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Selection of the Insight Landing Site M. Golombek1, D. Kipp1, N
Manuscript Click here to download Manuscript InSight Landing Site Paper v9 Rev.docx Click here to view linked References Selection of the InSight Landing Site M. Golombek1, D. Kipp1, N. Warner1,2, I. J. Daubar1, R. Fergason3, R. Kirk3, R. Beyer4, A. Huertas1, S. Piqueux1, N. E. Putzig5, B. A. Campbell6, G. A. Morgan6, C. Charalambous7, W. T. Pike7, K. Gwinner8, F. Calef1, D. Kass1, M. Mischna1, J. Ashley1, C. Bloom1,9, N. Wigton1,10, T. Hare3, C. Schwartz1, H. Gengl1, L. Redmond1,11, M. Trautman1,12, J. Sweeney2, C. Grima11, I. B. Smith5, E. Sklyanskiy1, M. Lisano1, J. Benardino1, S. Smrekar1, P. Lognonné13, W. B. Banerdt1 1Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109 2State University of New York at Geneseo, Department of Geological Sciences, 1 College Circle, Geneseo, NY 14454 3Astrogeology Science Center, U.S. Geological Survey, 2255 N. Gemini Dr., Flagstaff, AZ 86001 4Sagan Center at the SETI Institute and NASA Ames Research Center, Moffett Field, CA 94035 5Southwest Research Institute, Boulder, CO 80302; Now at Planetary Science Institute, Lakewood, CO 80401 6Smithsonian Institution, NASM CEPS, 6th at Independence SW, Washington, DC, 20560 7Department of Electrical and Electronic Engineering, Imperial College, South Kensington Campus, London 8German Aerospace Center (DLR), Institute of Planetary Research, 12489 Berlin, Germany 9Occidental College, Los Angeles, CA; Now at Central Washington University, Ellensburg, WA 98926 10Department of Earth and Planetary Sciences, University of Tennessee, Knoxville, TN 37996 11Institute for Geophysics, University of Texas, Austin, TX 78712 12MS GIS Program, University of Redlands, 1200 E. Colton Ave., Redlands, CA 92373-0999 13Institut Physique du Globe de Paris, Paris Cité, Université Paris Sorbonne, France Diderot Submitted to Space Science Reviews, Special InSight Issue v. -
Nasa Advisory Council Human Exploration and Operations
NASA ADVISORY COUNCIL HUMAN EXPLORATION AND OPERATIONS COMMITTEE NASA Headquarters Washington, DC January 13-14, 2021 MEETING REPORT _____________________________________________________________ N. Wayne Hale, Chair ____________________________________________________________ Bette Siegel, Executive Secretary Table of Contents Call to Order 3 Commercial Crew Program 5 Public Comments 8 Artemis Program 9 SMD Artemis CLPS Activities 11 Moon to Mars Update 12 Solar System and Beyond 12 HERMES Instrument Update Artemis III SDT Update Advancing Biological and Physical Sciences Through Lunar Exploration 14 SMD Mars Science Update 14 Artemis Accords 15 Planetary Protection Activities 15 Discussion/Findings and Recommendations 16 Appendix A- Attendees Appendix B- HEOC Membership Appendix C- Presentations Appendix D- Agenda Appendix E- Chat Transcript Prepared by Joan M. Zimmermann Zantech IT, Inc. 2 January 13, 2021 Call to order and welcome Dr. Bette Siegel, Executive Secretary of the Human Exploration and Operations Committee (HEOC), called the meeting to order, and provided details of the Federal Advisory Committee Act (FACA), which provides governance rules for the meeting. She introduced Mr. N. Wayne Hale, Chair of the HEOC. Mr. Hale noted to the public that this particular HEO meeting counts as the last meeting of 2020, and the next scheduled meeting in March/April will be the first meeting of 2021. Mr. Hale welcomed three new members, Ms. Lynn Cline, Mr. David Thompson, and Mr. Kwatsi Alibaruho. The present meeting is focused on an update on the HEO areas, and a joint meeting with the NASA Advisory Council (NAC) Science Committee. Mr. Hale asked if NAC Chair, General Lester Lyles, who was attending the meeting virtually, had any remarks to proffer. -
The Messenger Spacecraft Power System Design and Early Mission Performance
