Introduction to Aerospace Engineering



Similar documents
2. Orbits. FER-Zagreb, Satellite communication systems 2011/12

Can Hubble be Moved to the International Space Station? 1

Space Exploration. A Visual History. Philip Stooke

Section 4: The Basics of Satellite Orbits

Solar System Fundamentals. What is a Planet? Planetary orbits Planetary temperatures Planetary Atmospheres Origin of the Solar System

Name: Earth 110 Exploration of the Solar System Assignment 1: Celestial Motions and Forces Due in class Tuesday, Jan. 20, 2015

RS platforms. Fabio Dell Acqua - Gruppo di Telerilevamento

THE SOLAR SYSTEM - EXERCISES 1

Astrodynamics (AERO0024)

Grade 6 Standard 3 Unit Test A Astronomy. 1. The four inner planets are rocky and small. Which description best fits the next four outer planets?

Chapter 25.1: Models of our Solar System

Astronomy 110 Homework #04 Assigned: 02/06/2007 Due: 02/13/2007. Name:

Perspective and Scale Size in Our Solar System

Exam # 1 Thu 10/06/2010 Astronomy 100/190Y Exploring the Universe Fall 11 Instructor: Daniela Calzetti

Use the following information to deduce that the gravitational field strength at the surface of the Earth is approximately 10 N kg 1.

Name Class Period. F = G m 1 m 2 d 2. G =6.67 x Nm 2 /kg 2

Satellites and Space Stations

How Rockets Work Newton s Laws of Motion

Lecture 13. Gravity in the Solar System

Interplanetary Travel. Outline. In This Section You ll Learn to...

Earth Is Not the Center of the Universe

Chapter 5: Circular Motion, the Planets, and Gravity

Newton s Law of Gravity

7. Our Solar System. Planetary Orbits to Scale. The Eight Planetary Orbits

Delimitation and Commercial Use of Outer Space. Sang-Myon Rhee Seoul National University March 28, 2011

WELCOME to Aurorae In the Solar System. J.E. Klemaszewski

Notes: Most of the material in this chapter is taken from Young and Freedman, Chap. 13.

Study Guide: Solar System

Jr. Edition. Solar System. Trading Cards. Solar System Trading Cards, Jr. Edition. Learn more about the solar system on these websites:

Gravity? Depends on Where You Are!

Newton s Law of Universal Gravitation

HOW TO BUILD A NANORACKS PAYLOAD: NANOLABS

Lecture 07: Work and Kinetic Energy. Physics 2210 Fall Semester 2014

Chapter 7 Our Planetary System. Agenda. Intro Astronomy. Intro Astronomy. What does the solar system look like? A. General Basics

Lecture 12: The Solar System Briefly

Into the Final Frontier : America s Journey into Space

A long time ago, people looked

Our Planetary System. Earth, as viewed by the Voyager spacecraft Pearson Education, Inc.

Elements of Physics Motion, Force, and Gravity Teacher s Guide

G U I D E T O A P P L I E D O R B I T A L M E C H A N I C S F O R K E R B A L S P A C E P R O G R A M

Name Class Date. true

The Gravitational Field

Science 9 Worksheet 13-1 The Solar System

Chapter 7 Our Planetary System. What does the solar system look like? Thought Question How does the Earth-Sun distance compare with the Sun s radius

How Long Do You Need To Achieve Your Scientific Objectives?

