The Initial Flight Anomalies Ofskyla P 3
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Space Administration
https://ntrs.nasa.gov/search.jsp?R=19700024651 2020-03-23T18:20:34+00:00Z TO THE CONGRESSOF THE UNITEDSTATES : Transmitted herewith is the Twenty-first Semiannual Repol* of the National Aeronautics and Space Administration. Twen~-first SEMIANNUAL REPORT TO CONGRESS JANUARY 1 - JUNE 30, 1969 NATIONAL AERONAUTICS AND SPACE ADMINISTRATION WASHINGTON, D. C. 20546 Editors: G. B. DeGennaro, H. H. Milton, W. E. Boardman, Office of Public Affairs; Art work: A. Jordan, T. L. Lindsey, Office of Organiza- tion and Management. For sale by the Superintendent of Documents, U.S. Government Printing Office Washington, D.C. 20402-Price $1.25 THE PRESIDENT May 27,1970 The White House I submit this Twenty-First Semiannual Report of the National Aeronautics and Space Aldministration to you for transmitttal to Congress in accordance with section 206(a) of the National Aero- nautics and Space Act of 1958. It reports on aotivities which took place betiween January 1 and June 30, 1969. During this time, the Nation's space program moved forward on schedule. ApolIo 9 and 10 demonstrated the ability of ;the man- ned Lunar Module to operate in earth and lunar orbit and its 'eadi- ness to attempt the lunar landing. Unmanned observatory and ex- plorer class satellites carried on scientific studies of the regions surrounding the Earth, the Moon, and the Sun; a Biosatellite oarwing complex biological science experiment was orbited; and sophisticated weather satellites and advanced commercial com- munications spacecraft became operational. Advanced research projects expanded knowledge of space flighk and spacecraft engi- neering as well as of aeronautics. -
Ceramic Matrix Composites with Nano Technology–An Overview
International Review of Applied Engineering Research. ISSN 2248-9967 Volume 4, Number 2 (2014), pp. 99-102 © Research India Publications http://www.ripublication.com/iraer.htm Ceramic Matrix Composites with Nano Technology–An Overview Saubhagya Sharma, Samresh Kumar Shashi and Vikram Tomar Department of Material Science & Nano Technology, University of Petroleum & Energy Studies, Dehradun, Uttrakhand. Abstract Ceramic matrix composites (CMCs) are promising materials for use in high temperature structural applications. This class of materials offers high strength to density ratios. Also, their higher temperature capability over conventional super alloys may allow for components that require little or no cooling. This benefit can lead to simpler component designs and weight savings. These materials can also contribute in increasing the operating efficiency due to higher operating temperatures being achieved. Using carbon/carbon composites with the help of Nanotechnology is more beneficial in structural engineering and can decrease the production cost. They can withstand high stresses and temperatures than the traditional alumina, silicon carbide which fracture easily under mechanical loads Fundamental work in processing, characterization and analysis is important before the structural properties of this new class of Nano composites can be optimized. The fields of the Nano composite materials have received a lot of attention to scientists and engineers in recent years. The fabrication of such composites using Nano technology can make a revolution in the field of material science engineering and can make the composites able to be used in long lasting applications. 1. Introduction As we know that Composite materials are the type of materials that are formed by combining two or more materials of different physical and chemical properties. -
Progress Report on Apollo Program
PROGRESS REPORT ON APOLLO PROGRAM Michael Collins, LCol. USAF (M) Astronaut NASA-MANNED SPACECRAFT CENTER It is a great pleasure to be here today and to greet you hardy suMvors of the pool party. I will do my best to avoid loud noises and bright colors during my status report. Since the last SETP Symposium, the Apollo Program has been quite busy in a number of different areas. (Figure 1) My problem is to sift through this information and to talk only about those things of most interest to you. First, to review briefly our hardware, we are talking about two different spacecraft and two different boosters. (Figure 2) The Command Module is that part of the stack COLLINS which makes the complete round trip to the moon. Attached to it is the Service Module, containing expendables and a 20,000 pound thrust engine for maneuverability. The Lunar Module will be carried on later flights and is the landing vehicle and active rendezvous partner. The uprated Saturn I can put the Command and Service Modules into earth orbit; the Saturn V is required when the Lunar Module is added. Since the last symposium, we have flown the Command and Service Modules twice and the Lunar Module once, all unmanned. Apollo 4, the first Saturn V flight, was launched in November 1967. (Figure 3) The Saturn V did a beautiful, i.e. nominal, job of putting the spacecraft into earth parking orbit. After a coast period, the third stage (S-IVB by McDonnell Douglas) was ignited a second time, achieving a highly elliptical orbit. -
