Fourth Annual Heds-Up Forum

Total Page:16

File Type:pdf, Size:1020Kb

Fourth Annual Heds-Up Forum FOURTH ANNUAL HEDS-UP FORUM May 3-5, 2001 Lunar and Planetary Institute, Houston, Texas LPI Contribution No. 1106 FOURTH ANNUAL HEDS-UP FORUM May 3-5,2001 Lunar and Planetary Institute, Houston, Texas Edited by Kathleen M. Johnson Sponsored by Lunar and Planetary Institute National Aeronautics and Space Administration Office of Space Flight, Advanced Projects Office Lunar and Planetary Institute 3600 Bay Area Boulevard Houston TX 77058-1113 LPI Contribution No. 1106 ISSN No. 0161-5297 ii Fourth ttEDS-UP Forum Compiled in 2001 by LUNAR AND PLANETARY INSTITUTE The Institute is operated by the Universities Spac_ Research Association under Contract No, NASW-4574 with the National Aeronautics and Space Administration. Material in this volume may be copied without restraint for library, abstract service, education, or personal research purposes; however, republication of any paper or portion thereof requires the written permission of the authors as well as the appropriate acknowledgment of this publication. This volume may be cited as Johnson K. M., ed. (2001) Fourth Aroma! HEDS-UP Forum. LPI Contribution No. 1106, Lunar and Planetary Institute, Houston. 185 pp. This volume is distributed by ORDER DEPARTMENT Lunar and Planetary Institute 3600 Bay Area Boulevard Houston TX 77058-11 t3 Phone: 281-486-2172 Fax: 281-486-2186 E-mail: [email protected] Mail order requestors will be invoiced for the cost of shipping and handling. Cover design by team from the University of Colorado at Boulder. LPI Cmltribution No. 1 I06 iii PREFACE The HEDS-UP (Human Exploration and Development of Space-University Partners) program was instituted to build new relationships between university, faculty, students, and NASA in support of the Human Exploration and Development of Space. The program has provided a mechanism for university students to explore problems of interest to NASA through student eng!neering-design projects, led by a university professor or mentor, and aided by the HEDS-UP staff. HEDS-UP program management advised teams on the selection of projects that were aligned with the goals of the HEDS strategic enterprise, and provided contacts with NASA and industry professionals who served as mentors. Students became acquainted with objectives, strategies, development issues, and technologic characteristics of space exploration programs. In doing so, they prepared themselves for future engineering challenges, often discovering that the program was on their critical path to professional advancement. Many of the ideas were innovative and of interest to NASA. Industry benefitted from HEDS-UP as a mechanism to converge with talented students about to enter the work force. In addition, universities became more involved in the teaching of space exploration, and students were encouraged and mentored as they included education outreach as an element in their work. This in turn highlighted their performance to others and universities in their communities. The culmination of the HEDS-UP program each year has been the HEDS-UP Forum, held at the Lunar and Planetary Institute (LPI) in Houston, Texas. During the Forum, teams presented their design projects to the university and industry participants and NASA personnel via written reports, oral presentations, models, prototypes, and experiment demonstrations. NASA, industry, and academic professionals presented discussion of current issues and topics of interest in space exploration. Included at the Forum was an informal poster session, where all attendees further discussed the teams' research findings. The Fourth Annual HEDS-UP Forum was held May 3-5, 2001. This year's Forum included representation of 13 university teams, three of which were graduate student teams. Each team contributed a 15-20-page written report; these reports are reproduced in this volume. The agenda for the Forum shows the order of presentation talks by the university teams, NASA presenters, and LPI presenters. Invited speakers included Mr. John Connolly of the NASA Johnson Space Center, Dr. Alex Ignatiev of the University of Houston, Dr. Michael Duke and Dr. Paul Spudis of the LPI, and Dr. Larry Kuznetz of the University of California, Berkeley. The Forum was organized by Dr. Kathleen Johnson, Education Manager at the LPI. Other staff members at the LPI provided logistical, photography, and publications support. A special thanks and acknowledgment goes to Dr. Michael Duke for pioneering this stellar event. Funding'for the HEDS-UP Program was provided by the Office of Space Flight's Advanced Project Office at NASA Headquarters. Kathleen Johnson Education Manager Lunar and Planetary Institute 2 LPI Contributiml No. 1106 v CONTENTS Agenda ........................................................................................................................................................ 