DOCSLIB.ORG

Keynote Address

Total Page：16

File Type：pdf, Size：1020Kb

Download full-text PDF Read full-text
Keynote Address National Aeronautics and Space Administration Jet Propulsion Laboratory California Institute of Technology Pasadena, California Ground systems in support of space exploration for Ground Systems Architectures Workshop April 3, 2008 Charles Elachi, Director NASA Jet Propulsion Laboratory California Institute of Technology 4/3/08 Elachi GSAW 1 National Aeronautics and Space Administration Ground systems have supported Jet Propulsion Laboratory California Institute of Technology Pasadena, California space exploration for a half century • 1958: Explorer 1 news conference at National Academy with William Pickering, James van Allen, and Werner von Braun National Aeronautics and Where are we now? About 58 NASA Space Administration Jet Propulsion Laboratory robotic explorers, plus a number of California Institute of Technology Pasadena, California international missions (some examples) ESA Venus Express orbiting Venus ESA Rosetta to study Spitzer studying stars and Ulysses studying the comet in 2014 galaxies in the infrared sun Aqua studying Earth’s CALIPSO studying Earth’s Hubble studying the universe oceans climate Rovers “Spirit” and “Opportunity” studying Mars Two Voyagers on an Aura studying Earth’s interstellar mission atmosphere MESSENGER on its way to Mercury QuikScat, Jason 1, CloudSat, and GRACE (plus ASTER, MISR, AIRS, MLS and TES instruments) monitoring Earth. Chandra studying the ESA Mars Express orbiting Mars x-ray universe Japanese SELENE studying Earth’s moon New Horizons on its way to Pluto National Aeronautics and Space Administration Now: A continuous robotic presence Jet Propulsion Laboratory California Institute of Technology Pasadena, California on and in orbit around Mars 2001 Mars Odyssey Spirit Mars Reconnaissance Orbiter “Do not go where the path may lead, go instead where there is no path and leave a trail.” Opportunity Emerson. Mars Express (Opportunity’s tracks in Meridiani Planum) (ESA) National Aeronautics and Space Administration Mars Reconnaissance Orbiter zooms Jet Propulsion Laboratory California Institute of Technology in on Opportunity at Victoria crater Pasadena, California National Aeronautics and Space Administration Opportunity’s reconnaissance of Jet Propulsion Laboratory California Institute of Technology the cliffs of Victoria Crater Pasadena, California National Aeronautics and Space Administration Magellan Venus radar data processed Jet Propulsion Laboratory California Institute of Technology to show topography beneath clouds Pasadena, California National Aeronautics and Space Administration Galileo catches sulfur volcano Jet Propulsion Laboratory California Institute of Technology erupting on Jupiter’s moon Io Pasadena, California National Aeronautics and Space Administration Jupiter’s ring and its halo Jet Propulsion Laboratory California Institute of Technology Pasadena, California from Galileo National Aeronautics and Space Administration Jet PropulsionLooking Laboratory down on Saturn from Cassini orbiter California Institute of Technology Pasadena, California (1 billion miles from Earth) National Aeronautics and Space Administration Backlit Saturn from Cassini orbiter Jet Propulsion Laboratory California Institute of Technology Pasadena, California Earth Visions of Saturn’s rings from Cassini orbiter (Colors indicate particle sizes) National Aeronautics and Space Administration Jet Propulsion Laboratory California Institute of Technology Pasadena, California Celestial art: Dione, rings and Saturn from Cassini orbiter Saturn’s “spongy” pia07740 moon Hyperion from Cassini orbiter Saturn’s moon Phoebe from Cassini orbiter Saturn’s moon Enceledus with “tiger stripe” cracks in ice National Aeronautics and Space Administration Cassini