Light. Physics Gymnasium 15/06/00. Outline. Einstein s Theory of Relativity Outrageous, but true! What about Galileo and Newton? What about Einstein?
|
|
- Victor Weaver
- 7 years ago
- Views:
Transcription
1 Outline Einstein s Theory of Relativity Outrageous, but true! Galileo and Newton The start of eletromagnetism Einstein - The Theory of Speial Relativity Einstein - The Theory of General Relativity Physis Gymnasium, June 2000 by David N. Jamieson, PhD, FAIP Shool of Physis University of Melbourne Light What about Galileo and Newton? Light real light radio waves (x-rays, gamma rays, mirowaves, or any other sort of eletromagneti field) Speed is = 299,792,458 m/s (1 billion km/hr) fast but finite Alternative pitures of light: waves or partiles Galileo: The laws of Physis do not depend on absolute motion (does this inlude eletromagnetism?) Newton: An objet one set in motion remains in motion until ated upon by an external fore The universe is governed by a majesti lokwork where all loks everywhere at all times tik in perfet synhronisation. What about Einstein? Time, spae and gravity The theory of Speial Relativity for fast objets The theory of General Relativity for high objets Essential and entral to the funtioning of the Global Positioning System!! How fast are we going? Relative to surfae of Earth? Relative to the Sun?...entre of Galaxy?...origin of Big Bang? Can t use ordinary Mehanis to test this! What about eletromagnetism? Can we use properties of light? by Dr D.N. Jamieson 1
2 Galileo and Newton knew that, in the absene of frition, a ball would roll down a hill and up the same height on the other side. Galileo and Newton knew that, in the absene of frition, a ball would roll down a hill and up the same height on the other side. Galileo and Newton knew that, in the absene of frition, a ball would roll down a hill and up the same height on the other side. A flat bit in the middle makes no differene. A flat bit in the middle makes no differene. A flat bit in the middle makes no differene. Coasting at onstant speed by Dr D.N. Jamieson 2
3 What about if you get rid of the seond hill? What about if you get rid of the seond hill? To infinity at onstant speed How fast are we going anyway? Galileo (and Newton) knew that an objet, one set in motion, ontinues indefinitely at onstant speed unless ated upon by an external fore. Cannot detet this motion from inside Sun s Orbit around galaxy: 250 km/s Twie the speed of sound and not a drop spilled! Lifestyle of a Conorde passenger...or parked at the gate? Milky Way Galaxy trajetory towards Great Attrator: 7000 km/s Earth s Orbit around Sun: 30 km/s But eletromagnetism (and light) may be different Eletrostati fore: F = kqq/r 2 q r Q Magneti fore: F = qvb N S q...magneti fore depends on the speed, v! Light is an eletromagneti wave So experiments with light might allow us to detet our absolute speed through the osmos! So how does light behave? Possible Answers: Like Tennis Balls? Like Sound Waves? Like Something Else? by Dr D.N. Jamieson 3
4 Like tennis balls? Like tennis balls? 100 km/hr 0 km/hr 100 km/hr Like tennis balls? Like tennis balls? NO! v v? v Light signals would get out of syn!! True situation +v + v? +v Like sound waves? Like sound waves? Speed of sound in air always Mah 1 Mah 1 Mah 2 by Dr D.N. Jamieson 4
5 Like sound waves Like sound waves? Aether wind! Sound in Air Air has pressure Made of O, N, Ar Has mass You breath it... Light in Aether? Aether is insubstantial Very elasti Other properties??? 30 km/s? 30 km/s Like sound waves? NO!! Mihelson -Morley experiment found no differene! 30 km/s Summary Objet Us Them Us 0 v Them v 0 Tennis Ball 0 100km/hr Sound Wave speed of sound speed of sound v Light v Enter Einstein The Speial Theory of Relativity Light annot be used to measure an absolute speed! This is entirely onsistent with the rest of the laws of physis whih apply to mehanis And light does not behave like tennis balls light does not behave like sound waves What does this mean? Laws of Physis the same for everybody The speed Sun s of light the same for everybody moves at Let us look at speed a startling onsequene of these fats Sun s light moves at speed by Dr D.N. Jamieson 5
6 The Light Clok The Light Clok A photon bouning between mirrors may be used as a lok A photon bouning between mirrors may be used as a lok The Light Clok A photon bouning between mirrors may be used as a lok Moving Clok is slow! Speed Short distane Long distane Speed tik Moving loks run slow! The Twin Phenomenon Cosmi Rays reate fast muons in outer atmosphere Idential muons reated in the laboratory live for 2.2 millionths of a seond Even at speed of light, this is not long enough to reah sea level! Fast muons live longer than slow muons Fast muons reated here Expet to deay here See plenty here! by Dr D.N. Jamieson 6
