Power Subsystem Approach for the Europa Mission

Total Page:16

File Type:pdf, Size:1020Kb

Power Subsystem Approach for the Europa Mission E3S Web of Conferences 16, 13004 (2017) DOI: 10.1051/ e3sconf/20171613004 ESPC 2016 POWER SUBSYSTEM APPROACH FOR THE EUROPA MISSION Antonio Ulloa-Severino(1), Gregory A. Carr(1), Douglas J. Clark(1), Sonny M. Orellana(1), Roxanne Arellano(1), Marshall C. Smart(1), Ratnakumar V. Bugga(1), Andreea Boca(1), and Stephen F. Dawson(1) (1)Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA 91109 USA, Email: [email protected] ABSTRACT implementation of the spacecraft and instrument hardware. The mission design team is expending great NASA is planning to launch a spacecraft on a mission to efforts to minimize the amount of total dose radiation the Jovian moon Europa, in order to conduct a detailed the flight system would accumulate and maximize reconnaissance and investigation of its habitability. The science data return. spacecraft would orbit Jupiter and perform a detailed science investigation of Europa, utilizing a number of The NASA-selected instruments intend to characterize science instruments including an ice-penetrating radar to Europa by producing high-resolution images and determine the icy shell thickness and presence of surface composition maps. An ice-penetrating radar subsurface oceans. The spacecraft would be exposed to intends to determine the crust thickness, and a harsh radiation and extreme temperature environments. magnetometer would measure the magnetic field To meet mission objectives, the spacecraft power strength and direction to further help scientists subsystem is being architected and designed to operate determine ocean depth and salinity. A thermal efficiently, and with a high degree of reliability. instrument would be used to identify warmer water that could have erupted through the crust, while other 1. EUROPA MISSION OVERVIEW instruments would help detect water and particles in the The planned Europa mission’s main focus is to execute moon’s atmosphere. an in-depth science investigation of Jupiter’s icy moon Europa shown in Fig. 1 [1]. The moon has shown The nine NASA-selected instruments that would be evidence of a liquid water ocean underneath the used for the Europa mission are the following [2]: unknown thickness of icy surface. The ocean could provide an environment suitable for life due its 1) Plasma Instrument for Magnetic Sounding interaction with a volcanic seafloor. (PIMS) 2) Interior Characterization of Europa using Magnetometry (ICEMAG) 3) Mapping Imaging Spectrometer for Europa (MISE) 4) Europa Imaging System (EIS) 5) Radar for Europa Assessment and Sounding: Ocean to Near-surface (REASON) 6) Europa Thermal Emission Imaging System (E- THEMIS) 7) Mass Spectrometer for Planetary Exploration/Europa (MASPEX) 8) Ultraviolet Spectrograph/Europa (UVS) 9) Surface Dust Mass Analyser (SUDA) 2. POWER SUBSYSTEM ARCHITECTURE The power subsystem architecture design approach involves implementing a robust single-fault tolerant Figure 1: Cutaway diagram of Europa's interior. design with small fault containment regions, based on a Artwork credit: Michael Carroll similar approach used for the Cassini mission to Saturn. The design has focused on three main areas: the baseline The combination of harsh radiation, low temperature solar arrays, power management electronics, and (30 K) environments, and distance from the sun (5 AU batteries as shown in Fig 2. to 5.5 AU) creates challenges on design and © The Authors, published by EDP Sciences. This is an open access article distributed under the terms of the Creative Commons Attribution License 4.0 (http://creativecommons.org/licenses/by/4.0/). E3S Web of Conferences 16, 13004 (2017) DOI: 10.1051/ e3sconf/20171613004 ESPC 2016 Power Control and Distribution Assembly controlled via commands. Power control uses an N+K Power Bus architecture for the number of power stages, where N is Solar Array Safe/Arm number required for the mission and K is the number of Plug Battery Prop Bus A & B additional stages provided for redundancy, as shown in Plug Array & Battery Interface Slice Battery Deployment Fig. 3. The command and telemetry interface to the Bus A & B power management electronics is block redundant. Umbilical Switched loads Engineering Bus A/B Pulsed Regulation Power Bus RSB A RSB A/B Propulsion Module loads Stage FCR 1 SA Pwr Controller A (Incl. xRTI) Electronics A/B Voltage Control N Local Ctrl Power Bus Power Bus RSB B Power Bus Volt Controller B Control FCR A Ctrl Volt A Regulation Ctrl Volt B Stage 1 Power Switch Switched power Engineering Slice 1 Power Bus Communication Regulated Power Switch Control A Slice 2 Bus A Regulation Power Bus Stage FCR N SA Pwr Power Bus Power Switch Slice 3 Power Bus Voltage Control N Local Ctrl Power Bus Power Power Switch Control FCR B Volt Slice 4 Ctrl Volt A Regulation Distribution Stage N Function Power Switch Engineering Ctrl Volt B Slice 5 Power Bus Communication Control B Power Switch Bus B Regulation Slice 6 Stage FCR N+1 SA Pwr Voltage Control 1 Switched power Local Ctrl Power Bus Volt Regulation Figure 2. Baseline Power Subsystem