Applicability of STEM-RTG and High-Power SRG Power Systems to the Discovery and Scout Mission Capabilities Expansion (DSMCE) Study of ASRG-Based Missions
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Autonomous Onboard Science Data Analysis for Comet Missions
AUTONOMOUS ONBOARD SCIENCE DATA ANALYSIS FOR COMET MISSIONS David R. Thompson(1), Daniel Q. Tran(1), David McLaren(1), Steve A. Chien(1), Larry Bergman(1), Rebecca Castaño(1), Richard Doyle(1), Tara Estlin(1), Matthew Lenda(1), (1) Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Dr. Pasadena, CA 91109, USA Email: [email protected], all others [email protected] Figure 1. Plume detection by identifying the nucleus. Left: computational edge detection. Center: a convex hull of edge points. Right: bright areas outside the nucleus are plumes. Image credit: NASA/JPL/UMD. ABSTRACT active geologic processes including scarps and outflows [1]. Its surface undergoes continuous modification, Coming years will bring several comet rendezvous with visible change during the years between two missions. The Rosetta spacecraft arrives at Comet flybys. The EPOXI flyby of comet Hartley 2 shows 67P/Churyumov–Gerasimenko in 2014. Subsequent skyscraper-size spires, flat featureless plains that outgas rendezvous might include a mission such as the H O, regions of rough and mottled texture, bands of proposed Comet Hopper with multiple surface landings, 2 various shapes, and diverse surface albedo. Comets’ as well as Comet Nucleus Sample Return (CNSR) and active areas range from 10-90%, changing over time Coma Rendezvous and Sample Return (CRSR). These and distance to the sun. They manifest as both localized encounters will begin to shed light on a population that, jets and diffuse regions (Figure 1). Still more exotic, despite several previous flybys, remains mysterious and recently discovered “active asteroids” suggest that poorly understood. -
2020 Technology and Research Initiative Fund Annual Report
FISCAL YEAR 2020 TECHNOLOGY AND RESEARCH INITIATIVE FUND ABOUT THIS REPORT The fiscal year 2020 Arizona Board of Regents Technology and Research Initiative Fund filed in accordance with A.R.S. §15-1648(D) includes the prior year’s TRIF expenditures. The board adopted TRIF five-year project plans, available on the ABOR website, detailing anticipated budgets and expected outcomes. TRIF was established through Proposition 301 that increased the state’s sales tax to be dedicated to K-12, community colleges and Arizona’s public universities. Collection of the tax began on June 1, 2001, and the proposition was extended for another 20 years in 2018. Arizona law establishes TRIF using Proposition 301 sales tax revenue and gives the Arizona Board of Regents the responsibility to administer the fund. TRIF monies are continuously appropriated to ABOR and do not lapse at the end of the fiscal year. The fiscal year 2020 TRIF report details research goals, accomplishments and highlights from the universities that address challenges to the state and society as well as detailed financial information on how the funds were utilized. Through TRIF funds, the institutions are able to accomplish advances in vital research, including COVID-19 research, virus biotech detection, water resources and more. ABOUT THE ARIZONA BOARD OF REGENTS The Arizona Board of Regents is committed to ensuring access for qualified residents of Arizona to undergraduate and graduate institutions; promoting the discovery, application, and dissemination of new knowledge; extending the benefits of university activities to Arizona’s citizens outside the university; and maximizing the benefits derived from the state’s investment in education. -
Agile Science Operations David R
