Phase 1 Science Report Contents
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IMPLICATIONS for FUNCTION in MICROGRAVITY Introduction
Journal of Vestibular Research. Vol. 8. No.1. pp. 81-94.1998 Copyright I!:I 1998 Elsevier Science Inc. Printed in the USA. All rights reserved 0957-4271/98 $19.00 + .00 ELSEVIER PIT S0957-4271(97)00055-4 Review SLEEP AND VESTIBULAR ADAPTATION: IMPLICATIONS FOR FUNCTION IN MICROGRAVITY J. Allan Hobson, Robert Stickgold, Edward F. Pace-Schott, and Kenneth R. Leslie Laboratory of Neurophysiology. Massachusetts Mental Health Center, Harvard Medical School, Boston, Massachusetts : : ,. "" .. 1>.. .. I. II ~ ,... "" ,... " - r' - .... .. ,... .. ... ,. .. ~ 'f''''' .. .... p .... - - • .. _.... • - _ E-mail: [email protected] o Abstract - Optimal human performance de Introduction pends upon integrated sensorimotor and cognitive functions, both of which are known to be exquis The functions of sleep remain unknown. The itely sensitive to loss of sleep. Under the micro compelling idea that sleep subserves neuronal gravity conditions of space flight, adaptation of plasticity was first clearly articulated by Giuseppe both sensorimotor (especially vestibular) and cog nitive functions (especially orientation) must occur Moruzzi (1). This hypothesis has been tested in quickly-and be maintained-despite any concur many ways, induding the systematic perturba rent disruptions of sleep that may be caused by tion of the vestibular system. The close interre microgravity itself, or by the uncomfortable sleep lationship between the vestibular nuclei and the ing conditions of the spacecraft. It is the three-way sleep inducing structures of the pontine brain interaction between sleep quality, general work ef stem has been extensively studied by Moruzzi's ficiency, and sensorimotor integration that is the colleagues, especially Ottavio Pompeiano (2). It subject of this paper and the focus of new work in is the purpose of this paper to discuss the con our laboratory. -
Introduction to Astronomy from Darkness to Blazing Glory
Introduction to Astronomy From Darkness to Blazing Glory Published by JAS Educational Publications Copyright Pending 2010 JAS Educational Publications All rights reserved. Including the right of reproduction in whole or in part in any form. Second Edition Author: Jeffrey Wright Scott Photographs and Diagrams: Credit NASA, Jet Propulsion Laboratory, USGS, NOAA, Aames Research Center JAS Educational Publications 2601 Oakdale Road, H2 P.O. Box 197 Modesto California 95355 1-888-586-6252 Website: http://.Introastro.com Printing by Minuteman Press, Berkley, California ISBN 978-0-9827200-0-4 1 Introduction to Astronomy From Darkness to Blazing Glory The moon Titan is in the forefront with the moon Tethys behind it. These are two of many of Saturn’s moons Credit: Cassini Imaging Team, ISS, JPL, ESA, NASA 2 Introduction to Astronomy Contents in Brief Chapter 1: Astronomy Basics: Pages 1 – 6 Workbook Pages 1 - 2 Chapter 2: Time: Pages 7 - 10 Workbook Pages 3 - 4 Chapter 3: Solar System Overview: Pages 11 - 14 Workbook Pages 5 - 8 Chapter 4: Our Sun: Pages 15 - 20 Workbook Pages 9 - 16 Chapter 5: The Terrestrial Planets: Page 21 - 39 Workbook Pages 17 - 36 Mercury: Pages 22 - 23 Venus: Pages 24 - 25 Earth: Pages 25 - 34 Mars: Pages 34 - 39 Chapter 6: Outer, Dwarf and Exoplanets Pages: 41-54 Workbook Pages 37 - 48 Jupiter: Pages 41 - 42 Saturn: Pages 42 - 44 Uranus: Pages 44 - 45 Neptune: Pages 45 - 46 Dwarf Planets, Plutoids and Exoplanets: Pages 47 -54 3 Chapter 7: The Moons: Pages: 55 - 66 Workbook Pages 49 - 56 Chapter 8: Rocks and Ice: -
Sleep and Daily Rhythms