1 Scenes from the Forum ............................................................................................................................. 3 University Design Studies Water Extraction from Martian Soil Colorado School of Mines .......................................................................................................................... 11 - / Asteroid Rescue Mission Georgia Institute of Technology ................................................................................................................. 26- 2--- A Deployable hzstrument Package for Paleontological Research Massachusetts Institute of Technology ....................................................................................................... 43- 5 Mining the Foundation of the Future Pennsylvania State University .................................................................................................................... 54 "_7' The Modular Martian MILLIPEDE f Rowan University ....................................................................................................................................... 67 -5 Advanced Two-System Space Suit University of California, Berkeley .............................................................................................................. 81 -/_,,, Hyperbaric Chamber Pass-Through Mechanism Design University of Colorado at Boulder .............................................................................................................. 93 -7 Project LaMaR: Laser-powered Mars Rover University of Colorado at Boulder ............................................................................................................ 110_ if" A Basic Utility Rover for Research Operations University of Maryland, College Park ...................................................................................................... 125 - Clarke Station: An Artificial Gravity Space Station at the Earth-Moon LI Point University of Maryland, College Park ...................................................................................................... 140-/Q Designing a Closed Ecological System to Stq_port Animal Populations for Greater Than Thirty, Days: Pahn Sized Ecosystems University of Washington, Seattle ............................................................................................................ 155 -'-/t Incorporation of the Mini-Magnetospheric Plasma Propulsion System (M2P2) in a Manned Mission to Mars University of Washington, Seattle ............................................................................................................ 168 "/2-.----- List of Forum Participants ................................................................................................................... 183 LPI Contribution No. 1106 1 AGENDA Mqy 3 r 2001 7:30 a.m. Continental Breakfast 8:30 a.m. Welcome to LPI -- Kathteen Johnson 8:45 a.m. Michael Duke, Lunar and Planetary Institute -- "Future Goals and Initiatives for the HEDS Strategic Enterprise" 9:15 am. PauI Spudis, Lunar and Planetary Institute -- "Exploration of the Moon" 9:45 a.m. Alex Ignatiev, University of Houston -- "'Construction of Solar Cells on the Moon" 10:15 a.m Break 10:30 a.m. University of Colorado, Boulder -- "Hyperbaric Chamber Pass-through Module" 11:15 a.m. Embry-Riddle Aeronautical University -- "Mars Communication Outpost" 12:00 noon Lunch 1:30 p.m. Colorado School of Mines -- "Extraction of Water from Martian Regolith" 2:15 p.m. University of Maryland -- "Deep Space Human Space Station" 3:00 p.m Break 3:15 p.m. University of Washington -- "Mini-Magnetospheric Plasma Propulsion System for a Manned Mission to Mars" 4:00 p.m. Massachusetts Institute of Technology- "Experimental Package for Paleontological Research on Mars" 4:45 p.m. Pennsylvania State University -- "Adaptive Robotics for Martian Exploration" 6:00 p.m. Poster Session