Experimental Study of Cavitation and Flow Instabilities in Space Rocket Turbopumps and Hydrofoils
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National Aeronautics and Educational Product Space Administration Teachers I Grades 2-6 I Office of Education and Human Resources Education Division _o N N cO 0 u_ 0 N t_ I ,.-, CO ,4" U O" 0_ _ Z _ 0 0 tM < u Is LIJ I-. _-.q4" W_ O ul ,,_ W;Z. INWel I I,,-. UJ .... 0,. i,-,{ .... u4 uJ I-,- .. IU_ Z_ .1 i ! I i I j | ] ROCKETS Physical Science Teacher's Guide with Activities National Aeronautics and Space Administration Office of Human Resources and Education Education Division This publication is in the Public Domain and is not protected by copyright. Permission is not required for duplication. EP-291 July 1993 Acknowledgments This publication was developed for the National Aeronautics and Space Administra- tion with the assistance of the many educa- tors of the Aerospace Education Services Program, Oklahoma State University. Writer: Gregory L. Vogt, Ed.D. Teaching From Space Program NASA Johnson Space Center Houston, TX Editor: Carla R. Rosenberg Teaching From Space Program NASA Headquarters Washington, DC Table of Contents How To Use This Guide ............................... 1 Activities and Demonstration Matrix ............. 2 Brief History of Rockets ................................ 3 Rocket Principles ......................................... 8 Practical Rocketry ...................................... 12 Activities and Demonstrations .................... 19 Glossary ..................................................... 40 NASA Educational Materials And Suggested Readings .......................... 41 NASA Educational Resources ................... 42 Evaluation Card ..................................... Insert ii How To Use This Guide vehiclesockets arein theexistence.oldest formEarlyofrocketsself-containedwere in use more than two thousand years ago. Over a long and exciting history, rockets have evolved from simple tubes filled with black powder into mighty vehicles capable of launching a spacecraft out into the galaxy. -
Howard Seifert Papers
http://oac.cdlib.org/findaid/ark:/13030/tf0z09n4j4 No online items Guide to the Howard Seifert Papers Daniel Hartwig Stanford University. Libraries.Department of Special Collections and University Archives Stanford, California 2001 Copyright © 2015 The Board of Trustees of the Leland Stanford Junior University. All rights reserved. Note This encoded finding aid is compliant with Stanford EAD Best Practice Guidelines, Version 1.0. Guide to the Howard Seifert SC0173 1 Papers Overview Call Number: SC0173 Creator: Seifert, Howard, 1911-1977 Creator: Seifert,, 1911-1977. Title: Howard Seifert papers Dates: 1960-1977 Physical Description: 39.5 Linear feet Language(s): The materials are in English. Repository: Department of Special Collections and University Archives Green Library 557 Escondido Mall Stanford, CA 94305-6064 Email: [email protected] Phone: (650) 725-1022 URL: http://library.stanford.edu/spc Custodial History Gift of Mrs. Howard Seifert, 1977, and administrative transfer, Department of Aeronautics and Astronautics, 1979. Information about Access None. Ownership & Copyright Property rights reside with the repository. Literary rights reside with the creators of the documents or their heirs. To obtain permission to publish or reproduce, please contact the Public Services Librarian of the Dept. of Special Collections and University Archives. Cite As [Identification of item], Howard Seifert Papers, SC 173, Stanford University Archives, Stanford, Calif. Biography Howard Seifert, an authority on rocket propulsion of space vehicles, was professor of aeronautics and astronautics at Stanford from 1960 to 1976. He also directed the Physical Sciences Laboratory at the United Aircraft Corporation (1960-65) and was president of the American Rocket Society (1960). Before joining the Stanford faculty, he was on the staff at the Jet Propulsion Laboratory and Space Technology Laboratories and a visiting professor at UCLA. -
Review of Advance Rocket Engine
International Journal of Science and Research (IJSR) ISSN: 2319-7064 ResearchGate Impact Factor (2018): 0.28 | SJIF (2018): 7.426 Review of Advance Rocket Engine Sanjana Sharma Research Scholar, Chandigarh University, Punjab (India) Abstract: The rocket engine is the main and very important part of the space transportation system. In this paper an attempt has been made about the history of Rocket Engine, types of Rocket Engines and future scope in the technology of theRocket Engines. Also, an attempt about physics behind the jets, and advantages and disadvantages of every rocket engine is made in this review paper. 1. Introduction creating incendiary weapons from the mid-eighth to the end of the thirteenth century—two of which are rockets. The first Rocket Engines are basically used to store the rocket mass of recipe calls for one part, which is sulfur, added to six parts rocket propellant for forming its high speed propulsive jet. of saltpeter (potassium nitrate) dissolved in laurel oil, then Those vehicles which are propelled by rocket engines are inserted into hollow wood and lit to actually fly away commonly known as rockets. Rockets function on the whenever you want, to whatever destination you wish and principle of Newton’s 3rd law of motion. We always see that burn up everything. The second recipe combines a pound of most of the rocket engines use combustion, but non- sulfur, two pounds of charcoal, and six pounds of saltpeter— combusting (such as cold gas thrusters) forms also exist. all finely powdered on a marble slab. Then this powder mixture is packed firmly into a long and narrow case. -