Mobile Computing. Chapter 5: Satellite Systems

Lab 7: Gravity and Jupiter's Moons

1. Soaring Through Our Solar System By Laura G. Smith

WEIGHTLESS WONDER Reduced Gravity Flight

The Space Shuttle: Teacher s Guide

Earth Sciences -- Grades 9, 10, 11, and 12. California State Science Content Standards. Mobile Climate Science Labs

California Standards Grades 9 12 Boardworks 2009 Science Contents Standards Mapping

GRAVITATIONAL FIELDS PHYSICS 20 GRAVITATIONAL FORCES. Gravitational Fields (or Acceleration Due to Gravity) Symbol: Definition: Units:

Spacecraft Power for Cassini

Gravity. in the Solar System. Beyond the Book. FOCUS Book

The orbit of Halley s Comet

Educator Guide to S LAR SYSTEM El Prado, San Diego CA (619)

Second International Symposium on Advanced Radio Technologies Boulder Co, September 8-10, 1999

Group Leader: Group Members:

USING MS EXCEL FOR DATA ANALYSIS AND SIMULATION

Interaction of Energy and Matter Gravity Measurement: Using Doppler Shifts to Measure Mass Concentration TEACHER GUIDE

TOPO Trajectory Operations Officer

Asteroids. Earth. Asteroids. Earth Distance from sun: 149,600,000 kilometers (92,960,000 miles) Diameter: 12,756 kilometers (7,926 miles) dotted line

ROYAL CANADIAN AIR CADETS PROFICIENCY LEVEL TWO INSTRUCTIONAL GUIDE SECTION 6 EO C IDENTIFY PARTS OF A ROCKET PREPARATION

Solar System Facts & Fun

DIRECT ORBITAL DYNAMICS: USING INDEPENDENT ORBITAL TERMS TO TREAT BODIES AS ORBITING EACH OTHER DIRECTLY WHILE IN MOTION

National Aeronautics and Space Administration Office of Policy and Plans NASA History Office. NASA History Fact Sheet

Newton s Laws of Motion

Halliday, Resnick & Walker Chapter 13. Gravitation. Physics 1A PHYS1121 Professor Michael Burton

UNIVERSITY OF SASKATCHEWAN Department of Physics and Engineering Physics

Class 2 Solar System Characteristics Formation Exosolar Planets

Science Focus 9 Space Exploration Topic Test

circular motion & gravitation physics 111N

Version A Page The diagram shows two bowling balls, A and B, each having a mass of 7.00 kilograms, placed 2.00 meters apart.

EVALUAT ING ACADEMIC READINESS FOR APPRENTICESHIP TRAINING Revised for ACCESS TO APPRENTICESHIP

Examination Space Missions and Applications I (AE2103) Faculty of Aerospace Engineering Delft University of Technology SAMPLE EXAM

Solar System. 1. The diagram below represents a simple geocentric model. Which object is represented by the letter X?

5. Satellite Systems. History of Satellite Communications

Name: João Fernando Alves da Silva Class: 7-4 Number: 10

Forces. When an object is pushed or pulled, we say that a force is exerted on it.

CSSAR Space Science Cooperation

Penn State University Physics 211 ORBITAL MECHANICS 1

The Solar System. Unit 4 covers the following framework standards: ES 10 and PS 11. Content was adapted the following:

Physics 2A, Sec B00: Mechanics -- Winter 2011 Instructor: B. Grinstein Final Exam

1. Large ships are often helped into port by using two tug boats one either side of the ship. April 5, 1989 (Anchorage Daily News / Erik Hill)

DEOS. Deutsche Orbitale Servicing Mission. The In-flight Technology Demonstration of Germany s Robotics Approach to Service Satellites

Satellite technology

A Solar System Coloring Book

Newton s Law of Gravitation

Current Staff Course Unit/ Length. Basic Outline/ Structure. Unit Objectives/ Big Ideas. Properties of Waves A simple wave has a PH: Sound and Light

NJ Physics Professor Has the 'Right Stuff' Valorie Sands

FIZIKA ANGOL NYELVEN

Presentation of problem T1 (9 points): The Maribo Meteorite

Mobile Communications: Satellite Systems

How the Universe Works

A SOLAR SYSTEM COLORING BOOK

A Taxonomy for Space Curricula

Physical Science Chapter 2. Forces

Georgia Performance Standards Framework for Science Grade 6. Unit Organizer: UNIVERSE AND SOLAR SYSTEM (Approximate Time 3 Weeks)

