Files and their Relationships
|
|
- Dominick Stephens
- 5 years ago
- Views:
Transcription
1 Contents Preface Files and their Relationships 1 The Java Programming Language What is Java? Installing Java: A Simple Program Hello World Syntax Packages JAR Files Language Details Reserved Words Types and Variables Strings, Arrays, Pointers and null Operators Statements Exercises Object-Oriented Features Classes and Objects Encapsulation: public, private and protected Modiers: static and final Constructors and this Extending Classes and Inheritance Everything is an Object Casting Exercises Class-like Objects Exceptions Necessary Classes Useful Examples An Input Line Reader Finding Files Giving the User Choices A Dialog for Text Input iii ix xv
2 iv CONTENTS 2 Spatial Geometry Lines and Planes Translation and Rotation Using 4 4 Matrices Reection Two-dimensional Reection Three-dimensional Reection Projection Parallel Projection Perspective Projection Shading Spheres A Simple Shaded Sphere The Projection A Shading Model The Window Class The Drawing Class Mobile Eye The Drawing Class Keyboard and Mouse Events Geometry Drawable Sphere Overview Drawing the Curves Surface Features Viewing JPEG Files Pasting an Image A Sphere with Surface Details The Ellipse and Kepler's Laws Denition and Parts of the Ellipse Tangent to the Ellipse Polar Representation Kepler's Second and Third Laws Determining Perihelion and Aphelion Kepler's Equation An Animation Astronomy: Overview Introduction An Animation of the Sun and Earth Improved Sphere Class Keyboard Listener Sphere with Equator and Ecliptic A Simple Animation An Improved Animation Coordinate Systems Equatorial Coordinates
3 CONTENTS v Horizon Coordinates Ecliptic Coordinates Time Astronomy: Details Changing Coordinate Systems Hour Angle Right Ascension Equatorial Ecliptic Horizon Equatorial Code for Coordinate Conversion Long-term Variation of Coordinate Axes Qualitative Description Formulas Code for Precession and Nutation Animation of Precession Time Time: A Summary Time: Utility Code Animating the Equation of Time Factors that are Ignored Time Refraction Aberration Relativistic Eects Parallax The Shape of the Earth The JPL Data Chebyshev Polynomials Overview of the Data The ASCII Files The Binary Files Using the JPL Data Serialization Converting the JPL Data to Java Format Coordinates of the Planets Animating the JPL Data A Simple Animation Improving the Animation PlanetState MobileAnim MobilePane
4 vi CONTENTS 9 Adding the Stars Stellar Position and Proper Motion Data The Stars on the Celestial Sphere Displaying the Stars on an OutSphere The StarWindow main()-class Animation of Proper Motion The Planets on the Celestial Sphere Displaying the Planets on an OutSphere The JPLSphereAnim main()-class The Celestial Sphere with Stars and Planets Spaceship Earth View from Inside a Sphere: Code The InSphere Class Helper Classes Explanation of InSphere Projection Zooming In and Out Viewing the Stars InsideStarSphere InsideStarWindow The Stars and Planets InsideJPLSphere CEarthPane CEarthAnim View from Earth's Surface Generating a Static View Animating the View A Mathematical Review 297 A.1 Notation A.2 Trigonometry A.2.1 Inverse Trigonometric Functions A.2.2 Arc-tangent A.2.3 Trigonometric Identities A.3 Vectors A.3.1 The Dot Product A.3.2 The Cross Product A.3.3 Velocity Vector and Angular Velocity A.4 Polar and Spherical Coordinates A.5 Matrices A.5.1 Matrix Algebra A.5.2 The Determinant A.6 Linear Independence A.7 Spherical Trigonometry A.8 Under the Rug A.8.1 Tangents to a Curve or Surface
5 CONTENTS vii A.8.2 Area and Stretching A.9 Utility Code B Contents of the CD 331 B.1 List of Files B.2 Running the Programs B.3 The Java Front-end B.3.1 ListDialog B.3.2 Main B.3.3 CmdRunner B.3.4 CmdLineWindow B.3.5 LineListener B.3.6 InStreamGlue B.3.7 OutStreamGlue B.3.8 CmdLineDocFilter Bibliography 345 Index 351
Files and their Relationships
Files and their Relationships The tables below give an overview of the Java source-code les found on the accompanying CD. The les used by the rsf.jfe package 2 are not included in any of the tables here.
