Software Cost Estimation for COVID
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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'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 Sector Brochure
SPACE SPACE REVOLUTIONIZING THE WAY TO SPACE SPACECRAFT TECHNOLOGIES PROPULSION Moog provides components and subsystems for cold gas, chemical, and electric Moog is a proven leader in components, subsystems, and systems propulsion and designs, develops, and manufactures complete chemical propulsion for spacecraft of all sizes, from smallsats to GEO spacecraft. systems, including tanks, to accelerate the spacecraft for orbit-insertion, station Moog has been successfully providing spacecraft controls, in- keeping, or attitude control. Moog makes thrusters from <1N to 500N to support the space propulsion, and major subsystems for science, military, propulsion requirements for small to large spacecraft. and commercial operations for more than 60 years. AVIONICS Moog is a proven provider of high performance and reliable space-rated avionics hardware and software for command and data handling, power distribution, payload processing, memory, GPS receivers, motor controllers, and onboard computing. POWER SYSTEMS Moog leverages its proven spacecraft avionics and high-power control systems to supply hardware for telemetry, as well as solar array and battery power management and switching. Applications include bus line power to valves, motors, torque rods, and other end effectors. Moog has developed products for Power Management and Distribution (PMAD) Systems, such as high power DC converters, switching, and power stabilization. MECHANISMS Moog has produced spacecraft motion control products for more than 50 years, dating back to the historic Apollo and Pioneer programs. Today, we offer rotary, linear, and specialized mechanisms for spacecraft motion control needs. Moog is a world-class manufacturer of solar array drives, propulsion positioning gimbals, electric propulsion gimbals, antenna positioner mechanisms, docking and release mechanisms, and specialty payload positioners. -
VIPER: Virtual Intelligent Planetary Exploration Rover
Proceeding of the 6th International Symposium on Artificial Intelligence and Robotics & Automation in Space: i-SAIRAS 2001, Canadian Space Agency, St-Hubert, Quebec, Canada, June 18-22, 2001. VIPER: Virtual Intelligent Planetary Exploration Rover Laurence Edwards Lorenzo Fl¨uckiger∗ Laurent Nguyen† Richard Washington‡ Autonomy and Robotics Area, NASA Ames Research Center, Moffett Field, CA 94035 { edwards | lorenzo | nguyen | richw } @artemis.arc.nasa.gov Keywords: Simulation, 3D visualization, plan ex- your vehicle works. This is the world of scientist- ecution, planetary rovers. directed planetary rover exploration. Planetary rovers are scientific tools for exploring Abstract an unknown world. One focus of the Autonomy and Simulation and visualization of rover be- Robotics Area (ARA) at the NASA Ames Research havior are critical capabilities for scientists Center is to design and develop the tools and tech- and rover operators to construct, test, and niques that allow scientists to control a rover effi- validate plans for commanding a remote ciently and effectively. This presents challenges both rover. The VIPER system links these capa- in the user interface and in the underlying rover con- bilities, using a high-fidelity virtual-reality trol methods. (VR) environment, a kinematically accu- One important element of the planetary rover con- rate simulator, and a flexible plan execu- trol is the ability to simulate and visualize possible tive to allow users to simulate and visualize execution outcomes of a plan under development. possible execution outcomes of a plan under We have developed the VIPER system, which links development. plan execution, rover simulation, and a high-fidelity, This work is part of a larger vision of a realistic virtual-reality (VR) environment. -
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. -
NASA Program & Budget Update
NASA Update AAAC Meeting | June 15, 2020 Paul Hertz Director, Astrophysics Division Science Mission Directorate @PHertzNASA Outline • Celebrate Accomplishments § Science Highlights § Mission Milestones • Committed to Improving § Inspiring Future Leaders, Fellowships § R&A Initiative: Dual Anonymous Peer Review • Research Program Update § Research & Analysis § ROSES-2020 Updates, including COVID-19 impacts • Missions Program Update § COVID-19 impact § Operating Missions § Webb, Roman, Explorers • Planning for the Future § FY21 Budget Request § Project Artemis § Creating the Future 2 NASA Astrophysics Celebrate Accomplishments 3 SCIENCE Exoplanet Apparently Disappears HIGHLIGHT in the Latest Hubble Observations Released: April 20, 2020 • What do astronomers do when a planet they are studying suddenly seems to disappear from sight? o A team of researchers believe a full-grown planet never existed in the first place. o The missing-in-action planet was last seen orbiting the star Fomalhaut, just 25 light-years away. • Instead, researchers concluded that the Hubble Space Telescope was looking at an expanding cloud of very fine dust particles from two icy bodies that smashed into each other. • Hubble came along too late to witness the suspected collision, but may have captured its aftermath. o This happened in 2008, when astronomers announced that Hubble took its first image of a planet orbiting another star. Caption o The diminutive-looking object appeared as a dot next to a vast ring of icy debris encircling Fomalhaut. • Unlike other directly imaged exoplanets, however, nagging Credit: NASA, ESA, and A. Gáspár and G. Rieke (University of Arizona) puzzles arose with Fomalhaut b early on. Caption: This diagram simulates what astronomers, studying Hubble Space o The object was unusually bright in visible light, but did not Telescope observations, taken over several years, consider evidence for the have any detectable infrared heat signature. -