Activities Guide for Teachers National Space Biomedical Research Institute Houston, Texas The National Space Biomedical Research Institute (NSBRI) is combining the basic research capabilities of some of the nation’s leading biomedical research centers with operational and applied research conducted by the National Aeronautics and Space Administration (NASA) to understand and achieve safe and effective long-term human exploration and development of space. The NSBRI’s discoveries and research products will help to counter the effects of weightlessness and space radiation and will contribute to the health and well-being of all mankind. National Space Biomedical Research Institute One Baylor Plaza, NA-425 Houston, Texas 77030-3498 http://www.nsbri.org The activities described in this book are intended for school-age children under direct supervision of adults. The authors, Baylor College of Medicine and the National Space Biomedical Research Institute cannot be responsible for any accidents or injuries that may result from conduct of the activities, from not specifically following directions, or from ignoring cautions contained in the text. The opinions, findings and conclusions expressed in this publication are solely those of the authors and do not necessarily reflect the views of Baylor College of Medicine or the National Space Biomedical Research Institute. Authors: Nancy P. Moreno, Ph.D. and Barbara Z. Tharp, M.S. Cover Illustration: T Lewis Design and Production: Martha S. Young Acknowledgments The authors gratefully acknowledge the support of Bobby R. Alford, M.D.; Laurence R. Young, Sc.D.; and Ronald J. White, Ph.D.; as well as the contributions of the following science reviewers: Mary A. -
Tracing Subduction Zone Processes with Magnesium Isotopes
Tracing subduction zone processes with magnesium isotopes Yan Hu A dissertation submitted in partial fulfillment of the requirements for the degree of Doctor of Philosophy University of Washington 2018 Reading Committee: Fang-Zhen Teng, Chair Bruce K. Nelson Ronald S. Sletten Program Authorized to Offer Degree: Earth and Space Sciences © Copyright 2018 Yan Hu University of Washington Abstract Tracing subduction zone processes with magnesium isotopes Yan Hu Chair of the Supervisory Committee: Professor Fang-Zhen Teng Department of Earth and Space Sciences Subduction and recycling of oceanic plates change the chemical composition of mantle and affect its physical properties, thereby modulating Earth’s dynamics. Stable Mg isotopes (δ26Mg) can trace this recycling process as crustal materials are highly fractionated compared to the average mantle composition. This dissertation focuses on Mg isotope fractionation during subduction-related processes and the consequent mantle heterogeneity. The dissertation first compares inconsistent δ26Mg values of San Carlos peridotitic olivines that are published by several laboratories. We analyzed mineral grains from two San Carlos peridotites with disparate lithologies and determined that all mineral phases have indistinguishable δ26Mg values to within 0.07‰. With analytical precision and accuracy being confirmed, the significance of anomalous δ26Mg values can be understood in the context of mantle heterogeneity. The next paper investigates the Mg isotopic heterogeneity in mantle pyroxenites that have formed by multi-stage interactions between peridotites and melts with diverse origins. Pyroxenites formed by reaction with melts derived from subducted oceanic crust and carbonate sediments are shown to have variable δ26Mg values (−1.51‰ to −0.10‰). In contrast, pyroxenites that are formed by reaction with silicate melts from deep mantle has δ26Mg values similar to common mantle peridotites. -
March 21–25, 2016
FORTY-SEVENTH LUNAR AND PLANETARY SCIENCE CONFERENCE PROGRAM OF TECHNICAL SESSIONS MARCH 21–25, 2016 The Woodlands Waterway Marriott Hotel and Convention Center The Woodlands, Texas INSTITUTIONAL SUPPORT Universities Space Research Association Lunar and Planetary Institute National Aeronautics and Space Administration CONFERENCE CO-CHAIRS Stephen Mackwell, Lunar and Planetary Institute Eileen Stansbery, NASA Johnson Space Center PROGRAM COMMITTEE CHAIRS David Draper, NASA Johnson Space Center Walter Kiefer, Lunar and Planetary Institute PROGRAM COMMITTEE P. Doug Archer, NASA Johnson Space Center Nicolas LeCorvec, Lunar and Planetary Institute Katherine Bermingham, University of Maryland Yo Matsubara, Smithsonian Institute Janice Bishop, SETI and NASA Ames Research Center Francis McCubbin, NASA Johnson Space Center Jeremy Boyce, University of California, Los Angeles Andrew Needham, Carnegie Institution of Washington Lisa Danielson, NASA Johnson Space Center Lan-Anh Nguyen, NASA Johnson Space Center Deepak Dhingra, University of Idaho Paul Niles, NASA Johnson Space Center Stephen Elardo, Carnegie Institution of Washington Dorothy Oehler, NASA Johnson Space Center Marc Fries, NASA Johnson Space Center D. Alex Patthoff, Jet Propulsion Laboratory Cyrena Goodrich, Lunar and Planetary Institute Elizabeth Rampe, Aerodyne Industries, Jacobs JETS at John Gruener, NASA Johnson Space Center NASA Johnson Space Center Justin Hagerty, U.S. Geological Survey Carol Raymond, Jet Propulsion Laboratory Lindsay Hays, Jet Propulsion Laboratory Paul Schenk, -