THE MESSENGER SPACECRAFT POWER SYSTEM DESIGN AND EARLY MISSION PERFORMANCE G. Dakermanji, C. Person, J. Jenkins, L. Kennedy, D. Temkin Johns Hopkins University Applied Physics Laboratory, 11100 Johns Hopkins Rd., Laurel, Maryland, 20723-6099, USA Email: [email protected] ABSTRACT The MESSENGER (MErcury Surface, Space ENvironment, GEochemistry, and Ranging) spacecraft was launched on August 3, 2004. The spacecraft will be inserted into Mercury orbit in March 2011 for one year of orbital operation. During the mission, the spacecraft distance to the Sun will vary between approximately 1 and 0.3 Astronomical Units (AU), imposing severe requirements on the spacecraft thermal and power systems design. The spacecraft is maintained behind a sunshade. The two single-axis, gimbaled solar array panels are designed to withstand the expected high temperatures. A peak power tracking system has been selected to allow operation over the widely varying solar array I-V curves. In order to reduce cost and risk while increasing the likelihood of mission success, the approach taken in the power system design, including the solar arrays, was to use conventional design, materials, and fabrication techniques. 1. MISSION DESCRIPTION a. Launch Configuration Sunshade MESSENGER (MErcury Surface, Space ENvironment, GEochemistry, and Ranging), shown in Fig. 1, is a Battery NASA Discovery Program spacecraft designed and built by the Johns Hopkins University Applied Physics Laboratory (APL). It will orbit the planet Mercury for one Earth year of orbital operation. Most of what is known about Mercury comes from the Mariner 10 spacecraft. Using three flybys, Mariner 10 was able to map about 45% of the planet surface during a one-year period between 1974 and 1975. -
NASA's Ames Research Center
NASA’s Ames Research Center NASA’s center in Silicon Valley Ames Research Center, one of 10 NASA fi eld Ames provides NASA with advancements in: centers, is located in California’s Silicon Valley. For more than 70 years, Ames has been a leader in Entry systems: Safely delivering spacecraft to conducting world-class research and development. Earth and other celestial bodies. Location: California’s Silicon Valley, 40 miles Supercomputing: Enabling NASA’s advanced south of San Francisco; 12 miles north of San modeling and simulation. Jose, between Mountain View and Sunnyvale Next generation air transportation: Transforming Jobs: Approximately 2,500 on-site employees and the way we fl y. contractors Airborne science: Examining our own world and Economic impact: $1.3B annually for the U.S.; beyond from the sky. $932M for California and $877M for Bay Area, creating more than 8,400 jobs in the U.S. with Low-cost missions: Enabling high value science 5,900 in California (2010 Economic Benefi ts to low Earth orbit and the moon. Study). Biology and astrobiology: Understanding life on Established: Dec. 20, 1939 as part of the National Earth -- and in space. Advisory Committee for Aeronautics (NACA); became part of the National Aeronautics and Exoplanets: Finding worlds beyond our own. Space Administration (NASA) in 1958. Autonomy and robotics: Complementing Missions: Ames-related missions scheduled for humans in space. launch in 2013 include LADEE, PhoneSat, EDSN, EcAMSat, SporeSat and IRIS. Ames will launch Lunar science: Rediscovering our moon. several space biosciences payloads this year. The center is lead for the Mars Curiosity rover’s Human factors: Advancing human-technology Chemistry and Mineralogy (CheMin) instrument interaction for NASA missions. -
Space Communications and Navigation (Scan) Testbed
National Aeronautics and Space Administration Space Communication and Navigation Testbed: Communications Technology for Exploration Richard Reinhart NASA Glenn Research Center July 2013 ISS Research and Development Conference Sponsored by Space Communication and Navigation Program Titan Lunar Neptune Relay Satellite Saturn Uranus Pluto LADEE Charon Jupiter Near Earth Optical Relay Pathfinder Mars NISNNISN MCC MOCs SCaN2023202520182015 Add: Services Provide: ••IntegratedEnhancedDeepIntegratedStandard Space service-basedServicesOptical Network Optical Initial Management Initial and architectureCapability Interfaces Capability (INM) ••SpaceDeepSpaceIntegratedDelay Space internetworking InternetworkingTolerant Service Optical Networking Execution Relay (DTN throughout Pathfinder and (ISE) IP) Solar Venus Deep Space ••InternationalLunarSystemSpaceDeep SpaceRelay Internetworking interoperability Satellite Antenna Initial Array Capability Antenna Optical Relay ••AssuredSignificantOpticalLunar Optical Ground safety Increases and Pathfinder Terminal security in Bandwidth (LADEE) of missions Array Pathfinder ••SignificantRetirementNearTDRS Earth K, L increases Optical of Aging Initial RFin bandwidth Systems Capability Sun Mercury • TDRSIncreased M,N microwave link data rates • Lunar Relay Payload (potential) 2 Microwave Links Optical Links NISN Next Generation Communication and Navigation Technology – Optical Communications – Antenna Arraying Technology – Receive and Transmit – Software Defined Radio – Advanced Antenna Technology – Spacecraft RF -