flew within 50 km of Jet Propulsion Laboratory California Institute of Technology Enceladus on March 12 Pasadena, California 50 km 50 km 09034 Saturn’s moon Titan from Cassini orbiter Surface of Saturn’s moon Titan from Huygens lander Methane lakes on Saturn’s 09102 moon Titan from Cassini orbiter radar (at –300°F) Water ice jets on Saturn’s moon Enceladus from Cassini orbiter (At –300°F) National Aeronautics and Space Administration Ground software processes data from Jet Propulsion Laboratory California Institute of Technology Pasadena, California the most distant part of the universe • Hubble Space Telescope deep field image National Aeronautics and Space Administration Spitzer views the star-forming Jet Propulsion Laboratory California Institute of Technology Pasadena, California “Mountains of Creation” GL4029 IRAC [3.6][4.5] IRAC image Lori Allen and the IRAC team AFGL402 National Aeronautics and Space Administration A dying star from Jet Propulsion Laboratory California Institute of Technology Spitzer Space Telescope Pasadena, California National Aeronautics and Space Administration New ways to see a changing Earth Jet Propulsion Laboratory California Institute of Technology with robotic remote sensing Pasadena, California Atmospheric Infrared Jason provides global sea Gravity Recovery and QuikSCAT provides Sounder (AIRS) surface height maps every Climate Experiment near global (90%) ocean provides monthly global 10 days (GRACE) provides monthly surface wind maps temperature maps maps of Earth’s gravity every 24 hours Multi-angle Imaging Tropospheric Emission Microwave Limb Sounder CloudSat provides Spectro Radiometer Spectrometer (TES) (MLS) provides daily maps monthly maps of cloud (MISR) provides monthly provides monthly global of stratospheric chemistry ice water content global aerosol maps maps of Ozone National Aeronautics and Space Administration Shuttle Radar Topography Mission Jet Propulsion Laboratory California Institute of Technology Pasadena, California (SRTM) image of Los Angeles (2000) National Aeronautics and Space Administration Jet Propulsion Laboratory Ground Systems contribute to mission California Institute of Technology Pasadena, California success during all mission life-cycle phases Mission formulation Mission design Spacecraft development Ion engine Ground System cost modeling Ground System engineering Environmental test Assembly Real-time mission operations Integration Data processing, Launch and test visualization and distribution Verification, validation, launch, and flight operations 4/3/08 Elachi GSAW 27 Ion Engine (DS-1) National Aeronautics and Space Administration Ground system implementation Jet Propulsion Laboratory California Institute of Technology Pasadena, California challenge for JPL missions Multiple one-of-a-kind missions… each with unique challenges Common tracking, command, telemetry and data management services Flexible multi-mission operations infrastructure—processes, procedures, teams and facilities System H/W, S/W, Mission Nets & Comm Management Archive Mission Planning and Sequencing Adaptable multi- Data Manageme nt Navigation Analysis mission software Data Acquisition S/C and Command Operations Engineering Product Analysis Generation systems for mission- Science Analysis unique requirements Distributed ground system capabilities for science and engineering interoperability 4/3/08 Elachi GSAW 28 National Aeronautics and Space Administration Mars Exploration Rovers: An example of an Jet Propulsion Laboratory California Institute of Technology operationally responsive ground system Pasadena, California NASA “Software of the Predicted Opportunity: SOL 272 SKELETON -1.3 Ahr Energy Margin no deep sleep/2nd Switchback Drive Thursday Assess and analyze Start End DUR CPU Year” Maestro enables HGA 22720 10:40:00 11:00:00 0:20:00 Eng Keepout/MTES 