The Shuttle Problem
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Astrodynamics
Politecnico di Torino SEEDS SpacE Exploration and Development Systems Astrodynamics II Edition 2006 - 07 - Ver. 2.0.1 Author: Guido Colasurdo Dipartimento di Energetica Teacher: Giulio Avanzini Dipartimento di Ingegneria Aeronautica e Spaziale e-mail: [email protected] Contents 1 Two–Body Orbital Mechanics 1 1.1 BirthofAstrodynamics: Kepler’sLaws. ......... 1 1.2 Newton’sLawsofMotion ............................ ... 2 1.3 Newton’s Law of Universal Gravitation . ......... 3 1.4 The n–BodyProblem ................................. 4 1.5 Equation of Motion in the Two-Body Problem . ....... 5 1.6 PotentialEnergy ................................. ... 6 1.7 ConstantsoftheMotion . .. .. .. .. .. .. .. .. .... 7 1.8 TrajectoryEquation .............................. .... 8 1.9 ConicSections ................................... 8 1.10 Relating Energy and Semi-major Axis . ........ 9 2 Two-Dimensional Analysis of Motion 11 2.1 ReferenceFrames................................. 11 2.2 Velocity and acceleration components . ......... 12 2.3 First-Order Scalar Equations of Motion . ......... 12 2.4 PerifocalReferenceFrame . ...... 13 2.5 FlightPathAngle ................................. 14 2.6 EllipticalOrbits................................ ..... 15 2.6.1 Geometry of an Elliptical Orbit . ..... 15 2.6.2 Period of an Elliptical Orbit . ..... 16 2.7 Time–of–Flight on the Elliptical Orbit . .......... 16 2.8 Extensiontohyperbolaandparabola. ........ 18 2.9 Circular and Escape Velocity, Hyperbolic Excess Speed . .............. 18 2.10 CosmicVelocities -
Launch and Deployment Analysis for a Small, MEO, Technology Demonstration Satellite
46th AIAA Aerospace Sciences Meeting and Exhibit AIAA 2008-1131 7 – 10 January 20006, Reno, Nevada Launch and Deployment Analysis for a Small, MEO, Technology Demonstration Satellite Stephen A. Whitmore* and Tyson K. Smith† Utah State University, Logan, UT, 84322-4130 A trade study investigating the economics, mass budget, and concept of operations for delivery of a small technology-demonstration satellite to a medium-altitude earth orbit is presented. The mission requires payload deployment at a 19,000 km orbit altitude and an inclination of 55o. Because the payload is a technology demonstrator and not part of an operational mission, launch and deployment costs are a paramount consideration. The payload includes classified technologies; consequently a USA licensed launch system is mandated. A preliminary trade analysis is performed where all available options for FAA-licensed US launch systems are considered. The preliminary trade study selects the Orbital Sciences Minotaur V launch vehicle, derived from the decommissioned Peacekeeper missile system, as the most favorable option for payload delivery. To meet mission objectives the Minotaur V configuration is modified, replacing the baseline 5th stage ATK-37FM motor with the significantly smaller ATK Star 27. The proposed design change enables payload delivery to the required orbit without using a 6th stage kick motor. End-to-end mass budgets are calculated, and a concept of operations is presented. Monte-Carlo simulations are used to characterize the expected accuracy of the final orbit. -
The Speed of a Geosynchronous Satellite Is ___
Physics 106 Lecture 9 Newton’s Law of Gravitation SJ 7th Ed.: Chap 13.1 to 2, 13.4 to 5 • Historical overview • N’Newton’s inverse-square law of graviiitation Force Gravitational acceleration “g” • Superposition • Gravitation near the Earth’s surface • Gravitation inside the Earth (concentric shells) • Gravitational potential energy Related to the force by integration A conservative force means it is path independent Escape velocity Example A geosynchronous satellite circles the earth once every 24 hours. If the mass of the earth is 5.98x10^24 kg; and the radius of the earth is 6.37x10^6 m., how far above the surface of the earth does a geosynchronous satellite orbit the earth? G=6.67x10-11 Nm2/kg2 The speed of a geosynchronous satellite is ______. 1 Goal Gravitational potential energy for universal gravitational force Gravitational Potential Energy WUgravity= −Δ gravity Near surface of Earth: Gravitational force of magnitude of mg, pointing down (constant force) Æ U = mgh Generally, gravit. potential energy for a system of m1 & m2 G Gmm12 mm F = Attractive force Ur()=− G12 12 r 2 g 12 12 r12 Zero potential energy is chosen for infinite distance between m1 and m2. Urg ()012 = ∞= Æ Gravitational potential energy is always negative. 2 mm12 Urg ()12 =− G r12 r r Ug=0 1 U(r1) Gmm U =− 12 g r Mechanical energy 11 mM EKUrmvMVG=+ ( ) =22 + − mech 22 r m V r v M E_mech is conserved, if gravity is the only force that is doing work. 1 2 MV is almost unchanged. If M >>> m, 2 1 2 mM ÆWe can define EKUrmvG=+ ( ) = − mech 2 r 3 Example: A stone is thrown vertically up at certain speed from the surface of the Moon by Superman. -
