Review Article Application Prospect of Fission-Powered Spacecraft in Solar System Exploration Missions
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LISA, the Gravitational Wave Observatory
The ESA Science Programme Cosmic Vision 2015 – 25 Christian Erd Planetary Exploration Studies, Advanced Studies & Technology Preparations Division 04-10-2010 1 ESAESA spacespace sciencescience timelinetimeline JWSTJWST BepiColomboBepiColombo GaiaGaia LISALISA PathfinderPathfinder Proba-2Proba-2 PlanckPlanck HerschelHerschel CoRoTCoRoT HinodeHinode AkariAkari VenusVenus ExpressExpress SuzakuSuzaku RosettaRosetta DoubleDouble StarStar MarsMars ExpressExpress INTEGRALINTEGRAL ClusterCluster XMM-NewtonXMM-Newton CassiniCassini-H-Huygensuygens SOHOSOHO ImplementationImplementation HubbleHubble OperationalOperational 19901990 19941994 19981998 20022002 20062006 20102010 20142014 20182018 20222022 XMM-Newton • X-ray observatory, launched in Dec 1999 • Fully operational (lost 3 out of 44 X-ray CCD early in mission) • No significant loss of performances expected before 2018 • Ranked #1 at last extension review in 2008 (with HST & SOHO) • 320 refereed articles per year, with 38% in the top 10% most cited • Observing time over- subscribed by factor ~8 • 2,400 registered users • Largest X-ray catalogue (263,000 sources) • Best sensitivity in 0.2-12 keV range • Long uninterrupted obs. • Follow-up of SZ clusters 04-10-2010 3 INTEGRAL • γ-ray observatory, launched in Oct 2002 • Imager + Spectrograph (E/ΔE = 500) + X- ray monitor + Optical camera • Coded mask telescope → 12' resolution • 72 hours elliptical orbit → low background • P/L ~ nominal (lost 4 out 19 SPI detectors) • No serious degradation before 2016 • ~ 90 refereed articles per year • Obs -
Exploration of the Jovian System by EJSM (Europa Jupiter System Mission): Origin of Jupiter and Evolution of Satellites
Trans. JSASS Aerospace Tech. Japan Vol. 8, No. ists27, pp. Tk_35-Tk_38, 2010 Topics Exploration of the Jovian System by EJSM (Europa Jupiter System Mission): Origin of Jupiter and Evolution of Satellites 1) 2) 2) 2) 3) By Sho SASAKI , Masaki FUJIMOTO , Takeshi TAKASHIMA , Hajime YANO , Yasumasa KASABA , 4) 4) 2) 2) Yukihiro TAKAHASHI , Jun KIMURA , Tatsuaki OKADA , Yasuhiro KAWAKATSU , 2) 2) 2) 2) 2) Yuichi TSUDA , Jun-ichiro KAWAGUCHI , Ryu FUNASE , Osamu MORI , Mutsuko MORIMOTO , 5) 6) 7) Masahiro IKOMA , Takeshi NAGANUMA , Atsushi YAMAJI , 8) 9) Hauke HUSSMANN , Kei KURITA and JUPITER WORKING GROUP 1)National Astronomical Observatory of Japan, Oshu, Japan 2)The Institute of Space and Astronautical Science, JAXA, Sagamihara, Japan 3)Tohoku University, Sendai, Japan 4)Hokkaido University, Sapporo, Japan 5)Tokyo Institute of Technology, Tokyo, Japan 6)Hiroshima University, Higashi-Hiroshima, Japan 7)Kyoto University, Kyoto, Japan 8)German Aerospace Center, Berlin, Germany 9)Earthquake Research Institute, The University of Tokyo, Tokyo, Japan (Received July 16th, 2009) EJSM (Europa Jupiter System Mission) is a planned Jovian system mission with three spacecraft aiming at coordinated observations of the Jovian satellites especially Europa and the magnetosphere, atmosphere and interior of Jupiter. It was formerly called "Laplace" mission. In October 2007, it was selected as one of future ESA scientific missions Cosmic Vision (2015-2025). From the beginning, Japanese group is participating in the discussion process of the mission. JAXA will take a role on the magnetosphere spinner JMO (Jupiter Magnetosphere Orbiter). On the other hand, ESA will take charge of JGO (Jupiter Ganymede Orbiter) and NASA will be responsible for JEO (Jupiter Europa Orbiter). -
From the Moon to the Moons: Encedalus, Ganymede and Europa