Agile Science Operations David R. Thompson Machine Learning and Instrument Autonomy Jet Propulsion Laboratory, California Institute of Technology Engineering Resilient Space Systems Keck Institute Study, July 31 2012. A portion of this research was carried out at the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration. Copyright 2012 California Institute of Technology. All Rights Reserved; U. S. Government Support Acknowledged. Image: Hartley 2 (EPOXI), NASA/JPL/UMD Jet Propulsion Laboratory / California Institute of Technology / Solar System Exploration Directorate 1 Agenda Motivation: science at primitive bodies Critical Path Analysis and reaction time A survey of onboard science data analysis Case study – how could onboard data analysis impact missions? Image: Hartley 2 (EPOXI), NASA/JPL/UMD Jet Propulsion Laboratory / California Institute of Technology / Solar System Exploration Directorate 2 Primitive bodies Jet Propulsion Laboratory / California Institute of Technology / Solar System Exploration Directorate 3 Typical encounter (Lutetia 21, Rosetta) Jet Propulsion Laboratory / California Institute of Technology / Solar System Exploration Directorate 4 Primitive bodies: key measurements Reproduced from Castillo-Rogez, Pavone, Nesnas, Hoffman, “Expected Science Return of Spatially-Extended In-Situ Exploration at Small Solar System Bodies,” IEEE Aerospace 2012. Jet Propulsion Laboratory / California Institute of Technology / Solar System Exploration Directorate -
LAST CALL for the DAS Dinner Meeting Tuesday, May17th
Vol. 56, No. 5, May, 2011 Next Meeting – May 17th, 2011 at 6:00 PM ~ Annual Dinner Meeting at the Hilton Wilmington/Christiana ~ See Pages 4 & 5 for full Details on this Event Celebrating the DAS Amateur Astronomer of the Year FROM THE PRESIDENT ! Bill Hanagan To start off, I’d like to thank Bill McKibben for his LAST CALL for the presentation at the April meeting on the Ancient Astronomy of Machu Picchu and Greg Lee for his presentation on DAS Dinner Meeting “What’s Up in the Sky”. If you missed the April meeting, you also missed my presentation on the sizing, positioning, and th surface quality of Newtonian secondary mirrors. Tuesday, May 17 Our May meeting is the annual “dinner” meeting of the DAS and it will be held on Tuesday, May 17 at the Christiana You’ll need to call Treasurer McKibben Hilton, the same location as last year. Social hour begins at at this late hour for Reservations. 6:00 P.M. followed by dinner at 7:00 P.M. After dinner, we’ll view a short video of time lapse astrophotos followed by the Andrew K. Johnston presentation of the Amateur Astronomer of the Year Award. We’ll conclude the evening with a talk titled “Navigating across from the the Solar System” by Mr. Andrew K. Johnston from the National Smithsonian Air and Space Museum. Mr. Johnston is the co-author of the “Smithsonian Atlas of Space Exploration” and his talk will give National Air & us a look at the history and technology of solar system explora- tion. -
Io Volcano Observer
EPSC Abstracts Vol. 13, EPSC-DPS2019-996-1, 2019 EPSC-DPS Joint Meeting 2019 c Author(s) 2019. CC Attribution 4.0 license. Follow the Heat: Io Volcano Observer A. S. McEwen1, E. Turtle2, L. Kestay3, K. Khurana4, J. Westlake2, P. Wurz5, J. Helbert6, R. Park7, M. Bland3, D. Breuer6, L. Carter1, A. G. Davies7, C. W. Hamilton1, S. Horst8, X. Jia9, L. Jozwiak2, J. T. Keane10, K. de Kleer10, V. Lainey7, K. Mandt2, I. Matsuyama1, O. Mousis11, F. Nimmo12, C. Paranicas2, J. Perry1, A. Pommier13, J. Radebaugh14, J. Spencer15, S. Sutton1, N. Thomas5, A. Vorburger5 1LPL, University of Arizona, 2JHU APL, 3USGS, 4UCLA, 5UBE, 6DLR, 7JPL, 8JHU, 9U.Michigan, 10Caltech, 11AMU, 12UCSC, 13UCSD, 14BYU, 15SwRI. Abstract A promising avenue to address these questions is a new spacecraft mission making multiple close flybys The Io Volcano Observer (IVO) Discovery mission of Io, combined with research and analysis motivated proposal [1] has been re-focused in 2019 towards by the mission. IVO will address all of these understanding tidal heating as a fundamental questions, while still within the constraints of NASA planetary process. To “Follow the Heat”, IVO will Discovery program. IVO will characterize volcanic determine how heat is generated in Io’s interior, processes (Q1); test interior models via a set of transported to the surface, and how heat and mass are geophysical measurements (coupled with laboratory lost to space. experiments and theory; Q2 and Q3); measure the total heat flow and orbital evolution of Io (Q4); and 1. Tidal Heating analyze mass loss processes (Q5). No new technologies are required for this mission, which Tidal heating is key to the evolution and habitability leverages advances in radiation design and solar of many worlds across our Solar System and beyond. -
