Chapter3 on Board the Space Station
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Lift Off to the International Space Station with Noggin!
Lift Off to the International Space Station with Noggin! Activity Guide for Parents and Caregivers Developed in collaboration with NASA Learn About Earth Science Ask an Astronaut! Astronaut Shannon Children from across the country had a Walker unique opportunity to talk with astronauts aboard the International Space Station (ISS)! NASA (National Aeronautics and Space Administration) astronaut Shannon Astronaut Walker and JAXA (Japan Aerospace Soichi Noguchi Exploration Agency) astronaut Soichi Noguchi had all of the answers! View NASA/Noggin Downlink and then try some out-of-this- world activities with your child! Why is it important to learn about Space? ● Children are naturally curious about space and want to explore it! ● Space makes it easy and fun to learn STEM (Science, Technology, Engineering, and Math). ● Space inspires creativity, critical thinking and problem solving skills. Here is some helpful information to share with your child before you watch Ask an Astronaut! What is the International Space Station? The International Space Station (ISS) is a large spacecraft that orbits around Earth, approximately 250 miles up. Astronauts live and work there! The ISS brings together astronauts from different countries; they use it as a science lab to explore space. Learn Space Words! Astronauts Earth An astronaut is someone who is Earth is the only planet that people have trained to go into space and learn lived on. The Earth rotates - when it is day more about it. They have to wear here and our part of the Earth faces the special suits to help them breathe. Sun, it is night on the other side of the They get to space in a rocket. -
Mission to Jupiter
This book attempts to convey the creativity, Project A History of the Galileo Jupiter: To Mission The Galileo mission to Jupiter explored leadership, and vision that were necessary for the an exciting new frontier, had a major impact mission’s success. It is a book about dedicated people on planetary science, and provided invaluable and their scientific and engineering achievements. lessons for the design of spacecraft. This The Galileo mission faced many significant problems. mission amassed so many scientific firsts and Some of the most brilliant accomplishments and key discoveries that it can truly be called one of “work-arounds” of the Galileo staff occurred the most impressive feats of exploration of the precisely when these challenges arose. Throughout 20th century. In the words of John Casani, the the mission, engineers and scientists found ways to original project manager of the mission, “Galileo keep the spacecraft operational from a distance of was a way of demonstrating . just what U.S. nearly half a billion miles, enabling one of the most technology was capable of doing.” An engineer impressive voyages of scientific discovery. on the Galileo team expressed more personal * * * * * sentiments when she said, “I had never been a Michael Meltzer is an environmental part of something with such great scope . To scientist who has been writing about science know that the whole world was watching and and technology for nearly 30 years. His books hoping with us that this would work. We were and articles have investigated topics that include doing something for all mankind.” designing solar houses, preventing pollution in When Galileo lifted off from Kennedy electroplating shops, catching salmon with sonar and Space Center on 18 October 1989, it began an radar, and developing a sensor for examining Space interplanetary voyage that took it to Venus, to Michael Meltzer Michael Shuttle engines. -
Space Station Intergovernmental Agreement
AGREEMENT AMONG THE GOVERNMENT OF CANADA, GOVERNMENTS OF MEMBER STATES OF THE EUROPEAN SPACE AGENCY, THJ3 GOVERNMENT OF JAPAN, THE GOVERNMENT OF THE RUSSIAN FEDERATION, AND THE GOVERNMENT OF THE UNITED STATES OF AMERICA CONCERNING COOPERATION ON THE CIVIL INTERNATIONAL SPACE STATION , - Table of Contents Arkle 1 Object and Scope Art~le 2 International Rights and Obhgatlons Article 3 Detimtlons Artxle 4 Cooperatmg Agencies Article 5 Reglstratlon, lunsd~cl~on and Control Article 6 Ownershrp of Elements and Equipment Article 7 Management Artxle 8 De&&d Des1811and Development Artde 9 Utthzation Article 10 Operation Article I I crew Article I2 Transportation Article 13 Communlcatrons Article I4 Evolution Article I5 Fundmg Article 16 Cross-Waiver of Liability Article I7 Llabillty Convention Article 18 Customs and Immigmtlon Article 19 Exchange of Data and Goods Article 20 Treatment of Data and Goods in Transit Article 2 1 Intellectual Property tiicle 22 Crimmal Junsdic~on Artxle 23 Consultations Article 24 Space StatIon Cooperation Review Alticle 25 Entry into Force Arlicle 26 Opmti~e Effect as between Certain PartIes Artxle 27 Amendments Article 28 Withdrawal Annex Space Station Elements to be Provided by the Partners I - II I The Government of Canada (heremafter also “Canada”), The Governments of the Kingdom of Belgium, the Kmgdom of Denmark, the French Republic, the Federal Republic of Germany, the Italian Repubhc, the Kmgdom of the Netherlands, the Kingdom of Norway, the Kingdom of Spam, the Kingdom of Sweden, the Swiss Confederation, and -
