Fundamental Cosmology: 2.Homogeneity & Isotropy

Size: px
Start display at page:

Download "Fundamental Cosmology: 2.Homogeneity & Isotropy"

Transcription

1 Fundamental Cosmology: 2.Homogeneity & Isotropy When I trace at my pleasure the windings to and fro of the heavenly bodies, I no longer touch the earth with my feet: I stand in the presence of Zeus himself and take my fill of ambrosia, food of the gods. Ptolemy ( BC) 1

2 2.1: Ancient Cosmology Egyptian Cosmology (3000B.C.) Nun Atum Ra Shu ( ) Tefnut ( ) Geb Nut 2

3 2.1: Ancient Cosmology Ancient Greek Cosmology (700B.C.) {from Hesoid s s Theogony} Chaos Gaea ( ) Gaea ( ) Uranus ( ) Rhea Cronus ( ) The Titans Zeus The Olympians 3

4 2.1: Ancient Cosmology Aristotle and the Ptolemaic Geocentric Universe Ancient Greeks : Aristotle ( B.C.) - first Cosmological model. Stars fixed on a celestial sphere which rotated about the spherical Earth every 24 hours Planets, the Sun and the Moon, moved in the ether between the Earth and stars. Heavens composed of 55 concentric, crystalline spheres to which the celestial objects were attached and rotated at different velocities (w = constant for a given sphere) Ptolemy (90-168A.D.) (using work of Hipparchus 2 A.D.) Ptolemy's great system Almagest. Perfect motion should be in circles, so the stars and planets, being heavenly objects, moved in circles. Planets appear to periodically loop back upon themselves (retrograde motion), epicycles had to be introduced -> planets moved in circles upon circles about the fixed Earth. 4

5 2.2: The Development of Modern Cosmology The Copernican Heliocentric Universe Copernicus ( ) Revolution in Astronomy De Revolutionibus orbitum caelestium (On the revolution of the celestial spheres) The Universe does not revolve around the Earth! Circa 1514 Copernicus distributed a short, hand written book - The Little Commentary containing 7 axioms 1.There is no one centre in the Universe. 2.The Earth's centre is not the centre of the Universe. 3.The centre of the Universe is near the sun. 4.The distance from the Earth to the sun is imperceptible compared with the distance to the stars. 5.The rotation of the Earth accounts for the apparent daily rotation of the stars. 6.The apparent annual cycle of movements of the sun is caused by the Earth revolution around it. 7.The apparent retrograde motion of the planets is caused by the motion of the Earth from which one observes. Copernican Cosmological Principle : THE EARTH DOES NOT OCCUPY A SPECIAL PLACE IN THE UNIVERSE 5

6 2.2: The Development of Modern Cosmology From then until now c.168 : Ptolemy s Geocentric Universe. c.1514 : Copernicus Proposes Heliocentric Universe. c.1588 : Tcycho Brahe argues against Heliocentric model due to lack of observed Stellar Parallax. c.1609 : Kepler orbital laws : Key to Copernican Heliocentric model - Planets move in ellipses not circles. c.1610 : Galileo discovers moons orbiting Jupiter : Death blow for the Ptolemy s Geocentric model. c.1687 : Newton publishes Philosophiae naturalis principia mathematic. c.1838 : Bessel measures parallax of 61 Cygni showing it lies far beyond solar system. c.1915 : Einsteins Theory of Relativity. c.1917 : Friedmann formulates equations for expanding Universe. c.1929 : Hubble shows the nebulae are extragalactic in origin and moving away from us. c.1948 : Gamov postulates the initial singularity. c.1948 : Hoyle coins the phrase Big Bang. c.1964 : Penzias & Wilson discover the Cosmic Microwave Background (kills steady state model). 6

7 2.3: The Cosmological Principle DEFINITIONS : Fundamental Observer : Someone at rest with respect to the rest of the Universe in their locality. Universe ~ smooth fluid ~ substratum -> Fundamental observers are co-moving with it. Homogeneity : Same picture of the Universe at any time is seen by all Fundamental Observers. No preferred locations i.e. measure the same amounts of scalar quantities such as mass, density, temperature. Isotropy : The Universe looks the same in all directions to a Fundamental Observer. No preferred Directions 7