The International Space Transit Vehicle Concept
Construction of an International Space Transit Vehicle Using the Space Station Dan Roukos* and Madhu Thangavelu† University of Southern California, Los Angeles, CA 90089-1191 Figure 1: ISV in Space _______________________________ *Graduate Student, Department of Astronautical Engineering, Viterbi School of Engineering, University of Southern California, Los Angeles, CA †Conductor, ASTE 527 Space Concepts Studio, Department of Astronautical Engineering, Viterbi School of Engineering, Graduate Thesis Advisor, School of Architecture, University of Southern California, Los Angeles, CA, AIAA Member 1 Abstract After abandoning the possibility of directly evolving the ISS for cislunar, lunar orbital or interplanetary applications, we looked at the potential of the ISS as the prime and opportune assembly node for such missions beyond LEO. We note that space station concepts in the past have referred to such a facility in LEO for this purpose; a manned station in LEO to build large vehicles and structures for outbound destinations, since such systems cannot be lofted directly from the Earth, using current technology. The International Space Vehicle (ISV), as shown in figure 1, is a concept architecture for a new kind of spacecraft presented here as the initial platform for evolving systems for space exploration and extraterrestrial settlement goals set by the U.S. and shared by the world; namely manned return to the Moon and manned missions to Mars and beyond. The nature of these missions, using current technology, demand long duration manned space presence for several years. No vehicle built or planned yet, with the partial exception of the ISS, which requires constant logistics support from Earth, can effectively support life in space for such periods. -
Richard Nakka's Experimental Rocketry Web Site
Richard Nakka's Experimental Rocketry Web Site Solid Propellant Burn Rate • Introduction • What Influences Burning Rate? • Modification of Burning Rate • Combustion Process • Burn Rate Measurement Introduction The burning surface of a rocket propellant grain recedes in a direction perpendicular to this burning surface. The rate of regression, typically measured in inches per second (or mm per second), is termed burning rate (or burn rate). This rate can differ significantly for different propellants, or for one particular propellant, depending on various operating conditions as well as formulation. Knowing quantitatively the burning rate of a propellant, and how it changes under various conditions, is of fundamental importance in the successful design of a solid rocket motor. This web page discusses the factors that influence burn rate, how it may be modified, how the burn rate can be determined experimentally, and the physical processes that occur at the burning surface of a propellant that governs the burning rate. What Influences Burning Rate? An illustration of the concept of burning surface regression is given in Figure 1, for a section of a hollow cylindrical grain, with an inhibited outer surface ( "inhibited" means that the propellant surface is protected from the heat of combustion and as such, burning does not occur). Burning commences along the length of the central core, with the burning surface receding radially outward (shown at arbitrary times t1, t2, t3). Note that the burning surface area (represented by the arc length of the red lines in this figure) is continually increasing. Also note that the surface regression rate (burn rate) is not constant. -
Work Breakdown Structure (WBS) • Milestone Schedule • Funding and Personnel Resources • WBS Details PROGRAM ROAD MAP
INTRODUCTION • Background • Hydrogen vs. Water • Project Objective • Program Plan Status • Conclusions To Date ISRU BACKGROUND • "ISRU" -- Insitu Space Resource Utilization • The Utilization of Lunar Water Ice Near the Lunar Poles (cold traps) Is Expected to Have a Dramatic Effect on the Affordability of Future Lunar and Mars Exploration and Colonization • The Latest Lunar Prospector Data Indicates up to 260 Million Tons of Water Ice is Present • The Use of Water Includes: Hydrogen and Oxygen Propellants for: Space Transport Systems, Life Support, Food Production, Chemical Energy Storage, Rover Fuels/Oxidizers, Concrete Production for Infrastructure, etc. • The Discovery and Use of Water Ice on the Moon is a Tremendously Important Event for Man's Exploration and Colonization of the Solar System • In This Effort, We Are Developing a Detailed Program Plan that NASA May Choose to Use to “Discover, Extract and Use” Lunar Water or Lunar Hydrogen and Oxygen LUNAR PROSPECTOR DATA WATER VS. HYDROGEN • Lunar Prospector’s Neutron Spectrometer (NS) is Designed to Detect the Presence of Hydrogen, which Is Believed by Many to Indicate the Presence of Water Ice • Current Data Indicate up to 260 Million Metric Tons of Water Ice Have Been Predicted by the Science Team, (July 1999) • Estimates Indicate 200 Million MT at the South Pole and 60 Million MT at the North Pole • Ice Likely in Deposites of Pure Water Ice Burried Beneath ~5 cm of Dry Regolith in ~1.5% Concentrations • Concentrations Appear Higher at the North Pole • Kulcinski, Schmidt and Others -