7 Summary Galaxy rossing protons Constant speed of light leads to: Time dilation: 1 t = t t = γ. t whereγ v = 1 v Galaxy view proton speed v < (just) γ = Cross galaxy in t=10 5 years Proton view galaxy speed v < (just) L = L/γ = 10 5 /10 10 = 10-5 l.y. = 95 million km = 0.7 A.U. Hene t = L / = 10-5 years = 315 seonds Gamma is always greater than 1! (The bigger the better) Galaxy View L = 10 5 light years Proton View SS433 - The strangest objet in our galaxy Relativity and Spae Travel The entral engine produes jets of matter moving at 25% the speed of light! Neutron star Before Roket and fuel at rest Fuel After Fuel thrown away Roket goes forward by onservation of momentum Normal star Fuel Chemial Rokets Gravitational Slingshot Can use gravity to boune off a planet Pik up twie the orbital speed for a head-on ollision! v 2 = 29.6 km/s v o = 9.6 km/s NB: Essential that trajetory does not interset planet! v 1 = 10.4 km/s by Dr D.N. Jamieson 7
8 High Speed Exhaust - Ion Engine Use Hg +, Xe + or Cs + as reation mass Aelerate ions to 1% by eletri fields Low thrust (not many ions per seond) But be patient! Laboratory test In flight To the Stars Prelaunh High temperature exhaust - Nulear Engines High temperature exhaust: Nulear Engines NERVA nulear roket prototype Built in USA in 1960 s Suffered from failure of the nulear ore 1 2 For the future: high temperature fusion or even fission engines Extremely high exhaust temperatures 3 Nulear Pulse Jet Antimatter rokets Momentum from nulear explosions Conept tested with hemial explosives by Dr D.N. Jamieson 8
9 Ultra fast exhaust - Light Ramsoop: Burn the interstellar medium Starwisp interstellar probe Burn interstellar hydrogen Density 1 atom/m 3 DNJ Seal of Approval 1000 km 2 mylar with 20nm Si oating Ramsoop Maths Kineti Energy of Relativisti Spaeraft Speed (v/) γ = 1/(1-v 2 / 2 ) 1/2 Kineti Energy (J/kg) Compare: 100 km/hr USA annual eletri power (1982) 8.5x10 18 J World annual eletri power (1982) 4.5x10 3.1x10 10 J Solar flux on Earth for 1 year 5.3x10 24 J x x x x x , x Gev eletron in a storage ring at CERN General Relativity Equivalene Priniple... remained, for forty years after its disovery (by Einstein), an austere intelletual monument - a somewhat sterile topi isolated from the mainstream of physis and astronomy - whose pratitioners were magnifient ultural ornaments In the late 20thC, GR is an engineering subjet! Inertial mass: F = m i a Gravitational mass: F = GMm g /r 2 Newton knew m i = m g Why? by Dr D.N. Jamieson 9
10 Equivalene Priniple Experimental test of C=2πr Sine m i = m g these are equivalent (same laws of Physis, everything) Radius, r Measured C/r Cirumfrene, C 10 m 62.8 m m m m m m m ,000 km 40,0000 km 4.00 Yikes!! C<2πr Why?? Drawing the Big Cirle (on Earth) C<2πr for irles drawn on urved surfaes Drawing the Big Cirle (off Earth) Apply Equivalene Priniple Apply Equivalene Priniple Twenty 1 metre rulers laid down around rim by observer on ground Cirumfrene is 20 m = 2πr Veloity of rim View from rotating disk Artifiial gravity in the ontrol room of the Disovery (2001- A spae Odyssey) by Dr D.N. Jamieson 10
11 Apply Equivalene Priniple Apply Equivalene Priniple Observer on rim sees rulers going past at high speed I am standing on the bottom of a stationary ylinder wathing lots of rulers go past Cirumfrene now measued by ontrated rulers I am standing on the bottom of a stationary ylinder wathing lots of rulers go past They are shrunken to less than 1 m by Lorentz ontration! Fast moving shrunken ruler Same number as before, but shorter Cirumfrene is less than 2πr! Apply Equivalene Priniple Conlusion Gravity points outwards on rim of rotating disk C < 2πR there Gravity points inwards on Earth C > 2πr there Earth s gravity makes more spae! The Speed of Light is the same for everybody The Laws of Physis are the same for everybody Moving loks run slow Moving objets ontrat Gravity and aeleration are the same thing Spae is warped Experimental status: All OK! by Dr D.N. Jamieson 11
Relativity in the Global Positioning System
Relativity in the Global Positioning System Neil Ashby Department of Physis,UCB 390 University of Colorado, Boulder, CO 80309-00390 NIST Affiliate Email: ashby@boulder.nist.gov July 0, 006 AAPT workshop
More informationPhysics 43 HW 3 Serway Chapter 39 & Knight Chapter 37
Physis 43 HW 3 Serway Chapter 39 & Knight Chapter 37 Serway 7 th Edition Chapter 39 Problems: 15, 1, 5, 57, 60, 65 15. Review problem. An alien ivilization oupies a brown dwarf, nearly stationary relative
More informationTHE UNIVERSITY OF THE STATE OF NEW YORK THE STATE EDUCATION DEPARTMENT ALBANY, NY
P THE UNIVERSITY OF THE STATE OF NEW YORK THE STATE EDUCATION DEPARTMENT ALBANY, NY 4 Referene Tables for Physial Setting/PHYSICS 006 Edition List of Physial Constants Name Symbol Value Universal gravitational
More informationarxiv:astro-ph/0304006v2 10 Jun 2003 Theory Group, MS 50A-5101 Lawrence Berkeley National Laboratory One Cyclotron Road Berkeley, CA 94720 USA
LBNL-52402 Marh 2003 On the Speed of Gravity and the v/ Corretions to the Shapiro Time Delay Stuart Samuel 1 arxiv:astro-ph/0304006v2 10 Jun 2003 Theory Group, MS 50A-5101 Lawrene Berkeley National Laboratory
More information1.1 A Modern View of the Universe" Our goals for learning: What is our place in the universe?"