Gao-21-306, Nasa
United States Government Accountability Office Report to Congressional Committees May 2021 NASA Assessments of Major Projects GAO-21-306 May 2021 NASA Assessments of Major Projects Highlights of GAO-21-306, a report to congressional committees Why GAO Did This Study What GAO Found This report provides a snapshot of how The National Aeronautics and Space Administration’s (NASA) portfolio of major well NASA is planning and executing projects in the development stage of the acquisition process continues to its major projects, which are those with experience cost increases and schedule delays. This marks the fifth year in a row costs of over $250 million. NASA plans that cumulative cost and schedule performance deteriorated (see figure). The to invest at least $69 billion in its major cumulative cost growth is currently $9.6 billion, driven by nine projects; however, projects to continue exploring Earth $7.1 billion of this cost growth stems from two projects—the James Webb Space and the solar system. Telescope and the Space Launch System. These two projects account for about Congressional conferees included a half of the cumulative schedule delays. The portfolio also continues to grow, with provision for GAO to prepare status more projects expected to reach development in the next year. reports on selected large-scale NASA programs, projects, and activities. This Cumulative Cost and Schedule Performance for NASA’s Major Projects in Development is GAO’s 13th annual assessment. This report assesses (1) the cost and schedule performance of NASA’s major projects, including the effects of COVID-19; and (2) the development and maturity of technologies and progress in achieving design stability. -
Download Announcement
Moog Moog Inc. ▪ East Aurora, New York ▪ 14052 ▪ 716-652-2000 Announcement Moog to Exhibit Mission Critical Space Technology at the 36th Annual Space Symposium East Aurora, NY (August 14, 2021) – Moog Inc. (NYSE: MOG.A and MOG.B) will highlight its Space technology capabilities at the 36th annual Space Symposium in Colorado Springs, CO August 23-26. Moog with be at booth #1030 in the North Exhibit Hall at The Broadmoor. Visit us at Space Symposium to discover more about the following featured technologies: The Small Launch Orbital Maneuvering Vehicle (SL-OMV) is a propulsive tug for secondary payload deployment focused on Venture Class Launch Vehicles. It is payload configurable for cubesats through ESPA-Class spacecraft. It can be used to disperse cubesat constellations or deliver ESPA- Class spacecraft to their ideal orbit. The SL-OMV has its own avionics, power, green propulsion, and communications systems that are configurable for short duration missions. Additionally, Moog’s next generation, radiation-hardened Integrated Avionics Unit (IAU) will be on display. NASA recently selected our IAU and Spacecraft Energization and Power Interfacing Assembly to be the main computer and power source for the VIPER rover, which will land on the Moon’s South Pole to scout possible landing sites for NASA’s Artemis Program. Furthermore, Moog and industry Partner Unibap have teamed to produce next-generation Payload Graphics Processing Units (GPU) for LEO, MEO and GEO missions. We will have live demonstrations daily at 1 p.m. in booth #1030. Many of our solutions on display support human exploration, including NASA’s Artemis missions. -
NASA Ames Research Center Intelligent Systems and High End Computing
NASA Ames Research Center Intelligent Systems and High End Computing Dr. Eugene Tu, Director NASA Ames Research Center Moffett Field, CA 94035-1000 A 80-year Journey 1960 Soviet Union United States Russia Japan ESA India 2020 Illustration by: Bryan Christie Design Updated: 2015 Protecting our Planet, Exploring the Universe Earth Heliophysics Planetary Astrophysics Launch missions such as JWST to Advance knowledge unravel the of Earth as a Determine the mysteries of the system to meet the content, origin, and universe, explore challenges of Understand the sun evolution of the how it began and environmental and its interactions solar system and evolved, and search change and to with Earth and the the potential for life for life on planets improve life on solar system. elsewhere around other stars earth “NASA Is With You When You Fly” Safe, Transition Efficient to Low- Growth in Carbon Global Propulsion Operations Innovation in Real-Time Commercial System- Supersonic Wide Aircraft Safety Assurance Assured Ultra-Efficient Autonomy for Commercial Aviation Vehicles Transformation NASA Centers and Installations Goddard Institute for Space Studies Plum Brook Glenn Research Station Independent Center Verification and Ames Validation Facility Research Center Goddard Space Flight Center Headquarters Jet Propulsion Wallops Laboratory Flight Facility Armstrong Flight Research Center Langley Research White Sands Center Test Facility Stennis Marshall Space Kennedy Johnson Space Space Michoud Flight Center Space Center Center Assembly Center Facility -
Section 3 Report Executive Order 13287 Fiscal Years 2009-2011