High Frontier 4 All Module 1: by Phil Eklund & Jeffrey
HIGH FRONTIER 4 ALL MODULE 1: BY PHIL EKLUND & JEFFREY CHAMBERLAIN MODULE 1 - TERAWATT | HIGH FRONTIER 4 ALL | 1 High Frontier 4 Module for 1 to 5 players Updated Feb, 2021. 2 | HIGH FRONTIER 4 ALL | MODULE 1 - TERAWATT 1A. Module 1 This terawatt module introduces two new patent decks: Freighters (1B) and GW/TW Thrusters (1C). Freighters are a new type of patent card allowing the transport of valuable factory goods back to LEO. GW/TW thrusters are more powerful and efficient versions of the MW thrusters of the core game, allowing your Spacecraft to reach the outer planets more easily. This module also optionally introduces Futures, special game goals to earn victory points. a. The Cover Painting by Nick Stevens depicts the 2-stage starship Daedalus, designed by the British Interplanetary Society. It has a Wet Mass of 1350 and a Dry Mass of 100. First stage power is 40 TW. 1A1. Module 1 Components 1 Drawer Box 1 Rules Booklet 5 Playmat Extensions 5 Big Wooden Cubes (12mm, in 5 player colors) for Freighters 30 Gold Plastic Beads for Isotope FT 10 Wooden Stars for Futures. 8 Wooden Sticks for Space Elevators 7 GW/TW Thruster Cards 7 Freighter Fleets Cards 4 Ziplock Bags 1A2. Module 1 Setup Setup is per core setup (C), except during patent decks setup (C4) include Freighter cards and GW/TW thruster cards as two extra patent decks with Black-Side faceup, and give each player their big wooden cube for their Freighter Figure. a. Freighter Cards & GW/TW Thruster Cards are black on one side, and purple on the other. -
Propulsion to Moons of Jupiter Using Heat and Water Without Electrolysis Or Cryogenics
Space Exploration 2005 SESI Conference Series, Vol. 001, 2005 A. C. Zuppero Propulsion to Moons of Jupiter Using Heat and Water Without Electrolysis Or Cryogenics Anthony Zuppero1 1NeoKismet, L.L.C., 456 Montgomery Ste 1350, San Francisco, CA 44104 USA Abstract. Exploration of the inner solar system during the last 20 years revealed the existence of many water objects. They include hydrated minerals in the near earth asteroids, ice on Earth's moon, water ice moons, and ice lakes on planets and moons. Examination of the composition and hardness properties of the objects revealed that the use of heat alone, at temperatures well below the melting point of rock, would release water vapor or water. Research dating from the 1960's demonstrated the technology to use water as the coolant in nuclear reactors at temperatures up to 1100 Kelvin without significant wear or erosion of the nuclear system. In a nuclear rocket, nuclear heated coolants flow directly from the reactor core into a rocket nozzle bolted on the reactor. The coolants boil to vapor and propell the rocket. The combination of these elements permitted use of the water from space as a propellant for inner solar system exploration. Two mission options were compared. Each would deliver a net 10,000 tons of useful space ship payload to Callisto, a moon of Jupiter. The H2O option uses water as propellant and only thermal processes. The other, cryogenic option uses liquid hydrogen (LH2) as propellant and electricity to split water and for cryo systems. Both systems get all their water from space. -
Rockets Educator Guide
ROCKETS A Teacher's Guide with Activities In Science, Mathematics, and Technology National Aeronautics and Space Administration Office of Human Resources and Education Education Division Washington, DC Education Working Group NASA Johnson Space Center Houston, Texas This publication is in the Public Domain and is not protected by copyright. Permission is not required for duplication. EG-1999-06-108-HQ Acknowledgments This publication was developed for the National Aeronautics and Space Administration with the assistance of hundreds of teachers in the Texas Region IV area and educators of the Aerospace Education Services Program, Oklahoma State University. Writers: Deborah A. Shearer Gregory L. Vogt, Ed.D. Teaching From Space Program NASA Johnson Space Center Houston, TX Editor: Carla B. Rosenberg Teaching From Space Program NASA Headquarters Washington, DC Special Thanks to: Timothy J. Wickenheiser Chief, Advanced Mission Analysis Branch NASA Lewis Research Center Gordon W. Eskridge Aerospace Education Specialist Oklahoma State University Dale M. Olive Teacher, Hawaii i ii Table of Contents How To Use This Guide ............................... 1 Activity Format ............................................. 3 Brief History of Rockets................................ 5 Rocket Principles ....................................... 13 Practical Rocketry ...................................... 18 Launch Vehicle Family Album .................... 25 Activities ..................................................... 35 Activity Matrix ...................................... -