THE IO VOLCANO OBSERVER (IVO) for DISCOVERY 2015. A. S. Mcewen1, E. P. Turtle2, and the IVO Team*, 1LPL, University of Arizona, Tucson, AZ USA
46th Lunar and Planetary Science Conference (2015) 1627.pdf THE IO VOLCANO OBSERVER (IVO) FOR DISCOVERY 2015. A. S. McEwen1, E. P. Turtle2, and the IVO team*, 1LPL, University of Arizona, Tucson, AZ USA. 2JHU/APL, Laurel, MD USA. Introduction: IVO was first proposed as a NASA Discovery mission in 2010, powered by the Advanced Sterling Radioisotope Generators (ASRGs) to provide a compact spacecraft that points and settles quickly [1]. The 2015 IVO uses advanced lightweight solar arrays and a 1-dimensional pivot to achieve similar observing flexibility during a set of fast (~18 km/s) flybys of Io. The John Hopkins University Applied Physics Lab (APL) leads mission implementation, with heritage from MESSENGER, New Horizons, and the Van Allen Probes. Io, one of four large Galilean moons of Jupiter, is the most geologically active body in the Solar System. The enormous volcanic eruptions, active tectonics, and high heat flow are like those of ancient terrestrial planets and present-day extrasolar planets. IVO uses Figure 1. IVO will distinguish between two basic tidal heating advanced solar array technology capable of providing models, which predict different latitudinal variations in heat ample power even at Jovian distances of 5.5 AU. The flux and volcanic activity. Colors indicate heating rate and hazards of Jupiter’s intense radiation environment temperature. Higher eruption rates lead to more advective are mitigated by a comprehensive approach (mission cooling and thicker solid lids [2]. design, parts selection, shielding). IVO will generate Table 2: IVO Science Experiments spectacular visual data products for public outreach. Experiment Characteristics Narrow-Angle 5 µrad/pixel, 2k × 2k CMOS detector, color imaging Science Objectives: All science objectives from Camera (NAC) (filter wheel + color stripes over detector) in 12 bands from 300 to 1100 nm, framing images for movies of the Io Observer New Frontiers concept recommended dynamic processes and geodesy. -
Comet Hopper Moves to 'Final Round' in NASA Selection Process 12 May 2011
Comet Hopper moves to 'final round' in NASA selection process 12 May 2011 the team include Deputy PI Michael A'Hearn, who led NASA's Deep Impact and EPOXI comet missions. The Comet Hopper mission would be managed by NASA Goddard Space Flight Center in Greenbelt, Md. Other partners include Lockheed Martin, KinetX, the Johns Hopkins University Applied Physics Laboratory, University of Bern, Jet Propulsion Laboratory and Discovery Communications. "We've had some amazing cometary flybys but they have given us only snapshots of one point in time of what a comet is like," said Sunshine. "Comets are exciting because they are dynamic, changing throughout their orbits. With this new mission, we will start out with a comet that is in the cold, outer reaches of its orbit and watch its activity come alive as it moves closer and closer to the sun." The Comet Hopper mission would study the evolution of 46P/Wirtanen by landing on the comet Credit: NASA/GSFC/University of Maryland multiple times and observing its changes as it interacts with the sun. Comet Hopper would observe the comet by making detailed in situ measurements from various locations on the (PhysOrg.com) -- A University of Maryland-led surface and in the innermost coma as the comet mission proposal know as Comet Hopper has been moves through its orbit. The innermost coma is the chosen to compete for final selection as a new atmosphere of the comet just off the surface of the planetary mission in NASA's Discovery Program. nucleus where outgassing and jets originate. "We The team will receive $3 million to further develop would extensively explore the surface of a comet, its mission proposal concept. -
NASA's FY14 Management and Performance, Addressing