8 2.3: The Cosmological Principle Copernican Cosmological Principle The Earth does not occupy a special place in the Universe The Cosmological Principle At any single epoch, the Universe appears Homogeneous and Isotropic to all Fundamental Observers Perfect Cosmological Principle The Universe appears Homogeneous and Isotropic to all Fundamental Observers AT ALL TIMES Anthropic Cosmological Principle (WEAK) The conditions necessary for sentient life will only exist in a Universe where the laws of physics are the way they are as seen by us. (STRONG) There could be many different universes, or regions in a single Universe, where the laws of physics are different. 8

9 Examples 2.4: Homogeneity and Isotropy homogeneous inhomogeneous homogeneous (on scales>strip) but anisotropic isotropic but inhomogeneous isotropic (about centre) anisotropic 9

10 2.4: Homogeneity and Isotropy Isotropy + Copernican Principle implies Homogeneity Castor sees Isotropic Universe f x = f a = f y x Castor b a y Pollux Pollux sees Isotropic Universe f x = f b = f y 10

11 2.4: Homogeneity and Isotropy Cosmological Principle (Homogeneity) implies a cosmic time Since the Universe appears the same to all fundamental observers at any given time, All observers see the same sequence of events=> they can all synchronize their watches to some event which occurs in the history of the Universe, thereafter all the watches measure the same cosmological time 11

12 2.4: Homogeneity and Isotropy Is the real Universe really isotropic?? Matter: Small scales : Highly anisotropic Large scales > 100Mpc (Clusters / Superclusters) : fairly isotropic Radio Sources: isotropic to a few percent Radiation: CMB - Isotropic to 1 part in 10 5, 0.003%, 2mK 12

13 2.4: Homogeneity and Isotropy Is the real Universe really homogeneous?? For population of uniformly distributed objects of constant number density h, flux S, luminosity L; The number of objects per steradian out to some radius r, N = hr 3 /3 Ê S = L /r 2 fi r = L ˆ Á Ë S Ê N(S) = hp 3 / 2 ˆ Á S -3 / 2 Ë 3 1/ 2 We can measure the slope of galaxy counts!! log 10 N µ1.5log 10 S or m = A - 2.5log 10 S log 10 N = B + 0.6m (A & B are constants) unfortunately galaxies evolve 13

14 2.5: Hubbles Law The Recession of the galaxies Cosmological Doppler Effect z= redshift z = l o - l e l e 1912: Vesto Silpher (Lowell) measured blue shift from M31 By 1925 measured ~ 40 galaxies, all redshifted except local group 1929 Hubble relates redshift to distance (Cepheids) Linear Relation cz=h o r HUBBLE s LAW km/s/mpc Original Estimate Ho = 500 km/s/mpc (severely underestimated distances to galaxies Modern Estimate Ho = 70 km/s/mpc 14

15 2.5: Hubble s s Law Cosmological Principle: Derivation of Hubble s s Law How can Universe be homogeneous if all galaxies are running away from us!!?? v(r) v(r ) r = r - a (r,r,a = VECTORS) v (r ) = v(r) - v(a) v (r ) = v (r - a) Homogeneity => O & O see same events v (r - a) = v(r - a) O r v(a) a r -v(a) O General Solution v i (r,t) = v(r - a) = v(r) - v(a) 3 Âh(t) ij r j or j=1 Ê h 11 h 12 h 13 ˆ Ê Á Á h 21 h 22 h 23 Á Á Ë h 31 h 32 h 33 Ë h(t) is fn(t) Isotropy => matrix is rotationally invariant => h ij =0 for i j and h 11 = h 22 = h 33 = constant = H(t) So; v 1 = H(t)r 1 v 2 = H(t)r 2 v 13 = H(t)r 3 v = H(t)r r 1 r 2 r 3 ˆ Velocity of any co-moving particle is either zero (H=0) or moving radially away (H>0) or toward us (H<0) with a velocity proportional to the distance : i.e. HUBBLES LAW 15

