2007 Holiday Greetings from the Ames Center Director NASA Ames Study

Total Page:16

File Type:pdf, Size:1020Kb

2007 Holiday Greetings from the Ames Center Director NASA Ames Study National Aeronautics and Space Administration, Ames Research Center, Moffett Field, CA December 2007 2007 Holiday greetings from the Ames center director BY S. PETE WORDEN and help prepare NASA to put boots on see NASA in a whole new way. As 2007 draws to a close, it’s the moon by the end of the next decade. Next year promises to be even important to take time to pause and This year, NASA Ames helped fire- more exciting. NASA will be cel- reflect on our numerous accomplish- fighters battle some of the worst wildfires ebrating its 50th anniversary. In the ments. We had a great year. We made in California’s history. NASA flew a fall, we’re launching LCROSS on its major contributions in several key remotely piloted aircraft called the Ikhana mission to the moon. In 2009, we’re areas, including lunar exploration, over devastating wildfires in Southern looking forward to seeing the Kepler environment, collaborations and explo- California, Oregon and near Gilroy. Us- mission begin its search for habitable ration, establishing Ames as a premier ing its sophisticated imaging technology planets. It’s an exciting time to be research center. on board, Ames was able to help firefight- here at NASA Ames. NASA announced this year that ers peer through the dense smoke to see So as we say goodbye to 2007 the new Lunar Science Institute will how best to combat the fierce flames. and look forward to 2008, I want to be based at Ames, ensuring that our Ames forged key partnerships with express my sincere thanks to each center will play a key role in future some of the best and brightest compa- and every one of you for all your hard exploration as NASA returns to the nies on the planet, including our Silicon work and numerous contributions moon and later travels to Mars. Next Valley neighbors, Google and Microsoft. to the center. I know that with your year, the Lunar CRater Observation We are working with Google to develop help, we can make 2008 even better. and Sensing Satellite (LCROSS) will Google Moon so that everyone can take I wish you and your families happy slam into the moon and provide scien- a virtual trip to the lunar surface. With holidays and best wishes for the new tists with a wealth of data that will tell Microsoft, we are developing an immer- year. us a great deal about the lunar surface sive imaging technology that lets people NASA Ames study reveals less water in Mars’ clouds BY JOHN BLUCK “The martian clouds we are study- much harder to initiate cloud forma- Martian clouds may contain less ing are composed of water ice, like tion at these cloud temperatures than water than previously thought, ac- some clouds on Earth. However, they what we thought,” he explained. cording to a new NASA Ames study. are forming at very cold temperatures, “This difficulty results in larger New NASA laboratory measure- often below minus 100 degrees Cel- cloud particles, which fall out of the atmosphere more quickly and, thus, results in less cloud mass and a drier One place where water can be found on Mars is its colorful atmosphere,” Colaprete explained. clouds. In this photo, taken by Colaprete presented his findings Viking Orbiter 1, which visited Dec. 11, 2007, during the annual Amer- Mars in 1976, water clouds are ican Geophysical Union (AGU) fall visible just after sunrise in and meeting at San Francisco’s Moscone around a maze of canyons known Convention Center. as Noctis Labyrinthus. Scientists don’t yet know, however, why Previously, scientists believed that these clouds formed, and why martian clouds would form at 100 some stick to the canyons. One percent relative humidity, but the new possibility is that water sometimes study shows that martian air has to condenses in shaded regions of the be more supersaturated with water to canyons, only to evaporate into form clouds than scientists theorized clouds when exposed to the morn- before. ing sun. Water in any form on continued on page 2 the Mars might be important to sustaining life and possible future human exploration. On the Inside . Page 2 - Scientists assess possibilities of Photo: Viking Project, USGS, JPL, NASA water and life on Enceladus Page 5 - Ames top stories in 2007 ments of simulated martian clouds sius (minus 148 degrees Fahrenheit),” Page 7 - Ames transformed into ‘North Pole’ reveal that scientists may have been said Tony Colaprete, an Ames plan- overestimating the amount of water in etary scientist. “What we have found Page 8 - NASA flies Ikhana over wildfires the planet’s atmosphere. in our laboratory studies is that it is Page 13 - Classifieds www.nasa.gov Scientists assess possibilities of water and life on Enceladus BY JOHN BLUCK Life," on Dec. 10, There is a chance liquid water may 2007, at the Moscone exist on Saturn's moon, Enceladus – Convention Center and even a possibility that life could South in San Fran- be there, too – according to NASA cisco. photo NASA scientists who are studying data from Though Saturn's NASA's Cassini spacecraft. moons are far from High-resolution Cassini images the sun, there could show icy jets and towering plumes be liquid water on ejecting large quantities of particles Enceladus because very rapidly as seen in images taken the "general thought by the spacecraft. Scientists have is that there must found evidence the jets might be be some sort of Plumes of icy material extend above the southern polar region of Saturn’s erupting from near-surface pockets of tidal heating," said moon Enceladus as imaged by the Cassini spacecraft in February 2005. The monochrome view is presented along with a color-coded version on the right. liquid water above 32 degrees Fahr- McKay. The latter reveals a fainter and much more extended plume component. enheit, like cold versions of the Old Some scien- Faithful geyser in Yellowstone Nation- tists hypothesize might live on Enceladus. The bacte- al Park, according to NASA reports. that bacteria, living off hydrogen and ria would be "similar to subsurface, Scientists are eagerly anticipating carbon dioxide, and making methane, continued on page 9 the results from a closer Enceladus flyby proposed for an extended Cassi- Study reveals less water in Mars’ clouds ni mission, according to Christopher continued from front page McKay, a scientist at NASA Ames. and time,” Colaprete observed. Clouds "The geysers seem like good “We want to understand the climate of Mars and how the martian in the atmosphere largely control the evidence for liquid water," McKay ob- amount of water that comes off of the served. "The geysers and the methane water cycle operates,” Colaprete said. “Clouds are integral to this system, north pole and migrates to the south in them both seem to up the chances just as on Earth. However, assuming pole. for life. I would say that the chance for the clouds form or behave the same as “Water that reaches the southern life is good enough to warrant further on Earth may be a bad assumption.” winter pole freezes to the surface,” Co- investigation." According to Colaprete, more ac- laprete said. “In the southern spring, Scientists believe the methane curate understanding of the processes this water re-evaporates and returns could come from three potential that control martian clouds and water to the northern polar cap. The cycle is sources. Researchers say it could be cycle are critical to understanding repeated year after year.” primordial – very ancient – or it could Mars’ current and past climates. If all the water in the atmosphere be manufactured deep within Encela- A large water ice cap at the mar- were to freeze out to the surface, it dus, and lastly, and least likely, the tian north pole dominates the martian would make a layer of ice about one- methane could be biological in origin. water cycle. During the northern fifth the thickness of a human hair, McKay and Carolyn Porco, Space summer this water ice cap evaporates, according to Colaprete. Science Institute, Boulder, Colo., pre- and winds carry the resulting water “Cloud mass is typically only 10 to 20 percent of the total water content. sided over numerous scientific pre- vapor to the south pole, according to Colaprete. However, the thin martian atmosphere sentations during a morning session, is much more sensitive/reactive to the "Enceladus: Possibilities for Water and “The amount of water in the mar- tian atmosphere varies greatly in space influence of these clouds,” he said. American Geophysical Union conference held The annual American Geophysical Union, (AGU) conference took place from Dec. 10 - 14, 2007, at the Moscone Center in San Francisco (right photo). Chris McKay of Ames and Carolyn Porco, Space Science Institute, Boulder, Colo., presided over numerous scientific presentations during a morning session, ‘Enceladus: Pos- sibilities for Water and Life.’ Ames science writer John Bluck wrote several articles based upon recent discoveries that were the subject of some of the presentations at the conference. The articles, ‘NASA Study Reveals Less Water in Mars’ Clouds’ focuses on recent findings by NASA Ames planetary scientist, Tony Colaprete, photo by Eric James NASA who presented his study results on Dec. 11; the article ‘NASA Scientists Assess the Possibilities of Water and Life on Enceladus;’ and the story, ‘NASA Scientists Predict Major Ecosystem Carbon Loss in Western States,’ are all included in this issue of the Astrogram. 2 Astrogram December 2007 Scientists predict major ecosystem carbon loss in western states BY JOHN BLUCK Future climate scenarios of air tem- perature warming imply that ecosys- tems across the western United States will experience large carbon losses to the atmosphere and tree growth decline in the western United States, according to NASA Earth scientists.
