Celestial mechanics in an interplanetary flight

Similar documents
Ch. 22 Origin of Modern Astronomy Pretest

Celestial Mechanics and Satellite Orbits

Gat ew ay T o S pace AS EN / AS TR Class # 19. Colorado S pace Grant Consortium

History. Geocentric model (Ptolemy) Heliocentric model (Aristarchus of Samos)

PHYS 155 Introductory Astronomy

Overview of Astronautics and Space Missions

Gravitation and the Motion of the Planets

Earth Science, 13e Tarbuck & Lutgens

Design of Orbits and Spacecraft Systems Engineering. Scott Schoneman 13 November 03

Gravitation and the Waltz of the Planets

Gravitation and the Waltz of the Planets. Chapter Four

Earth Science, 11e. Origin of Modern Astronomy Chapter 21. Early history of astronomy. Early history of astronomy. Early history of astronomy

EXAM #2. ANSWERS ASTR , Spring 2008

Lecture #5: Plan. The Beginnings of Modern Astronomy Kepler s Laws Galileo

History of Astronomy. PHYS 1411 Introduction to Astronomy. Tycho Brahe and Exploding Stars. Tycho Brahe ( ) Chapter 4. Renaissance Period

Announcements. Topics To Be Covered in this Lecture

PHYS 160 Astronomy Test #1 Fall 2017 Version B

Planetary Mechanics:

Chapter. Origin of Modern Astronomy

How High Is the Sky? Bob Rutledge

Astronomy- The Original Science

Chapter 4. The Origin Of Modern Astronomy. Is okay to change your phone? From ios to Android From Android to ios

Copernican revolution Review

Space Notes Covers Objectives 1 & 2

Early Theories. Early astronomers believed that the sun, planets and stars orbited Earth (geocentric model) Developed by Aristotle

9/12/2010. The Four Fundamental Forces of Nature. 1. Gravity 2. Electromagnetism 3. The Strong Nuclear Force 4. The Weak Nuclear Force

Physics Unit 7: Circular Motion, Universal Gravitation, and Satellite Orbits. Planetary Motion

Models of the Solar System. The Development of Understanding from Ancient Greece to Isaac Newton

BROCK UNIVERSITY. 1. About 2300 years ago, Aristotle argued that the Earth is spherical based on a number of observations, one of which was that

The History of Astronomy

The following notes roughly correspond to Section 2.4 and Chapter 3 of the text by Bennett. This note focuses on the details of the transition for a

How Astronomers Learnt that The Heavens Are Not Perfect

Gravity. Newton s Law of Gravitation Kepler s Laws of Planetary Motion Gravitational Fields

Planetary Orbits: Kepler s Laws 1/18/07

Cosmology is the study of the universe. What is it s structure? How did it originate? How is it evolving? What is its eventual fate?

Chapter 02 The Rise of Astronomy

Gravitation Part I. Ptolemy, Copernicus, Galileo, and Kepler

Astronomy Notes Chapter 02.notebook April 11, 2014 Pythagoras Aristotle geocentric retrograde motion epicycles deferents Aristarchus, heliocentric

Conceptual Physics Projectiles Motion of Planets

Kepler, Newton, and laws of motion

18. Kepler as a young man became the assistant to A) Nicolaus Copernicus. B) Ptolemy. C) Tycho Brahe. D) Sir Isaac Newton.

Space Exploration. Chapter. hapte

Days of the week: - named after 7 Power (moving) objects in the sky (Sun, Moon, 5 planets) Models of the Universe:

Universal Gravitation

Conceptual Physics Projectiles Motion of Planets

chapter 10 questions_pictures removed.notebook September 28, 2017 Chapter 10 What We Know About the Universe Has Taken Us Thousands of Years to Learn

History of Astronomy. Historical People and Theories

Origin of Modern Astronomy Chapter 21

Chapter 2. The Rise of Astronomy. Copyright (c) The McGraw-Hill Companies, Inc. Permission required for reproduction or display.

Learning Objectives. one night? Over the course of several nights? How do true motion and retrograde motion differ?

ASTRONOMY LECTURE NOTES MIDTERM REVIEW. ASTRONOMY LECTURE NOTES Chapter 1 Charting the Heavens

AP Physics Multiple Choice Practice Gravitation

Basics of Kepler and Newton. Orbits of the planets, moons,

Chapter 18: Studying Space Astronomy: The Original Science

Name: Earth 110 Exploration of the Solar System Assignment 1: Celestial Motions and Forces Due on Tuesday, Jan. 19, 2016

2. See FIGURE B. This person in the FIGURE discovered that this planet had phases (name the planet)?

1. The bar graph below shows one planetary characteristic, identified as X, plotted for the planets of our solar system.

ASTR 1010 Spring 2016 Study Notes Dr. Magnani

Occam s Razor: William of Occam, 1340(!)

Chapter 22 Exam Study Guide

EARTH SCIENCE UNIT 9 -NOTES ASTRONOMY

THE SUN AND THE SOLAR SYSTEM

3) During retrograde motion a planet appears to be A) dimmer than usual. B) the same brightness as usual C) brighter than usual.

1) Kepler's third law allows us to find the average distance to a planet from observing its period of rotation on its axis.

