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The Solar Cruiser Mission: Demonstrating Large Solar Sails for Deep Space Missions
The Solar Cruiser Mission: Demonstrating Large Solar Sails for Deep Space Missions Les Johnson*, Frank M. Curran**, Richard W. Dissly***, and Andrew F. Heaton* * NASA Marshall Space Flight Center ** MZBlue Aerospace NASA Image *** Ball Aerospace Solar Sails Derive Propulsion By Reflecting Photons Solar sails use photon “pressure” or force on thin, lightweight, reflective sheets to produce thrust. NASA Image 2 Solar Sail Missions Flown (as of October 2019) NanoSail-D (2010) IKAROS (2010) LightSail-1 (2015) CanX-7 (2016) InflateSail (2017) NASA JAXA The Planetary Society Canada EU/Univ. of Surrey Earth Orbit Interplanetary Earth Orbit Earth Orbit Earth Orbit Deployment Only Full Flight Deployment Only Deployment Only Deployment Only 3U CubeSat 315 kg Smallsat 3U CubeSat 3U CubeSat 3U CubeSat 10 m2 196 m2 32 m2 <10 m2 10 m2 3 Current and Planned Solar Sail Missions CU Aerospace (2018) LightSail-2 (2019) Near Earth Asteroid Solar Cruiser (2024) Univ. Illinois / NASA The Planetary Society Scout (2020) NASA NASA Earth Orbit Earth Orbit Interplanetary L-1 Full Flight Full Flight Full Flight Full Flight In Orbit; Not yet In Orbit; Successful deployed 6U CubeSat 90 Kg Spacecraft 3U CubeSat 86 m2 >1200 m2 3U CubeSat 32 m2 20 m2 4 Near Earth Asteroid Scout The Near Earth Asteroid Scout Will • Image/characterize a NEA during a slow flyby • Demonstrate a low cost asteroid reconnaissance capability Key Spacecraft & Mission Parameters • 6U cubesat (20cm X 10cm X 30 cm) • ~86 m2 solar sail propulsion system • Manifested for launch on the Space Launch System (Artemis 1 / 2020) • 1 AU maximum distance from Earth Leverages: combined experiences of MSFC and JPL Close Proximity Imaging Local scale morphology, with support from GSFC, JSC, & LaRC terrain properties, landing site survey Target Reconnaissance with medium field imaging Shape, spin, and local environment NEA Scout Full Scale EDU Sail Deployment 6 Solar Cruiser Mission Concept Mission Profile Solar Cruiser may launch as a secondary payload on the NASA IMAP mission in October, 2024. -
The James Webb Space Telescope
The James Webb Space Telescope Jonathan P. Gardner NASA’s Goddard Space Flight Center http://jwst.nasa.gov Space Science Reviews, 2006, 123/4, 485 1 James Webb Space Telescope Integrated Science Primary Mirror Instrument Module (ISIM) • 6.6m Telescope • Successor to Hubble & Spitzer. • Demonstrator of deployed optics. Secondary • 4 instruments: 0.6 to 28.5 μm Mirror • Passively cooled to < 50 K. • Named for 2nd NASA Administrator 5 Layer Sunshield Spacecraft Bus • Complementary: 30m, ALMA, WFIRST, LSST • NASA + ESA + CSA: 14 countries • Lead: Goddard Space Flight Center • Prime: Northrop Grumman • Operations: STScI • Senior Project Scientist: Nobel Laureate John Mather • Launch date: October 2018 2 NIRCam: NIRSpec Imaging 0.6 – 5.0 µm Broad, med & narrow 10 sq. arcmin FOV 65 mas resolution Coronagraphy NIRCam FGS/NIRISS: NIRSpec: Guiding Multi-object: 10 sq. arcmin Slitless spectroscopy (R~150) IFU: 3x3 arcsec Exoplanet transits (R~750) R~100, R~1000, R~3000 Non-redundant mask MIRI: 5 – 28.5 µm 2 sq. arcmin FOV IFU R~3000 Coronagraphy FGS/NIRISS MIRI 4 Model-Dependent Rule of Thumb: Deep NIR Surveys • Ultra-deep, deep and deep-wide imaging surveys: • JWST will do at z~12 what HST is doing at z~6 • JWST will do at z~17 what HST is doing at z~9 CANDELS UDF COSMOS 5 15 Angular Resolution 2 mm 10 5 per 1 kpc 3.6 mm NIRCam Pixels 0 0 10 20 Redshift NIRCam resolution JWST + NIRCam have enough resolution to study the structure of distant galaxies. The plots at right show the two-pixel resolution at 2 microns. -
JWST Project Status