Recommended publications
  • Imagining Outer Space Also by Alexander C
    Imagining Outer Space Also by Alexander C. T. Geppert FLEETING CITIES Imperial Expositions in Fin-de-Siècle Europe Co-Edited EUROPEAN EGO-HISTORIES Historiography and the Self, 1970–2000 ORTE DES OKKULTEN ESPOSIZIONI IN EUROPA TRA OTTO E NOVECENTO Spazi, organizzazione, rappresentazioni ORTSGESPRÄCHE Raum und Kommunikation im 19. und 20. Jahrhundert NEW DANGEROUS LIAISONS Discourses on Europe and Love in the Twentieth Century WUNDER Poetik und Politik des Staunens im 20. Jahrhundert Imagining Outer Space European Astroculture in the Twentieth Century Edited by Alexander C. T. Geppert Emmy Noether Research Group Director Freie Universität Berlin Editorial matter, selection and introduction © Alexander C. T. Geppert 2012 Chapter 6 (by Michael J. Neufeld) © the Smithsonian Institution 2012 All remaining chapters © their respective authors 2012 All rights reserved. No reproduction, copy or transmission of this publication may be made without written permission. No portion of this publication may be reproduced, copied or transmitted save with written permission or in accordance with the provisions of the Copyright, Designs and Patents Act 1988, or under the terms of any licence permitting limited copying issued by the Copyright Licensing Agency, Saffron House, 6–10 Kirby Street, London EC1N 8TS. Any person who does any unauthorized act in relation to this publication may be liable to criminal prosecution and civil claims for damages. The authors have asserted their rights to be identified as the authors of this work in accordance with the Copyright, Designs and Patents Act 1988. First published 2012 by PALGRAVE MACMILLAN Palgrave Macmillan in the UK is an imprint of Macmillan Publishers Limited, registered in England, company number 785998, of Houndmills, Basingstoke, Hampshire RG21 6XS.