Satellites and Space Probes Space System Design, MAE 342, Princeton University Robert Stengel

Transcription:

Introduction to Aerospace Engineering Lecture slides Challenge the future 1

Introduction to Aerospace Engineering AE1102 Dept. Space Engineering Astrodynamics & Space Missions (AS) Prof. ir. B.A.C. Ambrosius Ir. R. Noomen Space Systems Engineering (SSE) Ir. J.M. Kuiper Ir. B.T.C. Zandbergen AE1102 Introduction to Aerospace Engineering (Space) 1

1-3 Why do we go in Space? What can we do there? What are the challenges? Historical highlights Differences with Aeronautics Characteristic conditions and numbers AE1102 Introduction to Aerospace Engineering (Space) 2 Part of the contents of this presentation originates from the lecture Space Engineering and Technology I, Part I (ae1-801/1), by R. Hamann.

What is Space Flight (Astronautics)? Learning goals Get acquainted with concepts of space flight Understand differences with aeronautics Learn about historical perspective Become aware of unique applications Understand principles of satellite orbits Understand principles of rockets Get acquainted with unique aspects of space technology Develop awareness of characteristic numbers and costs Develop ability to make simple (back-of the-envelope) calculations??? AE1102 Introduction to Aerospace Engineering (Space) 3

Why do we go in Space? BECAUSE: we are curious it is challenging we have the necessary technology it stimulates technological innovations we can afford it it provides a unique environment (vantage point) It enables new applications we can do new business it provides access to new worlds Etc??? it is there. AE1102 Introduction to Aerospace Engineering (Space) 4

AE1102 Introduction to Aerospace Engineering (Space) 5

What can we do in Space? Observe the universe Observe and monitor the Earth Experience and exploit weightlessness (ISS) Perform in-situ science Travel to new worlds (solar system exploration) Space Tourism ISS (2010) Make money Etc.??? Comet Hartly 2010 (Deep Impact) Virgin Galactic Spaceship-2 AE1102 Introduction to Aerospace Engineering (Space) 6

Important applications Space physics Space astronomy Telecommunication Navigation Meteorology Disaster monitoring Global change Micro-gravity research Solar system exploration Espionage and surveillance Space tourism Etc??? AE1102 Introduction to Aerospace Engineering (Space) 7

Example of applications (Communication) Satellites in geostationary orbit and sample missions (Inmarsat-4; Intelsat-10; ~6000 kg) AE1102 Introduction to Aerospace Engineering (Space) 8

Example of applications (Earth observation; Meteorology) Infrared cloud picture taken by geostationary satellite (7 November 2010) AE1102 Introduction to Aerospace Engineering (Space) 9

Example of applications (Earth observation; global change monitoring) Decrease of Iceland ice cap due to global warming AE1102 Introduction to Aerospace Engineering (Space) 10

Example of applications (Global Navigation Satellite System; GNSS) Constellation of GPS satellites and example of Block-I and Block-IIR-M satellites AE1102 Introduction to Aerospace Engineering (Space) 11

Example of applications (Space Astronomy) The Hubble Space Telescope and one of the first pictures after the last repair mission AE1102 Introduction to Aerospace Engineering (Space) 12

Example of applications (Solar system exploration) The Spirit rover on the surface of Mars and pictured by the MRO orbiter AE1102 Introduction to Aerospace Engineering (Space) 13

What are the challenges? To get there, stay there and return To do this in an affordable, efficient way To deal with a harsh and hostile environment To develop the technology To invent innovative applications To (remotely) operate the systems To automate and autonomate the systems To deal with the unexpected.. AE1102 Introduction to Aerospace Engineering (Space) 14

Enabling technologies Miniaturization of electronics Radio communication and radar technology Capability to build large light-weight structures Advanced heat resistant materials Light-weight, powerful gas turbines and pumps Liquid propellant rocket engines Active guidance using gyroscopes Solar cells Heat engines (Stirling principle) Digital computers Life support systems Etc??? AE1102 Introduction to Aerospace Engineering (Space) 15