PSAD-81-2 Support Service Contracting at Johnson Space
BY THEU.S. GENERAL ACCOUNTli’JG OFFICE Report To The Administrator, National Aeronautics And Space Administration S@pportService Contracting At Johnson Space Center Needs Strengthening T National Aeronautics and S ace Administration Sl about $175 million annual Py on support service Cl at Johnson Space Center. GAO tested the way si of these contracts are administered and found --a contractor was working without approved llllllllllllllll113606 work orders, --Government-furnished equipment was unac- counted for, --questionable reimbursements occurred for con- tractor costs, I --contract funds increased before the need was justified, I --contracting officers were unaware of their re- sponsibilitres and unfamiliar with contract terms, and I --some contracting officers had a general attitude that small dollar value contracts are not worthy of adequate attention. I ‘/A0 believes overreliance on cost-type contracts which quire greater administration efforts than fixed-price )ntracts contributes to these contracting weaknesses recommends that the National Aeronautics and ace Administration take corrective actions. mp81s2 OCTOBER 21,1900 + Request for copies of GAO reports should be sent to: U.S. General Accounting Office Document Handling and Information Services Facility P.O. Box 6015 Gaithersburg, Md. 20760 Telephone (202) 275-6241 The first five copies of individual reports are free of charge. Additional copies of bound audit reports are $3.25 each. Additional copies of unbound report (i.e., letter reports) and most other publications are $1.00 each. There will be a 25% discount on all orders for 100 or more copies mailed to a single address. Sales orders must be prepaid on a cash, check, or money order basis. -
588168 Amendment No. 56 NASA Glenn Research Center, License
NRC FORM 374 PAGE 1 OF 7 PAGES U.S. NUCLEAR REGULATORY COMMISSION Amendment No. 56 MATERIALS LICENSE Pursuant to the Atomic Energy Act of 1954, as amended, the Energy Reorganization Act of 1974 (Public Law 93-438), and Title 10, Code of Federal Regulations, Chapter I, Parts 30, 31, 32, 33, 34, 35, 36, 37, 39, 40, 70 and 71, and in reliance on statements and representations heretofore made by the licensee, a license is hereby issued authorizing the licensee to receive, acquire, possess, and transfer byproduct, source, and special nuclear material designated below; to use such material for the purpose(s) and at the place(s) designated below; to deliver or transfer such material to persons authorized to receive it in accordance with the regulations of the applicable Part(s). This license shall be deemed to contain the conditions specified in Section 183 of the Atomic Energy Act of 1954, as amended, and is subject to all applicable rules, regulations, and orders of the Nuclear Regulatory Commission now or hereafter in effect and to any conditions specified below. Licensee In accordance with letter dated 4. Expiration Date: March 31, 2025 March 28, 201 1. National Aeronautics & Space Administration R John H. Glenn Research Center 5. Docket No.: 030-05626 2. 21000 Brookpark Road Reference No.: Mailstop 6-4 Cleveland, OH 44135 6. Byproduct, source, 9. Authorized use and/or special nuclear material A. Any byproduct material A. Activation ~ucts A. For research and development as between atomic numbers described in 10 CFR 30.4. Possession 3 and 83 incident to the radiological characterization surveys of a shut-down cyclotron. -
March 21–25, 2016