James Webb Space Telescope JSTUC Project Status June 8, 2020 29 July 2011 11 Topics Project Status Observatory I&T Ground System and Operations Launch Vehicle Commissioning 2 Observatory Status 3 Observatory Major Accomplishments Completed Deployment Tower Assembly (DTA) deployment/stow (#1) Completed Sunshield Deployment Completed Sunshield Membrane Folding Completed anomalous Command/Telemetry Processor (CTP) and Traveling Wave Tube Amplifier (TWTA) replacements Root cause for both anomalous flight boxes identified – both random part failures which don’t impugn other units Deployed/Stowed Primary Mirror Wings as part of Observatory Pre- Environmental Deployments MIRI Cryocooler Fill Complete Sunshield (SS) Bi-Pod First Motion Test Successfully Complete DTA Deployment (#2) Complete Partial Stow SS Unitized Pallet Structure Complete 4 TWTA and CTP Replacement 5 Deployed Primary Mirror 6 Sunshield Preps For Folding 7 Remaining I&T Activities Spacecraft Elem. Observatory Observatory Post-environmental Pre-environmental Environmental Deployments Deployments Tests Completed In Progress Begins in Aug. Observatory Observatory Post-environmental Deployments Final Build 8 Remaining I&T Activities SCE Post SCE OTIS/SCE / Environment Reconfigure Deployments SCE for OTIS Integration OTIS Integration (Part 1) 2 DTA Deploy Sunshield Sunshield Fold J2 Panel Stow Deployment Sunshield Preps for Repairs & Sunshield Stow DTA #1 Opening Midbooms #1 Membranes Folding Updates Membranes Propulsion SCE Post-Env MRD Install GAA ROM SCE Deployment -
NASA Next Editor at the Gas Giant, Orbiting Jupiter 37 Core
MAY 2016 1 NASAnext National Aeronautics and Space Administration next NASAempowering the next generation of space explorers OSIRIS-REx NASA’s asteroid sampling mission takes off PAGE 6 www.nasa.gov MAY 2016 MAY 2016 2 3 NASAnext NASAnext Dear Reader, Humans are curious; they love to explore. Throughout our history, man has tirelessly pursued the next hori- zon. The same is true of our scientists and engineers. NASA’s missions and accomplish- ments are a direct result of this ines- capable curiosity and thirst for explo- ration. To many of our scientists and engineers, space is the final frontier — a place of endless discovery. Our eyes are fixed on this frontier. NASA’s Hubble Space Telescope has helped scientists uncover some of the most distant objects ever seen. We observed the Juno spacecraft make A meteor streaks across the sky during the annual Perseid meteor shower on Aug. its arrival at Jupiter this summer. In 12, 2016, in West Virginia. What have you seen in the night sky? NASA/Bill Ingalls fall, we watch as OSIRIS-REx trav- els to a near-Earth asteroid known as Bennu to retrieve a sample and send it back to Earth. SEPTEMBER 2016 But our scientists and engineers juno know that we also must keep a close meets a 3 Juno meets a giant eye on our own planet. Warmer than NASA/JPL-Caltech average temperatures and disappear- ing sea ice are indicators that our 4 NASA’s NICER planet is changing. NASA continuous- ly monitors and studies these chang- giant 5 One planet, two suns es to help us understand the future of upiter has captivated people sky, Jupiter’s magnetic field would ap- our home. -
James Webb Space Telescope
Integrated Science Instrument Module NASA’s Goddard Space Flight Center Optical Telescope Element Mid-infrared Instrument NASA/JPL, ESA Telescope Design and Deployment Near-infrared Spectrograph Northrop Grumman European Space Agency (ESA) Optical Telescope and Mirror Near-infrared Camera Design University of Arizona Ball Aerospace Fine Guidance Sensor Telescope Structures Canadian Space Agency Alliant Techsystems James Optical Telescope Integration and Test ITT/Exelis Webb Mirror Manufacturing Beryllium Mirror Blanks Brush Wellman Space Mirror Machining Axsys Technologies For more information, please contact: Telescope Mirror Grinding and Polishing SSG/Tinsley Laboratories Northrop Grumman Aerospace Systems Blake Bullock Milestone 310-813-8410 Achievements [email protected] in 2012 Christina Thompson 310-812-2375 [email protected] Spacecraft Bus Northrop Grumman Sunshield Northrop Grumman ManTech/NeXolve Webb Telescope Operating in space nearly a million miles from Earth and protected by its tennis court-sized, five-layer sunshield, the Webb Telescope will be shielded from sunlight and kept cool at a temperature of approximately www.northropgrumman.com 45 Kelvin (-380° F). This extreme cold enables Webb’s infrared © 2012 Northrop Grumman Systems Corporation Printed in USA sensors to see the most distant galaxies and to peer through galactic CBS Bethpage dust into dense clouds where star and galaxy formation take place. 12-2339 • AS • 12/12 • 43998-12 Northrop Grumman is under contract to NASA’s Goddard Space Flight Center in Greenbelt, Md., for the design and development of the Webb Telescope’s optics, sunshield and spacecraft. James Webb Space Telescope assembly is a critical component of the spacecraft that closes the Webb’s Far-reaching Achievements in 2012 mission data link to NASA’s Deep Space Network that will transmit the he James Webb Space Telescope is NASA’s top science mission telescope’s data from its orbit nearly a million miles from Earth. -