and Reception May 4, 2001 7:30 a.m. Continental Breakfast 8:15 a.m Sharon Steahle, LPI --"Logistics Dos and Don 'ts (Op, How to Get Reimbursed for your Travel)" 8:30 a.m. University of Maryland -- "Crewed Rover for Lunar and Mars EVA "' 9:15 a.m. University of California, Berkeley -- "Human Exploration of Mars" 10:00 a.m Break 10:15 a.m. Rowan University -- "Mars Mission Rocket Propulsion System" 11:00 a.m. Georgia Institute of Technology -- "Human Exploration of a Near-Earth Asteroid" 11:45 a.m University of Washington -- "Closed Ecological System" 12:30 p.m. Lunch 2:00 p.m. Embry Riddle Aeronautical University -- "Orbital Debris Collection System" 2:45 p.m. University of Colorado, Boulder -- "Project LaMar: l.xzser-pbwered Mars Rover" 3:30 p.m. Break 3:45 p.m. John Connolley, NASA Johnson
Recommended publications
  • New Horizons: Reconnaissance of the Pluto-Charon System and The
    C.T. Russell Editor New Horizons Reconnaissance of the Pluto-Charon System and the Kuiper Belt Previously published in Space Science Reviews Volume 140, Issues 1–4, 2008 C.T. Russell Institute of Geophysics & Planetary Physics University of California Los Angeles, CA, USA Cover illustration: NASA’s New Horizons spacecraft was launched on 2006 January 19, received a grav- ity assist during a close approach to Jupiter on 2007 February 28, and is now headed for a flyby with closest approach 12,500 km from the center of Pluto on 2015 July 14. This artist’s depiction shows the spacecraft shortly after passing above Pluto’s highly variegated surface, which may have black-streaked surface deposits produced from cryogenic geyser activity, and just before passing into Pluto’s shadow when solar and earth occultation experiments will probe Pluto’s tenuous, and possibly hazy, atmosphere. Sunlit crescents of Pluto’s moons Charon, Nix, and Hydra are visible in the background. After flying through the Pluto system, the New Horizons spacecraft could be re-targeted towards other Kuiper Belt Objects in an extended mission phase. This image is based on an original painting by Dan Durda. © Dan Durda 2001 All rights reserved. Back cover illustration: The New Horizons spacecraft was launched aboard an Atlas 551 rocket from the NASA Kennedy Space Center on 2008 January 19 at 19:00 UT. Library of Congress Control Number: 2008944238 DOI: 10.1007/978-0-387-89518-5 ISBN-978-0-387-89517-8 e-ISBN-978-0-387-89518-5 Printed on acid-free paper.
    [Show full text]
  • GUIDANCE, NAVIGATION, and CONTROL 2020 AAS PRESIDENT Carol S
    GUIDANCE, NAVIGATION, AND CONTROL 2020 AAS PRESIDENT Carol S. Lane Cynergy LLC VICE PRESIDENT – PUBLICATIONS James V. McAdams KinetX Inc. EDITOR Jastesh Sud Lockheed Martin Space SERIES EDITOR Robert H. Jacobs Univelt, Incorporated Front Cover Illustration: Image: Checkpoint-Rehearsal-Movie-1024x720.gif Caption: “OSIRIS-REx Buzzes Sample Site Nightingale” Photo and Caption Credit: NASA/Goddard/University of Arizona Public Release Approval: Per multimedia guidelines from NASA Frontispiece Illustration: Image: NASA_Orion_EarthRise.jpg Caption: “Orion Primed for Deep Space Exploration” Photo Credit: NASA Public Release Approval: Per multimedia guidelines from NASA GUIDANCE, NAVIGATION, AND CONTROL 2020 Volume 172 ADVANCES IN THE ASTRONAUTICAL SCIENCES Edited by Jastesh Sud Proceedings of the 43rd AAS Rocky Mountain Section Guidance, Navigation and Control Conference held January 30 to February 5, 2020, Breckenridge, Colorado Published for the American Astronautical Society by Univelt, Incorporated, P.O. Box 28130, San Diego, California 92198 Web Site: http://www.univelt.com Copyright 2020 by AMERICAN ASTRONAUTICAL SOCIETY AAS Publications Office P.O. Box 28130 San Diego, California 92198 Affiliated with the American Association for the Advancement of Science Member of the International Astronautical Federation First Printing 2020 Library of Congress Card No. 57-43769 ISSN 0065-3438 ISBN 978-0-87703-669-2 (Hard Cover Plus CD ROM) ISBN 978-0-87703-670-8 (Digital Version) Published for the American Astronautical Society by Univelt, Incorporated, P.O. Box 28130, San Diego, California 92198 Web Site: http://www.univelt.com Printed and Bound in the U.S.A. FOREWORD HISTORICAL SUMMARY The annual American Astronautical Society Rocky Mountain Guidance, Navigation and Control Conference began as an informal exchange of ideas and reports of achievements among local guidance and control specialists.