European Astronaut Selection ESA Prepares for the Missions of the 21 St Century
European Astronaut Selection ESA prepares for the missions of the 21 st century With the selection of its first astronauts ESA’s human spaceflight activities in 1978 and the first Spacelab mission are now entering a new era, with ESA in 1983, the European Space Agency astronauts working aboard the (ESA) took its first steps into human International Space Station (ISS), spaceflight. The advent of the Columbus Columbus starting operations, and orbital laboratory project required a the new ‘ATV’ cargo ship delivering second selection of astronauts in 1992. fresh supplies to the Station. The exploration of the Solar System will be one of humanity’s most exciting adventures in the near future. All of the world’s spacefaring nations are preparing for this huge enterprise, and an astronaut corps is essential for Europe, thanks to ESA, to take part in this endeavour. Now is the time for ESA to seek new talents to reinforce its astronaut team, to prepare for missions to the ISS, the Moon and beyond. T The Selection | How? When? Where? h e S e l e c t i o n How can I apply? You can apply online via the ESA web portal (www.esa.int/ astronautselection). Registration is in two steps: • pre-registration: provide identity information and a JAR-FCL 3, Class 2 medi- cal examination certificate, from an Aviation Medical Examiner who has been certified by his/her national Aviation Medical Authority; • a password then allows you to access the application form. T The Selection | How? When? Where? h e S e l e • initial selection according to basic criteria; c t i What are the o • psychological tests for selected candidates; n • second round of psychological tests and interviews; steps in the • medical tests; selection • job interview. -
Human Mars Mission Architecture Plan to Settle the Red Planet with 1000 People
Human Mars Mission Architecture Plan to Settle the Red Planet with 1000 People Malaya Kumar Biswal M1, Vishnu S2, Devika S Kumar3, Sairam M4 Pondicherry University, Kalapet, Puducherry, India - 605 014 Abstract Exploration is one of the attentive endeavor to mankind and a strategy for evolution. We have been incessantly reconnoitering our planet and universe from Mesopotamian era to modern era. The progression of rocketry and planetary science in past century engendered a futuristic window to explore Mars which have been a source of inspiration to hundreds of astronomers and scientists. Globally, it invigorated space exploration agencies to make expedition for planetary exploration to Mars and Human Mars Missions. Scientists and engineers have portrayed numerous Human Mars Mission proposals and plans but currently the design reference mission 5.0 of NASA is the only mission under study. Here we propose a mission architecture for permanent Human Mars Settlement with 1000 peoples with multiple launch of sufficient cargoes and scientific instruments. Introduction: This paper focuses on design of Human Mars Mission with reference to the instructions by Mars Society. We proposed mission architecture for carrying 1000 peoples onboard spaceship (Marship). Overall mission architecture outline map and Human Mars Settlement Map is provided next to this page. We divided the whole mission architecture into three phases starting from orbital launch of launch vehicles and Mars colony establishment. We proposed novel habitat for protection during robust dust storms, various method to make the colony economically successful, minerals and their applications, administrative methods, water extraction, plantation, landing patterns, estimation of masses of food to be carried out and customizable system for re-use and recycling. -
Landed Science at a Lunar Crustal Magnetic Anomaly