FORTY-SEVENTH LUNAR AND PLANETARY SCIENCE CONFERENCE PROGRAM OF TECHNICAL SESSIONS MARCH 21–25, 2016 The Woodlands Waterway Marriott Hotel and Convention Center The Woodlands, Texas INSTITUTIONAL SUPPORT Universities Space Research Association Lunar and Planetary Institute National Aeronautics and Space Administration CONFERENCE CO-CHAIRS Stephen Mackwell, Lunar and Planetary Institute Eileen Stansbery, NASA Johnson Space Center PROGRAM COMMITTEE CHAIRS David Draper, NASA Johnson Space Center Walter Kiefer, Lunar and Planetary Institute PROGRAM COMMITTEE P. Doug Archer, NASA Johnson Space Center Nicolas LeCorvec, Lunar and Planetary Institute Katherine Bermingham, University of Maryland Yo Matsubara, Smithsonian Institute Janice Bishop, SETI and NASA Ames Research Center Francis McCubbin, NASA Johnson Space Center Jeremy Boyce, University of California, Los Angeles Andrew Needham, Carnegie Institution of Washington Lisa Danielson, NASA Johnson Space Center Lan-Anh Nguyen, NASA Johnson Space Center Deepak Dhingra, University of Idaho Paul Niles, NASA Johnson Space Center Stephen Elardo, Carnegie Institution of Washington Dorothy Oehler, NASA Johnson Space Center Marc Fries, NASA Johnson Space Center D. Alex Patthoff, Jet Propulsion Laboratory Cyrena Goodrich, Lunar and Planetary Institute Elizabeth Rampe, Aerodyne Industries, Jacobs JETS at John Gruener, NASA Johnson Space Center NASA Johnson Space Center Justin Hagerty, U.S. Geological Survey Carol Raymond, Jet Propulsion Laboratory Lindsay Hays, Jet Propulsion Laboratory Paul Schenk, -
10 Things to Know About NASA's Glenn Research Center
National Aeronautics and Space Administration 10 Things to Know About NASA’s Glenn Research Center 1. NASA Glenn’s economic impact in Ohio exceeds $1.4 billion per year. According to an economic impact study by Cleveland State University’s Center for Economic Development, Glenn generates over $700 million annually in economic activity and creates over 7,000 jobs. NASA Glenn also generates nearly $500 million in labor income and approximately $120 million in tax revenue per year. 2. Glenn scientists and engineers are prolific inventors. The research center holds more than 725 patents and has won over 120 R&D 100 Awards, also known as the Oscars of innovation. That’s more than any other NASA center. Glenn strives to increase private sector revenue and contribute to private sector job growth by licensing its inventions. 3. Every U.S. aircraft has NASA Glenn technology on board. NASA is with you when you fly. Today’s commercial airliners are safer, quieter and more fuel efficient because of NASA Glenn technology. Glenn advancements such as ice detection and air traffic control systems have made flying safer. Glenn jet engine combustors have resulted in more efficient aircraft engines, and Glenn developed nozzle chevrons are used to make the Boeing 787 Dreamliner and new 737 MAX quieter. 4. Glenn is transforming aviation by developing revolutionary technologies for aircraft and the national airspace system. Glenn is working to dramatically improve efficiency, reduce costs and noise, and maintain safety in crowded skies. The center leads the agency’s effort to develop hybrid electric propulsion systems for commercial passenger aircraft. -
Cubex: a Compact X-Ray Telescope Enables Both X-Ray Fluorescence Imaging Spectroscopy and Pulsar Timing Based Navigation
SSC18-V-05 CubeX: A compact X-Ray Telescope Enables both X-Ray Fluorescence Imaging Spectroscopy and Pulsar Timing Based Navigation Jan Stupl, Monica Ebert, David Mauro SGT / NASA Ames NASA Ames Research Center, Moffett Field, CA; 650-604-4032 [email protected] JaeSub Hong Harvard University Cambridge, MA Suzanne Romaine, Almus Kenter, Janet Evans, Ralph Kraft Smithsonian Astrophysical Observatory Cambridge, MA Larry Nittler Carnegie Institution of Washington Washington, DC Ian Crawford Birkbeck College London, UK David Kring Lunar and Planetary Institute Houston, TX Noah Petro, Keith. Gendreau, Jason Mitchell, Luke Winternitz NASA Goddard Space Flight Center Greenbelt, MD Rebecca. Masterson, Gregory Prigozhin Massachusetts Institute of Technology Cambridge, MA Brittany Wickizer NASA Ames Research Center Moffett Field, CA Kellen Bonner, Ashley Clark, Arwen Dave, Andres Dono-Perez, Ali Kashani, Daniel Larrabee, Samuel Montez, Karolyn Ronzano, Tim Snyder MEI / NASA Ames Research Center Joel Mueting, Laura Plice Metis / NASA