    [Show full text]
  • Guidance, Navigation, and Control 2014
    GUIDANCE, NAVIGATION, AND CONTROL 2014 Edited by Alexander J. May Volume 151 ADVANCES IN THE ASTRONAUTICAL SCIENCES GUIDANCE, NAVIGATION, AND CONTROL 2014 AAS PRESIDENT Lyn D. Wigbels RWI International Consulting Services VICE PRESIDENT - PUBLICATIONS Richard D. Burns NASA Goddard Space Flight Center EDITOR Alexander J. May Lockheed Martin Space Systems Co. SERIES EDITOR Robert H. Jacobs Univelt, Incorporated Front Cover Illustration: Lockheed Martin is the prime contractor building the Orion multi-purpose crew vehicle, NASA’s first spacecraft designed for long-duration, human-rated deep space exploration. Orion will transport humans to interplanetary destinations beyond low Earth orbit, such as asteroids, the moon and eventually Mars, and return them safely back to Earth. Credit: Lockheed Martin. Frontispiece: Lockheed Martin’s state-of-the-art Space Operations Simulation Center (SOSC) has completed orbital simulation tests with hardware and data that was flown on NASA’s STS-134 space shut- tle Endeavour mission to the International Space Station. The tests have demonstrated the cen- ter’s ability to replicate on-orbit conditions that affect relative navigation, lighting and motion con- trol in space — providing a simulated space dynamics and lighting environment that is unparal- leled in the space industry. Credit: Lockheed Martin. iii iv GUIDANCE, NAVIGATION, AND CONTROL 2014 Volume 151 ADVANCES IN THE ASTRONAUTICAL SCIENCES Edited by Alexander J. May Proceedings of the 37th Annual AAS Rocky Mountain Section Guidance and Control Conference held January 31 – February 5, 2014, Breckenridge, Colorado. Published for the American Astronautical Society by Univelt, Incorporated, P.O. Box 28130, San Diego, California 92198 Web Site: http://www.univelt.com v Copyright 2014 by AMERICAN ASTRONAUTICAL SOCIETY AAS Publications Office P.O.
    [Show full text]
  • Guidance and Control 2011
    GUIDANCE AND CONTROL 2011 Edited by Kyle B. Miller Volume 141 ADVANCES IN THE ASTRONAUTICAL SCIENCES GUIDANCE AND CONTROL 2011 i CONFERENCE COMMITTEE Brent Abbott Surrey Space Vanessa Baez Lockheed Martin Space Systems Co. Lee Barker Lockheed Martin Space Systems Co. Jim Chapel Lockheed Martin Space Systems Co. Brian Clapp Lockheed Martin Space Systems Co. David A. Chart Lockheed Martin Space Systems Co. Michael Drews Lockheed Martin Space Systems Co. Bill Emery University of Colorado Scott Francis Lockheed Martin Space Systems Co. Kristen Francis Lockheed Martin Space Systems Co. Bill Frazier Ball Aerospace & Technologies Corp. Lis Garratt Ball Aerospace & Technologies Corp. Larry Germann Left Hand Design Ian Gravseth Ball Aerospace & Technologies Corp. Lisa Hardaway Ball Aerospace & Technologies Corp. Steven Jolly Lockheed Martin Space Systems Co. Mary A. Klaus Lockheed Martin Space Systems Co. Alex May Lockheed Martin Space Systems Co. James McQuerry Ball Aerospace & Technologies Corp. Shawn McQuerry Lockheed Martin Space Systems Co. Kyle Miller Ball Aerospace & Technologies Corp. Carolyn O’Brien Lockheed Martin Space Systems Co. Marv Odefey Left Hand Design Michael Osborne Lockheed Martin Space Systems Co. Brian Patterson Lockheed Martin Space Systems Co. Chris Randall Ball Aerospace & Technologies Corp. Ron Rausch United Launch Alliance (Retired) Jay Speed Ball Aerospace & Technologies Corp. Cheryl Walker TASC, Inc. Zach Wilson Lockheed Martin Space Systems Co. THE 35th ANNUAL ROCKY MOUNTAIN SECTION GUIDANCE AND CONTROL CONFERENCE Will be held at Breckenridge, Colorado, February 3–8, 2012, Michael Osborne, Lockheed Martin Space Systems Co., Chairing ii AAS PRESIDENT Frank A. Slazer Northrop Grumman VICE PRESIDENT - PUBLICATIONS Prof. David B. Spencer Pennsylvania State University EDITOR Kyle B.