James Webb Space Telescope | Handbook James Webb Space Telescope | Handbook
James Webb Space Telescope | Handbook James Webb Space Telescope | Handbook Contents 1. Introduction 2 2. Design 3 2.1 Development timeline 3 2.2 Testing 4 2.3 Sunshield 4 2.4 Mirror 6 2.5 Instruments 7 3. Mission 9 3.1 Infrared light 9 3.2 First light 10 3.3 Formation and evolution of galaxies 11 3.4 Formation of stars and planetary systems 12 3.5 Planetary systems and the origins of life 12 4. Taking Webb into schools 13 5. Glossary 14 6. Useful links 15 Note: numbers in square brackets, e.g. [1] refer to entries in the glossary. James Webb Space Telescope | Handbook 1. Introduction This guide contains information about the James Webb Space Telescope. Webb is a collaboration between ESA, NASA, and the Canadian Space Agency. It is named after the NASA administrator James E. Webb who oversaw the first human spaceflight programmes of Mercury and Gemini and the establishment of the Apollo missions. Webb is the largest space telescope ever built and it will see objects up to 100 times fainter than those the Hubble Space Telescope can see. Hubble observes mainly visible light but Webb will use infrared light. Infrared light allows scientists to see further back in time to when the earliest stars and galaxies formed and into areas where visible light cannot get through, such as clouds of gas where stars and planets form. Scientists will use these observations to understand as much as possible about how the Universe evolved into what is seen today. Thousands of engineers and scientists from across the world have worked together for over twenty years to design and develop the technologies required for such a large and complex telescope. -
To Appear in Cometary Nuc/Ei in Space and Time, Ed. M. F. A’Hearn, ASP Conference Series, 1999
To appear in Cometary Nuc/ei in Space and Time, ed. M. F. A’Hearn, ASP Conference Series, 1999 Comet Missions in NASA’s New Millennium Program Paul R. Weissman Earth and Space Sciences Division, Jet Propulsion Laboratory, Mail stop 183-601, 4800 Oak Grove Drive, Pasadena, CA 91109 USA Abstract. NASA’s New Millennium Program (NMP) is designed to develop, test, and flight validate new, advanced technologies for plane- tary and Earth exploration missions, using a series of low cost space- craft. Such new technologies include solar-electric propulsion, inflatable- rigidizable structures, autonomous navigation and maneuvers, advanced avionics with low mass and low power requirements, and advanced sensors and concepts for science instruments. Two of NMP’s currently identified interplanetary missions include encounters with comets. The first is the Deep Space 1 mission which was launched in October, 1998 and which will fly by asteroid 1992 KD in 1999 and possibly comet Wilson-Harrington and/or comet Borrelly in 2001. The second NMP comet mission is Deep Space 4/Champollion which will be launched in April, 2003 and which will rendezvous with, orbit and land on periodic comet Tempel 1 in 2006. DS-4/Champollion is a joint project with CNES, the French space agency. 1. Introduction The advent of small, low-cost space missions has brought with it a need for new, advanced technologies which can enable productive missions with the smaller launch vehicles and payloads employed. In order to promote such technologies, NASA has created the New Millennium Program (NMP), administered by the Jet Propulsion Laboratory. New Millennium provides flight opportunities to validate new spacecraft, instrument, and operations technologies through a series of low cost missions. -
Orbit Transfer Problems and the Results You Obtained