JUICE Red Book
ESA/SRE(2014)1 September 2014 JUICE JUpiter ICy moons Explorer Exploring the emergence of habitable worlds around gas giants Definition Study Report European Space Agency 1 This page left intentionally blank 2 Mission Description Jupiter Icy Moons Explorer Key science goals The emergence of habitable worlds around gas giants Characterise Ganymede, Europa and Callisto as planetary objects and potential habitats Explore the Jupiter system as an archetype for gas giants Payload Ten instruments Laser Altimeter Radio Science Experiment Ice Penetrating Radar Visible-Infrared Hyperspectral Imaging Spectrometer Ultraviolet Imaging Spectrograph Imaging System Magnetometer Particle Package Submillimetre Wave Instrument Radio and Plasma Wave Instrument Overall mission profile 06/2022 - Launch by Ariane-5 ECA + EVEE Cruise 01/2030 - Jupiter orbit insertion Jupiter tour Transfer to Callisto (11 months) Europa phase: 2 Europa and 3 Callisto flybys (1 month) Jupiter High Latitude Phase: 9 Callisto flybys (9 months) Transfer to Ganymede (11 months) 09/2032 – Ganymede orbit insertion Ganymede tour Elliptical and high altitude circular phases (5 months) Low altitude (500 km) circular orbit (4 months) 06/2033 – End of nominal mission Spacecraft 3-axis stabilised Power: solar panels: ~900 W HGA: ~3 m, body fixed X and Ka bands Downlink ≥ 1.4 Gbit/day High Δv capability (2700 m/s) Radiation tolerance: 50 krad at equipment level Dry mass: ~1800 kg Ground TM stations ESTRAC network Key mission drivers Radiation tolerance and technology Power budget and solar arrays challenges Mass budget Responsibilities ESA: manufacturing, launch, operations of the spacecraft and data archiving PI Teams: science payload provision, operations, and data analysis 3 Foreword The JUICE (JUpiter ICy moon Explorer) mission, selected by ESA in May 2012 to be the first large mission within the Cosmic Vision Program 2015–2025, will provide the most comprehensive exploration to date of the Jovian system in all its complexity, with particular emphasis on Ganymede as a planetary body and potential habitat. -
A Perspective on the Design and Development of the Spacex Dragon Spacecraft Heatshield
A Perspective on the Design and Development of the SpaceX Dragon Spacecraft Heatshield by Daniel J. Rasky, PhD Senior Scientist, NASA Ames Research Center Director, Space Portal, NASA Research Park Moffett Field, CA 94035 (650) 604-1098 / [email protected] February 28, 2012 2 How Did SpaceX Do This? Recovered Dragon Spacecraft! After a “picture perfect” first flight, December 8, 2010 ! 3 Beginning Here? SpaceX Thermal Protection Systems Laboratory, Hawthorne, CA! “Empty Floor Space” December, 2007! 4 Some Necessary Background: Re-entry Physics • Entry Physics Elements – Ballistic Coefficient – Blunt vs sharp nose tip – Entry angle/heating profile – Precision landing reqr. – Ablation effects – Entry G’loads » Blunt vs Lifting shapes – Lifting Shapes » Volumetric Constraints » Structure » Roll Control » Landing Precision – Vehicle flight and turn-around requirements Re-entry requires specialized design and expertise for the Thermal Protection Systems (TPS), and is critical for a successful space vehicle 5 Reusable vs. Ablative Materials 6 Historical Perspective on TPS: The Beginnings • Discipline of TPS began during World War II (1940’s) – German scientists discovered V2 rocket was detonating early due to re-entry heating – Plywood heatshields improvised on the vehicle to EDL solve the heating problem • X-15 Era (1950’s, 60’s) – Vehicle Inconel and Titanium metallic structure protected from hypersonic heating AVCOAT » Spray-on silicone based ablator for acreage » Asbestos/silicone moldable TPS for leading edges – Spray-on silicone ablator -
Chapter 3: Familiarizing Yourself with the Night Sky