Management and Performance ADDRESSING MANAGEMENT CHALLENGES AND IMPROVING PERFORMANCE An essential phase in NASA’s performance management cycle is to evaluate Agency performance against its plans. Managers assess performance throughout the year and pay particular attention when NASA’s performance falls short of its goals. They seek explanations, develop plans to improve performance, and track results for as long as necessary. NASA leadership also evaluates trends across the portfolio of programs and over longer periods of time to identify and resolve persistent issues. The Government Performance and Results Act Modernization Act of 2010 reinforced NASA’s approach to performance management by introducing requirements for unmet program performance. Specifically, Congress required agencies and the Office of Management and Budget to provide analysis of trends in unmet performance targets. When a NASA program does not meet its commitment as stated in the annual performance plan, responsible program officials must explain the performance shortfall and provide an improvement plan for correcting the issue. This section provides the explanations and performance improvement plans for any unmet performance measures in FY 2012 and, where applicable, the link to the prior year’s performance. For FY 2012, NASA discusses performance trends in the following categories: • Cost and Schedule Performance, • Commercial Spaceflight Development, and • Diversity. To provide better performance improvement plans, NASA assesses the explanations for unmet performance and looks for trends in root causes. The results of this root cause analysis inform senior management when crosscutting corrective actions are warranted. In addition, NASA uses information on management and performance challenges, as identified by NASA’s Office of Inspector General (OIG) and the Government Accountability Office (GAO), to better understand root causes and to guide setting improvement plans. -
Planetary Science Update & Perspectives on Venus Exploration
Planetary Science Update & Perspectives on Venus Exploration Presentation at VEXAG James L. Green Director, Planetary Science Division May 6, 2008 1 Outline • FY09 Presidents Budget • Venus exploration opportunities: – Plans for next New Frontiers – Plans for next Discovery – Plans for SALMON – R&A opportunities 2 BUDGET BY SCIENCE THEME 3 Planetary Division 4 Planetary Division 5 What Changed, What’s the Same What Changed: • Initiated an Outer Planets Flagship (OPF) study activity joint with ESA/JAXA. • Lunar Science Research augmented to include a series of small lunar spacecraft. • Augments and enhances R&A to return more results from Planetary missions. • Discovery Program: Includes the recently selected MoOs (EPOXI and Stardust-NExT), adds Aspera-3 2nd extension (ESA/Mars Express), and selected GRAIL. • Preserves critical ISP work FY08 thru FY10, but deletes outyear activities in favor of more critical R&A and RPS enhancements. • Completes the Advanced Stirling RPS development and prepares for flight demonstration. • Mars Scout 2011 delayed to 2013 due to conflict of interest discovered during proposal evaluation. • Direction to the Mars Program to study Mars Sample Return (MSR) as a next decade goal • Expands US participation on the ESA/ExoMars mission by funding the potential selection of BOTH candidate U.S. instruments and EDL support. What’s the Same: • Discovery Program: MESSENGER, Dawn, Mars Express/Aspera-3, Chandraayn/MMM • New Frontiers Program: Juno and New Horizons • Mars Program: Odyssey, MER, MRO, Phoenix, MSL • Research -
Headquarters Update
Outline Planetary Science Division Update • Administration • Upcoming Opportunities & Selections • National Academy Studies Presentation at the OPAG • Mars Science Laboratory • Mission Status and Plans James L. Green Director, Planetary Science Division November 6, 2008 1 2 Administration • Moving on: – John Rummel (Hq CS) - Astrobiology – Dennon Clardy (MSFC detailee) - Assistant for Flight Program – Kelly Snook (GSFC detailee) - Lunar Science Recent Selections, – Carlos Liceaga (LaRC detailee) - SALMON AO • Recent Personnel Additions: Opportunities & Studies – Mary Voytek (USGS detailee) - Astrobiology – Tibor Kremic (GRC detailee) - Assistant for Flight Program – Jennifer Heldmann (ARC detailee) - Lunar Science • Government transition: – Congress may pass budget before end of year – NASA preparing for the transition 3 4 Mars Scout-13 Selection Astrobiology