MS&E 315 and CME 304 Solar sailing between Earth and Mars 1 Overview In this project, you will use your knowledge of nonlinear optimization to help a space agency design a cargo mission. The mission consists of making a cargo spacecraft perform interplanetary orbit transfers between Earth and Mars, and the agency is considering using a solar sail to propel the spacecraft. They need you to determine how the spacecraft should be operated to perform these orbit transfers in the shortest possible time for different solar sail technologies. 2 Mission information 2.1 Simplifications The agency has determined that the following simplifications are acceptable for your analysis: 1. Orbits are heliocentric, circular and co-planar. 2. Gravitational effects due to celestial bodies other than the Sun are ignored. 3. The Sun and spacecraft are modeled as point masses. 4. The Sun has spherically symmetric gravitational and radiation fields. 2.2 Problem description The problem you have to solve consists of determining how the solar sail of the spacecraft should be oriented to make the spacecraft perform each of the interplanetary orbit transfers Earth-Mars and Mars-Earth in the shortest possible time. You have to perform this analysis for some, say three, of the available solar sail technologies so that the agency can choose the most appropriate one in terms of cost and performance. Each solar sail technology is identified by a characteristic acceleration, as described in the next subsection. Figure1 shows a diagram of the orbits of interest, where rE and !E denote the radius and angular velocity, respectively, of Earth's orbit around the Sun, and rM and !M denote the radius and angular velocity, respectively, of Mars's orbit around the Sun. -
Hybrid Solar Sails for Active Debris Removal Final Report
HybridSail Hybrid Solar Sails for Active Debris Removal Final Report Authors: Lourens Visagie(1), Theodoros Theodorou(1) Affiliation: 1. Surrey Space Centre - University of Surrey ACT Researchers: Leopold Summerer Date: 27 June 2011 Contacts: Vaios Lappas Tel: +44 (0) 1483 873412 Fax: +44 (0) 1483 689503 e-mail: [email protected] Leopold Summerer (Technical Officer) Tel: +31 (0)71 565 4192 Fax: +31 (0)71 565 8018 e-mail: [email protected] Ariadna ID: 10-6411b Ariadna study type: Standard Contract Number: 4000101448/10/NL/CBi Available on the ACT website http://www.esa.int/act Abstract The historical practice of abandoning spacecraft and upper stages at the end of mission life has resulted in a polluted environment in some earth orbits. The amount of objects orbiting the Earth poses a threat to safe operations in space. Studies have shown that in order to have a sustainable environment in low Earth orbit, commonly adopted mitigation guidelines should be followed (the Inter-Agency Space Debris Coordination Committee has proposed a set of debris mitigation guidelines and these have since been endorsed by the United Nations) as well as Active Debris Removal (ADR). HybridSail is a proposed concept for a scalable de-orbiting spacecraft that makes use of a deployable drag sail membrane and deployable electrostatic tethers to accelerate orbital decay. The HybridSail concept consists of deployable sail and tethers, stowed into a nano-satellite package. The nano- satellite, deployed from a mothership or from a launch vehicle will home in towards the selected piece of space debris using a small thruster-propulsion firing and magnetic attitude control system to dock on the debris. -
Propulsion Systems for Interstellar Exploration
The Future of Electric Propulsion: A Young Visionary Paper Competition 35th International Electric Propulsion Conference October 8-12, 2017 Atlanta, Georgia Propulsion Systems for Interstellar Exploration Steven L. Magnusen Embry-Riddle Aeronautical University, Daytona Beach, FL, USA Alfredo D. Tuesta∗ National Research Council Postdoctoral Associate, Washington, DC, USA [email protected] August 4, 2017 Abstract The idea of manned spaceships exploring nearby star systems, although difficult and unlikely in this generation or the next, is becoming less a tale of science fiction and more a concept of rigorous scientific interest. In 2003, NASA sent two rovers to Mars and returned images and data that would change our view of the planet forever. Already, scientists and engineers are proposing concepts for manned missions to the Red Planet. As we prepare to visit the planets in our solar system, we dare to explore the possibilities and venues to travel beyond. With NASA’s count of known exoplanets now over 3,000 and growing, interest in interstellar science is being renewed as well. In this work, the authors discuss the benefits and deficiencies of current and emerging technologies in electric propulsion for outer planet and extrasolar exploration and propose innovative and daring concepts to further the limits of present engineering. The topics covered include solar and electric sails and beamed energy as propulsion systems. I. Introduction Te Puke is the name for the voyaging canoe that the Polynesians developed to sail across vast distances in the Pacific Ocean at the turn of the first millennium. This primitive yet sophisticated canoe, made of two hollowed out tree trunks and crab claw sails woven together from leaves, allowed Polynesian sailors to navigate the open ocean by studying the stars. -