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 -
And Ground-Based Observations of Pulsating Aurora
University of New Hampshire University of New Hampshire Scholars' Repository Doctoral Dissertations Student Scholarship Spring 2010 Space- and ground-based observations of pulsating aurora Sarah Jones University of New Hampshire, Durham Follow this and additional works at: https://scholars.unh.edu/dissertation Recommended Citation Jones, Sarah, "Space- and ground-based observations of pulsating aurora" (2010). Doctoral Dissertations. 597. https://scholars.unh.edu/dissertation/597 This Dissertation is brought to you for free and open access by the Student Scholarship at University of New Hampshire Scholars' Repository. It has been accepted for inclusion in Doctoral Dissertations by an authorized administrator of University of New Hampshire Scholars' Repository. For more information, please contact [email protected]. SPACE- AND GROUND-BASED OBSERVATIONS OF PULSATING AURORA BY SARAH JONES B.A. in Physics, Dartmouth College 2004 DISSERTATION Submitted to the University of New Hampshire in Partial Fulfillment of the Requirements for the Degree of Doctor of Philosophy in Physics May, 2010 UMI Number: 3470104 All rights reserved INFORMATION TO ALL USERS The quality of this reproduction is dependent upon the quality of the copy submitted. In the unlikely event that the author did not send a complete manuscript and there are missing pages, these will be noted. Also, if material had to be removed, a note will indicate the deletion. UMT Dissertation Publishing UMI 3470104 Copyright 2010 by ProQuest LLC. All rights reserved. This edition of the work is protected against unauthorized copying under Title 17, United States Code. ProQuest LLC 789 East Eisenhower Parkway P.O. Box 1346 Ann Arbor, Ml 48106-1346 This dissertation has been examined and approved. -
Xii Multifunctional Composites 11 Thermal Protection Systems
xii Multifunctional Composites 11 Thermal protection systems, Maurizio Natali, Luigi Torre, and Jos´e Maria Kenny 337 11.1 The hyperthermal environment . 337 11.2 Non-ablative TPS materials . 339 11.2.1 NA-TPS on the Space Shuttle . 339 11.2.2 SSO reusable surface insulation . 341 11.2.3 Conclusion remarks on non-ablative TPS materials . 342 11.3 High temperature composites as polymeric ablatives . 342 11.4 Testing facilities . 348 11.4.1 The oxy-acetylene torch testbed - OATT . 349 11.4.2 The simulated solid rocket motor - SSRM . 349 11.4.3 Plasma jet torches . 351 11.4.4 Recession rate sensing techniques for TPSs . 352 11.5 PAs as thermal insulating materials . 356 11.5.1 Rigid HSMs . 356 11.5.2 Flexible HSMs for TPSs . 356 11.5.3 Elastomeric HSMs for SRMs . 357 11.6 Phenolic impregnated carbon ablators . 359 11.7 Differences between FRPAs and LCAs . 360 11.8 Nanostructured ablative materials . 360 11.8.1 Nanosilica as filler for traditional and nanostructured ablatives 363 Table of Contents xiii 11.8.2 Carbon nanofilaments based NRAMs . 366 11.9 Conclusions . 368 Bibliography . 369 Chapter 11 Thermal protection systems Maurizio Natali, Luigi Torre, and Jos´eMaria Kenny University of Perugia, Perugia, Italy Abstract Ablative materials play a vital role for the entire aerospace industry. Although some non-polymeric materials have been successfully used as ablatives, polymer ablatives (PA) represent the most versatile class of thermal protection system (TPS) materials. Compared with oxide, inorganic polymer, and metal based TPS materials, PAs have some intrinsic advantages, such as high heat shock resistance and low density. -
Highly Reliable 3-Dimensional Woven Thermal Protection System for Mars Sample Return