    [Show full text]
  • Go for Lunar Landing Conference Report
    CONFERENCE REPORT Sponsored by: REPORT OF THE GO FOR LUNAR LANDING: FROM TERMINAL DESCENT TO TOUCHDOWN CONFERENCE March 4-5, 2008 Fiesta Inn, Tempe, AZ Sponsors: Arizona State University Lunar and Planetary Institute University of Arizona Report Editors: William Gregory Wayne Ottinger Mark Robinson Harrison Schmitt Samuel J. Lawrence, Executive Editor Organizing Committee: William Gregory, Co-Chair, Honeywell International Wayne Ottinger, Co-Chair, NASA and Bell Aerosystems, retired Roberto Fufaro, University of Arizona Kip Hodges, Arizona State University Samuel J. Lawrence, Arizona State University Wendell Mendell, NASA Lyndon B. Johnson Space Center Clive Neal, University of Notre Dame Charles Oman, Massachusetts Institute of Technology James Rice, Arizona State University Mark Robinson, Arizona State University Cindy Ryan, Arizona State University Harrison H. Schmitt, NASA, retired Rick Shangraw, Arizona State University Camelia Skiba, Arizona State University Nicolé A. Staab, Arizona State University i Table of Contents EXECUTIVE SUMMARY..................................................................................................1 INTRODUCTION...............................................................................................................2 Notes...............................................................................................................................3 THE APOLLO EXPERIENCE............................................................................................4 Panelists...........................................................................................................................4
    [Show full text]
  • Ithaca Classified Business Directory 1935
    JAMIESON - McKINNEY COMPANY HOME HUMIDIFYING SYSTEMS AND HOT WATER 115-121 S. CAYUGA ST. PHONE 3434 1935-ITHAcA DIRECTORY-1935 379 MANNING'S Ithaca Classified Business Directory 1935 Copyright 1935, by H. A. Manning Co. *Indicates heading given by special arrangement with publishers *ABDOMINAL SUPPORTERS (BRANDS) FAHEY EMPLOYMENT AGENCY, 124 E PARADOX, AB Brooks & Son, 126 E State, State, see p 66 see p 67 Student Agencies (Inc), 409 College av ACCOUNTANTS AND AUDITORS Boynton Leland C, 1006 EState AGRICULTURAL IMPLEMENTS MAXFIELD TERRELL B, Savings Bank Anderson & Eddy Implement Co, 107 E bldg (219), see p 60 Green LANG JB ENGINE & GARAGE CO, 117 E *ACCOUNTING SCHOOLS Green, see p 43 (See Business Colleges) AIR BRUSH (PHOTOGRAPHY) *ACETYLENE WELDING FRANZ STUDIO THE, 214 E State, see p 80 CARL'S GARAGE, 201 E Tompkins, see back cover AIR CONDITIONING LANG'S PALACE GARAGE, 117-133 E JAMIESON-McKINNEY CO, 115-121 S Green, see p 43 Cayuga, see top margins REYNOLDS & DRAKE GARAGE CO, 216 S Cayuga, see front cover and p 45 AIRPORTS ADVERTISING AGENCIES Ithaca Flying Service, Taughannock blvd Agricultural Advertising and Research Ser­ Ithaca Municipal Airport, Taughannock blvd vice, 110 N Tioga Ithaca Sales & Pedigree Co, 513 N Tioga ALCOHOLIC BEVERAGE CONTRAl BUREAUS Roberts Grace E, 316 N Aurora Tompkins County Alcoholic Control Board 202 EState (601) *ADVERTISING SIGNS (See Sign Painters and Manufacturers) *ALUMINUM AND ENAMEL WARE AGENCIES ROTHSCHILD BROS, 155-59 E State and CO-OPERATIVE GLF EXCHANGE INC, 100-26 S Tioga, see p 7 Seneca bldg, 112 E Seneca RUMSEY CJ & CO, 206 E State, see p 64 CAREY BLDG.