Advancing Asteroid Surface Exploration Using Sublimate- Based Regenerative Micropropulsion and 3D Path Planning
Advancing Asteroid Surface Exploration Using Sublimate- Based Regenerative Micropropulsion And 3D Path Planning Item Type text; Electronic Thesis Authors Wilburn, Greg Publisher The University of Arizona. Rights Copyright © is held by the author. Digital access to this material is made possible by the University Libraries, University of Arizona. Further transmission, reproduction, presentation (such as public display or performance) of protected items is prohibited except with permission of the author. Download date 07/10/2021 15:36:40 Link to Item http://hdl.handle.net/10150/636641 ADVANCING ASTEROID SURFACE EXPLORATION USING SUBLIMATE-BASED REGENERATIVE MICROPROPULSION AND 3D PATH PLANNING by Greg Wilburn ____________________________ Copyright © Greg Wilburn 2019 A Thesis Submitted to the Faculty of the DEPARTMENT OF AEROSPACE AND MECHANICAL ENGINEERING In Partial Fulfillment of the Requirements For the Degree of MASTER OF SCIENCE In the Graduate College THE UNIVERSITY OF ARIZONA 2019 Acknowledgements The author would first like to thank his thesis committee members for their help and direction in solving some of the complex problems in this work. The author acknowledges the time and effort of his advisor, Dr. Jekan Thangavelauthum, for his guidance over the entire course of the project. Recognition is deserved for Dr. Erik Asphaug and Dr. Stephen Schwarz for their development of the AMIGO robot concept. The development of MEMS systems presented could not have been done without the coursework and guidance from Dr. Eniko Enikov. Special thanks goes to my friends and family who have supported and encouraged me through my graduate studies. I couldn’t have done it without you, Emilia! 3 Table of Contents I. -
Space Propulsion Technology for Small Spacecraft
Space Propulsion Technology for Small Spacecraft The MIT Faculty has made this article openly available. Please share how this access benefits you. Your story matters. Citation Krejci, David, and Paulo Lozano. “Space Propulsion Technology for Small Spacecraft.” Proceedings of the IEEE, vol. 106, no. 3, Mar. 2018, pp. 362–78. As Published http://dx.doi.org/10.1109/JPROC.2017.2778747 Publisher Institute of Electrical and Electronics Engineers (IEEE) Version Author's final manuscript Citable link http://hdl.handle.net/1721.1/114401 Terms of Use Creative Commons Attribution-Noncommercial-Share Alike Detailed Terms http://creativecommons.org/licenses/by-nc-sa/4.0/ PROCC. OF THE IEEE, VOL. 106, NO. 3, MARCH 2018 362 Space Propulsion Technology for Small Spacecraft David Krejci and Paulo Lozano Abstract—As small satellites become more popular and capa- While designations for different satellite classes have been ble, strategies to provide in-space propulsion increase in impor- somehow ambiguous, a system mass based characterization tance. Applications range from orbital changes and maintenance, approach will be used in this work, in which the term ’Small attitude control and desaturation of reaction wheels to drag com- satellites’ will refer to satellites with total masses below pensation and de-orbit at spacecraft end-of-life. Space propulsion 500kg, with ’Nanosatellites’ for systems ranging from 1- can be enabled by chemical or electric means, each having 10kg, ’Picosatellites’ with masses between 0.1-1kg and ’Fem- different performance and scalability properties. The purpose tosatellites’ for spacecrafts below 0.1kg. In this category, the of this review is to describe the working principles of space popular Cubesat standard [13] will therefore be characterized propulsion technologies proposed so far for small spacecraft.