Selections CAN #5 - 10 selections with a 27% success rate – 5 new 5 returning teams but 2 with new PIs • Mark Allen, JPL, Titan as a prebiotic chemical system • Ariel Anbar, ASU, Follow the elements • George Cody, Carnegie Inst. Wash., Astrobiology Pathways • David DesMarais, ARC, Early habitable environments • Chris House, PSU, Signatures of life • Isik Kanik, JPL, Icy Worlds • Karen Meech, UH, Water and its relation to life • Mike Mumma, GSFC, Organics in planetary systems Mars Atmosphere & Volatile EvolutioN • Doug Whittet, RPI, Setting the stage for life • Loren Williams, GIT, Ribosome adaption & evolution 5 6 Upcoming 2008 Opportunities Academy Studies • Congress: NASA will -
PAC March 9 10 2020 Report
NASA ADVISORY COUNCIL PLANETARY SCIENCE ADVISORY COMMITTEE March 9-10, 2020 NASA Headquarters Washington, DC MEETING REPORT _____________________________________________________________ Anne Verbiscer, Chair ____________________________________________________________ Stephen Rinehart, Executive Secretary Table of Contents Opening and Announcements, Introductions 3 PSD Update and Status 3 PSD R&A Status 5 Planetary Protection 7 Discussion 8 Mars Exploration Program 8 Lunar Exploration Program 9 PDCO 11 Planetary Data System 12 PDS at Headquarters 13 Findings and Discussion 13 General Comments 13 Exoplanets in Our Backyard 14 AP Assets for Solar System Observations 15 Solar System Science with JWST 16 Mercury Group 17 VEXAG 17 SBAG 18 OPAG 19 MEPAG 19 MAPSIT 20 LEAG 21 CAPTEM 21 Discussion 22 Findings and Recommendations Discussion 23 Appendix A- Attendees Appendix B- Membership roster Appendix C- Agenda Appendix D- Presentations Prepared by Joan M. Zimmermann Zantech, Inc. 2 Opening, Announcements, Around the Table Identification Executive Secretary of the Planetary Science Advisory Committee (PAC), Dr. Stephen Rinehart, opened the meeting and made administrative announcements. PAC Chair, Dr. Anne Verbiscer, welcomed everyone to the virtual meeting. Announcements were made around the table and on Webex. PSD Status Report Dr. Lori Glaze, Director of the Planetary Science Division, gave a status report. First addressing the President’s Budget Request (PBR) for Fiscal Year 2021 (FY21) for the Science Mission Directorate (SMD), Dr. Glaze noted that it was one of the strongest science budgets in NASA history, representing a 12% increase over the enacted FY20 budget. The total PBR keeps NASA on track to land on the Moon by 2024; and to help prepare for human exploration at Mars. -
Versatile Stirling Technology for Radioisotope and Fission Power Systems
VERSATILE STIRLING TECHNOLOGY FOR RADIOISOTOPE AND FISSION POWER SYSTEMS. L. S. Mason1, J. F. Zakrajsek1, and D.T. Palac1, 1NASA Glenn Research Center, 21000 Brookpark Road, Cleveland OH 44135, [email protected], [email protected], [email protected]. Introduction: Free-piston Stirling technology has The FPS Stirling development has been sponsored been under development at NASA Glenn Research by the Space Technology Mission Directorate (STMD) Center (GRC) since the 1970s. The current focus is on under the Nuclear Systems Project. A 12 kWe AC 100-watt class convertor technology for Radioisotope Power Conversion Unit (PCU) with two dual opposed Power Systems (RPS) and multi-kilowatt convertor and thermodynamically-coupled Stirling engines, technology for Fission Power Systems (FPS). shown in Fig. 3, is in the final stages of development at The NASA Science Mission Directorate (SMD) Sunpower with delivery to GRC expected in Spring has sponsored the RPS Stirling development. The 2014 [3]. technology is at a high Technology Readiness Level (TRL) based on the Advanced Stirling Convertor (ASC) from Sunpower Inc. The ASC, shown in Fig. 1, is designed to produce 80 We AC at 32% thermal-to- electric efficiency. The high efficiency allows a four- fold reduction in the amount of Pu-238 fuel as com- pared to Multi-Mission Radioisotope Thermoelectric Generator (MMRTG) technology. Figure 3. 12 kWe PCU The PCU will be integrated into a fission Technol- ogy Demonstration Unit (TDU) that includes an elec- trically-heated reactor simulator with a pumped sodi- um-potassium (NaK) heat transfer loop that couples directly to the Stirlings [4].