Ames Research Center NASA Ames Research Center, Moffett Field, CA Yueh-Liang Shen, Duy Nguyen Booz Allen Hamilton / NASA Ames NASA Ames Research Center, Moffett Field, CA Stupl 1 32nd Annual AIAA/USU Conference on Small Satellites ABSTRACT This paper describes the miniaturized X-ray telescope payload, CubeX, in the context of a lunar mission. The first part describes the payload in detail, the second part summarizes a small satellite mission concept that utilizes its compact form factor and performance. This instrument can be used for both X-ray fluorescence (XRF) imaging spectroscopy and X-ray pulsar timing-based navigation (XNAV). It combines high angular resolution (<1 arcminutes) Miniature Wolter-I X-ray optics (MiXO) with a common focal plane consisting of high spectral resolution (<150 eV at 1 keV) CMOS X-ray sensors and a high timing resolution (< 1 µsec) SDD X-ray sensor. -
MAVEN—Definitive Answers About Mars Climate History
Page 1 The Critical Path A Flight Projects Directorate Quarterly Publication Volume 20 number 3 A Newsletter Published for Code 400 Employees 2012 Winter INSIDE THIS ISSUE: MAVEN—Definitive Answers about MAVEN—Definitive Answers Mars Climate History Page 1 about Mars Climate History When the Mars Atmosphere and Volatile Evolution (MAVEN) Message From The Director Of Page 2 mission launches in November 2013 it will make history. Personality Tintypes Page 3 Even though there have been a number of Mars missions before, MAVEN is the first mission to focus its study on the Comings and Going Page 10 Mars upper atmosphere. MAVEN will study the evolution of the Mars atmosphere and climate, by examining the conduit NASA’s LADEE Spacecraft Gets Page 11 Final Science Instrument Installed through which the atmosphere has to pass as it is lost to space (i.e., the upper atmosphere). It is the first mission NASA's GPM Observatory Page 13 devoted to understanding the role that loss to space played in Completes First Dry Run the history of the atmosphere and climate. MAVEN will Three Former GSFC Leaders Page 15 provide a comprehensive picture of the Mars upper atmos- Pass On phere, ionosphere, solar energetic drivers, and atmospheric An Ode to McDonald Page 16 losses. It will deliver definitive answers to long-standing questions about the climate history and habitability of Mars. New Business News Page 17 MAVEN is a Principal Investigator-led mission and the first Knowledge Management Corner Page 20 Mars mission managed by the Goddard Space Flight Center 2012 Agency Honor Award (GSFC). -
EXPLORING the MOON in the 21St CENTURY
CosmoELEMENTS EXPLORING THE MOON IN THE 21st CENTURY Samuel J. Lawrence1 and Clive R. Neal2 DOI: 10.2138/gselements.15.5.360 INTRODUCTION In 2019, we are celebrating the 50th anniversary of NASA’s momentous Apollo expedi- tions to the Moon. The samples brought back by the astronauts, and the fieldwork those astro- The South Pole of the Moon, pictured here in an oblique view from FIGURE 1 NASA’s Lunar Reconnaissance Orbiter, is the landing site for the nauts performed on the lunar surface, cemented the Moon’s status as seventh human lunar landing. IMAGE COURTESY OF NAC M1195011983LR (NASA/ the cornerstone of the solar system. It is not an exaggeration to say GSFC/ARIZONA STATE UniVERSITY). that the Apollo expeditions transformed our understanding of our solar system, and, in fact, most of the discoveries made in planetary science since the 1960s can trace directly, or indirectly, from the scientific of the Sun’s evolution and history. Finally, this is another area where results of those Apollo expeditions. the Apollo expeditions represent a strength: there are five decades worth of planetary science hypotheses that lunar geological fieldwork Although some erroneously proclaim that the Moon is “Been there, will address. The lunar surface could also provide a unique and stable done that”, nothing could be further from the truth. After a long long-term platform for astronomy. In particular, manned radio obser- st hiatus, beginning in the first years of the 21 century, there has vatories or optical interferometers on the far side of the Moon could been a resurgence of interest in the Moon, including the Kaguya produce dramatic advances in astrophysics.