Chapter 1 Our Place in the Universe 1.1 A Modern View of the Universe What is our place in the universe? What is our place in the universe? How did we come to be? How can we know what the universe was
More informationPhysical and mathematical postulates behind relativity
Physial and mathematial postulates behind relativity Tuomo Suntola Physis Foundations Soiety, Finland, www.physisfoundations.org In this presentation we look for answers to questions: What was the problem
More information10.1 The Lorentz force law
Sott Hughes 10 Marh 2005 Massahusetts Institute of Tehnology Department of Physis 8.022 Spring 2004 Leture 10: Magneti fore; Magneti fields; Ampere s law 10.1 The Lorentz fore law Until now, we have been
More informationThe Sun and Solar Energy
I The Sun and Solar Energy One of the most important forces behind global change on Earth is over 90 million miles distant from the planet. The Sun is the ultimate, original source of the energy that drives
More informationAstronomy 110 Homework #04 Assigned: 02/06/2007 Due: 02/13/2007. Name:
Astronomy 110 Homework #04 Assigned: 02/06/2007 Due: 02/13/2007 Name: Directions: Listed below are twenty (20) multiple-choice questions based on the material covered by the lectures this past week. Choose
More informationDerivation of Einstein s Equation, E = mc 2, from the Classical Force Laws
Apeiron, Vol. 14, No. 4, Otober 7 435 Derivation of Einstein s Equation, E = m, from the Classial Fore Laws N. Hamdan, A.K. Hariri Department of Physis, University of Aleppo, Syria nhamdan59@hotmail.om,
More informationHow To Understand General Relativity
Chapter S3 Spacetime and Gravity What are the major ideas of special relativity? Spacetime Special relativity showed that space and time are not absolute Instead they are inextricably linked in a four-dimensional
More informationRelativistic Kinematics -a project in Analytical mechanics Karlstad University
Relativisti Kinematis -a projet in Analytial mehanis Karlstad University Carl Stigner 1th January 6 Abstrat The following text is a desription of some of the ontent in hapter 7 in the textbook Classial
More information5. The Nature of Light. Does Light Travel Infinitely Fast? EMR Travels At Finite Speed. EMR: Electric & Magnetic Waves
5. The Nature of Light Light travels in vacuum at 3.0. 10 8 m/s Light is one form of electromagnetic radiation Continuous radiation: Based on temperature Wien s Law & the Stefan-Boltzmann Law Light has
More informationName: Earth 110 Exploration of the Solar System Assignment 1: Celestial Motions and Forces Due in class Tuesday, Jan. 20, 2015
Name: Earth 110 Exploration of the Solar System Assignment 1: Celestial Motions and Forces Due in class Tuesday, Jan. 20, 2015 Why are celestial motions and forces important? They explain the world around
More information1 A Solar System Is Born
CHAPTER 3 1 A Solar System Is Born SECTION Formation of the Solar System BEFORE YOU READ After you read this section, you should be able to answer these questions: What is a nebula? How did our solar system
More informationClassical Electromagnetic Doppler Effect Redefined. Copyright 2014 Joseph A. Rybczyk
Classial Eletromagneti Doppler Effet Redefined Copyright 04 Joseph A. Rybzyk Abstrat The lassial Doppler Effet formula for eletromagneti waves is redefined to agree with the fundamental sientifi priniples
More information8.1 Radio Emission from Solar System objects
8.1 Radio Emission from Solar System objects 8.1.1 Moon and Terrestrial planets At visible wavelengths all the emission seen from these objects is due to light reflected from the sun. However at radio
More informationAnother Look at Gaussian CGS Units
Another Look at Gaussian CGS Units or, Why CGS Units Make You Cool Prashanth S. Venkataram February 24, 202 Abstrat In this paper, I ompare the merits of Gaussian CGS and SI units in a variety of different
More informationComay s Paradox: Do Magnetic Charges Conserve Energy?