More informationCELESTIAL MECHANICS. Part I. Mathematical Preambles
Chapter 1. Numerical Methods CELESTIAL MECHANICS Part I. Mathematical Preambles 1.1 Introduction 1.2 Numerical Integration 1.3 Quadratic Equations 1.4 The Solution of f(x) = 0 1.5 The Solution of Polynomial
More informationAy 1 Lecture 2. Starting the Exploration
Ay 1 Lecture 2 Starting the Exploration 2.1 Distances and Scales Some Commonly Used Units Distance: Astronomical unit: the distance from the Earth to the Sun, 1 au = 1.496 10 13 cm ~ 1.5 10 13 cm Light
More informationThe Celestial Sphere. GEK1506 Heavenly Mathematics: Cultural Astronomy
The Celestial Sphere GEK1506 Heavenly Mathematics: Cultural Astronomy Helmer Aslaksen Department of Mathematics National University of Singapore aslaksen@math.nus.edu.sg www.math.nus.edu.sg/aslaksen/ The
More informationHistory of Astronomy. Historical People and Theories
History of Astronomy Historical People and Theories Plato Believed he could solve everything through reasoning. Circles and Spheres are good because they are perfect (never ending) and pleasing to the
More informationPHYS 155 Introductory Astronomy
PHYS 155 Introductory Astronomy - observing sessions: Sunday Thursday, 9pm, weather permitting http://www.phys.uconn.edu/observatory - Exam - Tuesday March 20, - Review Monday 6:30-9pm, PB 38 Marek Krasnansky
More informationCSE P503 - Project 1: Navigation System.
CSE P503 - Project 1: Navigation System. 1. Introduction The goal of this project is to design and verify a probe navigation system. Assume a radio telescope (marked by the red dot) sits at the center
More informationPHYS 160 Astronomy Test #1 Fall 2017 Version B
PHYS 160 Astronomy Test #1 Fall 2017 Version B 1 I. True/False (1 point each) Circle the T if the statement is true, or F if the statement is false on your answer sheet. 1. An object has the same weight,
More informationCHARTING THE HEAVENS USING A VIRTUAL PLANETARIUM
Name Partner(s) Section Date CHARTING THE HEAVENS USING A VIRTUAL PLANETARIUM You have had the opportunity to look at two different tools to display the night sky, the celestial sphere and the star chart.
More informationEarth Science, 11e. Origin of Modern Astronomy Chapter 21. Early history of astronomy. Early history of astronomy. Early history of astronomy
2006 Pearson Prentice Hall Lecture Outlines PowerPoint Chapter 21 Earth Science 11e Tarbuck/Lutgens This work is protected by United States copyright laws and is provided solely for the use of instructors
More information2) The number one million can be expressed in scientific notation as: (c) a) b) 10 3 c) 10 6 d)
Astronomy Phys 181 Midterm Examination Choose the best answer from the choices provided. 1) What is the range of values that the coordinate Declination can have? (a) a) -90 to +90 degrees b) 0 to 360 degrees
More informationEarly history of astronomy. Early history of astronomy. Positions in the sky. Lecture 3: The Sun & Constellations
Lecture 3: The Sun & Constellations Professor Kenny L. Tapp Early history of astronomy Birth of modern astronomy Noted scientist Johannes Kepler (1571-1630) Ushered in new astronomy Planets revolve around
More informationASTROPHYSICS. K D Abhyankar. Universities Press S T A R S A ND G A L A X I E S
ASTROPHYSICS S T A R S A ND G A L A X I E S K D Abhyankar Universities Press Contents Foreword vii Preface ix 1 Introduction 1 1.1 ' Astronomy and astrophysics 1 1.2 Importance of astronomy 2 1.3 Methods
More informationxvi xxiii xxvi Construction of the Real Line 2 Is Every Real Number Rational? 3 Problems Algebra of the Real Numbers 7
About the Author v Preface to the Instructor xvi WileyPLUS xxii Acknowledgments xxiii Preface to the Student xxvi 1 The Real Numbers 1 1.1 The Real Line 2 Construction of the Real Line 2 Is Every Real
More informationLab 5. Parallax Measurements and Determining Distances. 5.1 Overview
Lab 5 Parallax Measurements and Determining Distances 5.1 Overview Exercise five centers on a hands-on activity where students perform their own parallax measurements, measuring angular shifts in nearby
More informationEarth Science, 13e Tarbuck & Lutgens
Earth Science, 13e Tarbuck & Lutgens Origins of Modern Astronomy Earth Science, 13e Chapter 21 Stanley C. Hatfield Southwestern Illinois College Early history of astronomy Ancient Greeks Used philosophical
More informationLOCATING CELESTIAL OBJECTS: COORDINATES AND TIME. a. understand the basic concepts needed for any astronomical coordinate system.