Optimisation of Propellant Consumption for Power Limited Rockets
Delft University of Technology Faculty Electrical Engineering, Mathematics and Computer Science Delft Institute of Applied Mathematics Optimisation of Propellant Consumption for Power Limited Rockets. What Role do Power Limited Rockets have in Future Spaceflight Missions? (Dutch title: Optimaliseren van brandstofverbruik voor vermogen gelimiteerde raketten. De rol van deze raketten in toekomstige ruimtevlucht missies. ) A thesis submitted to the Delft Institute of Applied Mathematics as part to obtain the degree of BACHELOR OF SCIENCE in APPLIED MATHEMATICS by NATHALIE OUDHOF Delft, the Netherlands December 2017 Copyright c 2017 by Nathalie Oudhof. All rights reserved. BSc thesis APPLIED MATHEMATICS \ Optimisation of Propellant Consumption for Power Limited Rockets What Role do Power Limite Rockets have in Future Spaceflight Missions?" (Dutch title: \Optimaliseren van brandstofverbruik voor vermogen gelimiteerde raketten De rol van deze raketten in toekomstige ruimtevlucht missies.)" NATHALIE OUDHOF Delft University of Technology Supervisor Dr. P.M. Visser Other members of the committee Dr.ir. W.G.M. Groenevelt Drs. E.M. van Elderen 21 December, 2017 Delft Abstract In this thesis we look at the most cost-effective trajectory for power limited rockets, i.e. the trajectory which costs the least amount of propellant. First some background information as well as the differences between thrust limited and power limited rockets will be discussed. Then the optimal trajectory for thrust limited rockets, the Hohmann Transfer Orbit, will be explained. Using Optimal Control Theory, the optimal trajectory for power limited rockets can be found. Three trajectories will be discussed: Low Earth Orbit to Geostationary Earth Orbit, Earth to Mars and Earth to Saturn. After this we compare the propellant use of the thrust limited rockets for these trajectories with the power limited rockets. -
Up, Up, and Away by James J
www.astrosociety.org/uitc No. 34 - Spring 1996 © 1996, Astronomical Society of the Pacific, 390 Ashton Avenue, San Francisco, CA 94112. Up, Up, and Away by James J. Secosky, Bloomfield Central School and George Musser, Astronomical Society of the Pacific Want to take a tour of space? Then just flip around the channels on cable TV. Weather Channel forecasts, CNN newscasts, ESPN sportscasts: They all depend on satellites in Earth orbit. Or call your friends on Mauritius, Madagascar, or Maui: A satellite will relay your voice. Worried about the ozone hole over Antarctica or mass graves in Bosnia? Orbital outposts are keeping watch. The challenge these days is finding something that doesn't involve satellites in one way or other. And satellites are just one perk of the Space Age. Farther afield, robotic space probes have examined all the planets except Pluto, leading to a revolution in the Earth sciences -- from studies of plate tectonics to models of global warming -- now that scientists can compare our world to its planetary siblings. Over 300 people from 26 countries have gone into space, including the 24 astronauts who went on or near the Moon. Who knows how many will go in the next hundred years? In short, space travel has become a part of our lives. But what goes on behind the scenes? It turns out that satellites and spaceships depend on some of the most basic concepts of physics. So space travel isn't just fun to think about; it is a firm grounding in many of the principles that govern our world and our universe. -
Spacecraft Trajectories in a Sun, Earth, and Moon Ephemeris Model
SPACECRAFT TRAJECTORIES IN A SUN, EARTH, AND MOON EPHEMERIS MODEL A Project Presented to The Faculty of the Department of Aerospace Engineering San José State University In Partial Fulfillment of the Requirements for the Degree Master of Science in Aerospace Engineering by Romalyn Mirador i ABSTRACT SPACECRAFT TRAJECTORIES IN A SUN, EARTH, AND MOON EPHEMERIS MODEL by Romalyn Mirador This project details the process of building, testing, and comparing a tool to simulate spacecraft trajectories using an ephemeris N-Body model. Different trajectory models and methods of solving are reviewed. Using the Ephemeris positions of the Earth, Moon and Sun, a code for higher-fidelity numerical modeling is built and tested using MATLAB. Resulting trajectories are compared to NASA’s GMAT for accuracy. Results reveal that the N-Body model can be used to find complex trajectories but would need to include other perturbations like gravity harmonics to model more accurate trajectories. i ACKNOWLEDGEMENTS I would like to thank my family and friends for their continuous encouragement and support throughout all these years. A special thank you to my advisor, Dr. Capdevila, and my friend, Dhathri, for mentoring me as I work on this project. The knowledge and guidance from the both of you has helped me tremendously and I appreciate everything you both have done to help me get here. ii Table of Contents List of Symbols ............................................................................................................................... v 1.0 INTRODUCTION -