    [Show full text]
  • Guidance and Control 2013
    GUIDANCE AND CONTROL 2013 Edited by Lisa R. Hardaway Volume 149 ADVANCES IN THE ASTRONAUTICAL SCIENCES GUIDANCE AND CONTROL 2013 i AAS PRESIDENT Lyn D. Wigbels RWI International Consulting Services VICE PRESIDENT - PUBLICATIONS Richard D. Burns NASA Goddard Space Flight Center EDITOR Dr. Lisa R. Hardaway Ball Aerospace & Technologies Corp. SERIES EDITOR Robert H. Jacobs Univelt, Incorporated Front Cover Illustration: The beautiful imagery and important science received from on-orbit telescopes would not be possible without the technologies of Guidance, Navigation and Control. (Photo Credit: NASA). Frontispiece: Kepler, with its star trackers visible, is installed into its launch fairing. (Image courtesy of Ball Aerospace & Technologies Corp.) iii iv GUIDANCE AND CONTROL 2013 Volume 149 ADVANCES IN THE ASTRONAUTICAL SCIENCES Edited by Lisa R. Hardaway Proceedings of the 36th Annual AAS Rocky Mountain Section Guidance and Control Conference held February 1–6, 2013, Breckenridge, Colorado. Published for the American Astronautical Society by Univelt, Incorporated, P.O. Box 28130, San Diego, California 92198 Web Site: http://www.univelt.com v Copyright 2013 by AMERICAN ASTRONAUTICAL SOCIETY AAS Publications Office P.O. Box 28130 San Diego, California 92198 Affiliated with the American Association for the Advancement of Science Member of the International Astronautical Federation First Printing 2013 Library of Congress Card No. 57-43769 ISSN 0065-3438 ISBN 978-0-87703-601-2 (Hard Cover Plus CD ROM) ISBN 978-0-87703-602-9 (CD ROM) Published for the American Astronautical Society by Univelt, Incorporated, P.O. Box 28130, San Diego, California 92198 Web Site: http://www.univelt.com Printed and Bound in the U.S.A.
    [Show full text]
  • Evidence for Widespread Hydrated Minerals on Asteroid (101955) Bennu
    ARTICLES https://doi.org/10.1038/s41550-019-0722-2 Evidence for widespread hydrated minerals on asteroid (101955) Bennu V. E. Hamilton 1*, A. A. Simon2, P. R. Christensen3, D. C. Reuter2, B. E. Clark4, M. A. Barucci 5, N. E. Bowles6, W. V. Boynton7, J. R. Brucato8, E. A. Cloutis9, H. C. Connolly Jr10, K. L. Donaldson Hanna6, J. P. Emery 11, H. L. Enos7, S. Fornasier5, C. W. Haberle3, R. D. Hanna 12, E. S. Howell7, H. H. Kaplan1, L. P. Keller13, C. Lantz14, J.-Y. Li15, L. F. Lim2, T. J. McCoy16, F. Merlin5, M. C. Nolan 7, A. Praet5, B. Rozitis17, S. A. Sandford18, D. L. Schrader 19, C. A. Thomas20, X.-D. Zou15, D. S. Lauretta7 and the OSIRIS-REx Team21 Early spectral data from the Origins, Spectral Interpretation, Resource Identification, and Security-Regolith Explorer (OSIRIS- REx) mission reveal evidence for abundant hydrated minerals on the surface of near-Earth asteroid (101955) Bennu in the form of a near-infrared absorption near 2.7 µm and thermal infrared spectral features that are most similar to those of aque- ously altered CM-type carbonaceous chondrites. We observe these spectral features across the surface of Bennu, and there is no evidence of substantial rotational variability at the spatial scales of tens to hundreds of metres observed to date. In the visible and near-infrared (0.4 to 2.4 µm) Bennu’s spectrum appears featureless and with a blue (negative) slope, confirming previous ground-based observations. Bennu may represent a class of objects that could have brought volatiles and organic chemistry to Earth.