UNIT 2 UNIT 2 LOCATING CELESTIAL OBJECTS: COORDINATES AND TIME Goals After mastery of this unit, you should: a. understand the basic concepts needed for any astronomical coordinate system. b. understand
More informationAn Introduction to Celestial Mechanics
An Introduction to Celestial Mechanics This accessible text on classical celestial mechanics the principles governing the motions of bodies in the solar system provides a clear and concise treatment of
More informationPosition 3. None - it is always above the horizon. Agree with student 2; star B never crosses horizon plane, so it can t rise or set.
Position 3 None - it is always above the horizon. N E W S Agree with student 2; star B never crosses horizon plane, so it can t rise or set. Imaginary plane No; the Earth blocks the view. Star A at position
More informationUnit 2: Celestial Mechanics
Unit 2: Celestial Mechanics The position of the Earth Ptolemy (90 168 AD) Made tables that allowed a user to locate the position of a planet at any past, present, or future date. In order to maintain circular
More informationASTRONOMICAL COORDINATE SYSTEMS CELESTIAL SPHERE
ASTRONOMICAL COORDINATE SYSTEMS CELESTIAL SPHERE To the naked eye, stars appear fixed on the sky with respect to one another. These patterns are often grouped into constellations. Angular measurements
More informationProfessor Emeritus in Astronomy, Honorary Lecturer and Senior Research Fellow, University of Glasgow
Astronomy: Principles and Practice Fourth Edition A E Roy, PhD, FRAS, FRSE, FBIS Professor Emeritus in Astronomy, Honorary Lecturer and Senior Research Fellow, University of Glasgow D Clarke, PhD, MInstP,
More informationLecture Module 2: Spherical Geometry, Various Axes Systems
1 Lecture Module 2: Spherical Geometry, Various Axes Systems Satellites in space need inertial frame of reference for attitude determination. In a true sense, all bodies in universe are in motion and inertial
More informationThe Position of the Sun. Berthold K. P. Horn. necessary to know the position of the sun in the sky. This is particularly
MASSACHUSETTS INSTITUTE OF TECHNOLOGY ARTIFICIAL INTELLIGENCE LABORATORY Working Paper No. 162 March 1978 The Position of the Sun Berthold K. P. Horn Abstract. The appearance of a surface depends dramatically
More informationASTR 2310: Chapter 2
Emergence of Modern Astronomy Early Greek Astronomy Ptolemaic Astronomy Copernican Astronomy Galileo: The First Modern Scientist Kepler's Laws of Planetary Motion Proof of the Earth's Motion Early Greek
More informationCHARTING THE HEAVENS USING A VIRTUAL PLANETARIUM
Name Partner(s) Section Date CHARTING THE HEAVENS USING A VIRTUAL PLANETARIUM You have had the opportunity to look at two different tools to display the night sky, the celestial sphere and the star chart.
More informationProper Motion of Barnards Star
How to use Virtual Observatory Proper Motion of Barnards Star Florian Freistetter, ZAH, Heidelberg florian@ari.uni-heidelberg.de Stars do move! Even if stars are called fixed stars sometime, y are not
More information[05] Historical Perspectives (9/12/17)
1 [05] Historical Perspectives (9/12/17) Upcoming Items 1. Homework #2 due now. 2. Read Ch. 4.1 4.2 and do self-study quizzes. 3. Homework #3 due in one week. Ptolemaic system http://static.newworldencyclopedia.org/thumb/3/3a/
More informationLearning Objectives. one night? Over the course of several nights? How do true motion and retrograde motion differ?