To Inhabit the Solar System\- CHAPTERS Drafts\To Occupy the Solar System GRAPHICS\Cromeo3.Jpg Nuclear Explosions Would Power Dyson's "Orion Starship"
copyright © 2009 by Anthony Zuppero 1 of 417 copyright © 2009 by Anthony Zuppero inhabit 20091203_1405.doc 12/3/2009 2:37:32 PM copyright © 2009 by Anthony Zuppero CHAPTER 1 The neo solar system The Exodus Path, My Struggle. and Jupiter, Saturn. Although I really did find a way to power the rockets to take hundreds of us throughout the solar system, the only product of my Water in space turned out to be everywhere, from the planet entire career struggle working in so-called "rocket science," was Mercury in its the forever dark craters, in the moon, and in that people wanted to hear the story. mostly everything to way past at least Pluto, As the "Featured Evening Speaker", again and again, they would Long ago, when people landed on the moon and when Star keep me long after I was finished talking, asking me questions. Trek inspired us, we thought we could just go there, to space, to What was so captivating? Was it the stories about how we can the moon, to other planets like Mars or Mercury. But at every actually leave the Earth? Or was it just that I was telling them turn, we discovered another bad thing to stop us. stories and entertaining them? Or was it my struggle against the real world and reality? I can't tell, so I am telling the story We did not find what we needed to live, like water. Our rocket ships were too feeble, too huge, too expensive, and blew up too The struggle to make a Vision come alive, a kind of Exodus Path often. -
PERMANENT – Chapter 3 – Transportation of Earth, Lunar and Asteroidal Materials 1 Overview – Transport of Earth, Lunar
PERMANENT – Chapter 3 – Transportation of Earth, Lunar and Asteroidal Materials Excerpts from a website developed by physicist Mark Prado on issues related to space transportation and resources. [www.permanent.com] 1 Overview – Transport of Earth, Lunar and Asteroidal Materials The main barrier to space development is the cost of getting there. For example, the current Space Shuttle cost is around $12,000 per kilogram, and near future rockets are almost certainly not going to be able to deliver for less than $2000/kg. That is why we are looking at using materials already in space – getting materials from asteroids near Earth and the Moon. After all, the settlers of America didn’t bring from Europe all their bricks, wood, cement, food, water, etc. This section explains the differences in transportation costs between delivery from Earth, the Moon, and asteroids near Earth, both theoretically and by practical engineering methods. Different transportation technologies are compared, with an emphasis on practical, near term solutions. There are two factors that determine the economics of space transportation: 1. Theoretical requirements, i.e., the minimum energy required to go from one place to another due to gravity without considering any other requirements, and 2. Practical means, i.e., the cost of producing and operating vehicles. The relative weight of these two factors varies, depending on origin and destination. The effort required to transport a particular payload from one point to another in space is often compared in terms of “delta-v” – the total velocity change you would need to impart in order to go to a different destination. -
16 Apr 2021 Gas Core Reactors for Deep Space Propulsion
Gas Core Reactors for Deep Space Propulsion Mikhail V. Shubov University of MA Lowell, One University Ave, Lowell, MA 01854 E-mail: [email protected] Abstract The operation of a nuclear power station powering Deep Space transport is presented in the pa- per. The power station consists of a Gas Core Reactor (GCR) with magnetohydrodynamic (MHD) generator. A new model of gas core reactor which has advantages by comparison with known models is suggested. It is shown that 200 ton system would generate 200 MW electricity. The gas core reactor consists of a spherical cavity of 1 m to 1.5 m radius surrounded by a 50 cm thick 235 liquid beryllium reflector within molybdenum–92 container. The fuel consists of UF4, KF, and K. It is demonstrated that such power station will work for gaseous fuel pressures of 50 atm to 100 atm. The Monte-Carlo simulations describing paths of thousands of neutrons are performed. These simulations yield neutronic results, i.e. the fractions of neutrons causing fission, being ab- sorbed by moderator, and escaping the reactor. From this information one can calculate minimum needed pressure inside the reactor, the reactor size, and moderator thickness. The conductivity of superheated fuel depending on temperature and pressure is also calculated. It is concluded that space propulsion is the best use of uranium resources. Keywords: Nuclear Space Power, Magnetohydrodynamic Energy Conversion, Gas Core Nuclear Reactors, Space Exploration Introduction Deep Space transportation of large payloads would use electrically powered magnetoplasmady- namic thrusters to provide momentum for maneuvers. These thrusters use lithium propellant. The 3 2 thrusters should provide a sustained acceleration of 10− m/s for the space transport.