Architecture. Legend: Ctrl Volt A Stage Ctrl voltage CMD Ctrl Volt B N+1 Power Voltage setpoint Functional FCR 2.1 Power Source Region Figure 3. Power Regulation Function FCRs. The solar array substrates, materials, and components are being tested under the relevant environmental The power distribution electronics are designed conditions to characterize their performance and with internal housekeeping power that provide reliability in the Jovian environment. The primary independent functional slices that can be utilized challenges for photovoltaic operation at Jupiter are the throughout the spacecraft. The power distribution extremely high radiation from both electrons and function incorporates a resettable circuit breaker power protons, extremely low temperatures (30 K), and low- switch to separate the fault containment region for each irradiance low-temperature (LILT) solar cell load interface. The power switch is part of the load fault performance. Also, mission design requirements dictate containment region as shown in Fig. 4 and is fail-safe that the solar array mass and size constraints are of off. Redundant functions on the spacecraft are powered critical importance. by another power switch in a separate fault containment region. Each power switch has a block redundant The solar array string design and layout has been command and telemetry interface to maintain the load- adjusted to match the capability of the radiation-hard level fault containment region. electronics. The number of cells in series was set by the Regulated PWR Bus topology of the power management electronics to Power Distribution CMD A Regulated Housekeeping Power Switch FCR deliver the most power at the end of the mission in the Power A PWR Bus most severe environment. The challenge was to obtain Power Power Switch S/C Load 1 Serial Switch Distribution Channel enough voltage for the power management electronics Bus A Drivers CMD A early in the mission, during the inner solar system Power Switch S/C Load 2 cruise, and then still produce efficient power at the end Power Distribution CMD B Channel Power of mission. The power management electronics was Serial Switch Distribution Power Bus B Drivers designed to deliver close to the maximum power CMD B Switch S/C Load X Channel available from the solar array at the end of mission in a Housekeeping Power B robust fault-tolerant architecture. The power management electronics has two primary functions, Regulated PWR Bus Legend: power control and power distribution. CMD Functional Regulated PWR Bus FCR Region Housekeeping PWR Driver 2.2 Power Electronics Figure 4. Power Distribution FCRs. The baseline power control design operates near the 2.3 Energy Storage maximum power point of the solar array throughout the Jovian tour based on solar cell telemetry and modelling. The preliminary battery architecture uses high specific Power control electronics can charge the battery after a energy small 18650-size lithium-ion cells, to capitalize flyby operating near the I-V (current-voltage) curve on their internal safety functions, high capacity, and maximum power point without collapsing the solar excellent cell-to-cell reproducibility. Utilizing such a array voltage. The design is single fault tolerant. Power format is advantageous, since the approach does not bus voltage and solar array voltage set points are 2 E3S Web of Conferences 16, 13004 (2017) DOI: 10.1051/ e3sconf/20171613004 ESPC 2016 require individual cell monitoring and balancing • determination of required power subsystem circuitry. Each string of battery cells is a separate capabilities, and electrical fault containment region. Each battery cell • design of interfaces, both within and external to the string power subsystem. 3. POWER SUBSYSTEM SYSTEM The set of power subsystem requirements is the formal ENGINEERING agreement between the power subsystem domain and 3.1 System Engineering Context, Requirements and the flight system domain. Requirements for the power Verification and Validation (V&V) subsystem are being developed and maintained in the Rational Dynamic Object Requirements System System engineering on the Europa Project is divided (DOORS) Next Generation web-based software tool. into the following domains: • Project system engineering, which is concerned Later, as the Project and subsystems proceed into with everything from securing funding to delivering implementation phases, the attention of power on the project’s stated science goals and subsystem engineers would shift into V&V activities. requirements. Verification involves the formal check that the delivered • Mission system engineering, which is concerned power subsystem products meet all their requirements. with the launched spacecraft, launch vehicle, flight- Validation is a check to ensure that the power subsystem to-ground communications networks, and the pre- would meet the project and mission objectives, when and post-launch operations of the Europa spacecraft operated in the context of the other subsystems, the and payload. flight system, and the mission system. • Flight system engineering, which is concerned with the Europa spacecraft and payload.