Kepler s Laws Learning Objectives! Do the planets move east or west over the course of one night? Over the course of several nights? How do true motion and retrograde motion differ?! What are geocentric
More informationKirkwood Gaps. Phil Peterman Physics 527 Computational Physics Project 1
Introduction Kirkwood Gaps Phil Peterman Physics 527 Computational Physics Project 1 Resonance phenomena, or tendencies for systems to oscillate at particular frequencies, occur in many distinct branches
More informationThe point in an orbit around the Sun at which an object is at its greatest distance from the Sun (Opposite of perihelion).
ASTRONOMY TERMS Albedo Aphelion Apogee A measure of the reflectivity of an object and is expressed as the ratio of the amount of light reflected by an object to that of the amount of light incident upon
More informationFoundations of Astrophysics
Foundations of Astrophysics Barbara Ryden The Ohio State University Bradley M. Peterson The Ohio State University Preface xi 1 Early Astronomy 1 1.1 The Celestial Sphere 1 1.2 Coordinate Systems on a Sphere
More informationTest 1 Review Chapter 1 Our place in the universe
Test 1 Review Bring Gator 1 ID card Bring pencil #2 with eraser No use of calculator or any electronic device during the exam We provide the scantrons Formulas will be projected on the screen You can use
More informationChapter 16 The Solar System
Chapter 16 The Solar System Finding the Standard Time and Date at Another Location Example When it is 12 noon in London, what is the standard time in Denver, Colorado (40 N, 105 W)? Section 15.3 Finding
More informationSkyGlobe Planetarium
SkyGlobe Planetarium Introduction: This exercise will simulate the night sky and demonstrate a number of principles of the celestial sphere and the motions of the Earth and planets. Getting Started: 1.
More informationTycho Brahe
Tycho Brahe 1546-1601 At the time of Shakespeare and Elizabeth I and Champlain Lost part of his nose in a duel over who was the best mathematician At 27 he measured the distance of a supernova and a comet
More informationAJJAR Astronomical Javascript/Java Applet Resource
AJJAR Astronomical Javascript/Java Applet Resource Siobahn Morgan Department of Earth Science University of Northern Iowa Siobahn.Morgan@uni.edu Abstract The AJJAR (Astronomical Javascript/Java Applet
More informationThe Flammarion engraving by an unknown artist, first documented in Camille Flammarion's 1888 book L'atmosphère: météorologie populaire.
The Flammarion engraving by an unknown artist, first documented in Camille Flammarion's 1888 book L'atmosphère: météorologie populaire. Horizon Coordinates: Altitude (angular height above horizon) Azimuth
More informationOUTSIDE LAB 4: Finding the Distances and Sizes of Remote Objects
OUTSIDE LAB 4: Finding the Distances and Sizes of Remote Objects OBJECTIVE: To use the principles of trigonometry to find the distances to remote objects and then to find their dimensions. DISCUSSION:
More informationIntroduction The Role of Astronomy p. 3 Astronomical Objects of Research p. 4 The Scale of the Universe p. 7 Spherical Astronomy Spherical
Introduction The Role of Astronomy p. 3 Astronomical Objects of Research p. 4 The Scale of the Universe p. 7 Spherical Astronomy Spherical Trigonometry p. 9 The Earth p. 12 The Celestial Sphere p. 14 The
More informationSpace-Time Reference Systems
Space-Time Reference Systems Bearbeitet von Michael Soffel, Ralf Langhans 1. Auflage 2012. Buch. xiv, 314 S. Hardcover ISBN 978 3 642 30225 1 Format (B x L): 15,5 x 23,5 cm Gewicht: 654 g Weitere Fachgebiete
More informationExam# 1 Review Gator 1 Keep the first page of the exam. Scores will be published using the exam number Chapter 0 Charting the Heavens
Exam# 1 Review Exam is Wednesday October 11 h at 10:40AM, room FLG 280 Bring Gator 1 ID card Bring pencil #2 (HB) with eraser. We provide the scantrons No use of calculator or any electronic device during
More informationAstronomy. 1. (3 pts.) What is meant by the apparent magnitude of a star?