16 2.5: Hubble s s Law Cosmological Principle: Hubble s s Law & the Scale Factor Rewrite the Hubble Parameter H(t) = 1 R(t) Solution Hubble Constant is really Hubble Parameter Such that R(t) is the SCALE FACTOR dr dt = 1 R(t) Where; R o = R(t o ) such that r=r o at t=t o dr(t) dt dr(t) dt r µ R(t) fi r = R(t) R o r r o All distances are scaled up by this factor R(t) with increasing time with simple isotropic expansion (note: Volume V(t)µ R(t) 3 16

17 2.6: Summary Over the last 2 millennia our place in the Universe has become less and less important Geocentric - Heliocentric - isotropic homogeneous expanding Universe The Cosmological Principle is a very simple but very powerful tool for Cosmology Unfortunately the evolution of galaxies makes it very difficult to prove homogeneity The Universe itself is isotropic on the largest scales Hubbles Law follows simply from the Cosmological Principle and its assumptions about Isotropy and Homogeneity The Universe can be thought of a set of fixed coordinates that are scaled by some scale factor as a function of time. 17

18 2.6: Summary Fundamental Cosmology 2. Homogeneity & Isotropy Fundamental Cosmology 3. Newtonian Cosmology 18

Origins of the Universe

Origins of the Universe Cosmology Origins of the Universe The study of the universe, its current nature, its origin, and evolution 1 2 The Theory Theory Expansion indicates a denser, hotter past uniform, hot gas that cools as

More information

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?

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? Cosmology 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? ANCIENT COSMOLOGIES The Ptolemaic Universe Claudius Ptolemy

More information

The great tragedy of science the slaying of a beautiful hypothesis by an ugly fact. -Thomas Huxley. Monday, October 3, 2011

The great tragedy of science the slaying of a beautiful hypothesis by an ugly fact. -Thomas Huxley. Monday, October 3, 2011 The great tragedy of science the slaying of a beautiful hypothesis by an ugly fact. -Thomas Huxley 1 Chapter 4 The Origin of Modern Astronomy Outline I. The Roots of Astronomy A. Archaeoastronomy B. The

More information

Section 3- The history and future of space exploration

Section 3- The history and future of space exploration Unit 1: Space Section 3- The history and future of space exploration Ancient Astronomer Speed Dating Remember: Speak to your partner, don t copy notes Keep points brief, don t write paragraphs Stick to

More information

Lecture 2 : Early Cosmology

Lecture 2 : Early Cosmology Lecture 2 : Early Cosmology Getting in touch with your senses Greek astronomy/cosmology The Renaissance (part 1) 8/28/13 1 Sidney Harris Discussion : What would an unaided observer deduce about the Universe?

More information

Test 1 Review Chapter 1 Our place in the universe

Test 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 information

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

Chapter 4. The Origin Of Modern Astronomy. Is okay to change your phone? From ios to Android From Android to ios Chapter 4 The Origin Of Modern Astronomy Slide 14 Slide 15 14 15 Is Change Good or Bad? Do you like Homer to look like Homer or with hair? Does it bother you when your schedule is changed? Is it okay to

More information

Earth Science, 13e Tarbuck & Lutgens

Earth 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 information

Practice Test DeAnza College Astronomy 04 Test 1 Spring Quarter 2009

Practice Test DeAnza College Astronomy 04 Test 1 Spring Quarter 2009 Practice Test DeAnza College Astronomy 04 Test 1 Spring Quarter 2009 Multiple Choice Identify the letter of the choice that best completes the statement or answers the question. Mark answer on Scantron.