    [Show full text]
  • Historical Painting Techniques, Materials, and Studio Practice
    Historical Painting Techniques, Materials, and Studio Practice PUBLICATIONS COORDINATION: Dinah Berland EDITING & PRODUCTION COORDINATION: Corinne Lightweaver EDITORIAL CONSULTATION: Jo Hill COVER DESIGN: Jackie Gallagher-Lange PRODUCTION & PRINTING: Allen Press, Inc., Lawrence, Kansas SYMPOSIUM ORGANIZERS: Erma Hermens, Art History Institute of the University of Leiden Marja Peek, Central Research Laboratory for Objects of Art and Science, Amsterdam © 1995 by The J. Paul Getty Trust All rights reserved Printed in the United States of America ISBN 0-89236-322-3 The Getty Conservation Institute is committed to the preservation of cultural heritage worldwide. The Institute seeks to advance scientiRc knowledge and professional practice and to raise public awareness of conservation. Through research, training, documentation, exchange of information, and ReId projects, the Institute addresses issues related to the conservation of museum objects and archival collections, archaeological monuments and sites, and historic bUildings and cities. The Institute is an operating program of the J. Paul Getty Trust. COVER ILLUSTRATION Gherardo Cibo, "Colchico," folio 17r of Herbarium, ca. 1570. Courtesy of the British Library. FRONTISPIECE Detail from Jan Baptiste Collaert, Color Olivi, 1566-1628. After Johannes Stradanus. Courtesy of the Rijksmuseum-Stichting, Amsterdam. Library of Congress Cataloguing-in-Publication Data Historical painting techniques, materials, and studio practice : preprints of a symposium [held at] University of Leiden, the Netherlands, 26-29 June 1995/ edited by Arie Wallert, Erma Hermens, and Marja Peek. p. cm. Includes bibliographical references. ISBN 0-89236-322-3 (pbk.) 1. Painting-Techniques-Congresses. 2. Artists' materials- -Congresses. 3. Polychromy-Congresses. I. Wallert, Arie, 1950- II. Hermens, Erma, 1958- . III. Peek, Marja, 1961- ND1500.H57 1995 751' .09-dc20 95-9805 CIP Second printing 1996 iv Contents vii Foreword viii Preface 1 Leslie A.
    [Show full text]
  • The Composition of the Lunar Crust: Radiative Transfer Modeling and Analysis of Lunar Visible and Near-Infrared Spectra
    THE COMPOSITION OF THE LUNAR CRUST: RADIATIVE TRANSFER MODELING AND ANALYSIS OF LUNAR VISIBLE AND NEAR-INFRARED SPECTRA A DISSERTATION SUBMITTED TO THE GRADUATE DIVISION OF THE UNIVERSITY OF HAWAI‘I IN PARTIAL FULFILLMENT OF THE REQUIREMENTS FOR THE DEGREE OF DOCTOR OF PHILOSOPHY IN GEOLOGY AND GEOPHYSICS DECEMBER 2009 By Joshua T.S. Cahill Dissertation Committee: Paul G. Lucey, Chairperson G. Jeffrey Taylor Patricia Fryer Jeffrey J. Gillis-Davis Trevor Sorensen Student: Joshua T.S. Cahill Student ID#: 1565-1460 Field: Geology and Geophysics Graduation date: December 2009 Title: The Composition of the Lunar Crust: Radiative Transfer Modeling and Analysis of Lunar Visible and Near-Infrared Spectra We certify that we have read this dissertation and that, in our opinion, it is satisfactory in scope and quality as a dissertation for the degree of Doctor of Philosophy in Geology and Geophysics. Dissertation Committee: Names Signatures Paul G. Lucey, Chairperson ____________________________ G. Jeffrey Taylor ____________________________ Jeffrey J. Gillis-Davis ____________________________ Patricia Fryer ____________________________ Trevor Sorensen ____________________________ ACKNOWLEDGEMENTS I must first express my love and appreciation to my family. Thank you to my wife Karen for providing love, support, and perspective. And to our little girl Maggie who only recently became part of our family and has already provided priceless memories in the form of beautiful smiles, belly laughs, and little bear hugs. The two of you provided me with the most meaningful reasons to push towards the "finish line". I would also like to thank my immediate and extended family. Many of them do not fully understand much about what I do, but support the endeavor acknowledging that if it is something I’m willing to put this much effort into, it must be worthwhile.