Astronomy Name NaSc 109 Summer 2018 Exam 2 Don't Panic! Take a big deep breath... hold it... holllld it now let it out. Use your available time on this exam very efficiently; if you don't know an answer
More informationPHYS 160 Astronomy Test #1 Name Answer Key Test Version A
PHYS 160 Astronomy Test #1 Name Answer Key Test Version A True False Multiple Choice 1. T 1. C 2. F 2. B 3. T 3. A 4. T 4. E 5. T 5. B 6. F 6. A 7. F 7. A 8. T 8. D 9. F 9. D 10. F 10. B 11. B 12. D Definitions
More informationr p L = = So Jupiter has the greater angular momentum.
USAAAO 2015 Second Round Solutions Problem 1 T 10000 K, m 5, d 150 pc m M 5 log(d/10) M m 5 log(d/10) 5 5 log(15) 0.88 We compare this with the absolute magnitude of the sun, 4.83. solar 100 (4.83 0.88)/5
More informationExam #1 Covers material from first day of class, all the way through Tides and Nature of Light Supporting reading chapters 1-5 Some questions are
Exam #1 Covers material from first day of class, all the way through Tides and Nature of Light Supporting reading chapters 1-5 Some questions are concept questions, some involve working with equations,
More informationToday. Planetary Motion. Tycho Brahe s Observations. Kepler s Laws of Planetary Motion. Laws of Motion. in physics
Planetary Motion Today Tycho Brahe s Observations Kepler s Laws of Planetary Motion Laws of Motion in physics Page from 1640 text in the KSL rare book collection That the Earth may be a Planet the seeming
More informationPhysics Lab #4: Learning Starry Night, Part 3
Physics 10293 Lab #4: Learning Starry Night, Part 3 Introduction In this lab, we will continue using Starry Night to explore some of the most important concepts we will cover in lecture. Continue with
More informationAST111 PROBLEM SET 2 SOLUTIONS. RA=02h23m35.65s, DEC=+25d18m42.3s (Epoch J2000).
AST111 PROBLEM SET 2 SOLUTIONS Home work problems 1. Angles on the sky and asteroid motion An asteroid is observed at two different times. The asteroid is located at RA=02h23m35.65s, DEC=+25d18m42.3s (Epoch
More informationChapter 0 2/19/2014. Lecture Outline. 0.1 The Obvious View. Charting the Heavens. 0.1 The Obvious View. 0.1 The Obvious View. Units of Chapter 0
Lecture Outline Chapter 0 Charting the Heavens Earth is average we don t occupy any special place in the universe Universe: Totality of all space, time, matter, and energy Astronomy: Study of the universe
More informationROCZNIK ASTRONOMICZNY (ASTRONOMICAL ALMANAC) OF THE INSTITUTE OF GEODESY AND CARTOGRAPHY AGAINST THE IAU 2000 RESOLUTIONS
ROCZNIK ASTRONOMICZNY (ASTRONOMICAL ALMANAC) OF THE INSTITUTE OF GEODESY AND CARTOGRAPHY AGAINST THE IAU 2000 RESOLUTIONS M. SĘKOWSKI Institute of Geodesy and Cartography ul. Modzelewskiego 27, Warsaw,
More informationThe Measurement of Time
CHAPTER TWO The Measurement of Time Solar Time In antiquity the time of day was measured by the direction of a shadow cast in sunlight. This resulted in the development of a wide variety of sophisticated
More informationREVIEW CH #0. 1) Right ascension in the sky is very similar to latitude on the Earth. 1)
REVIEW CH #0 TRUE/FALSE. Write 'T' if the statement is true and 'F' if the statement is false. 1) Right ascension in the sky is very similar to latitude on the Earth. 1) 2) Latitude and right ascension
More informationMapping Document. GCSE (9-1) Astronomy. Pearson Edexcel Level 1/Level 2 GCSE (9-1) in Astronomy (1AS0)
Mapping Document GCSE (9-1) Astronomy Pearson Edexcel Level 1/Level 2 GCSE (9-1) in Astronomy (1AS0) GCSE (9-1) Astronomy Mapping document This document is designed to help you compare the existing 2011
More informationCoordinate Systems fundamental circle secondary great circle a zero point
Astrometry Coordinate Systems There are different kinds of coordinate systems used in astronomy. The common ones use a coordinate grid projected onto the celestial sphere. These coordinate systems are
More informationA2 Principi di Astrofisica. Coordinate Celesti
A2 Principi di Astrofisica Coordinate Celesti ESO La Silla Tel. 3.6m Celestial Sphere Our lack of depth perception when we look into space creates the illusion that Earth is surrounded by a celestial sphere.