More information

Ancient Cosmology: A Flat Earth. Alexandria

Ancient Cosmology: A Flat Earth. Alexandria Today Competing Cosmologies Geocentric vs. Heliocentric Ptolemy vs. copernicus Retrograde Motion Phases of Venus Galileo FIRST HOMEWORK DUE How d it work? Ancient Cosmology: A Flat Earth Here there be

More information

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

Chapter 2. The Rise of Astronomy. Copyright (c) The McGraw-Hill Companies, Inc. Permission required for reproduction or display. Chapter 2 The Rise of Astronomy Copyright (c) The McGraw-Hill Companies, Inc. Permission required for reproduction or display. Periods of Western Astronomy Western astronomy divides into 4 periods Prehistoric

More information

Wednesday, January 28

Wednesday, January 28 Ptolemy to Copernicus Wednesday, January 28 Astronomy of the ancients Many ancient cultures took note of celestial objects and celestial lphenomena. They noted tdcertain ti patterns in the heavens and

More information

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

Lecture #5: Plan. The Beginnings of Modern Astronomy Kepler s Laws Galileo Lecture #5: Plan The Beginnings of Modern Astronomy Kepler s Laws Galileo Geocentric ( Ptolemaic ) Model Retrograde Motion: Apparent backward (= East-to-West) motion of a planet with respect to stars Ptolemy

More information

II. The Universe Around Us. ASTR378 Cosmology : II. The Universe Around Us 23

II. The Universe Around Us. ASTR378 Cosmology : II. The Universe Around Us 23 II. The Universe Around Us ASTR378 Cosmology : II. The Universe Around Us 23 Some Units Used in Astronomy 1 parsec distance at which parallax angle is 1 ; 1 pc = 3.086 10 16 m ( 3.26 light years; 1 kpc

More information

Chapter 1 Introduction. Particle Astrophysics & Cosmology SS

Chapter 1 Introduction. Particle Astrophysics & Cosmology SS Chapter 1 Introduction Particle Astrophysics & Cosmology SS 2008 1 Ptolemäus (85 165 b.c.) Kopernicus (1473 1543) Kepler (1571 1630) Newton (1643 1727) Kant (1724 1630) Herschel (1738 1822) Einstein (1917)

More information

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

History of Astronomy. PHYS 1411 Introduction to Astronomy. Tycho Brahe and Exploding Stars. Tycho Brahe ( ) Chapter 4. Renaissance Period PHYS 1411 Introduction to Astronomy History of Astronomy Chapter 4 Renaissance Period Copernicus new (and correct) explanation for retrograde motion of the planets Copernicus new (and correct) explanation

More information

How big is the Universe and where are we in it?

How big is the Universe and where are we in it? Announcements Results of clicker questions from Monday are on ICON. First homework is graded on ICON. Next homework due one minute before midnight on Tuesday, September 6. Labs start this week. All lab

More information

A brief history of cosmological ideas

A brief history of cosmological ideas A brief history of cosmological ideas Cosmology: Science concerned with the origin and evolution of the universe, using the laws of physics. Cosmological principle: Our place in the universe is not special

More information

History of Astronomy. Historical People and Theories

History 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 information

Copernican Revolution. Motions of the sky. Motions of the sky. Copernican Revolution: questions on reading assignment

Copernican Revolution. Motions of the sky. Motions of the sky. Copernican Revolution: questions on reading assignment Copernican Revolution Motion of the sun & planets Ptolemy s Almagest Copernicus de Revolutionibus Orbium Caelestium, (Concerning Revolutions of the Heavenly Spheres), 1543 Galileo refutes Ptolemy with

More information

Hawking & the Universe

Hawking & the Universe Hawking & the Universe This is a supplement to the lecture given on Jan 26, 2015, by Dr. Mounib El Eid, Physics department, AUB. It may motivate the reader to explore some of the presented issues. There

More information

Lecture 3: History of Astronomy. Astronomy 111 Monday September 4, 2017

Lecture 3: History of Astronomy. Astronomy 111 Monday September 4, 2017 Lecture 3: History of Astronomy Astronomy 111 Monday September 4, 2017 Reminders Labs start this week Homework #2 assigned today Astronomy of the ancients Many ancient cultures took note of celestial objects

More information

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

Earth 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 information

How High Is the Sky? Bob Rutledge

How High Is the Sky? Bob Rutledge How High Is the Sky? Bob Rutledge Homer s Physics: Feb 16 2007 The Sun 8 Light Minutes Away 2 The Pleiades 300 Light Years Away (and inside our galaxy) [The nearest star, Proxima Cen, is only 4.2 light

More information

Ch. 22 Origin of Modern Astronomy Pretest

Ch. 22 Origin of Modern Astronomy Pretest Ch. 22 Origin of Modern Astronomy Pretest Ch. 22 Origin of Modern Astronomy Pretest 1. True or False: Early Greek astronomers (600 B.C. A.D. 150) used telescopes to observe the stars. Ch. 22 Origin of

More information

The Continuing Copernican Revolution...