    [Show full text]
  • Ralph: a Visible/Infrared Imager for the New Horizons Pluto/Kuiper Belt Mission
    Please verify that (1) all pages are present, (2) all figures are acceptable, (3) all fonts and special characters are correct, and (4) all text and figures fit within the margin lines shown on this review document. Return to your MySPIE ToDo list and approve or disapprove this submission. Ralph: A visible/infrared imager for the New Horizons Pluto/Kuiper Belt Mission Dennis Reuter1, Alan Stern2, James Baer3, Lisa Hardaway3, Donald Jennings1, Stuart McMuldroch4, Jeffrey Moore5, Cathy Olkin2, Robert Parizek3, Derek Sabatke3, John Scherrer6, John Stone6, Jeffrey Van Cleve3 and Leslie Young2 1NASA/GSFC, Code 693, Greenbelt, MD 20771 2Dept. of Space Studies, SWRI, 1050 Walnut St., Suite 400, Boulder CO, 80302 3BATC, 1600 Commerce St, Boulder, CO 80301 4SSG Precision Optronics, 65 Jonspin Rd., Wilmington MA, 01887 5NASA/Ames Research Center, MS 245-3, Moffett Field, CA 94035-1000 6SWRI, 6220 Culebra Rd., San Antonio TX, 78228 ABSTRACT The instrument named Ralph is a visible/NIR imager and IR hyperspectral imager that would fly as one of the core instruments on New Horizons, NASA’s mission to the Pluto/Charon system and the Kuiper Belt. It is a compact, power efficient, and robust instrument with excellent imaging characteristics and sensitivity, and is well suited to this long- duration flyby reconnaissance mission. 1. INTRODUCTION Ralph is a visible and IR remote sensing instrument scheduled to fly on the New Horizons Mission to the Pluto/Charon system and the Kuiper Belt. The instrument’s primary purpose is to measure surface characteristics, including geological processes, geomorphology, photometric properties, and surface composition. Surface temperature would be inferred from the spectral band shapes and positions of well-established, thermally-diagnostic reflectance spectral features in ices.
    [Show full text]
  • Ralph: a Visible/Infrared Imager for the New Horizons Pluto/Kuiper Belt Mission
    Ralph: A Visible/Infrared Imager for the New Horizons Pluto/Kuiper Belt Mission Dennis C. Reuter1, S. Alan Stern2, John Scherrer3, Donald E. Jennings1, James Baer4, John Hanley3, Lisa Hardaway4, Allen Lunsford1, Stuart McMuldroch5, Jeffrey Moore6, Cathy Olkin7, Robert Parizek4, Harold Reitsma4, Derek Sabatke4, John Spencer7, John Stone3, Henry Throop7, Jeffrey Van Cleve4, Gerald E. Weigle3 and Leslie A.Young7 1NASA/GSFC, Code 693, Greenbelt, MD 20771 2Space Sciences and Engineering Division, Southwest Research Institute (SwRI), 1050 Walnut St., Suite 400, Boulder CO, 80302 3SwRI, 6220 Culebra Rd., San Antonio TX, 78228 4Ball Aerospace and Technology Corporation (BATC), 1600 Commerce St, Boulder, CO 80301 5SSG Precision Optronics, 65 Jonspin Rd., Wilmington MA, 01887 6NASA/Ames Research Center, MS 245-3, Moffett Field, CA 94035-1000 7Dept. of Space Studies, Southwest Research Institute (SwRI), 1050 Walnut St., Suite 400, Boulder CO, 80302 ABSTRACT The New Horizons instrument named Ralph is a visible/near infrared multi-spectral imager and a short wavelength infrared spectral imager. It is one of the core instruments on New Horizons, NASA's first mission to the Pluto/Charon system and the Kuiper Belt. Ralph combines panchromatic and color imaging capabilities with IR imaging spectroscopy. Its primary purpose is to map the surface geology and composition of these objects, but it will also be used for atmospheric studies and to map the surface temperature. It is a compact, low-mass (10.5 kg) power efficient (7.1 W peak), and robust instrument with good sensitivity and excellent imaging characteristics. Other than a door opened once in flight, it has no moving parts.