    [Show full text]
  • NASA Ames to Establish Nationwide Lunar Science Institute
    November 2007 Worden gives upbeat message about future work for Ames BY JOHN BLUCK "We have switched material to In an upbeat talk to a crowd that phenolic impregnated carbon abla- filled the Ames main auditorium, tor (PICA), a (heat shield) material Ames Center Director S. Pete Worden developed here," Worden noted. His outlined an exciting future at Ames projected slide also listed Ames as that includes new work in exploration, leading PICA development and test- science and aeronautics -- each about a ing both for the Crew Exploration Ve- third of the center's efforts, he said. "I hicle, now called Orion, and the Mars have a gazillion charts to go through," Science Laboratory (MSL), which has photo by Eric James NASA he said. a planned launch date in fall 2009. His wide-ranging presentation Worden said that Ames' arc jets about Ames touched on moon explo- facility "a unique facility in the world." ration, a lunar institute, moon dust re- He added, "We want to upgrade search, heat shield work for spacecraft them." destined for the moon and Mars, a Mars sample "cache box" assignment, Life Sciences rising supercomputer capability, small "We are getting additional life Ames Center Director S. Pete Worden responds satellite work with a potential for support tasks assigned by Johnson to a question during the recent upbeat talk he many missions, increased astrobiology (and Marshall)," Worden said. "This is gave to the center about the future of Ames. work, growing cooperation among significant." continued on page 5 academia, and commercial partners and Ames and much more.
    [Show full text]
  • South Pole-Aitken Basin
    Feasibility Assessment of All Science Concepts within South Pole-Aitken Basin INTRODUCTION While most of the NRC 2007 Science Concepts can be investigated across the Moon, this chapter will focus on specifically how they can be addressed in the South Pole-Aitken Basin (SPA). SPA is potentially the largest impact crater in the Solar System (Stuart-Alexander, 1978), and covers most of the central southern farside (see Fig. 8.1). SPA is both topographically and compositionally distinct from the rest of the Moon, as well as potentially being the oldest identifiable structure on the surface (e.g., Jolliff et al., 2003). Determining the age of SPA was explicitly cited by the National Research Council (2007) as their second priority out of 35 goals. A major finding of our study is that nearly all science goals can be addressed within SPA. As the lunar south pole has many engineering advantages over other locations (e.g., areas with enhanced illumination and little temperature variation, hydrogen deposits), it has been proposed as a site for a future human lunar outpost. If this were to be the case, SPA would be the closest major geologic feature, and thus the primary target for long-distance traverses from the outpost. Clark et al. (2008) described four long traverses from the center of SPA going to Olivine Hill (Pieters et al., 2001), Oppenheimer Basin, Mare Ingenii, and Schrödinger Basin, with a stop at the South Pole. This chapter will identify other potential sites for future exploration across SPA, highlighting sites with both great scientific potential and proximity to the lunar South Pole.
    [Show full text]
  • Appendix a Recovery of Ejecta Material from Confirmed, Probable
    Appendix A Recovery of Ejecta Material from Confirmed, Probable, or Possible Distal Ejecta Layers A.1 Introduction In this appendix we discuss the methods that we have used to recover and study ejecta found in various types of sediment and rock. The processes used to recover ejecta material vary with the degree of lithification. We thus discuss sample processing for unconsolidated, semiconsolidated, and consolidated material separately. The type of sediment or rock is also important as, for example, carbonate sediment or rock is processed differently from siliciclastic sediment or rock. The methods used to take and process samples will also vary according to the objectives of the study and the background of the investigator. We summarize below the methods that we have found useful in our studies of distal impact ejecta layers for those who are just beginning such studies. One of the authors (BPG) was trained as a marine geologist and the other (BMS) as a hard rock geologist. Our approaches to processing and studying impact ejecta differ accordingly. The methods used to recover ejecta from unconsolidated sediments have been successfully employed by BPG for more than 40 years. A.2 Taking and Handling Samples A.2.1 Introduction The size, number, and type of samples will depend on the objective of the study and nature of the sediment/rock, but there a few guidelines that should be followed regardless of the objective or rock type. All outcrops, especially those near industrialized areas or transportation routes (e.g., highways, train tracks) need to be cleaned off (i.e., the surface layer removed) prior to sampling.