Recommended publications
  • An Impacting Descent Probe for Europa and the Other Galilean Moons of Jupiter
    An Impacting Descent Probe for Europa and the other Galilean Moons of Jupiter P. Wurz1,*, D. Lasi1, N. Thomas1, D. Piazza1, A. Galli1, M. Jutzi1, S. Barabash2, M. Wieser2, W. Magnes3, H. Lammer3, U. Auster4, L.I. Gurvits5,6, and W. Hajdas7 1) Physikalisches Institut, University of Bern, Bern, Switzerland, 2) Swedish Institute of Space Physics, Kiruna, Sweden, 3) Space Research Institute, Austrian Academy of Sciences, Graz, Austria, 4) Institut f. Geophysik u. Extraterrestrische Physik, Technische Universität, Braunschweig, Germany, 5) Joint Institute for VLBI ERIC, Dwingelo, The Netherlands, 6) Department of Astrodynamics and Space Missions, Delft University of Technology, The Netherlands 7) Paul Scherrer Institute, Villigen, Switzerland. *) Corresponding author, [email protected], Tel.: +41 31 631 44 26, FAX: +41 31 631 44 05 1 Abstract We present a study of an impacting descent probe that increases the science return of spacecraft orbiting or passing an atmosphere-less planetary bodies of the solar system, such as the Galilean moons of Jupiter. The descent probe is a carry-on small spacecraft (< 100 kg), to be deployed by the mother spacecraft, that brings itself onto a collisional trajectory with the targeted planetary body in a simple manner. A possible science payload includes instruments for surface imaging, characterisation of the neutral exosphere, and magnetic field and plasma measurement near the target body down to very low-altitudes (~1 km), during the probe’s fast (~km/s) descent to the surface until impact. The science goals and the concept of operation are discussed with particular reference to Europa, including options for flying through water plumes and after-impact retrieval of very-low altitude science data.