11:02 11:15 0:13 1 Execute Comm Blip 11:04 11:09 0:05 Drive 11:15 11:45 0:30 1 visodom 11:45 13:15 1:30 1 Post drive imaging + Tau 13:15 14:00 0:45 1 Shutdown 14:00 0:09 1 NAP 14:00 16:44 2:44 VME on 0:06 1 remote scientists to ODY Mtes & Disable D.S. (e2023) 16:44 17:09 0:25 1 RUHF 42721 14:59:52 15:12:53 0:13 RUHF 42723 (30Mb) 16:52:32 17:08:45 0:16 Shutdown 17:12 0:09 1 NAP 17:12 3:36 10:23 Wakeup 0:14 1 RUHF 42730 (60Mb) 3:36 3:52 0:15 1 actively participate in RUHF 42732 5:22 5:35 0:13 Shutdown 3:52 0:09 1 Wakeup 0:06 1 SA stomp- heating - cloud observation 8:00 8:45 0:45 1 Shutdown 8:45 0:09 1 Wakeup 0:06 1 AM Science (note: late HGA = longer science) 10:35 11:19 0:44 1 HGA 22730 10:59:59 11:19:59 0:20:00 rover planning activities Generate data products Plan observations and measurements Tactical Timeline reduced from 16 hours to 8 hours with ground system Communicate and acquire improvements Integrate activity plan Prepare command products 4/3/08 Elachi GSAW Sequence and simulate 29 National Aeronautics and Space Administration Mars Science Laboratory (MSL): Jet Propulsion Laboratory California Institute of Technology Infusion example of ground system Pasadena, California software technologies MSLICE (MSL Operations Interface) • Seamless integration of cutting edge visualization and planning tools for Mars surface missions. • Allows scientists to rapidly search spacecraft data temporally and spatially. • Automatically validates plans against flight rules and science constraints. • Enables collaboration by geographically distributed users. Mission Data Processing System • Multi-mission, DISA-compliant downlink processing framework. • Event-driven capabilities enabled by component architecture. • Supports flight system integration and test through operations, starting with flight software test bed. 4/3/08 Elachi GSAW 30 National Aeronautics and Space Administration JPL’s ground system is the product of a Jet Propulsion Laboratory California Institute of Technology
Load more

Recommended publications
  • The IRM the Iron That Binds: the Unexpectedly Strong Magnetism Of
    ISSN: 2152-1972 The IRM Inside... Visiting Fellows' Reports 2 Current Articles 4 QuarterlySummer 2014, Vol. 24 No.2 The iron that binds: The unexpectedly strong magnetism of high-temperature ceramic cements commonly used in rock magnetic experiments. Evgeniya Khakhalova and Josh M. Feinberg IRM The main goal of many IRM visitors is to better understand the composition of the mag- netic remanence carriers in their samples. Typically, a material’s Curie or Néel temperature serves as the primary means for estimat- ing its mineralogical composi- tion. However, many of the most commonly used techniques, such as high temperature susceptibil- ity and thermal demagnetization experiments, have to be inter- preted carefully due to the com- plicating effects of grain size. For example, single-domain grains contribute less signal to suscep- tibility experiments than super- Fig 1. RT SIRM curves on cooling from 300 K to 10 K and warming from 10 K to 300 K and SIRM warming curves from paramagnetic and multidomain 10 K to 300 K after field-cooling (FC) and zero-field-cooling (ZFC) of samples (a) Omega700_3, (b) Omega600, and (c) grains of the same material, and OmegaCC. SIRM was imparted using a field of 2.5 T. thermal demagnetization experi- ments are insensitive to superparamagnetic grains. Fur- ples dominated by hematite, goethite, and ferrihydrite). ther, the unblocking temperatures observed in a thermal In these instances, any source of magnetic contamination demagnetization experiment will typically be lower than in a strong-field thermomagnetic experiment can lead to the Curie or Néel temperature of the material. an incorrect interpretation of a sample’s magnetic miner- In this context, strong-field thermomagnetic ex- alogy.