    [Show full text]
  • Odd Year Nur-Rn-Lic-30550 G
    LicenseNumber FirstName MiddleName LastName RenewalGroup NUR-LPN-LIC-6174 DOLORES ROSE AABERG 2019 - ODD YEAR NUR-RN-LIC-30550 GRETCHEN ELLEN AAGAARD-SHIVELY 2019 - ODD YEAR NUR-RN-LIC-128118 CAMBRIA LAUREN AANERUD 2019 - ODD YEAR NUR-RN-LIC-25862 SOPHIA SABINA AANSTAD 2018 - EVEN YEAR NUR-APRN-LIC-124944 ERIN EDWARD AAS 2018 - EVEN YEAR NUR-RN-LIC-105371 ERIN EDWARD AAS 2018 - EVEN YEAR NUR-RN-LIC-34536 BRYON AAS 2019 - ODD YEAR NUR-RN-LIC-39208 JULIA LYNN AASEN 2018 - EVEN YEAR NUR-APRN-LIC-130522 LORI ANN AASEN 2019 - ODD YEAR NUR-RN-LIC-130520 LORI ANN AASEN 2019 - ODD YEAR NUR-RN-LIC-21015 DEBBIE ABAR 2018 - EVEN YEAR NUR-APRN-LIC-130757 LUKE G ABAR 2018 - EVEN YEAR NUR-RN-LIC-130756 LUKE GORDON ABAR 2019 - ODD YEAR NUR-RN-LIC-31911 AIMEE KRISTINE ABBOTT 2018 - EVEN YEAR NUR-RN-LIC-29448 DENISE M ABBOTT 2018 - EVEN YEAR NUR-RN-LIC-131150 SARAH FRANCES ABBOTT 2018 - EVEN YEAR NUR-LPN-LIC-31701 ANGIE ABBOTT 2019 - ODD YEAR NUR-LPN-LIC-33325 HEIDI ABBOTT 2019 - ODD YEAR NUR-LPN-LIC-4920 LORI ANN ABBOTT 2019 - ODD YEAR NUR-LPN-LIC-97426 DAYMON ABBOTT Expired - 2018 - EVEN YEAR NUR-RN-LIC-13260 ROBERT C ABBOTT Expired - 2018 - EVEN YEAR NUR-RN-LIC-17858 MONICA MAY ABDALLAH 2018 - EVEN YEAR NUR-RN-LIC-48890 STEVEN P ABDALLAH 2019 - ODD YEAR NUR-APRN-LIC-101391 LANEICE LORRAINE ABDEL-SHAKUR Expired - 2018 - EVEN YEAR NUR-RN-LIC-101333 LANEICE LORRAINE ABDEL-SHAKUR Expired - 2018 - EVEN YEAR NUR-RN-LIC-96606 RENDI L ABEL 2018 - EVEN YEAR NUR-RN-LIC-97338 LAURA ANN ABEL 2019 - ODD YEAR NUR-RN-LIC-69876 LACEY ANN ABELL 2019 - ODD YEAR NUR-RN-LIC-131932
    [Show full text]
  • R-700 MIT's ROLE in PROJECT APOLLO VOLUME I PROJECT
    R-700 MIT’s ROLE IN PROJECT APOLLO FINAL REPORT ON CONTRACTS NAS 9-153 AND NAS 9-4065 VOLUME I PROJECT MANAGEMENT SYSTEMS DEVELOPMENT ABSTRACTS AND BIBLIOGRAPHY edited by James A. Hand OCTOBER 1971 CAMBRIDGE, MASSACHUSETTS, 02139 ACKNOWLEDGMENTS This report was prepared under DSR Project 55-23890, sponsored by the Manned Spacecraft Center of the National Aeronautics and Space Administration. The description of project management was prepared by James A. Hand and is based, in large part, upon discussions with Dr. C. Stark Draper, Ralph R. Ragan, David G. Hoag and Lewis E. Larson. Robert C. Millard and William A. Stameris also contributed to this volume. The publication of this document does not constitute approval by the National Aeronautics and Space Administration of the findings or conclusions contained herein. It is published for the exchange and stimulation of ideas. @ Copyright by the Massachusetts Institute of Technology Published by the Charles Stark Draper Laboratory of the Massachusetts Institute of Technology Printed in Cambridge, Massachusetts, U. S. A., 1972 ii The title of these volumes, “;LJI’I”s Role in Project Apollo”, provides but a mcdest hint of the enormous range of accomplishments by the staff of this Laboratory on behalf of the Apollo program. Rlanss rush into spaceflight during the 1060s demanded fertile imagination, bold pragmatism, and creative extensions of existing tecnnologies in a myriad of fields, The achievements in guidance and control for space navigation, however, are second to none for their critical importance in the success of this nation’s manned lunar-landing program, for while powerful space vehiclesand rockets provide the environment and thrust necessary for space flight, they are intrinsicaily incapable of controlling or guiding themselves on a mission as complicated and sophisticated as Apollo.