Example of energy supply in Space Envisat solar panel Power: 6.55 kw Dimension: 5x14 m 2 Silicium solar cells Vanguard-1 (1958) First solar cells in space (invented in 1954 by Bell Telephone Lab) Power: 10 mw Dimension: 6x25 cm 2 Satellite mass: 1.5 kg AE1102 Introduction to Aerospace Engineering (Space) 16

Important dates and people - The theory 1571-1630 Kepler solves the mystery of celestial mechanics 1642 1727 Newton defines the physical principles of force, motion and gravitational attraction 1865 Jules Verne describes a virtual trip to the Moon 1903 Tsiolkowski publishes his theoretical study on rocket propulsion and multi-stage rocket motion 1920 s Oberth pioneers the theoretical fundamentals of space flight 1925 Hohmann analyzes the method to perform interplanetary flight AE1102 Introduction to Aerospace Engineering (Space) 17

Important dates and events - The hardware 1920-1940 Goddard launches first liquid propellant rocket in the US Koroljev does the same in Russia 1940-1945 Von Braun develops the first operational shortrange missile (V2 rocket) 1950-1960 Russia and the US develop Inter-mediate range and Inter-continental range Ballistic Missiles (IRBM s & ICBM s) R.H. Goddard 1926 Koroljev 1933 GIRD-X 1933 Korolev AE1102 Introduction to Aerospace Engineering (Space) 18

Important dates and events - Spaceflight 1957 Launch of Sputnik I 1958 Launch of Explorer I 1959 Luna 2 makes a hard landing on the moon 1961 First manned satellite flight (Gagarin; Vostok I) 1962 First US manned satellite flight (Glenn; Mercury) Sputnik I Launch: 4 oktober 1957 Shape: sphere Radius: 0.58 m Mass: 83.6 kg Radio frequencies: 20 and 40 MHz Low earth orbit: 227 x 941 km Inclination: 65.1º AE1102 Introduction to Aerospace Engineering (Space) 19

Important dates and events Spaceflight (cnt d) 1962 Mariner II to Venus 1965 First EVA (Extra Vehicular Activity) by Leonov; Voskhod 2 1967 First launch of largest rocket ever (Saturn-V) 1968 First European scientific satellite (ESRO II) 1969 First men on the moon (Amstrong & Aldrin; Apollo 11) 1974 First Dutch satellite (ANS) 1976 First soft landing on Mars (Viking 1/2) AE1102 Introduction to Aerospace Engineering (Space) 20

Important dates and events Spaceflight (cnt d) 1977 Voyager-2 to Jupiter, Saturn, Uranus and Neptune 1979 First successful flight of the European Ariane launcher 1981 First flight of the Space Shuttle 1986 First launch of MIR, the permanent Russian Space Station 1990 Launch of Hubble Space Telescope 1998 Launch of the first element of the ISS, the Russian Zarya module AE1102 Introduction to Aerospace Engineering (Space) 21

Differences with aeronautics Short-duration powered flight Free flight after launch Extremely high velocities Limited steering capability after launch No physical access to hardware after launch Vacuum environment Weightlessness Expendable propulsion High vantage point for observations Fast global coverage Tailored design for each mission Expensive!!?? Etc??? AE1102 Introduction to Aerospace Engineering (Space) 22

What is Space? Vacuum Where does it start (> 120km) No (small) lift and drag No breathing atmosphere No oxygen for propulsion Fluids evaporate (lubrication problems) Aggressive environment (atomic oxygen erodes plastics) Outgassing of materials Source: Fortescue AE1102 Introduction to Aerospace Engineering (Space) 23

What is Space? (Cnt d) Thermal Environment Extremely hot and cold Without special measures material temperatures may vary between -270 and +120 C (near Earth) Solar flux at Earth surface 400 to 600 W/m 2 (depending on cloud cover, latitude and time of day), in space 1400 W/m 2 Earth surface temperature ~293 K Deep space temperature 4 K No convection (because no air and no gravity) but Radiation (internally and to environment) and Conduction (internally) AE1102 Introduction to Aerospace Engineering (Space) 24