The Continuing Copernican Revolution... The Continuing Copernican Revolution... from Heliocentricity to the Cosmological Principle Astro 203 Vanderbilt University 2006/10/19 Prof. Rob Knop Slides online at: http://brahms.phy.vanderbilt.edu/~rknop/classes/talkslides#awayfmctr

More information

Ptolemy (125 A.D.) Ptolemy s Model. Ptolemy s Equant. Ptolemy s Model. Copernicus Model. Copernicus ( )

Ptolemy (125 A.D.) Ptolemy s Model. Ptolemy s Equant. Ptolemy s Model. Copernicus Model. Copernicus ( ) Ptolemy (125 A.D.) Designed a complete geometrical model of the universe that accurately predicted planetary motions with errors within 5 0 Most of the geometric devices and basic foundations of his model

More information

Evidence that the Earth does not move: Greek Astronomy. Aristotelian Cosmology: Motions of the Planets. Ptolemy s Geocentric Model 2-1

Evidence that the Earth does not move: Greek Astronomy. Aristotelian Cosmology: Motions of the Planets. Ptolemy s Geocentric Model 2-1 Greek Astronomy Aristotelian Cosmology: Evidence that the Earth does not move: 1. Stars do not exhibit parallax: 2-1 At the center of the universe is the Earth: Changeable and imperfect. Above the Earth

More information

History of Astronomy - Part I. Ancient Astronomy. Ancient Greece. Astronomy is a science that has truly taken shape only in the last couple centuries

History of Astronomy - Part I. Ancient Astronomy. Ancient Greece. Astronomy is a science that has truly taken shape only in the last couple centuries History of Astronomy - Part I Astronomy is a science that has truly taken shape only in the last couple centuries Many advances have been made in your lifetime However, astronomical concepts and ideas

More information

2 1 History of Astronomy

2 1 History of Astronomy History of Astronomy 2 1 Introduction 2 2 Together with theology, astronomy one of the oldest professions in the world. History 1 Introduction 2 2 Together with theology, astronomy one of the oldest professions

More information

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

Introduction to Astronomy & Astrophysics (PHY F215) Kaushar Vaidya Ph.D. (Astronomy) Introduction to Astronomy & Astrophysics (PHY F215) Kaushar Vaidya Ph.D. (Astronomy) vastness and scales (sizes, time, temperature-pressure) (philosophical, exo-planets, detection, alien) nothing like

More information

cosmogony geocentric heliocentric How the Greeks modeled the heavens

cosmogony geocentric heliocentric How the Greeks modeled the heavens Cosmogony A cosmogony is theory about ones place in the universe. A geocentric cosmogony is a theory that proposes Earth to be at the center of the universe. A heliocentric cosmogony is a theory that proposes

More information

Was Ptolemy Pstupid?

Was Ptolemy Pstupid? Was Ptolemy Pstupid? Why such a silly title for today s lecture? Sometimes we tend to think that ancient astronomical ideas were stupid because today we know that they were wrong. But, while their models

More information

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

Gravitation Part I. Ptolemy, Copernicus, Galileo, and Kepler Gravitation Part I. Ptolemy, Copernicus, Galileo, and Kepler Celestial motions The stars: Uniform daily motion about the celestial poles (rising and setting). The Sun: Daily motion around the celestial

More information

The History of Astronomy

The History of Astronomy The History of Astronomy The History of Astronomy Earliest astronomical record: a lunar calendar etched on bone from 6500 B.C. Uganda. Also we find early groups noted the Sun, Moon, Mercury, Venus, Earth,

More information

Today FIRST HOMEWORK DUE. Ancient Astronomy. Competing Cosmologies. Geocentric vs. Heliocentric. Ptolemy vs. copernicus.