    [Show full text]
  • Planetary Report Report
    The PLANETARYPLANETARY REPORT REPORT Volume XXIX Number 1 January/February 2009 Beyond The Moon From The Editor he Internet has transformed the way science is On the Cover: Tdone—even in the realm of “rocket science”— The United States has the opportunity to unify and inspire the and now anyone can make a real contribution, as world’s spacefaring nations to create a future brightened by long as you have the will to give your best. new goals, such as the human exploration of Mars and near- In this issue, you’ll read about a group of amateurs Earth asteroids. Inset: American astronaut Peggy A. Whitson who are helping professional researchers explore and Russian cosmonaut Yuri I. Malenchenko try out training Mars online, encouraged by Mars Exploration versions of Russian Orlan spacesuits. Background: The High Rovers Project Scientist Steve Squyres and Plane- Resolution Camera on Mars Express took this snapshot of tary Society President Jim Bell (who is also head Candor Chasma, a valley in the northern part of Valles of the rovers’ Pancam team.) Marineris, on July 6, 2006. Images: Gagarin Cosmonaut Training This new Internet-enabled fun is not the first, Center. Background: ESA nor will it be the only, way people can participate in planetary exploration. The Planetary Society has been encouraging our members to contribute Background: their minds and energy to science since 1984, A dust storm blurs the sky above a volcanic caldera in this image when the Pallas Project helped to determine the taken by the Mars Color Imager on Mars Reconnaissance Orbiter shape of a main-belt asteroid.
    [Show full text]
  • Operation and Performance of the Mars Exploration Rover Imaging System on the Martian Surface
    Operation and Performance of the Mars Exploration Rover Imaging System on the Martian Surface Justin N. Maki Jet Propulsion Laboratory California Institute of Technology Pasadena, CA USA [email protected] Todd Litwin, Mark Schwochert Jet Propulsion Laboratory California Institute of Technology Pasadena, CA USA Ken Herkenhoff United States Geological Survey Flagstaff, AZ USA Abstract - The Imaging System on the Mars Exploration Rovers has successfully operated on the surface of Mars for over one Earth year. The acquisition of hundreds of panoramas and tens of thousands of stereo pairs has enabled the rovers to explore Mars at a level of detail unprecedented in the history of space exploration. In addition to providing scientific value, the images also play a key role in the daily tactical operation of the rovers. The mobile nature of the MER surface mission requires extensive use of the imaging system for traverse planning, rover localization, remote sensing instrument targeting, and robotic arm placement. Each of these activity types requires a different set of data compression rates, surface Figure 1. The Mars Exploration Spirit Rover, as viewed by coverage, and image acquisition strategies. An overview the Navcam shortly after lander egress early in the mission. of the surface imaging activities is provided, along with a presents an overview of the operation and performance of summary of the image data acquired to date. the MER Imaging System. Keywords: Imaging system, cameras, rovers, Mars, 1.2 Imaging System Design operations. The MER cameras are classified into five types: Descent cameras, Navigation cameras (Navcam), Hazard Avoidance 1 Introduction cameras (Hazcam), Panoramic cameras (Pancam), and Microscopic Imager (MI) cameras.
    [Show full text]
  • A Retrospective Snapshot of the Planning Processes in MER Operations After 5 Years
    A Retrospective Snapshot of the Planning Processes in MER Operations After 5 Years Anthony Barrett, Deborah Bass, Sharon Laubach, and Andrew Mishkin Jet Propulsion Laboratory California Institute of Technology 4800 Oak Grove Drive M/S 301-260 {firstname.lastname}@jpl.nasa.gov Abstract Over the past five years on Mars, the Mars Exploration Rovers have traveled over 20 kilometers to climb tall hills and descend into craters. Over that period the operations process has continued to evolve as deep introspection by the MER uplink team suggests streamlining improvements and lessons learned adds complexity to handle new problems. As such, the operations process and its supporting tools automate enough of the drudgery to circumvent staff burnout issues while being nimble and safe enough to let an operations staff respond to the problems that Mars throws up on a daily basis. This paper describes the currently used integrated set of planning processes that support rover operations on a daily basis after five years of evolution. Figure 1. Mars Exploration Rover For communications, each rover has a high gain antenna Introduction for receiving instructions from Earth, and a low gain On January 3 & 24, 2004 Spirit and Opportunity, the twin antenna for transmitting data to the Odyssey or Mars Mars Exploration Rovers (MER), landed on opposite sides Reconnaissance orbiters with subsequent relay to Earth. of Mars at Gusev Crater and Meridiani Planum Given that it takes between 6 and 44 minutes for a signal to respectively. Each rover was originally expected to last 90 travel to and from the rovers, simple joystick operations Sols (Martian days) due to dust accumulation on the solar are not feasible.