Comay s Paradox: Do Magneti Charges Conserve Energy? 1 Problem Kirk T. MDonald Joseph Henry Laboratories, Prineton University, Prineton, NJ 08544 (June 1, 2015; updated July 16, 2015) The interation energy
More informationExam # 1 Thu 10/06/2010 Astronomy 100/190Y Exploring the Universe Fall 11 Instructor: Daniela Calzetti
Exam # 1 Thu 10/06/2010 Astronomy 100/190Y Exploring the Universe Fall 11 Instructor: Daniela Calzetti INSTRUCTIONS: Please, use the `bubble sheet and a pencil # 2 to answer the exam questions, by marking
More informationUse the following information to deduce that the gravitational field strength at the surface of the Earth is approximately 10 N kg 1.
IB PHYSICS: Gravitational Forces Review 1. This question is about gravitation and ocean tides. (b) State Newton s law of universal gravitation. Use the following information to deduce that the gravitational
More informationChapter 1: Our Place in the Universe. 2005 Pearson Education Inc., publishing as Addison-Wesley
Chapter 1: Our Place in the Universe Topics Our modern view of the universe The scale of the universe Cinema graphic tour of the local universe Spaceship earth 1.1 A Modern View of the Universe Our goals
More informationChapter 1 Our Place in the Universe
Chapter 1 Our Place in the Universe Syllabus 4 tests: June 18, June 30, July 10, July 21 Comprehensive Final - check schedule Website link on blackboard 1.1 Our Modern View of the Universe Our goals for
More informationCarol and Charles see their pencils fall exactly straight down.
Section 24-1 1. Carol is in a railroad car on a train moving west along a straight stretch of track at a constant speed of 120 km/h, and Charles is in a railroad car on a train at rest on a siding along
More informationUNIT V. Earth and Space. Earth and the Solar System
UNIT V Earth and Space Chapter 9 Earth and the Solar System EARTH AND OTHER PLANETS A solar system contains planets, moons, and other objects that orbit around a star or the star system. The solar system
More informationLesson 6: Earth and the Moon
Lesson 6: Earth and the Moon Reading Assignment Chapter 7.1: Overall Structure of Planet Earth Chapter 7.3: Earth s Interior More Precisely 7-2: Radioactive Dating Chapter 7.5: Earth s Magnetosphere Chapter
More informationClass 2 Solar System Characteristics Formation Exosolar Planets
Class 1 Introduction, Background History of Modern Astronomy The Night Sky, Eclipses and the Seasons Kepler's Laws Newtonian Gravity General Relativity Matter and Light Telescopes Class 2 Solar System
More informationQ3.2.a The gravitational force exerted by a planet on one of its moons is 3e23 newtons when the moon is at a particular location.
Q3.2.a The gravitational force exerted by a planet on one of its moons is 3e23 newtons when the moon is at a particular location. If the mass of the moon were three times as large, what would the force
More informationBeginning of the Universe Classwork 6 th Grade PSI Science
Beginning of the Universe Classwork Name: 6 th Grade PSI Science 1 4 2 5 6 3 7 Down: 1. Edwin discovered that galaxies are spreading apart. 2. This theory explains how the Universe was flattened. 3. All
More informationIntroduction to the Solar System
Introduction to the Solar System Lesson Objectives Describe some early ideas about our solar system. Name the planets, and describe their motion around the Sun. Explain how the solar system formed. Introduction
More informationAdvanced Topics in Physics: Special Relativity Course Syllabus
Advanced Topics in Physics: Special Relativity Course Syllabus Day Period What How 1. Introduction 2. Course Information 3. Math Pre-Assessment Day 1. Morning 1. Physics Pre-Assessment 2. Coordinate Systems
More informationPretest Ch 20: Origins of the Universe
Name: _Answer key Pretest: _2_/ 58 Posttest: _58_/ 58 Pretest Ch 20: Origins of the Universe Vocab/Matching: Match the definition on the left with the term on the right by placing the letter of the term
More informationNewton s Law of Gravity
Gravitational Potential Energy On Earth, depends on: object s mass (m) strength of gravity (g) distance object could potentially fall Gravitational Potential Energy In space, an object or gas cloud has
More informationFriday 20 January 2012 Morning
THIS IS A NEW SPECIFICATION H Friday 20 January 2012 Morning GCSE TWENTY FIRST CENTURY SCIENCE PHYSICS A A181/02 Modules P1 P2 P3 (Higher Tier) *A131500112* Candidates answer on the Question Paper. A calculator
More informationLecture 7 Formation of the Solar System. Nebular Theory. Origin of the Solar System. Origin of the Solar System. The Solar Nebula
Origin of the Solar System Lecture 7 Formation of the Solar System Reading: Chapter 9 Quiz#2 Today: Lecture 60 minutes, then quiz 20 minutes. Homework#1 will be returned on Thursday. Our theory must explain
More informationFrom lowest energy to highest energy, which of the following correctly orders the different categories of electromagnetic radiation?