More informationAdvanced Astronomy, C.P.
East Penn School District Secondary Curriculum A Planned Course Statement for Advanced Astronomy, C.P. Course # 422 Grade(s) 10, 11,12 Department: Science ength of Period (mins.) 40 Total Clock Hours:
More informationAST 2010 Descriptive Astronomy Study Guide Exam I
AST 2010 Descriptive Astronomy Study Guide Exam I Wayne State University 1 Introduction and overview Identify the most significant structures in the universe: Earth, planets, Sun, solar system, stars,
More informationFundamental Astronomy
H. Karttunen P. Kroger H. Oja M.Poutanen K.J. Donner (Eds.) Fundamental Astronomy Fifth Edition With 449 Illustrations Including 34 Colour Plates and 75 Exercises with Solutions < J Springer VII 1. Introduction
More informationToday. Planetary Motion. Tycho Brahe s Observations. Kepler s Laws Laws of Motion. Laws of Motion
Today Planetary Motion Tycho Brahe s Observations Kepler s Laws Laws of Motion Laws of Motion In 1633 the Catholic Church ordered Galileo to recant his claim that Earth orbits the Sun. His book on the
More informationANNEX 1. DEFINITION OF ORBITAL PARAMETERS AND IMPORTANT CONCEPTS OF CELESTIAL MECHANICS
ANNEX 1. DEFINITION OF ORBITAL PARAMETERS AND IMPORTANT CONCEPTS OF CELESTIAL MECHANICS A1.1. Kepler s laws Johannes Kepler (1571-1630) discovered the laws of orbital motion, now called Kepler's laws.
More informationKEELE UNIVERSITY SCHOOL OF CHEMICAL AND PHYSICAL SCIENCES Year 1 ASTROPHYSICS LAB. WEEK 1. Introduction
KEELE UNIVERSITY SCHOOL OF CHEMICAL AND PHYSICAL SCIENCES Year 1 ASTROPHYSICS LAB WEEK 1. Introduction D. E. McLaughlin January 2011 The purpose of this lab is to introduce you to some astronomical terms
More informationInternational Olympiad on Astronomy and Astrophysics (IOAA)
Syllabus of International Olympiad on Astronomy and Astrophysics (IOAA) General Notes 1. Extensive contents in basic astronomical concepts are required in theoretical and practical problems. 2. Basic concepts
More informationIf Earth had no tilt, what else would happen?
A more in depth explanation from last week: If Earth had no tilt, what else would happen? The equator would be much hotter due to the direct sunlight which would lead to a lower survival rate and little
More informationThe Revolution of the Moons of Jupiter
The Revolution of the Moons of Jupiter Overview: During this lab session you will make use of a CLEA (Contemporary Laboratory Experiences in Astronomy) computer program generously developed and supplied
More informationarxiv: v1 [astro-ph.ep] 18 Oct 2016
Demonstrating the Elliptical Orbit of Mars using Naked Eye Data Kevin Krisciunas 1 ABSTRACT arxiv:1610.05750v1 [astro-ph.ep] 18 Oct 2016 Over the course of eleven months we determined the position of Mars
More information3) During retrograde motion a planet appears to be A) dimmer than usual. B) the same brightness as usual C) brighter than usual.
Descriptive Astronomy (ASTR 108) Exam 1 B February 17, 2010 Name: In each of the following multiple choice questions, select the best possible answer. In the line on the scan sheet corresponding to the
More information1) Kepler's third law allows us to find the average distance to a planet from observing its period of rotation on its axis.