    [Show full text]
  • Science Concept 3: Key Planetary
    Science Concept 6: The Moon is an Accessible Laboratory for Studying the Impact Process on Planetary Scales Science Concept 6: The Moon is an accessible laboratory for studying the impact process on planetary scales Science Goals: a. Characterize the existence and extent of melt sheet differentiation. b. Determine the structure of multi-ring impact basins. c. Quantify the effects of planetary characteristics (composition, density, impact velocities) on crater formation and morphology. d. Measure the extent of lateral and vertical mixing of local and ejecta material. INTRODUCTION Impact cratering is a fundamental geological process which is ubiquitous throughout the Solar System. Impacts have been linked with the formation of bodies (e.g. the Moon; Hartmann and Davis, 1975), terrestrial mass extinctions (e.g. the Cretaceous-Tertiary boundary extinction; Alvarez et al., 1980), and even proposed as a transfer mechanism for life between planetary bodies (Chyba et al., 1994). However, the importance of impacts and impact cratering has only been realized within the last 50 or so years. Here we briefly introduce the topic of impact cratering. The main crater types and their features are outlined as well as their formation mechanisms. Scaling laws, which attempt to link impacts at a variety of scales, are also introduced. Finally, we note the lack of extraterrestrial crater samples and how Science Concept 6 addresses this. Crater Types There are three distinct crater types: simple craters, complex craters, and multi-ring basins (Fig. 6.1). The type of crater produced in an impact is dependent upon the size, density, and speed of the impactor, as well as the strength and gravitational field of the target.
    [Show full text]
  • Global Challenges
    6–10 JANUARY 2020 | ORLANDO, FL DRIVING AEROSPACE SOLUTIONS FOR GLOBAL CHALLENGES What’s going on in Page 25 aiaa.org/scitech #aiaaSciTech From the forefront of innovation to the frontlines of the mission. No matter the mission, Lockheed Martin uses a proven approach: engineer with purpose, innovate with passion and define the future. We take time to understand our customer’s challenges and provide solutions that help them keep the world secure. Their mission defines our purpose. Learn more at lockheedmartin.com. © 2019 Lockheed Martin Corporation FG19-23960_002 AIAA sponsorship.indd 1 12/10/19 3:20 PM Live: n/a Trim: H: 8.5in W: 11in Job Number: FG18-23208_002 Bleed: .25 all around Designer: Kevin Gray Publication: AIAA Sponsorship Gutter: None Communicator: Ryan Alford Visual: Male and female in front of screens. Resolution: 300 DPI Due Date: 12/10/19 Country: USA Density: 300 Color Space: CMYK NETWORK NAME: SciTech ON-SITE Wi-Fi From the forefront of innovation › PASSWORD: 2020scitech to the frontlines of the mission. CONTENTS Technical Program Committee .................................................................4 Welcome ........................................................................................................5 Sponsors and Supporters ..........................................................................7 Forum Overview ...........................................................................................8 Pre-Forum Activities .................................................................................
    [Show full text]