What is Space? (Cnt d) Radiation no atmosphere to shield from dangerous and destructive electromagnetic radiation (e.g. UV, X-rays) destroys living tissue, electronics, plastics Full EM spectrum observable! High energy particles High-energy protons and electrons Van Allen radiation belts South-Atlantic anomaly Solar flares / eruptions (even noticeable on Earth) Source: Fortescue AE1102 Introduction to Aerospace Engineering (Space) 25

Movie of the day (17-11-2011) http://www.space.com/13627-time-lapse-video-earth-aurorasiss.html AE1102 Introduction to Aerospace Engineering (Space) 26

What is space? (Cnt d) Weightlessness!! After launch the satellite and its contents are in a state of: CONTINUOUS FREE FALL Why? (Basics of astrodynamics: Newton s laws) Conservation of momentum (mass times velocity = constant) Force equals mass times acceleration (F=Ma) Reactive force = - Action force ( Action equals reaction ) Gravitational force: proportional to the masses of the attracting bodies and inversely proportional to the square of the distance to the center of the bodies AE1102 Introduction to Aerospace Engineering (Space) 27

What is Space (Cnt d) Earth gravity force on a S/C in circular orbit at height h orbit (assume S/C is a point-mass) Newton s 4 th law M M S / C E Fg = G = M 2 S / C g ( RE + horbit ) M µ g = G = ( R h ) ( R h ) E 2 2 E + orbit E + orbit M µ g G N B h g g 2 E E 0 = = (.. 0) 2 2 orbit = ==> = 0 2 RE RE ( RE + horbit ) UNIVERSAL gravitational constant: G = 6.673 * 10-11 (m 3 kg -1 s -2 ) g / g 0 = Gravitational acceleration at S/C altitude and Earth surface, resp. R E = Earth radius (assuming spherical Earth) h orbit = Height of the S/C above the Earth s surface N.B. In a circular orbit F g acts normal to the velocity vector V orbit = constant R Newton s 2 nd law AE1102 Introduction to Aerospace Engineering (Space) 28

What is Space (Cnt d) How does a satellite (S/C) stay in a (circular) orbit? Equilibrium between gravity force and centrifugal force Gravity force F g = M S / C g = M S / C g 0 2 RE ( RE + horbit ) 2 Apparent centrifugal force (circular orbit) F = M c S / C E 2 orbit V R + h orbit Equilibrium F g g = Fc 0 Vorbit = V ( horbit ) = R E R + h E orbit Orbital period T 2 π ( RE + horbit ) = V orbit See example in notes below AE1102 Introduction to Aerospace Engineering (Space) 29 GENERAL NOTE: All expressions can also be used INVERSELY!!! Example: If the orbital period T, the Earth radius Re and the height of the orbit h orbit are given, you can calculate the velocity of the S/C using the formula for the orbital period. Assume T = 90 minutes, Re = 6378 km and h orbit = 275 km Compute V orbit Answer: 7.74 km/s N.B. Always be careful with the units. Make sure you are always consistent. So don t mix up km and m, or min, hrs and seconds

Example problems Velocity and orbital period of a satellite in a circular Earth orbit Compute the value of g 0 at the Earth s surface (GM Earth = 398601.3 km 3 /s 2 ; Re = 6378 km) Compute the velocity of a satellite at 800 km altitude (Envisat) Compute the velocity of the Moon around the Earth (Average Earth-Moon distance = 384000 km) Compute the orbital height of a geostationary satellite (Orbital period = 23 hr 56 min) AE1102 Introduction to Aerospace Engineering (Space) 30 Answers: g 0 = 9.80 m/s2 V envisat = 7.4519 km/s V moon = 1.0118 km/s H geo-sat = 35785 km