From lowest energy to highest energy, which of the following correctly orders the different categories of electromagnetic radiation? From lowest energy to highest energy, which of the following correctly
More informationCELESTIAL CLOCK - THE SUN, THE MOON, AND THE STARS
INTRODUCTION CELESTIAL CLOCK - THE SUN, THE MOON, AND THE STARS This is a scientific presentation to provide you with knowledge you can use to understand the sky above in relation to the earth. Before
More informationastronomy 2008 1. A planet was viewed from Earth for several hours. The diagrams below represent the appearance of the planet at four different times.
1. A planet was viewed from Earth for several hours. The diagrams below represent the appearance of the planet at four different times. 5. If the distance between the Earth and the Sun were increased,
More informationName Class Period. F = G m 1 m 2 d 2. G =6.67 x 10-11 Nm 2 /kg 2
Gravitational Forces 13.1 Newton s Law of Universal Gravity Newton discovered that gravity is universal. Everything pulls on everything else in the universe in a way that involves only mass and distance.
More informationThe University of Texas at Austin. Gravity and Orbits
UTeach Outreach The University of Texas at Austin Gravity and Orbits Time of Lesson: 60-75 minutes Content Standards Addressed in Lesson: TEKS6.11B understand that gravity is the force that governs the
More informationPlanets beyond the solar system
Planets beyond the solar system Review of our solar system Why search How to search Eclipses Motion of parent star Doppler Effect Extrasolar planet discoveries A star is 5 parsecs away, what is its parallax?
More informationScience Standard 4 Earth in Space Grade Level Expectations
Science Standard 4 Earth in Space Grade Level Expectations Science Standard 4 Earth in Space Our Solar System is a collection of gravitationally interacting bodies that include Earth and the Moon. Universal
More informationSummary: Four Major Features of our Solar System
Summary: Four Major Features of our Solar System How did the solar system form? According to the nebular theory, our solar system formed from the gravitational collapse of a giant cloud of interstellar
More informationASTR 100. Lecture 14: Formation of the Solar System and A Brief History of Space Exploration
ASTR 100 Lecture 14: Formation of the Solar System and A Brief History of Space Exploration Reading: Formation of SS (Ch. 6), The Sun (Ch. 10) Friday: Quiz and Ex. 4 due Tuesday: Feb 18 th : Midterm Done
More informationWeek 1-2: Overview of the Universe & the View from the Earth
Week 1-2: Overview of the Universe & the View from the Earth Hassen M. Yesuf (hyesuf@ucsc.edu) September 29, 2011 1 Lecture summary Protein molecules, the building blocks of a living organism, are made
More informationName Class Date. true
Exercises 131 The Falling Apple (page 233) 1 Describe the legend of Newton s discovery that gravity extends throughout the universe According to legend, Newton saw an apple fall from a tree and realized
More informationPractice TEST 2. Explain your reasoning
Practice TEST 2 1. Imagine taking an elevator ride from the1 st floor to the 10 th floor of a building. While moving between the 1 st and 2 nd floors the elevator speeds up, but then moves at a constant
More informationFXA 2008. UNIT G485 Module 5 5.5.1 Structure of the Universe. Δλ = v λ c CONTENTS OF THE UNIVERSE. Candidates should be able to :
1 Candidates should be able to : CONTENTS OF THE UNIVERSE Describe the principal contents of the universe, including stars, galaxies and radiation. Describe the solar system in terms of the Sun, planets,
More informationOrigins of the Cosmos Summer 2016. Pre-course assessment
Origins of the Cosmos Summer 2016 Pre-course assessment In order to grant two graduate credits for the workshop, we do require you to spend some hours before arriving at Penn State. We encourage all of
More information165 points. Name Date Period. Column B a. Cepheid variables b. luminosity c. RR Lyrae variables d. Sagittarius e. variable stars
Name Date Period 30 GALAXIES AND THE UNIVERSE SECTION 30.1 The Milky Way Galaxy In your textbook, read about discovering the Milky Way. (20 points) For each item in Column A, write the letter of the matching
More informationBig bang, red shift and doppler effect
Big bang, red shift and doppler effect 73 minutes 73 marks Page of 26 Q. (a) Scientists have observed that the wavelengths of the light from galaxies moving away from the Earth are longer than expected.