Highly Reliable 3-Dimensional Woven Thermal Protection System for Mars Sample Return Don Ellerby Presenting for Keith Peterson [email protected] (512) 650-0885 Co-Authors (alphabetical by last name), E. Christiansen, D. Ellerby, P. Gage, M. Gasch, D. Prabhu, J. Vander Kam , E. Venkatapathy, T. W hite This work is funded by NASA Ames IRAD PI: E. Venkatapathy ; Technical Lead: K. Peterson; 1 3D Woven for MSR - Overview • The MSR Challenge: – Reliability requirements for a Mars Sample Return (MSR) Earth Entry Vehicle (EEV) are expected to be more stringent than any mission flown to date. • This flows down to all EEV subsystems, including heat-shield TPS • Likely to be the key driver for design decisions in many subsystem trades. • The MSR formulation is holding an option to on-ramp a 3D-woven system. The goal of this effort is to: –Provide a recommended 3D woven TPS architecture for MSR using Risk Informed Decision Making (RIDM). • Risk Informed DeCision Making (RIDM): – MSR formulation will institute RIDM processes to select configurations it pursues in future design cycles. • RIDM is a deliberative process that uses a diverse set of performance measures, together with other considerations, to inform decision making. – RIDM acknowledges the inevitable gaps in technical information, and the need for incorporating the cumulative wisdom of experienced personnel to integrate technical and nontechnical factors in order to produce sound decisions. 2 Why 3D Woven on MSR? • All TPS systems under consideration have their own set of challenges: – Carbon-Carbon (Hot Structure): • Certification of thermal-structural performance during re-entry and at temperature under the high strain landing impact environment will be challenging. -
Aerothermodynamic Design of the Mars Science Laboratory Heatshield
Aerothermodynamic Design of the Mars Science Laboratory Heatshield Karl T. Edquist∗ and Artem A. Dyakonovy NASA Langley Research Center, Hampton, Virginia, 23681 Michael J. Wrightz and Chun Y. Tangx NASA Ames Research Center, Moffett Field, California, 94035 Aerothermodynamic design environments are presented for the Mars Science Labora- tory entry capsule heatshield. The design conditions are based on Navier-Stokes flowfield simulations on shallow (maximum total heat load) and steep (maximum heat flux, shear stress, and pressure) entry trajectories from a 2009 launch. Boundary layer transition is expected prior to peak heat flux, a first for Mars entry, and the heatshield environments were defined for a fully-turbulent heat pulse. The effects of distributed surface roughness on turbulent heat flux and shear stress peaks are included using empirical correlations. Additional biases and uncertainties are based on computational model comparisons with experimental data and sensitivity studies. The peak design conditions are 197 W=cm2 for heat flux, 471 P a for shear stress, 0.371 Earth atm for pressure, and 5477 J=cm2 for total heat load. Time-varying conditions at fixed heatshield locations were generated for thermal protection system analysis and flight instrumentation development. Finally, the aerother- modynamic effects of delaying launch until 2011 are previewed. Nomenclature 1 2 2 A reference area, 4 πD (m ) CD drag coefficient, D=q1A D aeroshell diameter (m) 2 Dim multi-component diffusion coefficient (m =s) ci species mass fraction H total enthalpy -
Enceladus, Moon of Saturn
National Aeronautics and and Space Space Administration Administration Enceladus, Moon of Saturn www.nasa.gov Enceladus (pronounced en-SELL-ah-dus) is an icy moon of Saturn with remarkable activity near its south pole. Covered in water ice that reflects sunlight like freshly fallen snow, Enceladus reflects almost 100 percent of the sunlight that strikes it. Because the moon reflects so much sunlight, the surface temperature is extremely cold, about –330 degrees F (–201 degrees C). The surface of Enceladus displays fissures, plains, corrugated terrain and a variety of other features. Enceladus may be heated by a tidal mechanism similar to that which provides the heat for volca- An artist’s concept of Saturn’s rings and some of the icy moons. The ring particles are composed primarily of water ice and range in size from microns to tens of meters. In 2004, the Cassini spacecraft passed through the gap between the F and G rings to begin orbiting Saturn. noes on Jupiter’s moon Io. A dramatic plume of jets sprays water ice and gas out from the interior at ring material, coating itself continually in a mantle Space Agency. The Jet Propulsion Laboratory, a many locations along the famed “tiger stripes” at of fresh, white ice. division of the California Institute of Technology, the south pole. Cassini mission data have provided manages the mission for NASA. evidence for at least 100 distinct geysers erupting Saturn’s Rings For images and information about the Cassini on Enceladus. All of this activity, plus clues hidden Saturn’s rings form an enormous, complex struc- mission, visit — http://saturn.jpl.nasa.gov/ in the moon’s gravity, indicates that the moon’s ture. -
Earthrise- Contents and Chapter 1