National Aeronautics and Space Administration Section 3 Report Executive Order 13287 Fiscal Years 2009-2011 www.nasa.gov Crowds flock to watch the last flight of the Space Shuttle Program with the launch of Atlantis on July 8, 2011. Abbreviations for NASA Centers: ARC Ames Research Center DFC Dryden Flight Center GDSCC Goldstrone Deep Space Communication Complex GRC Glen Research Center GSFC Goddard Space Flight Center JPL Jet Propulsion Laboratory JSC Johnson Space Center KSC Kennedy Space Center LaRC Langley Research Center MAF Michoud Assembly Facility MSFC Marshall Space Flight Center PBS Plum Brook Station SSFL Santa Susana Field Laboratory SSC Stennis Scpace Center WFF Walllops Flight Facility WSTF White Sands Test Facility INTRODUCTION This report is submitted to the Advisory Council on His- toric Preservation (ACHP) by the National Aeronautics and Space Administration (NASA) in compliance with Executive Order (EO) 13287, Preserve America. Sec- tion 3 of EO 13287 requires NASA to submit a triennial report on its progress in identifying, protecting, and us- ing historic properties in the Agency’s ownership. This is NASA’s fourth report, the second triennial report, to be submitted. The report responds to the 18 questions posed by the ACHP in its “Advisory Guidelines Imple- menting Executive Order 13287, Preserve America” and reports progress made by NASA toward the EO goals. NASA continues to make strides in its stewardship re- sponsibilities as the cultural resources management and historic preservation program matures. Over the past 3 years, our Cultural Resources Management Panel has finalized the internal NASA Procedural Requirements that will guide Agency personnel across the country Submitted by NASA Headquarters in meeting NASA’s cultural resource stewardship re- 300 E Street SW sponsibilities. -
Planetary Science Update
Planetary Science Division Status Report Jim Green NASA, Planetary Science Division October 11, 2017 Presentation at LEAG Planetary Science Missions Events 2016 March – Launch of ESA’s ExoMars Trace Gas Orbiter July 4 – Juno inserted in Jupiter orbit * Completed September 8 – Launch of Asteroid mission OSIRIS – REx to asteroid Bennu September 30 – Landing Rosetta on comet CG October 19 – ExoMars EDM landing and TGO orbit insertion 2017 January 4 – Discovery Mission selection announced February 9-20 - OSIRIS-REx began Earth-Trojan search April 22 – Cassini begins plane change maneuver for the “Grand Finale” August 22 – Solar Eclipse across America September 15 – Cassini end of mission at Saturn September 22 – OSIRIS-REx Earth flyby October 28 – International Observe the Moon night (1st quarter) 2018 May 5 - Launch InSight mission to Mars August – OSIRIS-REx arrival at Bennu October – Launch of ESA’s BepiColombo to Mercury November 26 – InSight landing on Mars 2019 January 1 – New Horizons flyby of Kuiper Belt object 2014MU69 Formulation Implementation Primary Ops BepiColombo Lunar Extended Ops (ESA) Reconnaissance Orbiter Lucy New Horizons Psyche Juno Dawn JUICE (ESA) ExoMars 2016 MMX MAVEN MRO (ESA) (JAXA) Mars Express Mars (ESA) Odyssey OSIRIS-REx ExoMars 2020 (ESA) Mars Rover Opportunity Curiosity InSight 2020 Rover Rover NEOWISE Europa Clipper Discovery Program Discovery Program NEO characteristics: Mars evolution: Lunar formation: Nature of dust/coma: Solar wind sampling: NEAR (1996-1999) Mars Pathfinder (1996-1997) Lunar Prospector -
The Lunar Crater Observation and Sensing Satellite (LCROSS) Payload Development and Performance in Flight
Space Sci Rev (2012) 167:23–69 DOI 10.1007/s11214-011-9753-4 The Lunar Crater Observation and Sensing Satellite (LCROSS) Payload Development and Performance in Flight Kimberly Ennico · Mark Shirley · Anthony Colaprete · Leonid Osetinsky Received: 8 October 2010 / Accepted: 25 January 2011 / Published online: 19 February 2011 © US Government 2011 Abstract The primary objective of the Lunar Crater Observation and Sensing Satellite (LCROSS) was to confirm the presence or absence of water ice in a permanently shad- owed region (PSR) at a lunar pole. LCROSS was classified as a NASA Class D mission. Its payload, the subject of this article, was designed, built, tested and operated to support a condensed schedule, risk tolerant mission approach, a new paradigm for NASA science missions. All nine science instruments, most of them ruggedized commercial-off-the-shelf (COTS), successfully collected data during all in-flight calibration campaigns, and most im- portantly, during the final descent to the lunar surface on October 9, 2009, after 112 days in space. LCROSS demonstrated that COTS instruments and designs with simple interfaces, can provide high-quality science at low-cost and in short development time frames. Building upfront into the payload design, flexibility, redundancy where possible even with the science measurement approach, and large margins, played important roles for this new type of pay- load. The environmental and calibration approach adopted by the LCROSS team, compared to existing standard programs, is discussed. The description, capabilities, calibration and in- flight performance of each instrument are summarized. Finally, this paper goes into depth about specific areas where the instruments worked differently than expected and how the flexibility of the payload team, the knowledge of instrument priority and science trades, and proactive margin maintenance, led to a successful science measurement by the LCROSS payload’s instrument complement.