Descriptive Astronomy (ASTR 108) Exam 1 A February 17, 2010 Name: In each of the following multiple choice questions, select the best possible answer. In the line on the scan sheet corresponding to the
More informationTransforming from Geographic to Celestial Coordinates
Transforming from Geographic to Celestial Coordinates Michael McEllin 1 Introduction The simplest astronomical observation of all is that the stars appear to move around the Earth (which, of course is
More informationMASSACHUSETTS INSTITUTE OF TECHNOLOGY Physics Exploring Black Holes General Relativity and Astrophysics Spring 2003
MASSACHUSETTS INSTITUTE OF TECHNOLOGY Physics 8.224 Exploring Black Holes General Relativity and Astrophysics Spring 2003 ASSIGNMENT WEEK 5 NOTE: Exercises 6 through 8 are to be carried out using the GRorbits
More informationThe Mass of Jupiter Student Guide
The Mass of Jupiter Student Guide Introduction: In this lab, you will use astronomical observations of Jupiter and its satellites to measure the mass of Jupiter. We will use the program Stellarium to simulate
More informationNotes 10-3: Ellipses
Notes 10-3: Ellipses I. Ellipse- Definition and Vocab An ellipse is the set of points P(x, y) in a plane such that the sum of the distances from any point P on the ellipse to two fixed points F 1 and F
More information1. The Moon appears larger when it rises than when it is high in the sky because
2-1 Copyright 2016 All rights reserved. No reproduction or distribution without the prior written consent of 1. The Moon appears larger when it rises than when it is high in the sky because A. you are
More informationContents. List of Applications. Basic Concepts 1. iii
46891_01_FM_pi_pxviii.QXD 10/1/09 3:25 PM Page iii 1 List of Applications ix Preface xiii Basic Concepts 1 Unit 1A REVIEW OF OPERATIONS WITH WHOLE NUMBERS 2 1.1 Review of Basic Operations 2 1.2 Order of
More informationThe Earth and the Sky
The Earth and the Sky In this class, we want to understand why the objects in the sky as seen from the Earth - appear as they do. Even though we haven t yet discussed the details, I am assuming that there
More informationAstronomy 1143 Quiz 1 Review
Astronomy 1143 Quiz 1 Review Prof. Pradhan September 7, 2017 I What is Science? 1. Explain the difference between astronomy and astrology. Astrology: nonscience using zodiac sign to predict the future/personality
More informationDAY LABORATORY EXERCISE #5: PARALLAX & TRIANGULATION
AS102 - Day Laboratory Exercise: Parallax Page 1 DAY LABORATORY EXERCISE #5: PARALLAX & TRIANGULATION Goals: To use trigonometry to determine distances and sizes of objects To gain experience in measuring
More informationIn the space below, write an explanation for why we observe phases of the moon, based upon your current knowledge:
IDS 102 Phases of the Moon PART II In the space below, write an explanation for why we observe phases of the moon, based upon your current knowledge: As you discovered yesterday, when we observe the Earth
More informationBasic Physics. Remaining Topics. Gravitational Potential Energy. PHYS 1403 Introduction to Astronomy. Can We Create Artificial Gravity?
PHYS 1403 Introduction to Astronomy Basic Physics Chapter 5 Remaining Topics Gravitational Potential Energy Escape Velocity Artificial Gravity Gravity Assist An Alternate Theory of Gravity Gravitational
More informationIntroduction to Astronomy Laboratory Exercise #1. Intro to the Sky
Introduction to Astronomy Laboratory Exercise #1 Partners Intro to the Sky Date Section Purpose: To develop familiarity with the daytime and nighttime sky through the use of Stellarium. Equipment: Computer
More informationD. A system of assumptions and principles applicable to a wide range of phenomena that has been repeatedly verified
ASTRONOMY 1 EXAM 1 Name Identify Terms - Matching (20 @ 1 point each = 20 pts.) 1 Solar System G 7. aphelion N 14. eccentricity M 2. Planet E 8. apparent visual magnitude R 15. empirical Q 3. Star P 9.