    [Show full text]
  • PDS Mission Interface for Europa Mission Status of Planning for Data Archiving
    PDS Mission Interface for Europa Mission Status of Planning for Data Archiving CARTOGRAPHY AND IMAGING SCIENCES (“Imaging”) NODE PDS Lead Node Lisa Gaddis (USGS, Astrogeology) August 2016 Overview Common goals PDS4 Archiving roles, responsibilities EM archiving deliverables Data and Archive Working Group (DAWG) Archiving assignments Archiving activities to date Archiving schedule Current archiving activities Where we are now August 2016 2 Common Goals The PDS and Europa Mission (EM) will work together to ensure that we Organize, document and format EM digital planetary data in a standardized manner Collect complete, well-documented, peer-reviewed planetary data into archives Make planetary data available and useful to the science community ○ Provide online data delivery tools & services Ensure the long-term preservation and usability of the data August 2016 3 PDS4 The new PDS, an integrated data system to improve access ○ Required for all missions (e.g., used by LADEE, MAVEN) A re-architected, modern, online data system ○ Data are organized into bundles Includes all data for a particular instrument (e.g., PDF/A documents) ○ Bundles have collections Grouped files with a similar origin (e.g., Document Collection) Improves efficiency of ingestion and distribution of data ○ Uses Extensible Markup Language (XML) and standard data format templates ○ Self-consistent information model & software system ○ Information for Data Providers https://pds.nasa.gov/pds4/about ○ PDS4 Concepts Document https://pds.nasa.gov/pds4/doc/concepts/Concepts_150909.pdf
    [Show full text]
  • Using the Galileo Solid-State Imaging Instrument As a Sensor of Jovian
    Using the Galileo Solid-State Imaging Instrument as a Sensor of Jovian Energetic Electrons Ashley Carlton1, Maria de Soria-Santacruz Pich2, Insoo Jun2, Wousik Kim2, and Kerri Cahoy1 1Massachusetts Institute of Technology, Cambridge, 02139, USA (e-mail: [email protected]) 2Jet Propulsion Laboratory, California Institute of Technology, Pasadena, 91109, USA respectively. For the most part, information about the Jovian I. INTRODUCTION environment comes from the Galileo spacecraft Energetic Harsh radiation in the form of ionized, highly energetic Particle Detector (EPD) [Williams et al., 1992] (in Jovian particles is part of the space environment and can affect orbit from December 1995 to September 2003), which had a spacecraft. These particles not only sweep through the solar nearly equatorial orbit. Juno, a NASA spacecraft that entered system in the solar wind and flares and are ejected from Jovian orbit in July 2016, and Europa Clipper, a NASA galactic and extra-galactic supernovae, but also are trapped as mission planned for the 2020s, do not carry instruments belts in planetary magnetic fields. Jupiter’s magnetosphere is capable of measuring high-energy (>1 MeV) electrons. Juno is the largest and strongest of a planet in the solar system. in a polar orbit; Europa Clipper is planned to be in a highly Similar to Earth, Jupiter is roughly a magnetic dipole with a elliptical Jovian orbit, flying-by Jupiter’s moon, Europa, in tilt of ~11° [Khurana et al., 2004]. Jupiter’s magnetic field each orbit. strength is an order of magnitude larger than Earth, and its We develop a technique to extract the high-energy magnetic moment is roughly 18,000 times larger [Bagenal et electron environment using scientific imager data.
    [Show full text]
  • Europa Clipper Mission: Preliminary Design Report
    Europa Clipper Mission: Preliminary Design Report Todd Bayer, Molly Bittner, Brent Buffington, Karen Kirby, Nori Laslo Gregory Dubos, Eric Ferguson, Ian Harris, Johns Hopkins University Applied Physics Maddalena Jackson, Gene Lee, Kari Lewis, Jason Laboratory 11100 Johns Hopkins Road Laurel, Kastner, Ron Morillo, Ramiro Perez, Mana MD 20723-6099 Salami, Joel Signorelli, Oleg Sindiy, Brett Smith, [email protected] Melissa Soriano Jet Propulsion Laboratory California Institute of Technology 4800 Oak Grove Dr. Pasadena, CA 91109 818-354-4605 [email protected] Abstract—Europa, the fourth largest moon of Jupiter, is 1. INTRODUCTION believed to be one of the best places in the solar system to look for extant life beyond Earth. Exploring Europa to investigate its Europa’s subsurface ocean is a particularly intriguing target habitability is the goal of the Europa Clipper mission. for scientific exploration and the hunt for life beyond Earth. The 2011 Planetary Decadal Survey, Vision and Voyages, The Europa Clipper mission envisions sending a flight system, states: “Because of this ocean’s potential suitability for life, consisting of a spacecraft equipped with a payload of NASA- Europa is one of the most important targets in all of planetary selected scientific instruments, to execute numerous flybys of Europa while in Jupiter orbit. A key challenge is that the flight science” [1]. Investigation of Europa’s habitability is system must survive and operate in the intense Jovian radiation intimately tied to understanding the three “ingredients” for environment, which is especially harsh at Europa. life: liquid water, chemistry, and energy. The Europa Clipper mission would investigate these ingredients by The spacecraft is planned for launch no earlier than June 2023, comprehensively exploring Europa’s ice shell and liquid from Kennedy Space Center, Florida, USA, on a NASA supplied ocean interface, surface geology and surface composition to launch vehicle.