Introduction to Astronomy & Astrophysics (PHY F215) Kaushar Vaidya Ph.D. (Astronomy)

ASTRO 6570 Lecture 1

Lecture 13. Gravity in the Solar System

Introduction To Modern Astronomy I

Lesson 2 - The Copernican Revolution

Chapter 2 The Science of Life in the Universe

1. The Moon appears larger when it rises than when it is high in the sky because

9.2 Worksheet #3 - Circular and Satellite Motion

Pull out a ½ sheet or use the back of your old quiz

CH 8. Universal Gravitation Planetary and Satellite Motion

Scientific Method. Ancient Astronomy. Astronomy in Ancient Times

BROCK UNIVERSITY. 1. The observation that the intervals of time between two successive quarter phases of the Moon are very nearly equal implies that

By; Jarrick Serdar, Michael Broberg, Trevor Grey, Cameron Kearl, Claire DeCoste, and Kristian Fors

Astronomy Lesson 8.1 Astronomy s Movers and Shakers

Unit 2: Celestial Mechanics

EARTH SCIENCE UNIT 9 -KEY ASTRONOMY

Introduction To Modern Astronomy II

The History of Astronomy. Please pick up your assigned transmitter.

Chapter 1 The Copernican Revolution

Section 3- The history and future of space exploration

The History of Astronomy. Theories, People, and Discoveries of the Past

Astronomy. 1. (3 pts.) What is meant by the apparent magnitude of a star?

6. Summarize Newton s Law of gravity and the inverse square concept. Write out the equation

Chapter 10 Space Exploration Page 1 of 6

Physics Mechanics. Lecture 29 Gravitation

Physics 107 Ideas of Modern Physics (uw.physics.wisc.edu/~rzchowski/phy107) Goals of the course. What will we cover? How do we do this?

SCIENCE 9 CHAPTER 10 SECTION 1

Chapter 14 Satellite Motion

Claudius Ptolemaeus Second Century AD. Jan 5 7:37 AM

Early Models of the Universe. How we explained those big shiny lights in the sky

Section Study Guide. Teacher Notes and Answers. Circular Motion and Gravitation

2. See FIGURE B. In the Renaissance times, he proposed this model of the solar system (name this person).

ASTRONOMY CURRICULUM Unit 1: Introduction to Astronomy

AP Physics C Textbook Problems

Astronomy 1010 Planetary Astronomy Sample Questions for Exam 1

Chapter 6 More complicated orbits and spacecraft trajectories

Transcription:

Department of Physics, Umeå University October 10, 2008

Contents 1 Introduction History Theory 2 Rockets Plots of orbits 3 Aerobrake 4 References Introduction History Theory

History Theory What is celestial mechanics? Branch of astrophysics that deals with the motions of celestial objects: stars, galaxies, planets, (artificial) satellites, etc.. The field applies principles of physics to produce ephemeris data.

History Theory History Started probably when human discovered movement on the celestial sphere, however, problem of planetary motion has been known to Babylonian astronomers (3000 yrs bp). Notable astronomers in the field Aristarchus of Samos creator of the heliocentric model, proved later by Seleucus of Seleucia; Claudius Ptolemy author of the Almages, explained epicycles; Nicolaus Copernicus ; Galileo Galilei; Johannes Kepler; Isaac Newton; Joseph-Louis Lagrange.

History Theory Newton s cannonball

History Theory Escape velocity E Earth = E p + E k = mgr + mv 2 2, (1) E = mv 2 2, (2) mgr + mv 2 = mv 2 2 2, (3) v = 2gr. (4) [ ] [ ] [ ] m 2 m km 2 9.81 6, 357, 000 s 2 = 11, 356 11.4. s s

History Theory Types of orbits Centric classifications: galactocentric, heliocentric, geocentric, areocentric, lunar... Altitude classifications: LEO, MEO, GEO, HEO... Inclination classifications: polar, equatorial... Eccentricity classifications: circular, elliptic, parabolic, hiperbolic... Synchronous classifications: synchronous, geosynchronous, supersynchronous (disposal/graveyard), heliosynchronous...

History Theory Main types of orbits

History Theory Lagrange points

Introduction Rockets Plots of orbits Rocket... Remigiusz Pospieszyn ski

Rockets Plots of orbits...rocket...

Rockets Plots of orbits...rocket!

Rockets Plots of orbits Space Launch Facilities

Rockets Plots of orbits Hohmann transfer

Rockets Plots of orbits Bi-elliptic transfer

Rockets Plots of orbits Gravitational slingshot

Rockets Plots of orbits

Rockets Plots of orbits Cassini s tour

Rockets Plots of orbits Venus Express

Aerobrake Mars Reconnaissance orbiter

Aerobrake Apollo Command Module

References Conlusions 1 In order to send a spaceship to a celestial body one must know precise locations of all bodies involved. 2 Very precise timing is crucial for the good fortune of any mission. 3 Longer route can take less time than shorter. 4 When the target body has no atmosphere you need to take your fuel with you.

References Thank you for your attention! Presentation available at www.dywanik.eu

References http://en.wikipedia.org/wiki/newton s cannonball http://en.wikipedia.org/wiki/low Earth orbit http://en.wikipedia.org/wiki/lagrange points http://en.wikipedia.org/wiki/rocket http://www.arianespace.com http://maps.google.com http://en.wikipedia.org/wiki/hohmann transfer orbit http://en.wikipedia.org/wiki/bi-elliptic transfer http://en.wikipedia.org/wiki/gravitational slingshot http://saturn.jpl.nasa.gov

References http://www.astronomy.com/asy/default.aspx?c=a&id=3649 http://en.wikipedia.org/wiki/mars Reconnaissance Orbiter http://en.wikipedia.org/wiki/interplanetary travel