More informationA User s Guide to the Sky
A User s Guide to the Sky Constellations Betelgeuse Rigel Stars are named by a Greek letter ( ) according to their relative brightness within a given constellation plus the possessive form of the name
More informationCoordinate Systems fundamental circle secondary great circle a zero point
Astrometry Coordinate Systems There are different kinds of coordinate systems used in astronomy. The common ones use a coordinate grid projected onto the celestial sphere. These coordinate systems are
More informationIAU 2006 NFA GLOSSARY
IAU 2006 NFA GLOSSARY Prepared by the IAU Division I Working Group Nomenclature for Fundamental Astronomy'' (latest revision: 20 November 2007) Those definitions corresponding to the IAU 2000 resolutions
More informationAstronomy. The Seasons
Astronomy The Seasons The seasons are caused by the inclination of the Earth s axis: when a hemisphere is tipped toward the Sun, the Sun is more directly above it. At the Summer Solstice the tilt is most
More informationPLANETARIUM SIMULATION SYSTEM
PLANETARIUM SIMULATION SYSTEM Prof. Dr. W. Kowalk FB Informatik Universität Oldenburg, Germany Ammerländer Heerstraße 114-128, D-26129 Oldenburg Kowalk@informatik.uni-oldenburg.de Abstract This paper describes
More informationAstronomy 291. Professor Bradley M. Peterson
Astronomy 291 Professor Bradley M. Peterson The Sky As a first step, we need to understand the appearance of the sky. Important points (to be explained): The relative positions of stars remain the same
More informationAssignment 1. Due Feb. 11, 2019
Assignment 1 Due Feb. 11, 2019 Show all work and turn in answers on separate pages, not on these pages. Circle your final answers for clarity. Be sure to show/explain all of your reasoning and that your
More informationSurvey of Astronomy ASTRO 110-5
Survey of Astronomy ASTRO 110-5 Prof. Istvan Szapudi Institute for Astronomy IfA B204/WAT 401 Phone: 956 6196 Email: szapudi@ifa.hawaii.edu Class meets TTh 12:00 to 13:15 WAT 112 Office Hours after class
More informationCHAPTER 8 PLANETARY MOTIONS
1 CHAPTER 8 PLANETARY MOTIONS 8.1 Introduction The word planet means wanderer (πλάνητες αστέρες wandering stars); in contrast to the fixed stars, the planets wander around on the celestial sphere, sometimes
More information60 C From Bicycle to Space. Dionysis Konstantinou Corina Toma. Space Travel
60 C From Bicycle to Space Dionysis Konstantinou Corina Toma C Space Travel From Bicycle Length to Space of the CDay61 introduction Imagine travelling from one planet to another Why is it that we have
More informationChapter 2. Altitude Measurement
Chapter Altitude Measurement Although altitudes and zenith distances are equally suitable for navigational calculations, most formulas are traditionally based upon altitudes which are easily accessible
More informationReading Reminders. Your Questions via JiTT2
ASTR1010 Lecture 5 29 Jan 13 Today How the Sky Works: Stars, Seasons, Phases Announcements: Old-Fashioned Homework 1 released tonight on D2L, due ON PAPER next Tuesday at the start of class If you brought
More informationOrbital Mechanics. CTLA Earth & Environmental Science
Orbital Mechanics CTLA Earth & Environmental Science The Earth Spherical body that is flattened near the poles due to centrifugal force (rotation of the Earth) 40,074 KM across at the Equator 40,0007 KM
More informationASTRO 6570 Lecture 1
ASTRO 6570 Lecture 1 Historical Survey EARLY GREEK ASTRONOMY: Earth-centered universe - Some radical suggestions for a sun-centered model Shape of the Earth - Aristotle (4 th century BCE) made the first
More informationResearch Article Geodesic Effect Near an Elliptical Orbit
Applied Mathematics Volume 2012, Article ID 240459, 8 pages doi:10.1155/2012/240459 Research Article Geodesic Effect Near an Elliptical Orbit Alina-Daniela Vîlcu Department of Information Technology, Mathematics
More informationOrbital and Celestial Mechanics
Orbital and Celestial Mechanics John P. Vinti Edited by Gim J. Der TRW Los Angeles, California Nino L. Bonavito NASA Goddard Space Flight Center Greenbelt, Maryland Volume 177 PROGRESS IN ASTRONAUTICS
More informationAstronomical coordinate systems. ASTR320 Monday January 22, 2018
Astronomical coordinate systems ASTR320 Monday January 22, 2018 Special public talk this week: Mike Brown, Pluto Killer Wednesday at 7:30pm in MPHY204 Other news Munnerlyn lab is hiring student engineers
More informationThe Stars. Background & History The Celestial Sphere: Fixed Stars and the Luminaries
The Stars Background & History The Celestial Sphere: Fixed Stars and the Luminaries The Appearance of Stars on the Sky Brightness and Brightness Variations Atmospheric Effects: Twinkling Variable Stars
More information