GRAVITATION UNIT H.W. ANS KEY Question 1
GRAVITATION UNIT H.W. ANS KEY Question 1. Question 2. Question 3. Question 4. Two stars, each of mass M, form a binary system. The stars orbit about a point a distance R from the center of each star, as shown in the diagram above. The stars themselves each have radius r. Question 55.. What is the force each star exerts on the other? Answer D—In Newton's law of gravitation, the distance used is the distance between the centers of the planets; here that distance is 2R. But the denominator is squared, so (2R)2 = 4R2 in the denominator here. Two stars, each of mass M, form a binary system. The stars orbit about a point a distance R from the center of each star, as shown in the diagram above. The stars themselves each have radius r. Question 65.. In terms of each star's tangential speed v, what is the centripetal acceleration of each star? Answer E—In the centripetal acceleration equation the distance used is the radius of the circular motion. Here, because the planets orbit around a point right in between them, this distance is simply R. Question 76.. A Space Shuttle orbits Earth 300 km above the surface. Why can't the Shuttle orbit 10 km above Earth? (A) The Space Shuttle cannot go fast enough to maintain such an orbit. (B) Kepler's Laws forbid an orbit so close to the surface of the Earth. (C) Because r appears in the denominator of Newton's law of gravitation, the force of gravity is much larger closer to the Earth; this force is too strong to allow such an orbit. -
Compatibility Mode
Toward the Final Frontier of Manned Space Flight Ryann Fame Luke Bruneaux Emily Russell Image: Milky Way NASA Toward the Final Frontier of Manned Space Flight Part I: How we got here: Background and challenges (Ryann) Part II: Why boldly go? Why not? (Luke) Part III: Where are we going? (Emily) Toward the Final Frontier of Manned Space Flight Part I: How we got here: Background and challenges (Ryann) Part II: Why boldly go? Why not? (Luke) Part III: Where are we going? (Emily) Challenges in Human Space Travel • Challenge 1: Leaving Earth (Space!) • Challenge 2: Can humans live safely in space? • Challenge 3: Destination Travel Curiosity and Explorative Spirit Image: NASA Curiosity and Explorative Spirit Image: NASA How did we get here? 1903 Images: Library of Congress,US Gov. Military, NASA How did we get here? 1903 1947 Images: Library of Congress,US Gov. Military, NASA How did we get here? 1903 1947 1961 Images: Library of Congress,US Gov. Military, NASA How did we get here? 1903 1947 1961 1969 Images: Library of Congress,US Gov. Military, NASA How did we get here? 1903 1947 1971 1961 1969 Images: Library of Congress,US Gov. Military, NASA How did we get here? 1903 1981-2011 1947 1971 1961 1969 Images: Library of Congress,US Gov. Military, NASA Ballistic rockets for missiles X X Images: Library of Congress,US Gov. Military, NASA Leaving Earth (space!) 1946 Image: US Gov. Military Fuel Image: Wikimedia: Matthew Bowden Chemical combustion needs lots of oxygen 2 H2 + O2 → 2 H2O(g) + Energy Chemical combustion needs lots of oxygen 2 H2 -
Effects of Space Exploration Objective: Students Will Be Able To: 1
Lesson Topic: Effects of Space Exploration Objective: Students will be able to: 1. Identify and describe how space exploration affects the state of Florida. 2. Describe the nature of the Kennedy Space Center. 3. Identify the components of a space shuttle 4. Apply the importance of space exploration to the Florida culture through design. Time Required: 75 minutes Materials Needed: ● Teacher computer with internet access ● Projector/Smartboard ● 1 computer/laptop/iPad per student with internet access ● Effects of Space Exploration handout (attached) ● Space Exploration Video: Escape Velocity - A Quick History of Space Exploration ● Space Shuttle Website: Human Space Flight (HSF) - Space Shuttle ● Kennedy Space Center Website: Visit Kennedy Space Center Visitor Complex at Cape Canaveral ● Coloring pencils/Markers Teacher Preparation: ● Assign a Legends of Learning Content Review Quick Play playlist for the day(s) you will be teaching the lesson. ○ Content Review - Middle School - Effects of Space Exploration ● Make copies of Effects of Space Exploration Worksheet (1 per student) Engage (10 minutes): 1. Pass out the Effects of Space Exploration Handout. 2. Ask students “What do you know about space exploration? a. Draw the words “Space Exploration” on the board with a circle around it. i. As students share their answers write their answers on the board and link them to the Space Exploration circle with a line. 3. Tell students “We are going to watch a short video about the history of space exploration and how it has evolved over time. In the space provided on the handout, jot down any notes that you find interesting or important. 4. -