Chapter 3: Familiarizing Yourself With the Night Sky Introduction People of ancient cultures viewed the sky as the inaccessible home of the gods. They observed the daily motion of the stars, and grouped them into patterns and images. They assigned stories to the stars, relating to themselves and their gods. They believed that human events and cycles were part of larger cosmic events and cycles. The night sky was part of the cycle. The steady progression of star patterns across the sky was related to the ebb and flow of the seasons, the cyclical migration of herds and hibernation of bears, the correct times to plant or harvest crops. Everywhere on Earth people watched and recorded this orderly and majestic celestial procession with writings and paintings, rock art, and rock and stone monuments or alignments. When the Great Pyramid in Egypt was constructed around 2650 BC, two shafts were built into it at an angle, running from the outside into the interior of the pyramid. The shafts coincide with the North-South passage of two stars important to the Egyptians: Thuban, the star closest to the North Pole at that time, and one of the stars of Orion’s belt. Orion was The Ishango Bone, thought to be a 20,000 year old associated with Osiris, one of the Egyptian gods of the lunar calendar underworld. The Bighorn Medicine Wheel in Wyoming, built by Plains Indians, consists of rocks in the shape of a large circle, with lines radiating from a central hub like the spokes of a bicycle wheel. -
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: -
TAKE-HOME EXP. # 1 Naked-Eye Observations of Stars and Planets
TAKE-HOME EXP. # 1 Naked-Eye Observations of Stars and Planets Naked-eye observations of some of the brightest stars, constellations, and planets can help us locate our place in the universe. Such observations—plus our imaginations—allow us to actively participate in the movements of the universe. During the last few thousand years, what humans have said about the universe based on naked-eye observations of the night and day skies reveals the tentativeness of physical models based solely on sensory perception. Create, in your mind's eye, the fixed celestial sphere. See yourself standing on the Earth at Observer's the center of this sphere. As you make the zenith + star-pattern drawings of this experiment, your perception may argue that the entire sphere of fixed star patterns is moving around the Earth and you. To break that illusion, you probably have to consciously shift your frame of º reference—your mental viewpoint, in this 50 up from the horizon case— to a point far above the Earth. From South there you can watch the globe of Earth slowly Observer on local horizon plane rotate you , while the universe remains essentially stationary during your viewing It is you that turns slowly underneath a fixed and unchanging pattern of lights. Naked eye observations and imagination has led to constellation names like "Big Bear" or "Big Dipper". These names don't change anything physically —except, and very importantly, they aid humans' memory and use of star patterns. A. Overview This experiment involves going outside to a location where you can observe a simple pattern of stars, including at least 2, but preferably 3 or 4 stars. -
Nature Detectives
Winter 2015 Star Light, Star Bright, Let’s Find Some Stars Tonight! Finding specific stars in the night sky might seem overwhelming. All those stars! At a glance stars look like a million twinkling points of light that are impossible to sort out. But with a little information, you may discover hunting some stars is not so difficult. Turns out we don’t see a million stars. Less than a couple thousand – and usually many fewer than that – are visible to most people’s unaided eyes. The brightest and nearest stars are easily found without a telescope or binoculars. Stars Are Not Star-shaped Stars are big balls of gas that give off heat and light. Sound familiar? Isn’t that what our Sun does? Guess what, our Sun is a star. It seems confusing, but all stars are suns. Like our Sun, stars are also in the daytime sky. During the day, the Sun lights up the atmosphere so we can’t see other suns… er…stars. Pull Out and Save Our Sun isn’t even the brightest star. In fact all the stars we see at night are bigger and brighter than the Sun. It wins the brightness contest during the day simply because it is incredibly closer than all the other stars. (At night we don’t see the Sun because of Earth’s rotation. Our Sun is shining on the opposite side of Earth and we are in darkness.) Suns or Stars Appear to Rise and Set Our view of the stars changes through the night as Earth makes its daily rotation. -
The International Space Station and the Space Shuttle