Journal of Cosmology, 2010, Vol 5, pages xxx In PRESS Cosmology, January 13, 2010 From the Moon to the Moons: Encedalus, Ganymede and Europa. The Search for Life and Reliable Biomarkers J. Chela-Flores, Ph.D., The Abdus Salam ICTP, Strada Costiera 11, 34014 Trieste, Italia, and Instituto de Estudios Avanzados, IDEA, Caracas 1015A, República Bolivariana de Venezuela Abstract The recent renewal of interest in exploring the Moon has led to further novel possibilities for the exploration of the Solar System. It is in the outer Solar System where the biggest challenges await our efforts, both in the development of instrumentation and in the clarification of the biosignatures that should be clear indications of life, as opposed to non-life signals. We argue that in the present-day larger scope of cosmology we can undertake one of the most important missions of the space sciences within our own solar system, namely the search for and discovery of a second genesis. This may be accomplished by landing on Europa's surface. We conclude that the implementation of penetrators in future exploration of the outer solar system is worthy of all the financial and technical support that will be needed, both at the national, as well as at the international level. Keywords: Astrobiology, instrumentation, exploration of the solar system, Europa, Enceladus, Biosignatures 1. Introduction It seems appropriate for a journal devoted to cosmology to encompass the field of astrobiology and to move beyond the "anthropic principle" of quantum physics, the standard astroparticle physics and astrophysics that dominate the field of classical cosmology. -
Title: Exploration of Europa Cynthia B
Title: Exploration of Europa Cynthia B. Phillips1, D. L. Blaney2, R. T. Pappalardo2, H. Hussman3, G. Collins4, R. M. Mastrapa1, J. F. Cooper5, R. Greeley6, J. B. Dalton2, T. A. Hurford5, E. B. Bierhaus7, F. Nimmo8, D. A. Williams6, D. A. Senske2, W. B. McKinnon9 1SETI Institute, 2NASA JPL/Caltech, 3DLR Institute of Planetary Research, Berlin, 4Wheaton College, 5NASA Goddard, 6Arizona State University, 7Lockheed Martin Corporation, 8 Univ. Calif. Santa Cruz, 9Washington University in St. Louis Corresponding Author: Cynthia B. Phillips Carl Sagan Center for the Study of Life in the Universe SETI Institute 515 N. Whisman Rd. Mountain View, CA 94043 [email protected] 650-810-0230 1. Introduction Data from the Galileo spacecraft revealed that Europa's icy surface likely hides a global subsurface ocean with a volume nearly three times that of Earth's oceans. The existence of liquid water in the outer solar system was once thought a remote possibility, but the combination of geological, gravitational, and magnetic field observations and theory make it appear likely that liquid water exists beneath Europa's icy surface. It is now recognized that oceans may exist within many large icy moons and potentially even within icy dwarf planets, but Europa's inferred thin ice shell, potentially active surface- ocean and ocean-silicate mantle exchange, and chemical resources from surface irradiation elevate its priority for astrobiological exploration. A Europa mission is the first step in understanding the potential for icy satellites as abodes for life. Many unanswered questions remain following the Galileo mission. How thick is the ice shell? Is Europa currently geologically active? How does the ocean interact with the ice shell and with the underlying rocky layer? What is the composition of Europa’s surface and ocean? Are there organic or inorganic biosignatures? These questions can only be answered by a new mission to Europa and the Jupiter system. -
Leonid Gurvits JIVE and TU Delft June 3, 2021 ©Cristian Fattinanzi Piter Y Moons Xplorer
Leonid Gurvits JIVE and TU Delft June 3, 2021 ©Cristian Fattinanzi piter y moons xplorer Why a mission to Jupiter? Bits of history Mission challenges Where radio astronomy comes in • ~2000–2005: success of Cassini and Huygens missions (NASA, ESA, ASI) • 2006: Europlanet meeting in Berlin – “thinking aloud” on a Jovian mission • 2008: ESA-NASA jointly exploring a mission to giant planets’ satellites • ESA "Laplace" mission proposal (Blanc et al. 2009) • ESA Titan and Enceladus Mission (TandEM, Coustenis et al., 2009) • NASA Titan Explorer • 2009: two joint (ESA+NASA) concepts selected for further studies: • Europa Jupiter System Mission (EJSM) • Titan Saturn System Mission (TSSM: Coustenis et al., 2009) • 2010: EJSM-Laplace selected, consisting of two spacecraft: • ESA’s Jupiter Ganymede Orbiter (JGO) • NASA’s Jupiter Europa Orbiter (JEO) • 2012: NASA drops off; EJSM-Laplace/JGO becomes JUICE • 2013: JUICE payload selection completed by ESA; JUICE becomes an L-class mission of ESA’s Vision 2015-2025 • 2015: NASA selects Europa Clipper mission (Pappalardo et al., 2013) Voyager 1, 1979 ©NASA HOW DOES IT SEARCH FOR ORIGINS & WORK? LIFE FORMATION HABITABILITY Introduction Overarching questions JUICE JUICE Science Themes • Emergence of habitable worlds around gas giants • Jupiter system as an archetype for gas giants JUICE concept • European-led mission to the Jovian system • First orbiter of an icy moon • JGO/Laplace scenario with two Europa flybys and moderate-inclination phase at Jupiter • Science payload selected in Feb 2013, fully compatible -