    [Show full text]
  • 2020 Crew Health & Performance EVA Roadmap
    NASA/TP-20205007604 Crew Health and Performance Extravehicular Activity Roadmap: 2020 Andrew F. J. Abercromby1 Omar Bekdash4 J. Scott Cupples1 Jocelyn T. Dunn4 E. Lichar Dillon2 Alejandro Garbino3 Yaritza Hernandez4 Alexandros D. Kanelakos1 Christine Kovich5 Emily Matula6 Matthew J. Miller7 James Montalvo6 Jason Norcross4 Cameron W. Pittman7 Sudhakar Rajulu1 Richard A. Rhodes1 Linh Vu8 1NASA Johnson Space Center, Houston, Texas 2University of Texas Medical Branch, Galveston, Texas 3GeoControl Systems Inc., Houston, Texas 4KBR, Houston, Texas 5The Aerospace Corporation, Houston, Texas 6Stinger Ghaffarian Technologies (SGT) Inc., Houston, Texas 7Jacobs Technology, Inc., Houston, Texas 8MEI Technologies, Inc., Houston, Texas National Aeronautics and Space Administration Johnson Space Center Houston, Texas 77058 October 2020 The NASA STI Program Office ... in Profile Since its founding, NASA has been dedicated to the • CONFERENCE PUBLICATION. advancement of aeronautics and space science. The Collected papers from scientific and NASA scientific and technical information (STI) technical conferences, symposia, seminars, program plays a key part in helping NASA or other meetings sponsored or maintain this important role. co-sponsored by NASA. The NASA STI program operates under the • SPECIAL PUBLICATION. Scientific, auspices of the Agency Chief Information Officer. technical, or historical information from It collects, organizes, provides for archiving, and NASA programs, projects, and missions, disseminates NASA’s STI. The NASA STI often concerned with subjects having program provides access to the NTRS Registered substantial public interest. and its public interface, the NASA Technical Report Server, thus providing one of the largest • TECHNICAL TRANSLATION. collections of aeronautical and space science STI in English-language translations of foreign the world. Results are published in both non-NASA scientific and technical material pertinent to channels and by NASA in the NASA STI Report NASA’s mission.
    [Show full text]
  • Of Curiosity in Gale Crater, and Other Landed Mars Missions
    44th Lunar and Planetary Science Conference (2013) 2534.pdf LOCALIZATION AND ‘CONTEXTUALIZATION’ OF CURIOSITY IN GALE CRATER, AND OTHER LANDED MARS MISSIONS. T. J. Parker1, M. C. Malin2, F. J. Calef1, R. G. Deen1, H. E. Gengl1, M. P. Golombek1, J. R. Hall1, O. Pariser1, M. Powell1, R. S. Sletten3, and the MSL Science Team. 1Jet Propulsion Labora- tory, California Inst of Technology ([email protected]), 2Malin Space Science Systems, San Diego, CA ([email protected] ), 3University of Washington, Seattle. Introduction: Localization is a process by which tactical updates are made to a mobile lander’s position on a planetary surface, and is used to aid in traverse and science investigation planning and very high- resolution map compilation. “Contextualization” is hereby defined as placement of localization infor- mation into a local, regional, and global context, by accurately localizing a landed vehicle, then placing the data acquired by that lander into context with orbiter data so that its geologic context can be better charac- terized and understood. Curiosity Landing Site Localization: The Curi- osity landing was the first Mars mission to benefit from the selection of a science-driven descent camera (both MER rovers employed engineering descent im- agers). Initial data downlinked after the landing fo- Fig 1: Portion of mosaic of MARDI EDL images. cused on rover health and Entry-Descent-Landing MARDI imaged the landing site and science target (EDL) performance. Front and rear Hazcam images regions in color. were also downloaded, along with a number of When is localization done? MARDI thumbnail images. The Hazcam images were After each drive for which Navcam stereo da- used primarily to determine the rover’s orientation by ta has been acquired post-drive and terrain meshes triangulation to the horizon.