Landed Science at a Lunar Crustal Magnetic Anomaly David T. Blewett, Dana M. Hurley, Brett W. Denevi, Joshua T.S. Cahill, Rachel L. Klima, Jeffrey B. Plescia, Christopher P. Paranicas, Benjamin T. Greenhagen, Lauren Jozwiak, Brian A. Anderson, Haje Korth, George C. Ho, Jorge I. Núñez, Michael I. Zimmerman, Pontus C. Brandt, Sabine Stanley, Joseph H. Westlake, Antonio Diaz-Calderon, R. Ter ik Daly, and Jeffrey R. Johnson Space Science Branch, Johns Hopkins University Applied Physics Lab, USA Lunar Science for Landed Missions Workshop – January, 2018 1 Lunar Magnetic Anomalies • The lunar crust contains magnetized areas, a few tens to several hundred kilometers across, known as "magnetic anomalies". • The crustal fields are appreciable: Strongest anomalies are ~10-20 nT at 30 km altitude, perhaps a few hundred to 1000 nT at the surface. Lunar Prospector magnetometer Btot map (Richmond & Hood 2008 JGR) over LROC WAC 689-nm mosaic 2 Lunar Magnetic Anomalies: Formation Hypotheses • Magnetized basin ejecta: ambient fields amplified by compression as impact-generated plasma converged on the basin antipode (Hood and co-workers) Lunar Prospector magnetometer Btot (Richmond & Hood 2008 JGR) over LROC WAC 689- nm mosaic 3 Lunar Magnetic Anomalies: Formation Hypotheses • Magnetized basin ejecta: ambient fields amplified by compression as impact-generated plasma converged on the basin antipode (Hood and co-workers) • Magnetic field impressed on the surface by plasma interactions when a cometary coma struck the Moon (Schultz) Lunar Prospector magnetometer Btot (Richmond & Hood 2008 JGR) over LROC WAC 689- nm mosaic 4 Lunar Magnetic Anomalies: Formation Hypotheses • Magnetized basin ejecta: ambient fields amplified by compression as impact-generated plasma converged on the basin antipode (Hood and co-workers) • Magnetic field impressed on the surface by plasma interactions when a cometary coma struck the Moon (Schultz) • Magmatic intrusion or impact melt magnetized in an early lunar dynamo field (e.g., Purucker et al. -
Appendix Program Managers/Acknowledgments
Flight Information Appendix Program Managers/Acknowledgments Selected Readings Acronyms Contributors’ Biographies Index Image of a Legac y—The Final Re-entry Appendix 517 Flight Information Approx. Orbiter Enterprise STS Flight No. Orbiter Crew Launch Mission Approach and Landing Test Flights and Crew Patch Name Members Date Days 1 Columbia John Young (Cdr) 4/12/1981 2 Robert Crippen (Plt) Captive-Active Flights— High-speed taxi tests that proved the Shuttle Carrier Aircraft, mated to Enterprise, could steer and brake with the Orbiter perched 2 Columbia Joe Engle (Cdr) 11/12/1981 2 on top of the airframe. These fights featured two-man crews. Richard Truly (Plt) Captive-Active Crew Test Mission Flight No. Members Date Length 1 Fred Haise (Cdr) 6/18/1977 55 min 46 s Gordon Fullerton (Plt) 2 Joseph Engle (Cdr) 6/28/1977 62 min 0 s 3 Columbia Jack Lousma (Cdr) 3/22/1982 8 Richard Truly (Plt) Gordon Fullerton (Plt) 3 Fred Haise (Cdr) 7/26/1977 59 min 53 s Gordon Fullerton (Plt) Free Flights— Flights during which Enterprise separated from the Shuttle Carrier Aircraft and landed at the hands of a two-man crew. 4 Columbia Thomas Mattingly (Cdr) 6/27/1982 7 Free Flight No. Crew Test Mission Henry Hartsfield (Plt) Members Date Length 1 Fred Haise (Cdr) 8/12/1977 5 min 21 s Gordon Fullerton (Plt) 5 Columbia Vance Brand (Cdr) 11/11/1982 5 2 Joseph Engle (Cdr) 9/13/1977 5 min 28 s Robert Overmyer (Plt) Richard Truly (Plt) William Lenoir (MS) 3 Fred Haise (Cdr) 9/23/1977 5 min 34 s Joseph Allen (MS) Gordon Fullerton (Plt) 4 Joseph Engle (Cdr) 10/12/1977 2 min 34 s Richard Truly (Plt) 5 Fred Haise (Cdr) 10/26/1977 2 min 1 s 6 Challenger Paul Weitz (Cdr) 4/4/1983 5 Gordon Fullerton (Plt) Karol Bobko (Plt) Story Musgrave (MS) Donald Peterson (MS) The Space Shuttle Numbering System The first nine Space Shuttle flights were numbered in sequence from STS -1 to STS-9. -
2021 Program Guide Summer Supplement