    [Show full text]
  • New Horizons Mission to Pluto Featuring Ball Aerospace Ralph Camera Video Script 6/15 - W/42 Productions
    Ball Aerospace/NASA New Horizons Mission to Pluto Featuring Ball Aerospace Ralph Camera Video Script 6/15 - w/42 Productions VIDEO Products AUDIO Words on screen: Agility to innovate…strength to deliver Music Bed Deep Impact CRASH into the meteor VOICEOVER: Sometimes a voyage of exploration lasts HiRISE only months. Other discoveries take a few years. But Hubble when you’re going to the most distant worlds in our solar Spitzer system it can take almost a decade. Hello Pluto! WISE Lower Third: Makenzie Lystrup, Ball Aerospace Planetary Lystrup: 9:36 – The thing is that nobody has ever been Astronomer out to Pluto, right?… Launch footage VOICEOVER: New Horizons has been traveling to Pluto since 2006… Lystrup: - 9:55…so everything about this mission is going to be about not rewriting the textbooks but writing the textbooks. Spacecraft build images VOICEOVER: The New Horizons mission is anchored by the Southwest Research Institute for NASA. Lower Third: Alan Stern, Principal Investigator Stern: 1:30 - I hope it’s remembered as the scientific mission that cracked open..and dwarf planets…. Photo images of Ralph camera/integration VOICEOVER: The New Horizons camera system includes a remote-sensing instrument built by Ball Aerospace called RALPH. Lower Third: Lisa Hardaway, Ball Aerospace Ralph Program Hardaway: 51:50- Ralph is a nod….planet. Manager Ralph camera and sensor images VOICEOVER: Ball Aerospace began building Ralph in 2004 – with only 22 months to complete the science instrument. Lower Third: Jim Baer, Ralph Optical Engineer Lead Baer: 14:15 – 14:15 - We knew we could do it…we knew we could do it Ralph photo images VOICEOVER: Because the voyage to Pluto takes so long… Ralph had to be small, made out of light-weight aluminum with the power level of a night light.
    [Show full text]
  • Appendices Appendix A: Technical Exhibits
    APPENDICES APPENDIX A: TECHNICAL EXHIBITS SESSION II The Technical Exhibits Session was a unique opportunity to observe displays and dem- onstrations of state-of-the-art hardware, design and analysis tools, and services applica- ble to advancement of guidance, navigation, and control technology. The latest commer- cial tools for GN&C simulations, analysis, and graphical displays were demonstrated in a hands-on, interactive environment, including lessons learned and undocumented fea- tures. Associated papers not presented in other sessions were also provided and could be discussed with the authors. Local Chairpersons: Kristen Francis Lockheed Martin Space Systems Meredith Larson Ball Aerospace & Technologies Corp The Technical Exhibits did not consist of formal written text, and therefore papers for this session were not available for publication. The following papers and paper numbers were not available for publication, or were not assigned: AAS 11-021 to -030 1021 APPENDIX B: CONFERENCE PROGRAM PROGRAM Becky Petteys, (MathWorks ) th 36 ANNUAL AAS GUIDANCE & 13-005 GRAVMOD2: A New Tool for Precise CONTROL CONFERENCE Gravitational Modelling of Planetary Moons February 1 to February 6, 2013 and Small Bodies, Zuccarelli, V. (Astos Breckenridge, Colorado Solutions, Germany), Cadenas, R.(GMV, Spain), Huertas, I. (ESTEC, European Space Beaver Run Conference Center Agency), Weikert, S. (Astos Solutions, Germany), Astos Solutions, GMV, (ESTEC ESA) FRIDAY, FEBRUARY 1ST Room check-in at the Beaver Run Resort Local Chairperson front desk 4:00 PM daily. Michael Osborne, Lockheed Martin Space Systems, [email protected], 303- Conference registration 977-5867 Friday 5:00 to 8:00 PM Daily 6:30 to 10:00 AM and 4:00 to 6:00 PM SATURDAY, FEBRUARY 2ND Session 0……………….7:00-10:00 AM daily 7am Conference Opening POSTER SESSION by Lisa Hardaway AVAILABLE EVERY DAY The Poster Session will be available for viewing Session I……………………..7:10-10:30 AM every day and authors will be on hand to discuss their projects and answer questions.