    [Show full text]
  • Pre-Mission Insights on the Interior of Mars Suzanne E
    Pre-mission InSights on the Interior of Mars Suzanne E. Smrekar, Philippe Lognonné, Tilman Spohn, W. Bruce Banerdt, Doris Breuer, Ulrich Christensen, Véronique Dehant, Mélanie Drilleau, William Folkner, Nobuaki Fuji, et al. To cite this version: Suzanne E. Smrekar, Philippe Lognonné, Tilman Spohn, W. Bruce Banerdt, Doris Breuer, et al.. Pre-mission InSights on the Interior of Mars. Space Science Reviews, Springer Verlag, 2019, 215 (1), pp.1-72. 10.1007/s11214-018-0563-9. hal-01990798 HAL Id: hal-01990798 https://hal.archives-ouvertes.fr/hal-01990798 Submitted on 23 Jan 2019 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. Open Archive Toulouse Archive Ouverte (OATAO ) OATAO is an open access repository that collects the wor of some Toulouse researchers and ma es it freely available over the web where possible. This is an author's version published in: https://oatao.univ-toulouse.fr/21690 Official URL : https://doi.org/10.1007/s11214-018-0563-9 To cite this version : Smrekar, Suzanne E. and Lognonné, Philippe and Spohn, Tilman ,... [et al.]. Pre-mission InSights on the Interior of Mars. (2019) Space Science Reviews, 215 (1).
    [Show full text]
  • Martian Sub-Surface Ionising Radiation: Abstract Introduction ∗ Biosignatures and Geology Conclusions References Tables Figures L
    Biogeosciences Discuss., 4, 455–492, 2007 Biogeosciences www.biogeosciences-discuss.net/4/455/2007/ Discussions BGD © Author(s) 2007. This work is licensed 4, 455–492, 2007 under a Creative Commons License. Biogeosciences Discussions is the access reviewed discussion forum of Biogeosciences Martian radiation L. R. Dartnell et al Title Page Martian sub-surface ionising radiation: Abstract Introduction ∗ biosignatures and geology Conclusions References Tables Figures L. R. Dartnell1, L. Desorgher2, J. M. Ward3, and A. J. Coates4 1CoMPLEX (Centre for Mathematics & Physics in the Life Sciences and Experimental J I Biology), University College London, UK J I 2Physikalisches Institut, University of Bern, Switzerland 3Department of Biochemistry and Molecular Biology, University College London, UK Back Close 4Mullard Space Science Laboratory, University College London, UK Full Screen / Esc Received: 8 January 2007 – Accepted: 7 February 2007 – Published: 9 February 2007 Correspondence to: L. R. Dartnell ([email protected]) Printer-friendly Version Interactive Discussion EGU ∗Invited contribution by L. R. Dartnell, one of the Union Young Scientist Award winners 2006. 455 Abstract BGD The surface of Mars, unshielded by thick atmosphere or global magnetic field, is ex- posed to high levels of cosmic radiation. This ionizing radiation field is deleterious to 4, 455–492, 2007 the survival of dormant cells or spores and the persistence of molecular biomarkers in 5 the subsurface, and so its characterisation is of prime astrobiological interest. Previous Martian radiation research has attempted to address the question of biomarker persistence by inappro- priately using dose profiles weighted specifically for cellular survival. Here, we present L. R. Dartnell et al modelling results of the unmodified physically absorbed radiation dose as a function of depth through the Martian subsurface.