Weightlessness The International Space Station (ISS) AE1102 Introduction to Aerospace Engineering (Space) 31

Weightlessness (Cnt d) How do we move (heavy) objects in space? (robot arms exerting torque) What is torque (in Dutch: koppel of moment )? Torque is also called moment or moment of force It is the product of force (N) times arm (m) It acts like a lever which causes a rotational motion about a fulcrum or pivot point Examples: wrench or electrical screw driver AE1102 Introduction to Aerospace Engineering (Space) 32

Weightlessness (Cnt d) WRIST ROLL -185 o +185 o 11.3 m ECC +120 o -120 o +120 o WRIST PITCH -120 o -176 o +30 o ELBOW PITCH WRIST YAW SHOULDER ROLL +185 o -185 o -120 o +120 o -120 o +120 o SHOULDER PITCH SHOULDER YAW The European Robot Arm (ERA); Courtesy Dutch Space AE1102 Introduction to Aerospace Engineering (Space) 33

Weightlessness (Cnt d) Example A robot arm of 10 m length (l) has to move a payload of 6000 kg mass. The actuator at the root of the arm exercises 300 Nm torque. What time does it take to move the payload over 180 degrees? Force F, acceleration a and displacement s at the end of the arm: Torque 300 F = = = 30N l 10 F 30 a = = = 0.005 m / s payload mass 6000 s = α R = π.10 (NB. s equals distance traveled for α = 90 degrees) 2 90 degree arc with full acceleration/deceleration covered in t= (2 s / a) = (2 l (π /2) / a) = (10 π /0.005) = 79.3 s 180 degrees covered in less than 160 seconds What is the velocity of the payload at 90 degrees? 2 AE1102 Introduction to Aerospace Engineering (Space) 34 Answer: The velocity equals time times acceleration, giving ~ 0.4 m/s

Example questions (weightlessness) Is the orbital velocity of a spacecraft dependent of its mass or not? (motivate your answer) What happens to a free-floating astronaut, when he swings a hammer and hits the nail? What happens to a free-floating astronaut when he torques a bolt? What is the motion of an object within the ISS if it remains untouched? Why is it possible to move heavy objects near the ISS with small force? Why is it possible to dock a 120 ton Space Shuttle with a 330 ton ISS? AE1102 Introduction to Aerospace Engineering (Space) 35

Characteristic numbers Payload mass (3kg 100,000kg) Large aircraft (70,000kg) Launch mass (20,000kg 3,000,000kg) Large aircraft (250,000kg) Minimal orbital velocity (7.8 km/s = 28,000km/hr) Aircraft (900km/hr 3000km/hr) Minimal orbital height (250km) Aircraft (10km 20km) Typical satellite lifetime (3yr 15yr) Aircraft (25yr) AE1102 Introduction to Aerospace Engineering (Space) 36

Example of spacecraft size and mass ENVISAT (ESA; 2002; size: school bus; mass: 3000kg) Delfi-C3 (DUT; 2008; size: milk pack; mass: 3kg) AE1102 Introduction to Aerospace Engineering (Space) 37

Characteristic numbers (Cnt d) Cost of a Space Shuttle launch (500 MEuro) Long-range aircraft (~0.5 MEuro) Cost of a large communications satellite (250 MEuro) Inter-continental glass fiber cable (??? MEuro) Cost of Galileo navigation system (4,000 MEuro) Annual ESA budget (3,500 MEuro) Annual NASA budget (22,000 MUS$) Etc??? AE1102 Introduction to Aerospace Engineering (Space) 38

Characteristic numbers (Cnt d) Non-ESA 3% Space technology research 1% Other 17% Launch vehicles 19% Budget growth 2710 M (2000) 2903 M (2006) 3500 M (2009) Navigation 3% Microgravity 4% Telecommunications 6% Earth observation 17% Scientific program 13% ESA budget (2000) Manned spaceflight 17% Source: Space News, January 24, 2000 AE1102 Introduction to Aerospace Engineering (Space) 39