Power Systems Design
Power Systems Design • Lecture #17 – October 27, 2020 • Definitions of energy and power • Power generation systems • Energy storage systems • Integrated systems analysis © 2020 David L. Akin - All rights reserved http://spacecraft.ssl.umd.edu U N I V E R S I T Y O F Space Power Systems Design ENAE 483/788D - Principles of Space Systems Design MARYLAND 1 Energy and Power - Not the Same!!! • Energy - the capacity of a physical system to do work (J, N-m, kWhr) • Power - time rate of change of energy (W, N-m/ sec, J/sec) • We are interested in generating power; we store and use energy at a given power level. U N I V E R S I T Y O F Space Power Systems Design ENAE 483/788D - Principles of Space Systems Design MARYLAND 2 Solar Power • Insolation constant = 1394 W/m2 at 1 AU • Varies with inverse square of distance • Power conversion technologies – Photovoltaic – Thermodynamic cycle U N I V E R S I T Y O F Space Power Systems Design ENAE 483/788D - Principles of Space Systems Design MARYLAND 3 Solar Flux at Mars From Mason, Kilopower: Small Fission Power Systems for Mars and Beyond NASA FISO Working Group, Feb. 1, 2017 U N I V E R S I T Y O F Space Power Systems Design ENAE 483/788D - Principles of Space Systems Design MARYLAND 4 Photovoltaic Cell Efficiency U N I V E R S I T Y O F Space Power Systems Design ENAE 483/788D - Principles of Space Systems Design MARYLAND 5 Triple-Junction Photovoltaic Cell U N I V E R S I T Y O F Space Power Systems Design ENAE 483/788D - Principles of Space Systems Design MARYLAND 6 Individual Cell Efficiencies From Wertz, Everett, and Puschell, Space Mission Engineering: The New SMAD Microcosm Press, 2011 U N I V E R S I T Y O F Space Power Systems Design ENAE 483/788D - Principles of Space Systems Design MARYLAND 7 Photovoltaic Array Examples From Fortescue, Swinerd, and Stark, Spacecraft Systems Engineering, 4th ed. -
Securing Japan an Assessment of Japan´S Strategy for Space
Full Report Securing Japan An assessment of Japan´s strategy for space Report: Title: “ESPI Report 74 - Securing Japan - Full Report” Published: July 2020 ISSN: 2218-0931 (print) • 2076-6688 (online) Editor and publisher: European Space Policy Institute (ESPI) Schwarzenbergplatz 6 • 1030 Vienna • Austria Phone: +43 1 718 11 18 -0 E-Mail: [email protected] Website: www.espi.or.at Rights reserved - No part of this report may be reproduced or transmitted in any form or for any purpose without permission from ESPI. Citations and extracts to be published by other means are subject to mentioning “ESPI Report 74 - Securing Japan - Full Report, July 2020. All rights reserved” and sample transmission to ESPI before publishing. ESPI is not responsible for any losses, injury or damage caused to any person or property (including under contract, by negligence, product liability or otherwise) whether they may be direct or indirect, special, incidental or consequential, resulting from the information contained in this publication. Design: copylot.at Cover page picture credit: European Space Agency (ESA) TABLE OF CONTENT 1 INTRODUCTION ............................................................................................................................. 1 1.1 Background and rationales ............................................................................................................. 1 1.2 Objectives of the Study ................................................................................................................... 2 1.3 Methodology -
Cosmic Visions