    [Show full text]
  • Wide Crater in Older Meridiani Planum, Mars
    EPSC Abstracts Vol. 15, EPSC2021-143, 2021 https://doi.org/10.5194/epsc2021-143 Europlanet Science Congress 2021 © Author(s) 2021. This work is distributed under the Creative Commons Attribution 4.0 License. Mineralogical and Geomorphological Characterisation of a 20-km- wide Crater in Older Meridiani Planum, Mars Beatrice Baschetti1,2, Francesca Altieri2, Cristian Carli2, Alessandro Frigeri2, and Maria Sgavetti3 1Department of Physics, Sapienza University of Rome, p.le Aldo Moro 2, 00185 Rome, Italy ([email protected]) 2INAF/IAPS, via del Fosso del Cavaliere 100, 00133 Rome, Italy 3Department of Chemistry, Life Sciences and Environmental Sustainability, Università degli Studi di Parma, Viale delle Scienze 157/A, 43121 Parma Introduction: Meridiani Planum is a relatively plain area located at the Martian equator, south of Arabia Terra, approximately ranging from longitude 350°E to 10°E. Heavily cratered Noachian-aged terrains constitute the oldest geological unit in the region, where several channels and valley networks have left their imprint on the surface [1]. A series of younger terrains were then emplaced in some areas, likely during Late Noachian/Early Hesperian epochs [2]. Meridiani Planum shows signs of a diversified and complex history of aqueous activity in many locations. In addition to the evidence provided by the numerous valley networks, data from OMEGA and CRISM orbital spectrometers have revealed the presence of Fe/Mg phyllosilicates and sulfates throughout the area [3]. These hydrated minerals usually form by alteration in aqueous environments. Older, Noachian-aged, areas are generally characterized by the presence of Fe/Mg phyllosilicates, while younger capping units may display both phyllosilicates and sulfates.
    [Show full text]
  • Geological Analysis of Martian Rover-Derived Digital Outcrop Models 2 Using the 3D Visualisation Tool, Planetary Robotics 3D Viewer – Pro3d
    View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by Spiral - Imperial College Digital Repository Confidential manuscript submitted to Planetary Mapping: Methods, Tools for Scientific Analysis and Exploration (JGR Planets/Earth and Space Science Special Issue) 1 Geological analysis of Martian rover-derived Digital Outcrop Models 2 using the 3D visualisation tool, Planetary Robotics 3D Viewer – PRo3D. 3 4 Robert Barnes1, Sanjeev Gupta1, Christoph Traxler2, Thomas Ortner2, Arnold Bauer3, 5 Gerd Hesina2, Gerhard Paar3, Ben Huber3†, Kathrin Juhart3, Laura Fritz2, Bernhard 6 Nauschnegg3, Jan-Peter Muller4, Yu Tao4. 7 1Department of Earth Science and Engineering, Imperial College London, London, SW7 2AZ, 8 UK. 9 2VRVis Zentrum für Virtual Reality und Visualisierung Forschungs-GmbH, Donau-City- 10 Strasse 11, 1220, Vienna, Austria. 11 3Joanneum Research, Steyregasse 17, 8010, Graz, Austria. 12 4Mullard Space Science Laboratory, University College London, Holmbury Hill Rd, Dorking 13 RH5 6NT, UK. 14 †Presently at ETH Zürich. 15 16 Corresponding author: Robert Barnes ([email protected]) 17 18 Key Points: 19 • Processing of images from stereo-cameras on Mars rovers produces 3D Digital 20 Outcrop Models (DOMs) which are rendered and analysed in PRo3D. 21 • PRo3D enables efficient, real-time rendering and geological analysis of the DOMs, 22 allowing extraction of large amounts of quantitative data. 23 • Methodologies for sedimentological and structural DOM analyses in PRo3D are 24 presented at four localities along the MSL and MER traverses. 1 Confidential manuscript submitted to Planetary Mapping: Methods, Tools for Scientific Analysis and Exploration (JGR Planets/Earth and Space Science Special Issue) 25 Abstract 26 Panoramic camera systems on robots exploring the surface of Mars are used to collect images 27 of terrain and rock outcrops which they encounter along their traverse.