Order Code RL33568 The International Space Station and the Space Shuttle Updated November 9, 2007 Carl E. Behrens Specialist in Energy Policy Resources, Science, and Industry Division The International Space Station and the Space Shuttle Summary The International Space Station (ISS) program began in 1993, with Russia joining the United States, Europe, Japan, and Canada. Crews have occupied ISS on a 4-6 month rotating basis since November 2000. The U.S. Space Shuttle, which first flew in April 1981, has been the major vehicle taking crews and cargo back and forth to ISS, but the shuttle system has encountered difficulties since the Columbia disaster in 2003. Russian Soyuz spacecraft are also used to take crews to and from ISS, and Russian Progress spacecraft deliver cargo, but cannot return anything to Earth, since they are not designed to survive reentry into the Earth’s atmosphere. A Soyuz is always attached to the station as a lifeboat in case of an emergency. President Bush, prompted in part by the Columbia tragedy, made a major space policy address on January 14, 2004, directing NASA to focus its activities on returning humans to the Moon and someday sending them to Mars. Included in this “Vision for Space Exploration” is a plan to retire the space shuttle in 2010. The President said the United States would fulfill its commitments to its space station partners, but the details of how to accomplish that without the shuttle were not announced. The shuttle Discovery was launched on July 4, 2006, and returned safely to Earth on July 17. -
Butina Keynote
Vision A human outpost in space bringing nations together for the benefit of life on Earth… and beyond. We will make revolutionary discoveries and establish a permanent international presence of humans in space, to advance the exploration of the solar system and enable commerce in space. U.S. Core complete Mission Safely build, operate, and utilize a continuously inhabited orbital research facility through a partnership of governments, industries, and academia. International partner complete dimensions: 171 ft. long, 240 ft. wide, 90 ft. high, 15,000 cubic feet of living space. weight: 197 tons (404,000 lbs.) ISS today science capabilities: laboratories from four space agencies planned, U.S. Lab “Destiny” operating since Feb. 2001. orbital inclination/path: 51.6 degrees, covering 90% of the world’s population. altitude: approximately 240 miles above the Earth. speed: 17,500 miles per hour, orbiting the Earth 16 times a day. The International Space Station is more powerful, and 4 times larger, than any human space craft ever built. Over 100 people have visited the ISS so far, 17% for the second time. United States 16 International Participants Canada Russia Europe 5 International Partners Japan ISS Technical Configuration Elements Currently on Orbit Elements Pending US Shuttle Launch Science Power Module (SPM) Elements Pending Russian Launch Docking Compartment (DC) 1 Zarya Control Module Zvezda Service Module PMA 1 S1 Truss SO Truss Port SM MMOD Shields Segment Segment Photovoltaic AMS ULC1 P1 Truss Arrays ULC2 Port MT/ CETA Research Module (RM) Mobile Segment Rails S3/4 Truss Servicing Segment System P6 Truss Multipurpose Laboratory Segment Module (MLM) Express Pallets Starboard MT/ CETA Rails P5 Truss S6 Truss Segment Segment ESP-3 P3/4 Truss S5 Truss Segment Segment ESP-4 Canadarm2 Starboard Photovoltaic Arrays Dextre (SPDM) Mobile Remote Servicer Base System (MBS), JEM ELM-PS Mobile Transporter (MT) ESP-2 Z1 Truss Segment JEM RMS & Exposed Facility Airlock PMA 3 Node 1 Cupola U.S. -
Cubesat Mission: from Design to Operation
applied sciences Article CubeSat Mission: From Design to Operation Cristóbal Nieto-Peroy 1 and M. Reza Emami 1,2,* 1 Onboard Space Systems Group, Department of Computer Science, Electrical and Space Engineering, Luleå University of Technology, Space Campus, 981 92 Kiruna, Sweden 2 Aerospace Mechatronics Group, University of Toronto Institute for Aerospace Studies, Toronto, ON M3H 5T6, Canada * Correspondence: [email protected]; Tel.: +1-416-946-3357 Received: 30 June 2019; Accepted: 29 July 2019; Published: 1 August 2019 Featured Application: Design, fabrication, testing, launch and operation of a particular CubeSat are detailed, as a reference for prospective developers of CubeSat missions. Abstract: The current success rate of CubeSat missions, particularly for first-time developers, may discourage non-profit organizations to start new projects. CubeSat development teams may not be able to dedicate the resources that are necessary to maintain Quality Assurance as it is performed for the reliable conventional satellite projects. This paper discusses the structured life-cycle of a CubeSat project, using as a reference the authors’ recent experience of developing and operating a 2U CubeSat, called qbee50-LTU-OC, as part of the QB50 mission. This paper also provides a critique of some of the current poor practices and methodologies while carrying out CubeSat projects. Keywords: CubeSat; miniaturized satellite; nanosatellite; small satellite development 1. Introduction There have been nearly 1000 CubeSats launched to the orbit since the inception of the concept in 2000 [1]. An up-to-date statistics of CubeSat missions can be found in Reference [2]. A summary of CubeSat missions up to 2016 can also be found in Reference [3].