Honors Project 4: Escape Velocity
Math164,DueDate: Name(s): Honors Project 4: Escape Velocity Objective If a ball is thrown straight up into the air, it will travel upward, stop, and then fall back to earth. If a bullet is shot straight up into the air, it will travel upward, stop (at an altitude higher than the ball, unless the person who threw the ball was a real zealot), and then fall back to earth. In this project we discuss the problem of determining the velocity with which an object needs to be propelled straight up into the air so that the object goes into orbit; that is, so that it never falls back to earth. This is the escape velocity for the earth. (We add the phrase “for the earth” since the escape velocity, as we will see, depends on the mass of the body — whether it be a planet, or moon, or ... — from which the object is propelled.) We make two simplifying assumptions in our derivation: First, that there is no air resistance. Second, that the object has constant mass throughout its flight. This second assumption is significant since it means our analysis does not apply to a rocket, for example, since the mass of the rocket changes as the rocket burns fuel. Background Required Improper integrals. Narrative Newton’s Second Law of Motion states that if an object with mass m travels along a straight-line path parametrized by x = x(t) then the force which it will exert on a particle at a point along its path is given by F = ma where a = d2x/dt2. -
Spacex Rocket Data Satisfies Elementary Hohmann Transfer Formula E-Mail: [email protected] and [email protected]
IOP Physics Education Phys. Educ. 55 P A P ER Phys. Educ. 55 (2020) 025011 (9pp) iopscience.org/ped 2020 SpaceX rocket data satisfies © 2020 IOP Publishing Ltd elementary Hohmann transfer PHEDA7 formula 025011 Michael J Ruiz and James Perkins M J Ruiz and J Perkins Department of Physics and Astronomy, University of North Carolina at Asheville, Asheville, NC 28804, United States of America SpaceX rocket data satisfies elementary Hohmann transfer formula E-mail: [email protected] and [email protected] Printed in the UK Abstract The private company SpaceX regularly launches satellites into geostationary PED orbits. SpaceX posts videos of these flights with telemetry data displaying the time from launch, altitude, and rocket speed in real time. In this paper 10.1088/1361-6552/ab5f4c this telemetry information is used to determine the velocity boost of the rocket as it leaves its circular parking orbit around the Earth to enter a Hohmann transfer orbit, an elliptical orbit on which the spacecraft reaches 1361-6552 a high altitude. A simple derivation is given for the Hohmann transfer velocity boost that introductory students can derive on their own with a little teacher guidance. They can then use the SpaceX telemetry data to verify the Published theoretical results, finding the discrepancy between observation and theory to be 3% or less. The students will love the rocket videos as the launches and 3 transfer burns are very exciting to watch. 2 Introduction Complex 39A at the NASA Kennedy Space Center in Cape Canaveral, Florida. This launch SpaceX is a company that ‘designs, manufactures and launches advanced rockets and spacecraft. -
Space Medicine*
31 Desember 1960 S~A. TYDSKRIF VIR GENEESKUNDE 1117 mielitis ingelui het. Suid Afrika staan saam met' ander herhaal. Maar, onlangs het daar uit Japan 'n verdere lande in 'n omvattende poging om, onder andere, deur ontstellende berigO gekom dat daar in 1955 in die gebiede middel van die toediening van lewende verswakte polio wat jare gelede betrokke was by ontploffing van atoom slukentstof, poliomielitis geheel en al die hoof te bied. bomme, ongeveer twintig kinder gebore i wat op een of In hierdie verband weet ons dat al die gegewens daarop ander manier mi maak i . In die olgende jaar, 1956, wa dui dat ons in hierdie land die veiligste en die mees doel hierdie syfer yf-en-dertig, en in 1957, vyf-en- estig. Die treffende lewende polio-entstof wat beskikbaar is, ver aantal het du meer a erdriedubbel in drie jaar. Wat die vaardig. Soos ons aangetoon het toe hierdie saak bespreek implikasies van hierdie feite is, weet ons nie; a hulle is," spruit daar uit ons optrede in hierdie verband in die egter beteken wat huHe skyn te beteken, kan dit wee verlede egter 'n groot verantwoordelikheid vir die toekoms, dat veel meer skade berokken i aan die vroee onont om naamlik toe te sien dat hierdie onderneming op 'n wikkelde ovum, as wat moontlik geag is. 'n Ernstige waar volledige gemeenskapsbasis aangepak word. Dit sal dus skuwing om na te dink oor die gevolge van ons dade op goed wees om hier weer die waarskuwing te herhaal dat, 'n globale grondslag, kan ons skaars bedink.