    [Show full text]
  • Initial Results from the New Horizons Exploration of 2014 MU69, a Small Kuiper Belt Object
    Initial results from the New Horizons exploration of 2014 MU69, a small Kuiper Belt Object Corresponding Author: S.A. Stern, [email protected] S. A. Stern,1 H. A. Weaver,2 J. R. Spencer,1 C. B. Olkin,1 G. R. Gladstone,3 W. M. Grundy,4 J. M. Moore,5 D. P. Cruikshank,5 H. A. Elliott,3,48 W. B. McKinnon,6 J. Wm. Parker,1 A. J. Verbiscer,7 L. A. Young,1 D. A. Aguilar,8 J. M. Albers,2 T. Andert,9 J. P. Andrews,1 F. Bagenal,10 M. E. Banks,11 B. A. Bauer,2 J. A. Bauman,12 K. E. Bechtold,2 C. B. Beddingfield,13,5 N. Behrooz,2 K. B. Beisser,2 S. D. Benecchi,14 E. Bernardoni,10 R. A. Beyer,13,5 S. Bhaskaran,15 C. J. Bierson,16 R. P. Binzel,17 E. M. Birath,1 M. K. Bird,18,28 D. R. Boone,15 A. F. Bowman,2 V. J. Bray,19 D. T. Britt,20 L. E. Brown,2 M. R. Buckley,2 M. W. Buie,1 B. J. Buratti,15 L. M. Burke,2 S. S. Bushman,2 B. Carcich,21,2 A. L. Chaikin,22 C. L. Chavez,13,5 A. F. Cheng,2 E. J. Colwell,2 S. J. Conard,2 M. P. Conner,2 C. A. Conrad,1 J. C. Cook,23 S. B. Cooper,2 O. S. Custodio,2 C. M. Dalle Ore,13,5 C. C. Deboy,2 P. Dharmavaram,2 R. D. Dhingra,24 G. F. Dunn,3 A.
    [Show full text]
  • Ralph: a Visible/Infrared Imager for the New Horizons Pluto/Kuiper Belt Mission
    Ralph: A Visible/Infrared Imager for the New Horizons Pluto/Kuiper Belt Mission Dennis C. Reuter1, S. Alan Stern2, John Scherrer3, Donald E. Jennings1, James Baer4, John Hanley3, Lisa Hardaway4, Allen Lunsford1, Stuart McMuldroch5, Jeffrey Moore6, Cathy Olkin7, Robert Parizek4, Harold Reitsma4, Derek Sabatke4, John Spencer7, John Stone3, Henry Throop7, Jeffrey Van Cleve4, Gerald E. Weigle3 and Leslie A.Young7 1NASA/GSFC, Code 693, Greenbelt, MD 20771 2Space Sciences and Engineering Division, Southwest Research Institute (SwRI), 1050 Walnut St., Suite 400, Boulder CO, 80302 3SwRI, 6220 Culebra Rd., San Antonio TX, 78228 4Ball Aerospace and Technology Corporation (BATC), 1600 Commerce St, Boulder, CO 80301 5SSG Precision Optronics, 65 Jonspin Rd., Wilmington MA, 01887 6NASA/Ames Research Center, MS 245-3, Moffett Field, CA 94035-1000 7Dept. of Space Studies, Southwest Research Institute (SwRI), 1050 Walnut St., Suite 400, Boulder CO, 80302 ABSTRACT The New Horizons instrument named Ralph is a visible/near infrared multi-spectral imager and a short wavelength infrared spectral imager. It is one of the core instruments on New Horizons, NASA’s first mission to the Pluto/Charon system and the Kuiper Belt. Ralph combines panchromatic and color imaging capabilities with IR imaging spectroscopy. Its primary purpose is to map the surface geology and composition of these objects, but it will also be used for atmospheric studies and to map the surface temperature. It is a compact, low-mass (10.5 kg) power efficient (7.1 W peak), and robust instrument with good sensitivity and excellent imaging characteristics. Other than a door opened once in flight, it has no moving parts.
    [Show full text]