projected by the leader whom Ronald Syme considered to be the first Roman emperor. The Ara Pacis Augustae and the Res Gestae Divi Augustae embody the legacy the Emperor wished to establish, and each of these cultural works contain significant references to the Vestal Virgins. The study of history Livy undertook also emphasized the pathetic plight of Rhea Silvia as she was compelled to become a Vestal. Livy and his contemporary Dionysius of Halicarnassus explored the foundation of the Vestal Order and each writer had his own explanation about how Numa founded it. The Roman poets Virgil, Horace, Ovid, and Tibullus incorporated Vesta and the Vestals into their work in a way that offers further proof of the way Augustus insinuated himself into the fabric of Roman cultural identity by associating his public image with these honored priestesses.