Declaration of Interest in science instrumentation in response to the Announcement of Opportunity for Europa Jupiter System Mission (EJSM/Laplace) Cosmic Vision Candidate Surface Element Penetrators Proposers: Robert Gowen1, Alan Smith1, Richard Ambrosi6, Olga Prieto Ballesteros16, Simeon Barber2, Dave Barnes11, Chris Braithwaite9, John Bridges6, Patrick Brown5, Phillip Church10, Glyn Collinson1, Andrew Coates1, Gareth Collins5, Ian Crawford3, Veronica Dehant21, Michele Dougherty5, Julian Chela--Flores17, Dominic Fortes7, George Fraser6, Yang Gao4, Manuel Grande11, Andrew Griffiths1, Peter Grindrod7, Leonid Gurvits19, Axel Hagermann2, Toby Hopf5, Hauke Hussmann13, Ralf Jaumann13, Adrian Jones7, Geraint Jones1, Katherine Joy3, Ozgur Karatekin21, Günter Kargl20, Antonella Macagnano14, Anisha Mukherjee5, Peter Muller1, Ernesto Palomba12, Tom Pike5, Bill Proud9, Derek Pullen6, Francois Raulin15, Lutz Richter18, Simon Sheridan2, Mark Sims6, Frank Sohl13, Joshua Snape7, Jon Sykes6, Vincent Tong3, Tim Stevenson6, Lionel Wilson2, Ian Wright2, John Zarnecki2. Affiliations: 1:Mullard Space Science Laboratory, University College London, UK., 2:Planetary and Space Sciences Research Institute, Open University, UK. 3:Birkbeck College, University of London, UK. 4:Surrey Space Centre, Guildford, UK. 5:Imperial College, London, UK. 6:University of Leicester, UK. 7:University College London, UK. 8:University of Lancaster, UK. 9: Cavendish Laboratory, Cambridge, UK. 10:QinetiQ, 11: University of Aberystwyth, UK. 12: Istituto di Fisica dello Spazio Interplanetario-INAF, Roma, Italy. 13: DLR, Berlin, Germany. 14:Institute of Microelectronics and Microsystem -CNR, Roma, Italy. 15: Université Paris, France. 16: Centro de Astrobiologia-INTA-CSIC, España. 17: Abdus Salam International Centre for Theoretical Physics (ICTP), Trieste, Italy. 18: DLR, Bremen, Germany. 19: Joint Institute for VLBI in Europe (JIVE), Dwingeloo, The Netherlands. 20: IAF, Space Research Institute, Graz, Austria. -
EJSM/Jupiter Europa Orbiter Design and Status Karla B
EJSM/Jupiter Europa Orbiter Design and Status Karla B. Clark NASA–JEO Study Lead Jet Propulsion Laboratory California Institute of Technology January 18, 2010 3rd EJSM Instrument Workshop Jupiter Europa Orbiter The NASA Element of the Europa Jupiter System Mission For Discussion and Planning Purposes Only © 2010. All rights reserved. JEO Baseline Mission Overview • Objectives: Jupiter System, Europa • Launch vehicle: Atlas V 551 • Power source: 5 MMRTG • Mission timeline: – Launch: 2018 to 2022, nominally 2020 • Uses 6-year Venus-Earth-Earth gravity assist trajectory – Jovian system tour phase: 30 months • Multiple satellite flybys: 4 Io, 6 Ganymede, 6 Europa, and 9 Callisto – Europa orbital phase: 9 months – End of prime mission: 2029 – Spacecraft final disposition: Europa surface impact • 11 Instruments, including radio science • Optimized for science, cost, and risk • Radiation dose: 2.9 Mrad (behind 100 mils of Al) – Handled using a combination of rad-hard parts and tailored component shielding – Key rad-hard parts are available, with the required heritage – Team is developing and providing design information and approved parts list for prospective suppliers of components, including instruments 1/18/10 For Discussion and Planning Purposes Only 2 Mission Radiation Challenge Launch 2020 (Si))* (Mrad Point Launch Design 2020 Launch Launch 2011 Radiation 1989 * Behind 100 mil (2.5mm) of aluminum Estimated radiation dose levels unprecedented for NASA/ESA missions 1/18/10 For Discussion and Planning Purposes Only 3 JEO Mission Design Overview -
Cassini–Huygens, New Horizons, and the Galileo Orbiter
Outline • Characteristics of Jupiter • Exploration of Jupiter • Data and Images from JUNO spacecraft 2 Characteristics of Jupiter • Orbit Size Around Sun Scientific Notation: 7.7834082 × 108 푘푚 Astronomical Units: 5.2028870 퐴. 푈. • Mass Scientific Notation: 1.8981 × 1027 푘푔 (By Comparison: 317.828 × Earth) • Equatorial Radius Scientific Notation: 6.9911 × 104 푘푚 (By Comparison: 10.9733 × Earth) • Volume Scientific Notation: 1.43128 × 1015 푘푚3 (By Comparison: 1321.337 × Earth) • Density Scientific Notation: 1.3056 × 104 푚/푠 (By Comparison: 0.438 × Earth) 1 day (Jupiter) = 9.92 hours (Earth) 1 year (Jupiter) = 11.86 years (Earth) Number of moons: 69 • Features Ring • Features Strong magnetic field • Features Red spot Exploration of Jupiter Exploration of Jupiter Exploration of Jupiter Mission type: flyby Pioneer 10&11 (先鋒者 10&11 ) Time: Pioneer 10 1972 launch 