Today FIRST HOMEWORK DUE. Ancient Astronomy. Competing Cosmologies. Geocentric vs. Heliocentric. Ptolemy vs. copernicus. Today FIRST HOMEWORK DUE Ancient Astronomy Competing Cosmologies Geocentric vs. Heliocentric Ptolemy vs. copernicus Retrograde Motion Phases of Venus Galileo 1 3.1 The Ancient Roots of Science Our goals

More information

The Birth of Astronomy. Lecture 3 1/24/2018

The Birth of Astronomy. Lecture 3 1/24/2018 The Birth of Astronomy Lecture 3 1/24/2018 Fundamental Questions of Astronomy (life?) What is the shape of the Earth? How big is the planet we live on? Why do the stars move across the sky? Where is Earth

More information

Competing Models. The Ptolemaic system (Geocentric) The Copernican system (Heliocentric)

Competing Models. The Ptolemaic system (Geocentric) The Copernican system (Heliocentric) Competing Models The Ptolemaic system (Geocentric) The Copernican system (Heliocentric) How did Galileo solidify the Copernican revolution? Galileo overcame major objections to the Copernican view. Three

More information

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

Models of the Solar System. The Development of Understanding from Ancient Greece to Isaac Newton Models of the Solar System The Development of Understanding from Ancient Greece to Isaac Newton Aristotle (384 BC 322 BC) Third in line of Greek thinkers: Socrates was the teacher of Plato, Plato was the

More information

Astronomy- The Original Science

Astronomy- The Original Science Astronomy- The Original Science Imagine that it is 5,000 years ago. Clocks and modern calendars have not been invented. How would you tell time or know what day it is? One way to tell the time is to study

More information

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

Early Theories. Early astronomers believed that the sun, planets and stars orbited Earth (geocentric model) Developed by Aristotle Planetary Motion Early Theories Early astronomers believed that the sun, planets and stars orbited Earth (geocentric model) Developed by Aristotle Stars appear to move around Earth Observations showed

More information

Astro 13 Galaxies & Cosmology LECTURE 4 Tues 18 Jan 2011 P. Madau. I Cosmological Principles 25m II Why is the Sky Dark? (Olber s

Astro 13 Galaxies & Cosmology LECTURE 4 Tues 18 Jan 2011 P. Madau. I Cosmological Principles 25m II Why is the Sky Dark? (Olber s Astro 13 Galaxies & Cosmology LECTURE 4 Tues 18 Jan 2011 P. Madau 20m I Cosmological Principles 25m II Why is the Sky Dark? (Olber s Paradox) 10m III Break 15m IV Expanding Univ. - Hubble Constant 20m

More information

Announcements. Topics To Be Covered in this Lecture

Announcements. Topics To Be Covered in this Lecture Announcements! Tonight s observing session is cancelled (due to clouds)! the next one will be one week from now, weather permitting! The 2 nd LearningCurve activity was due earlier today! Assignment 2

More information

Directions: Read each slide

Directions: Read each slide Directions: Read each slide and decide what information is needed. Some slides may have red or yellow or orange underlined. This information is a clue for you to read more carefully or copy the information

More information

COSMIC DISTANCE LADDER

COSMIC DISTANCE LADDER ASTC02 - PROF. HANNO REIN COSMIC DISTANCE LADDER ADAPTED FROM SLIDES BY TERENCE TAO (UCLA) HOW FAR AWAY IS COSMIC DISTANCE LADDER Work out the answer in steps (rungs) Starting with short distances ( human

More information

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

Early Models of the Universe. How we explained those big shiny lights in the sky Early Models of the Universe How we explained those big shiny lights in the sky The Greek philosopher Aristotle (384 322 BCE) believed that the Earth was the center of our universe, and everything rotated

More information

Chapter 02 The Rise of Astronomy

Chapter 02 The Rise of Astronomy Chapter 02 The Rise of Astronomy Multiple Choice Questions 1. The moon appears larger when it rises than when it is high in the sky because A. You are closer to it when it rises (angular-size relation).