2021 PROGRAM GUIDE SUPPLEMENTsummer HELLO GIRL SCOUT! The Program Guide Summer Supplement is full of opportunities to try something new, dive deeper into that which interests you, and have FUN this summer with GSOSW! NAVIGATING THIS GUIDE This guide is organized by date. When you find events that are just right for you, visit girlscoutsosw.org/events to find more detailed information about the events and sign up! Special icons in this guide indicate where you can spend your program credits ( ), and if the event is in person ( ). These icons will SAMPLE ACTIVITY LISTING tell you if you can use program This is where credits and if the the event FARM TO FORK: COMPOST event is in person title, program AND CHEESE or virtual. In this example the partner and GSOSW location can event is in person Medford, OR be found. and you can use program credits. Get your hands dirty in the garden and Learn about learn about compost and worms from this event and Bugs R Us! Afterward, learn how to make The time of the whether it’s ricotta cheese in the kitchen. activity and which something grade levels can you would like 7/13/21 3:30 - 5:30 p.m. participate are to do! $10/girl All ages located here. Abbreviations are as follows: The date and D (Daisies), BR cost of the (Brownies), JR events are (Juniors), CAD listed here. (Cadettes), SR (Seniors) and AMB (Ambassadors). COVID-19 UPDATE GSOSW is excited to be offering a handful of in-person events this summer! GSOSW has collaborated with our program partners to ensure that all COVID-19 In-Person Troop/Group Meeting Guidelines laid out in Girl Scouts Together will be upheld and followed at all in-person events. -
Evidence Report: Risk of Adverse Cognitive Or Behavioral Conditions
Evidence Report: Risk of Adverse Cognitive or Behavioral Conditions and Psychiatric Disorders Human Research Program Behavioral Health and Performance Approved for Public Release: April 11, 2016 National Aeronautics and Space Administration Lyndon B. Johnson Space Center Houston, Texas 1 CURRENT CONTRIBUTING AUTHORS: Kelley J. Slack, Ph.D. Wyle Science Technology & Engineering Thomas J. Williams, Ph.D. Wyle Science Technology & Engineering Jason S. Schneiderman, Ph.D. Wyle Science Technology & Engineering Alexandra M. Whitmire, Ph.D. Wyle Science Technology & Engineering James J. Picano, Ph.D. Universities Space Research Association PREVIOUS CONTRIBUTING AUTHORS: Lauren B. Leveton, Ph.D. NASA Johnson Space Center Lacey L. Schmidt, Ph.D. Minerva Work Solutions Camille Shea, Ph.D. Houston Police Department 2 TABLE OF CONTENTS I. PRD RISK TITLE: RISK OF ADVERSE COGNITIVE OR BEHAVIORAL CONDITIONS AND PSYCHIATRIC DISORDERS ............................................................................................. 6 II. EXECUTIVE SUMMARY .................................................................................................... 9 III. INTRODUCTION ................................................................................................................ 11 IV. EVIDENCE ........................................................................................................................... 14 A. Space Flight Evidence .................................................................................................... 17 1. Sources -
Apollo 17 Index: 70 Mm, 35 Mm, and 16 Mm Photographs
General Disclaimer One or more of the Following Statements may affect this Document This document has been reproduced from the best copy furnished by the organizational source. It is being released in the interest of making available as much information as possible. This document may contain data, which exceeds the sheet parameters. It was furnished in this condition by the organizational source and is the best copy available. This document may contain tone-on-tone or color graphs, charts and/or pictures, which have been reproduced in black and white. This document is paginated as submitted by the original source. Portions of this document are not fully legible due to the historical nature of some of the material. However, it is the best reproduction available from the original submission. Produced by the NASA Center for Aerospace Information (CASI) Preparation, Scanning, Editing, and Conversion to Adobe Portable Document Format (PDF) by: Ronald A. Wells University of California Berkeley, CA 94720 May 2000 A P O L L O 1 7 I N D E X 7 0 m m, 3 5 m m, A N D 1 6 m m P H O T O G R A P H S M a p p i n g S c i e n c e s B r a n c h N a t i o n a l A e r o n a u t i c s a n d S p a c e A d m i n i s t r a t i o n J o h n s o n S p a c e C e n t e r H o u s t o n, T e x a s APPROVED: Michael C .