More informationLecture 10 Formation of the Solar System January 6c, 2014
1 Lecture 10 Formation of the Solar System January 6c, 2014 2 Orbits of the Planets 3 Clues for the Formation of the SS All planets orbit in roughly the same plane about the Sun. All planets orbit in the
More informationThe Universe. The Solar system, Stars and Galaxies
The Universe The Universe is everything. All us, the room, the U.S. the earth, the solar system, all the other stars in the Milky way galaxy, all the other galaxies... everything. How big and how old is
More informationImpact Simulation of Extreme Wind Generated Missiles on Radioactive Waste Storage Facilities
Impat Simulation of Extreme Wind Generated issiles on Radioative Waste Storage Failities G. Barbella Sogin S.p.A. Via Torino 6 00184 Rome (Italy), barbella@sogin.it Abstrat: The strutural design of temporary
More informationIsaac Newton. Translated into English by
THE MATHEMATICAL PRINCIPLES OF NATURAL PHILOSOPHY (BOOK 1, SECTION 1) By Isaa Newton Translated into English by Andrew Motte Edited by David R. Wilkins 2002 NOTE ON THE TEXT Setion I in Book I of Isaa
More informationChapter 1 Student Reading
Chapter 1 Student Reading Chemistry is the study of matter You could say that chemistry is the science that studies all the stuff in the entire world. A more scientific term for stuff is matter. So chemistry
More informationTest 2 --- Natural Sciences 102, Professors Rieke --- VERSION B March 3, 2010
Enter your answers on the form provided. Be sure to write your name and student ID number on the first blank at the bottom of the form. Please mark the version (B) in the Key ID space at the top of the
More informationData Provided: A formula sheet and table of physical constants is attached to this paper. DARK MATTER AND THE UNIVERSE
Data Provided: A formula sheet and table of physical constants is attached to this paper. DEPARTMENT OF PHYSICS AND ASTRONOMY Autumn Semester (2014-2015) DARK MATTER AND THE UNIVERSE 2 HOURS Answer question
More informationUnit 8 Lesson 2 Gravity and the Solar System
Unit 8 Lesson 2 Gravity and the Solar System Gravity What is gravity? Gravity is a force of attraction between objects that is due to their masses and the distances between them. Every object in the universe
More informationOn the Notion of the Measure of Inertia in the Special Relativity Theory
www.senet.org/apr Applied Physis Researh Vol. 4, No. ; 1 On the Notion of the Measure of Inertia in the Speial Relativity Theory Sergey A. Vasiliev 1 1 Sientifi Researh Institute of Exploration Geophysis
More informationSHAFTS: TORSION LOADING AND DEFORMATION
ECURE hird Edition SHAFS: ORSION OADING AND DEFORMAION A. J. Clark Shool of Engineering Department of Civil and Environmental Engineering 6 Chapter 3.1-3.5 by Dr. Ibrahim A. Assakkaf SPRING 2003 ENES 220
More informationA. 81 2 = 6561 times greater. B. 81 times greater. C. equally strong. D. 1/81 as great. E. (1/81) 2 = 1/6561 as great.
Q12.1 The mass of the Moon is 1/81 of the mass of the Earth. Compared to the gravitational force that the Earth exerts on the Moon, the gravitational force that the Moon exerts on the Earth is A. 81 2
More informationThursday 23 May 2013 Morning
THIS IS A NEW SPECIFICATION H Thursday 23 May 2013 Morning GCSE TWENTY FIRST CENTURY SCIENCE PHYSICS A A181/02 Modules P1 P2 P3 (Higher Tier) *A137270613* Candidates answer on the Question Paper. A calculator
More informationThe Gravitational Field
The Gravitational Field The use of multimedia in teaching physics Texts to multimedia presentation Jan Hrnčíř jan.hrncir@gfxs.cz Martin Klejch martin.klejch@gfxs.cz F. X. Šalda Grammar School, Liberec
More informationThe Birth of the Universe Newcomer Academy High School Visualization One
The Birth of the Universe Newcomer Academy High School Visualization One Chapter Topic Key Points of Discussion Notes & Vocabulary 1 Birth of The Big Bang Theory Activity 4A the How and when did the universe
More information7. In which part of the electromagnetic spectrum are molecules most easily detected? A. visible light B. radio waves C. X rays D.