    [Show full text]
  • Remote Characterization of Physical Surface Characteristics of Mars Using Diurnal Variations in Apparent Thermal Inertia
    University of Tennessee, Knoxville TRACE: Tennessee Research and Creative Exchange Masters Theses Graduate School 12-2018 Remote Characterization of Physical Surface Characteristics of Mars Using Diurnal Variations in Apparent Thermal Inertia Cameron Blake McCarty University of Tennessee, [email protected] Follow this and additional works at: https://trace.tennessee.edu/utk_gradthes Recommended Citation McCarty, Cameron Blake, "Remote Characterization of Physical Surface Characteristics of Mars Using Diurnal Variations in Apparent Thermal Inertia. " Master's Thesis, University of Tennessee, 2018. https://trace.tennessee.edu/utk_gradthes/5344 This Thesis is brought to you for free and open access by the Graduate School at TRACE: Tennessee Research and Creative Exchange. It has been accepted for inclusion in Masters Theses by an authorized administrator of TRACE: Tennessee Research and Creative Exchange. For more information, please contact [email protected]. To the Graduate Council: I am submitting herewith a thesis written by Cameron Blake McCarty entitled "Remote Characterization of Physical Surface Characteristics of Mars Using Diurnal Variations in Apparent Thermal Inertia." I have examined the final electronic copy of this thesis for form and content and recommend that it be accepted in partial fulfillment of the equirr ements for the degree of Master of Science, with a major in Geology. Jeff Moersch, Major Professor We have read this thesis and recommend its acceptance: Joshua P. Emery, Christopher M. Fedo Accepted for the Council: Dixie L. Thompson Vice Provost and Dean of the Graduate School (Original signatures are on file with official studentecor r ds.) Remote Characterization of Physical Surface Characteristics of Mars Using Diurnal Variations in Apparent Thermal Inertia A Thesis Presented for the Master of Science Degree The University of Tennessee, Knoxville Cameron Blake McCarty December 2018 Copyright © 2018 by Cameron Blake McCarty All rights reserved ii Dedication Mom, I'll love you forever, I'll like you for always.
    [Show full text]
  • 2005 Astronomy Magazine Index
    2005 Astronomy Magazine Index Subject index flyby of Titan, 2:72–77 Einstein, Albert, 2:30–53 Cassiopeia (constellation), 11:20 See also relativity, theory of Numbers Cassiopeia A (supernova), stellar handwritten manuscript found, 3C 58 (star remnant), pulsar in, 3:24 remains inside, 9:22 12:26 3-inch telescopes, 12:84–89 Cat's Eye Nebula, dying star in, 1:24 Einstein rings, 11:27 87 Sylvia (asteroid), two moons of, Celestron's ExploraScope telescope, Elysium Planitia (on Mars), 5:30 12:33 2:92–94 Enceladus (Saturn's moon), 11:32 2003 UB313, 10:27, 11:68–69 Cepheid luminosities, 1:72 atmosphere of water vapor, 6:22 2004, review of, 1:31–40 Chasma Boreale (on Mars), 7:28 Cassini flyby, 7:62–65, 10:32 25143 (asteroid), 11:27 chonrites, and gamma-ray bursts, 5:30 Eros (asteroid), 11:28 coins, celestial images on, 3:72–73 Eso Chasma (on Mars), 7:28 color filters, 6:67 Espenak, Fred, 2:86–89 A Comet Hale-Bopp, 7:76–79 extrasolar comets, 9:30 Aeolis (on Mars), 3:28 comets extrasolar planets Alba Patera (Martian volcano), 2:28 from beyond solar system, 12:82 first image of, 4:20, 8:26 Aldrin, Buzz, 5:40–45 dust trails of, 12:72–73 first light from, who captured, 7:30 Altair (star), 9:20 evolution of, 9:46–51 newly discovered low-mass planets, Amalthea (Jupiter's moon), 9:28 extrasolar, 9:30 1:68–71 amateur telescopes. See telescopes, Conselice, Christopher, 1:20 smallest, 9:26 amateur constellations whether have diamond layers, 5:26 Andromeda Galaxy (M31), 10:84–89 See also names of specific extraterrestrial life, 4:28–34 disk of stars surrounding, 7:28 constellations eyepieces, telescope.
    [Show full text]