    [Show full text]
  • 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,
    [Show full text]
  • IAC-17-F1.2.3 Page 1 of 23 IAC-17-C1.7.8 EVOLUTION OF
    68th International Astronautical Congress (IAC), Adelaide, Australia, 25-29 September 2017. Copyright © 2017 California Institute of Technology. Government sponsorship acknowledged. IAC-17-C1.7.8 EVOLUTION OF TRAJECTORY DESIGN REQUIREMENTS ON NASA’S PLANNED EUROPA CLIPPER MISSION Brent Buffingtona*, Try Lamb, Stefano Campagnolab, Jan Ludwinskic, Eric Fergusonc, Ben Bradleyc a Europa Clipper Mission Design Manager, Jet Propulsion Laboratory / California Institute of Technology 4800 Oak Grove Drive, Pasadena, CA, 91109-8099, [email protected] b Mission Design Engineer, Jet Propulsion Laboratory / California Institute of Technology 4800 Oak Grove Drive, Pasadena, CA, 91109-8099 c Mission Planning Engineer, Jet Propulsion Laboratory / California Institute of Technology 4800 Oak Grove Drive, Pasadena, CA, 91109-8099 * Corresponding Author Abstract Europa is one of the most scientifically intriguing targets in planetary science due to its potential suitability for extant life. As such, NASA has funded the California Institute of Technology Jet Propulsion Laboratory and the Johns Hopkins University Applied Physics Laboratory to jointly develop the planned Europa Clipper mission—a multiple Europa flyby mission architecture aimed to thoroughly investigate the habitability of Europa and provide reconnaissance data to determine a landing site that maximizes the probability of both a safe landing and high scientific value for a potential future Europa lander. The trajectory design—a major enabling component for this Europa Clipper mission concept—was developed to maximize science from a set of eight model payload instruments determined by a NASA-appointed Europa Science Definition Team (SDT) between 2011-2015. On May 26, 2015, NASA officially selected 10 instruments from 6 different U.S.
    [Show full text]
  • 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.
    [Show full text]
  • Europa Mission Update: Beyond Payload Selection
    Europa Mission Update: Beyond Payload Selection Todd Bayer, Brent Buffington, Jean- Karen Kirby Francois Castet, Maddalena Jackson, Johns Hopkins University Gene Lee, Kari Lewis, Jason Applied Physics Laboratory Kastner, Kathy Schimmels 11100 Johns Hopkins Road Jet Propulsion Laboratory Laurel, MD 20723-6099 California Institute of Technology [email protected] 4800 Oak Grove Dr. Pasadena, CA 91109 818-354-4605 [email protected] Abstract—Europa, the fourth largest moon of Jupiter, is believed 2. MISSION OVERVIEW ................................2 to be one of the best places in the solar system to look for 3. FLIGHT SYSTEM OVERVIEW ..................7 extant life beyond Earth. The 2011 Planetary Decadal Survey, Vision and Voyages, states: “Because of this ocean’s potential 4. FUTURE WORK .................................... 11 suitability for life, Europa is one of the most important targets 5. SUMMARY AND CONCLUSIONS .................... 11 in all of planetary science.” Exploring Europa to investigate its habitability is the goal of the planned Europa Mission. This ACKNOWLEDGMENTS ................................ 11 exploration is intimately tied to understanding the three “ingre- REFERENCES ......................................... 11 dients” for life: liquid water, chemistry, and energy. The Europa BIOGRAPHY .......................................... 11 Mission would investigate these ingredients by comprehensively exploring Europa’s ice shell and liquid ocean interface, surface geology and surface composition to glean insight into the inner workings of this fascinating moon. In addition, a lander mission 1. INTRODUCTION is seen as a possible future step, but current data about the Jo- vian radiation environment and about potential landing site haz- Scientific motivation for studying the habitability of Europa ards and potential safe landing zones is insufficient.