1. Most interstellar matter is too cold to be observed optically. Its radiation can be detected in which part of the electromagnetic spectrum? A. gamma ray B. ultraviolet C. infrared D. X ray 2. The space
More informationThe Hidden Lives of Galaxies. Jim Lochner, USRA & NASA/GSFC
The Hidden Lives of Galaxies Jim Lochner, USRA & NASA/GSFC What is a Galaxy? Solar System Distance from Earth to Sun = 93,000,000 miles = 8 light-minutes Size of Solar System = 5.5 light-hours What is
More informationLecture 24: Spinodal Decomposition: Part 3: kinetics of the
Leture 4: Spinodal Deoposition: Part 3: kinetis of the oposition flutuation Today s topis Diffusion kinetis of spinodal deoposition in ters of the onentration (oposition) flutuation as a funtion of tie:
More informationASTR 115: Introduction to Astronomy. Stephen Kane
ASTR 115: Introduction to Astronomy Stephen Kane ASTR 115: Introduction to Astronomy Textbook: The Essential Cosmic Perspective, 7th Edition Homework will be via the Mastering Astronomy web site: www.pearsonmastering.com
More information5- Minute Refresher: Daily Observable Patterns in the Sky
5- Minute Refresher: Daily Observable Patterns in the Sky Key Ideas Daily Observable Patterns in the Sky include the occurrence of day and night, the appearance of the moon, the location of shadows and
More informationWELCOME to Aurorae In the Solar System. J.E. Klemaszewski
WELCOME to Aurorae In the Solar System Aurorae in the Solar System Sponsoring Projects Galileo Europa Mission Jupiter System Data Analysis Program ACRIMSAT Supporting Projects Ulysses Project Outer Planets
More informationIntroduction to Nuclear Physics
Introduction to Nuclear Physics 1. Atomic Structure and the Periodic Table According to the Bohr-Rutherford model of the atom, also called the solar system model, the atom consists of a central nucleus
More information) ( )( ) ( ) ( )( ) ( ) ( ) (1)
OPEN CHANNEL FLOW Open hannel flow is haraterized by a surfae in ontat with a gas phase, allowing the fluid to take on shapes and undergo behavior that is impossible in a pipe or other filled onduit. Examples
More informationStudy Guide: Solar System
Study Guide: Solar System 1. How many planets are there in the solar system? 2. What is the correct order of all the planets in the solar system? 3. Where can a comet be located in the solar system? 4.
More informationx 1 ' = x 1 vt 1 x 1 ' = 4.0 m t 1 = 1.0 s x 2 vt 2 ' = 4.0 m t 2 ' = x 2 = 3.0 s x 1 = x 2 x 1 ' + vt 1 ' + vt 2 v (t 1 t 2 ) = x 2 ' x 1 ' = x 2
Physics 2220 Module 16 Homework 01. A firecracker explodes in reference frame S at t 1 1.0 seconds. A second firecracker explodes at the same position at t 2 3.0 seconds. In reference frame S', which moves
More informationThe Solar System. Source http://starchild.gsfc.nasa.gov/docs/starchild/solar_system_level1/solar_system.html
The Solar System What is the solar system? It is our Sun and everything that travels around it. Our solar system is elliptical in shape. That means it is shaped like an egg. Earth s orbit is nearly circular.
More informationChemical Building Blocks: Chapter 3: Elements and Periodic Table
Name: Class: Date: Chemical Building Blocks: Chapter 3: Elements and Periodic Table Study Guide Multiple Choice Identify the letter of the choice that best completes the statement or answers the question.
More informationNuclear fusion in stars. Collapse of primordial density fluctuations into galaxies and stars, nucleosynthesis in stars
Nuclear fusion in stars Collapse of primordial density fluctuations into galaxies and stars, nucleosynthesis in stars The origin of structure in the Universe Until the time of formation of protogalaxies,
More informationWorld of Particles Big Bang Thomas Gajdosik. Big Bang (model)
Big Bang (model) What can be seen / measured? basically only light (and a few particles: e ±, p, p, ν x ) in different wave lengths: microwave to γ-rays in different intensities (measured in magnitudes)
More informationSTAAR Science Tutorial 30 TEK 8.8C: Electromagnetic Waves
Name: Teacher: Pd. Date: STAAR Science Tutorial 30 TEK 8.8C: Electromagnetic Waves TEK 8.8C: Explore how different wavelengths of the electromagnetic spectrum such as light and radio waves are used to
More informationSolar Nebula Theory. Basic properties of the Solar System that need to be explained:
Solar Nebula Theory Basic properties of the Solar System that need to be explained: 1. All planets orbit the Sun in the same direction as the Sun s rotation 2. All planetary orbits are confined to the
More informationSTUDY GUIDE: Earth Sun Moon
The Universe is thought to consist of trillions of galaxies. Our galaxy, the Milky Way, has billions of stars. One of those stars is our Sun. Our solar system consists of the Sun at the center, and all
More informationSize and Scale of the Universe
Size and Scale of the Universe (Teacher Guide) Overview: The Universe is very, very big. But just how big it is and how we fit into the grand scheme can be quite difficult for a person to grasp. The distances
More informationNeutron Stars. How were neutron stars discovered? The first neutron star was discovered by 24-year-old graduate student Jocelyn Bell in 1967.