EARTHRISE: HOW MAN FIRST SAW THE EARTH Contents 1. Earthrise, seen for the first time by human eyes 2. Apollo 8: from the Moon to the Earth 3. A Short History of the Whole Earth 4. From Landscape to Planet 5. Blue Marble 6. An Astronaut’s View of Earth 7. From Cold War to Open Skies 8. From Spaceship Earth to Mother Earth 9. Gaia 10. The Discovery of the Earth 1. Earthrise, seen for the first time by human eyes On Christmas Eve 1968 three American astronauts were in orbit around the Moon: Frank Borman, James Lovell, and Bill Anders. The crew of Apollo 8 had been declared by the United Nations to be the ‘envoys of mankind in outer space’; they were also its eyes.1 They were already the first people to leave Earth orbit, the first to set eyes on the whole Earth, and the first to see the dark side of the Moon, but the most powerful experience still awaited them. For three orbits they gazed down on the lunar surface through their capsule’s tiny windows as they carried out the checks and observations prescribed for almost every minute of this tightly-planned mission. On the fourth orbit, as they began to emerge from the far side of the Moon, something happened. They were still out of radio contact with the Earth, but the on- board voice recorder captured their excitement. Borman: Oh my God! Look at that picture over there! Here’s the Earth coming up. Wow, that is pretty! Anders: Hey, don’t take that, it’s not scheduled. -
Final Report of the Opgt/Mjs Plasma Wave Science Team
1 September 1972 FINAL REPORT OF THE OPGT/MJS PLASMA WAVE SCIENCE TEAM Prepared by F. L. Scarf, Team Leader for National Aeronautical and Space Administration Washington, D.C. 205*t6 Contract NASW 2228 Space Sciences Department TRW Systems Group One Space Park Redondo Beach, California 902?8 4 Page 1 1. TEAM ORGANIZATION AND MEMBERSHIP The Plasma Wave Team Leader is Dr. F. L. Scarf of TRW Systems, and the official team members are Dr. D. A. Gurnett (University of Iowa), Dr. R. A. Helliwell (Stanford University), Dr. R. E. Holzer (UCLA), Dr. P. J. Kellogg (University of Minnesota), Dr. E. J. Smith (JPL), and Dr. E. Ungstrup (Danish Space Research Institute). Mr. A. M. A. Frandsen of JPL serves as Team Member and Experiment Representative. In addition, the Plasma Wave Team solicited the continuing support and assistance of several other outstanding scientists, and we have designated these participants as Team Associates; the Associates are Dr. N. M. Brice (Cornell University), Dr. D. Cartwright (University of Minnesota), Dr. R. W. Fredricks (TRW), Dr. H. B. Liemohn (Boeing), Dr. C. F. Kennel (UCLA), and Dr. R. Thome (UCLA) . 2. GENERAL TEAM ACTIVITIES FEBRUARY 1972-AUGUST 31, 1972 (See the mid-year report for a summary of the earlier work) During this period Dr. Scarf attended all SSG Meetings except the last one, where Dr. E. J. Smith represented the Plasma Wave Team. There were a number of Team Meetings and several additional .conferences at JPL concerning EMI and other potential spacecraft problems. The major development during this interval involved the decision not to go ahead with the Grand Tour. -
RECOVERY HELICOPTERS by John Stonesifer
RECOVERY HELICOPTERS By John Stonesifer The planning throughout the Mercury, Gemini, Apollo, Skylab, and Apollo-Soyuz Test Project (ASTP) programs to recover astronauts from a water landing after returning from space was to use helicopters operating from a carrier-type ship positioned in the Planned Landing Area. Early Mercury flights (Shepard, Freedom 7; Grissom, Liberty Bell 7; Glenn, Friendship 7) were supported by Marine squadrons using UH34D helicopters (Photo #1) operating from carrier-type ships for the Atlantic ocean recoveries. Carpenter’s flight, Aurora 7 following Glenn’s orbital flight, was again planned to land in the Atlantic and be supported by the Marine helicopters aboard the USS Intrepid. Recovery support for Carpenter’s landing rapidly changed when it was learned the spacecraft landed approximately 250 miles downrange from the Planed Landing Area. The landing was beyond the range for the Marine helicopters to immediately depart for the landing area. Aboard the Intrepid was a squadron of the larger, faster, greater- range SH-3A Sea King helicopters (Photo #2) that were just recently introduced to the fleet. Their mission during this deployment was primarily to practice their role of anti- submarine warfare while at sea en route to the assigned recovery station. However, when information became available that Carpenter was a considerable range downrange, decisions were made to utilize the SH-3A helicopters rather than the UH34D helicopters to fly to the landing. The swim teams and photographers quickly transferred their gear to the SH-3As and they sped to the scene. At the scene, pararescue jumpers had already parachuted from an Air Force plane to install the flotation collar and render assistance to Carpenter in his raft.