    [Show full text]
  • Europa Mission
    Europa Mission Lisa Gaddis (USGS, Astrogeology) PDS Cartography and Imaging Sciences Node (You can still call us “Imaging” or PDS-IMG or IMG) Feb 5, 2016 Europa Mission Interface Mission Status Instruments PDS Current Status: Node Assignments ○ Identify Lead Node, Instrument Support Nodes Feb 5, 2016 Europa Mission Now called “Europa Multiple Flyby Mission” Europa Clipper Orbiter and a Lander Explores potential for subsurface ocean & habitability on Jupiter’s moon Europa Ice shell and ocean, composition, geology Performs 45 close flybys of Europa from orbit around Jupiter Topographic survey, ice thickness, plumes? 7 to 10 days to transmit data between flybys Solar powered Joint investigation between JPL & APL Nine instruments on orbiter Nanosatellites for plume samples? Lander configuration is TBD Feb 5, 2016 Europa Clipper Orbital Instruments PIMS: Plasma Instrument for Magnetic Sounding PI: Joseph Westlake, APL ICEMAG: Interior Characterization of Europa using Magnetometry PI: Carol Raymond, JPL MISE: Mapping Imaging Spectrometer for Europa PI: Diana Blaney, JPL EIS: Europa Imaging System PI: Elizabeth Turtle, APL REASON: Radar for Europa Assessment and Sounding: Ocean to Near- Surface PI: Donald Blankenship, Univ. Texas E-THEMIS: Europa Thermal Emission Imaging System PI: Philip Christensen, Arizona State Univ. MASPEX: Mass Spectrometer for Planetary Exploration/Europa PI: Jack Waite, Southwest Research Institute UVS: Ultraviolet Spectrograph/Europa PI: Kurt Retherford, SWRI SUDA: Surface Dust Mass
    [Show full text]
  • Space Telescopes and Instrumentation 2018: Optical, Infrared, and Millimeter Wave
    PROCEEDINGS OF SPIE Space Telescopes and Instrumentation 2018: Optical, Infrared, and Millimeter Wave Makenzie Lystrup Howard A. MacEwen Giovanni G. Fazio Editors 10–15 June 2018 Austin, Texas, United States Sponsored by 4D Technology (United States) • Andor Technology, Ltd. (United Kingdom) • Astronomical Consultants & Equipment, Inc. (United States) • Giant Magellan Telescope (Chile) • GPixel, Inc. (China) • Harris Corporation (United States) • Materion Corporation (United States) • Optimax Systems, Inc. (United States) • Princeton Infrared Technologies (United States) • Symétrie (France) Teledyne Technologies, Inc. (United States) • Thirty Meter Telescope (United States) •SPIE Cooperating Organizations European Space Organisation • National Radio Astronomy Observatory (United States) • Science & Technology Facilities Council (United Kingdom) • Canadian Astronomical Society (Canada) Canadian Space Association ASC (Canada) • Royal Astronomical Society (United Kingdom) Association of Universities for Research in Astronomy (United States) • American Astronomical Society (United States) • Australian Astronomical Observatory (Australia) • European Astronomical Society (Switzerland) Published by SPIE Volume 10698 Part One of Three Parts Proceedings of SPIE 0277-786X, V. 10698 SPIE is an international society advancing an interdisciplinary approach to the science and application of light. The papers in this volume were part of the technical conference cited on the cover and title page. Papers were selected and subject to review by the editors and conference program committee. Some conference presentations may not be available for publication. Additional papers and presentation recordings may be available online in the SPIE Digital Library at SPIEDigitalLibrary.org. The papers reflect the work and thoughts of the authors and are published herein as submitted. The publisher is not responsible for the validity of the information or for any outcomes resulting from reliance thereon.