1973 flyby Pioneer 11 1973 launch 1974 flyby Launched on March 2, 1972, Pioneer 10 was the first spacecraft to pass through the asteroid belt and the first to make direct observations and obtain close-up images of Jupiter. Pioneer 11 was launched on a similar trajectory on April 5, 1973, like Pioneer 10 Pioneer 10 was the first spacecraft to pass through the asteroid belt, considered a spectacular achievement, and then headed toward Jupiter. Pioneer 10 also charted Jupiter’s intense radiation belts, located the planet’s magnetic field, and established that Jupiter is predominantly a liquid planet. Exploration of Jupiter Mission type: orbiter Time: 1989 launch 1995 Orbital insertion Galileo In October 1989, Galileo was launched from the cargo bay of the Space Shuttle Atlantis Galileo didn't have enough fuel to fly directly to Jupiter, but the spacecraft could borrow enough energy from Venus and Earth to make the long journey. -
Los Alamos National Laboratory
Spotlight on National Labs Los Alamos National Laboratory Thom Mason, Director of Los Alamos National Laboratory Alan Carr, Historian of Los Alamos National Laboratory Leslie Sherrill, Group Leader, XTD-IDA (Integrated Design and Assessment) Alexis Trahan, Engineer, NEN-1 (Safeguards Science and Technology) Joetta Goda, Engineer, NEN-2 (Advanced Nuclear Technology) Dave Poston, Chief Reactor Designer, NEN-5 (Systems Design and Analysis) Moderator Nicholas Thompson, Engineer, NEN-2 (Advanced Nuclear Technology) May 6, 2020 ANS Spotlight on National Labs Los Alamos National Laboratory Thom Mason Director of LANL May 6, 2020 LA-UR-20-23309 75+ years serving the nation • In 1943, Los Alamos Laboratory was founded with a single, urgent purpose: build an atomic bomb • The future holds no shortage of national security threats, but there is no shortage of innovative ways to combat those threats • LANL leverages strategic nuclear deterrence to solve challenges to our nation’s security LANL’s national security focus means we are uniquely qualified to tackle big, novel problems such as COVID-19 Los Alamos National Laboratory 4/30/20 | 3 Our 12,866 employees rely on cutting-edge equipment and facilities to solve grand challenges on Earth and in space • 37.8 sq. mile campus (about the size of D.C.) • Flagship research facilities For plutonium, explosives, simulations, chemistry, and more, enabling work that’s impossible anywhere else • Much of our stockpile research is applied to complex challenges in: – Climate change – Vaccine development & epidemic -
Leveraging Commercial Nuclear Reactors to Power Space Exploration
Leveraging Commercial Nuclear Reactors to Power Space Exploration Ben Johnson Brigham Young University, Provo, UT 84602, 970-822-7177, [email protected] This study is aimed at exploring the I. INTRODUCTION adaptation of commercial nuclear reactors as NASA has had a goal of a crewed an alternative to NASA’s current high-power 1 fission reactor systems, particularly with respect mission to Mars since the 1960s . Current to applications on the surface of Mars. The architecture for this manned mission study concludes that while the Kilopower recommends In Situ Resource Utilization architecture is brilliantly poised to provide (IRSU) on the surface of Mars and even the affordable, near-term power in the 1-10 Moon to produce fuel needed for travel to 2 kilowatts electric (kWe) range, the financial and from Mars. The power needed to barrier to higher power scaling of such systems convert the atmosphere and regolith into fuel is significant. This financial barrier adds risk to was initially estimated at 80 kWe, although the development of greater than 10kWe recent studies show that actual power systems and is likely to result in the failure to requirements for a 500 day mission with a successfully scale the technology to higher crew of six on Mars require at least 36 kWe powers for space exploration applications. To of energy.3 Producing consistent electricity investigate the feasibility of commercial reactor on Mars and the Moon is challenging in adaptation, the study first explores which some respects because the long lunar night general reactor concepts would be the most and dust storms on Mars’ surface make solar likely to succeed in space applications.