Neutron Stars How were neutron stars discovered? The first neutron star was discovered by 24-year-old graduate student Jocelyn Bell in 1967. Using a radio telescope she noticed regular pulses of radio
More information2. Orbits. FER-Zagreb, Satellite communication systems 2011/12
2. Orbits Topics Orbit types Kepler and Newton laws Coverage area Influence of Earth 1 Orbit types According to inclination angle Equatorial Polar Inclinational orbit According to shape Circular orbit
More informationGeorgia Performance Standards Framework for Science Grade 6. Unit Organizer: UNIVERSE AND SOLAR SYSTEM (Approximate Time 3 Weeks)
The following instructional plan is part of a GaDOE collection of Unit Frameworks, Performance Tasks, examples of Student Work, and Teacher Commentary. Many more GaDOE approved instructional plans are
More informationA Universe of Galaxies
A Universe of Galaxies Today s Lecture: Other Galaxies (Chapter 16, pages 366-397) Types of Galaxies Habitats of Galaxies Dark Matter Other Galaxies Originally called spiral nebulae because of their shape.
More informationThe Expanding Universe
Stars, Galaxies, Guided Reading and Study This section explains how astronomers think the universe and the solar system formed. Use Target Reading Skills As you read about the evidence that supports the
More informationChapter 15 Cosmology: Will the universe end?
Cosmology: Will the universe end? 1. Who first showed that the Milky Way is not the only galaxy in the universe? a. Kepler b. Copernicus c. Newton d. Hubble e. Galileo Ans: d 2. The big bang theory and
More informationGrade 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?
Grade 6 Standard 3 Unit Test A Astronomy Multiple Choice 1. The four inner planets are rocky and small. Which description best fits the next four outer planets? A. They are also rocky and small. B. They
More informationFrom Aristotle to Newton
From Aristotle to Newton The history of the Solar System (and the universe to some extent) from ancient Greek times through to the beginnings of modern physics. The Geocentric Model Ancient Greek astronomers
More informationG 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
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 CONTENTS Foreword... 2 Forces... 3 Circular Orbits... 8 Energy... 10 Angular Momentum... 13 FOREWORD
More informationThe Layout of the Solar System
The Layout of the Solar System Planets fall into two main categories Terrestrial (i.e. Earth-like) Jovian (i.e. Jupiter-like or gaseous) [~5000 kg/m 3 ] [~1300 kg/m 3 ] What is density? Average density
More informationPart I Special Relativity
Part I Speial Relativity G. W. Gibbons D.A.M.T.P., Cambridge University, Wilberfore Road, Cambridge CB3 0WA, U.K. February 14, 2008 The views of spae and time whih I wish to lay before you have sprung
More informationTHE SOLAR SYSTEM. Worksheets UNIT 1. Raül Martínez Verdún
Worksheets UNIT 1 October-December 2009 NAME: DATE: Worksheet 1A Cut out these 9 circles and then order them from the smallest to the biggest. NAME: DATE: Worksheet 1B NAME: DATE: Worksheet 2 Read the
More informationObjectives 404 CHAPTER 9 RADIATION
Objectives Explain the difference between isotopes of the same element. Describe the force that holds nucleons together. Explain the relationship between mass and energy according to Einstein s theory
More informationThe Solar System. Unit 4 covers the following framework standards: ES 10 and PS 11. Content was adapted the following:
Unit 4 The Solar System Chapter 7 ~ The History of the Solar System o Section 1 ~ The Formation of the Solar System o Section 2 ~ Observing the Solar System Chapter 8 ~ The Parts the Solar System o Section
More informationPractice final for Basic Physics spring 2005 answers on the last page Name: Date:
Practice final for Basic Physics spring 2005 answers on the last page Name: Date: 1. A 12 ohm resistor and a 24 ohm resistor are connected in series in a circuit with a 6.0 volt battery. Assuming negligible
More informationEducator Guide to S LAR SYSTEM. 1875 El Prado, San Diego CA 92101 (619) 238-1233 www.rhfleet.org
Educator Guide to S LAR SYSTEM 1875 El Prado, San Diego CA 92101 (619) 238-1233 www.rhfleet.org Pre-Visit Activity: Orbital Paths Materials: Plastic Plate Marble Scissors To Do: 1. Put the plate on a flat
More informationUnit 5: Space Exploration
Unit 5: Space Exploration Topic 1: Our Eyes Only Define FRAME OF REFERENCE: a set of axes of any kind that is used to describe the positions or motions of things Define CONSTELLATIONS: groupings of stars
More information