    [Show full text]
  • Blocks Size Frequency Distribution in the Enceladus Tiger Stripes Area: Implications on Their Formative Processes
    universe Article Blocks Size Frequency Distribution in the Enceladus Tiger Stripes Area: Implications on Their Formative Processes Maurizio Pajola 1,* , Alice Lucchetti 1 , Lara Senter 2 and Gabriele Cremonese 1 1 INAF-Astronomical Observatory of Padova, Vicolo dell’Osservatorio 5, 35122 Padova, Italy; [email protected] (A.L.); [email protected] (G.C.) 2 Department of Physics and Astronomy “G. Galilei”, Università di Padova, 35122 Padova, Italy; [email protected] * Correspondence: [email protected] Abstract: We study the size frequency distribution of the blocks located in the deeply fractured, geologically active Enceladus South Polar Terrain with the aim to suggest their formative mechanisms. Through the Cassini ISS images, we identify ~17,000 blocks with sizes ranging from ~25 m to 366 m, and located at different distances from the Damascus, Baghdad and Cairo Sulci. On all counts and for both Damascus and Baghdad cases, the power-law fitting curve has an index that is similar to the one obtained on the deeply fractured, actively sublimating Hathor cliff on comet 67P/Churyumov- Gerasimenko, where several non-dislodged blocks are observed. This suggests that as for 67P, sublimation and surface stresses favor similar fractures development in the Enceladus icy matrix, hence resulting in comparable block disaggregation. A steeper power-law index for Cairo counts may suggest a higher degree of fragmentation, which could be the result of localized, stronger tectonic disruption of lithospheric ice. Eventually, we show that the smallest blocks identified are located Citation: Pajola, M.; Lucchetti, A.; from tens of m to 20–25 km from the Sulci fissures, while the largest blocks are found closer to the Senter, L.; Cremonese, G.
    [Show full text]
  • The Europa Imaging System (EIS): High-Resolution, 3-D Insight Into Europa’S Geology, Ice Shell, and Potential for Current Activity
    EPSC Abstracts Vol. 13, EPSC-DPS2019-832-2, 2019 EPSC-DPS Joint Meeting 2019 c Author(s) 2019. CC Attribution 4.0 license. The Europa Imaging System (EIS): High-Resolution, 3-D Insight into Europa’s Geology, Ice Shell, and Potential for Current Activity E. P. Turtle (1), A. S. McEwen (2), M. Bland (3), G. C. Collins (4), I. J. Daubar (5), C. M. Ernst (1), L. Fletcher (6), C. J. Hansen (7), S. E. Hawkins (1), A. G. Hayes (8), D. Humm (1), T. A. Hurford (9), R. L. Kirk (3), N. Kutsop (8), A. C. Barr Mlinar (7), F. Nimmo (10), G. W. Patterson (1), C. B. Phillips (5), A. Pommerol (11), L. Prockter (12), L. C. Quick (13), E. L. Reynolds (1), K. A. Slack (1), J. M. Soderblom (14), S. Sutton (2), N. Thomas (11), H. Winters (1) (1) Johns Hopkins Applied Physics Laboratory, Laurel, Maryland, USA, (2) Univ. Arizona, Tucson, Arizona, USA, (3) U.S. Geological Survey, Flagstaff, AZ, USA, (4) Wheaton College, Norton, MA, USA, (5) Jet Propulsion Laboratory, Pasadena, CA, USA, (6) Univ. Leicester, Leicester, UK, USA, (7) Planetary Science Institute, Tucson, AZ, USA, (8) Cornell Univ., Ithaca, NY, USA, (9) NASA Goddard Space Flight Center, Greenbelt, MD, USA, (10) Univ. California, Santa Cruz, CA, USA, (11) Univ. Bern, Bern, Switzerland, USA, (12) Lunar and Planetary Institute, Houston, TX, USA, (13) Smithsonian Institution, Washington, DC, USA, (14) Massachusetts Institute of Technology, Cambridge, MA, USA. ([email protected]) Abstract 1. EIS Narrow-angle Camera (NAC) Designed for NASA's Europa Clipper Mission [1–3], The NAC, with a 2.3° x 1.2° field of view (FOV) and EIS combines a narrow-angle camera and a wide- a 10-µrad instantaneous FOV (IFOV), achieves 0.5- angle camera (Fig.
    [Show full text]