More information

b. Remember, Sun is a second or third generation star the nebular cloud of dust and gases was created by a supernova of a preexisting

b. Remember, Sun is a second or third generation star the nebular cloud of dust and gases was created by a supernova of a preexisting 1. Evolution of the Solar System Nebular hypothesis, p 10 a. Cloud of atoms, mostly hydrogen and helium b. Gravitational collapse contracted it into rotating disc c. Heat of conversion of gravitational

More information

The Copernican System: A Detailed Synopsis

The Copernican System: A Detailed Synopsis Oglethorpe Journal of Undergraduate Research Volume 5 Issue 1 Article 2 April 2015 The Copernican System: A Detailed Synopsis John Cramer Dr. jcramer@oglethorpe.edu Follow this and additional works at:

More information

V. Astronomy Section

V. Astronomy Section EAS 100 Planet Earth Lecture Topics Brief Outlines V. Astronomy Section 1. Introduction, Astronomical Distances, Solar System Learning objectives: Develop an understanding of Earth s position in the solar

More information

Motions of the Planets ASTR 2110 Sarazin

Motions of the Planets ASTR 2110 Sarazin Motions of the Planets ASTR 2110 Sarazin Motion of Planets Retrograde Motion Inferior Planets: Mercury, Venus Always near Sun on Sky Retrograde motion when very close to Sun on sky (Every other time) Superior

More information

This Week... Week 3: Chapter 3 The Science of Astronomy. 3.1 The Ancient Roots of Science. How do humans employ scientific thinking?

This Week... Week 3: Chapter 3 The Science of Astronomy. 3.1 The Ancient Roots of Science. How do humans employ scientific thinking? Week 3: Chapter 3 The Science of Astronomy This Week... The Copernican Revolution The Birth of Modern Science Chapter 2 Walkthrough Discovering the solar system Creating a clockwork Universe 3.1 The Ancient

More information

o Terms to know o Big Bang Theory o Doppler Effect o Redshift o Universe

o Terms to know o Big Bang Theory o Doppler Effect o Redshift o Universe Standard 1: Students will understand the scientific evidence that supports theories that explain how the universe and the solar system developed. They will compare Earth to other objects in the solar system.

More information

Copernican Revolution. ~1500 to ~1700

Copernican Revolution. ~1500 to ~1700 ~1500 to ~1700 Copernicus (~1500) Brahe (~1570) Kepler (~1600) Galileo (~1600) Newton (~1670) The Issue: Geocentric or Heliocentric Which model explains observations the best? Copernicus (~1500) Resurrected

More information

Chapter 3 The Science of Astronomy

Chapter 3 The Science of Astronomy Chapter 3 The Science of Astronomy 3.1 The Ancient Roots of Science Our goals for learning: In what ways do all humans employ scientific thinking? How did astronomical observations benefit ancient societies?

More information

Lecture #4: Plan. Early Ideas of the Heavens (cont d): Geocentric Universe Heliocentric Universe

Lecture #4: Plan. Early Ideas of the Heavens (cont d): Geocentric Universe Heliocentric Universe Lecture #4: Plan Early Ideas of the Heavens (cont d): Shape & size of the Earth Size & distance of Moon & Sun Geocentric Universe Heliocentric Universe Shape of the Earth Aristotle (Greece, 384 322 B.C.)

More information

Review of previous concepts!! Earth s orbit: Year, seasons, observed constellations, Polaris (North star), day/night lengths, equinoxes

Review of previous concepts!! Earth s orbit: Year, seasons, observed constellations, Polaris (North star), day/night lengths, equinoxes Review of previous concepts!! Earth s orbit: Year, seasons, observed constellations, Polaris (North star), day/night lengths, equinoxes Celestial poles, celestial equator, ecliptic, ecliptic plane (Fig

More information

Physics 107 Ideas of Modern Physics. Goals of the course. How is this done? What will we cover? Where s the math?

Physics 107 Ideas of Modern Physics. Goals of the course. How is this done? What will we cover? Where s the math? Physics 107 Ideas of Modern Physics (uw.physics.wisc.edu/~rzchowski/phy107) Modern Physics: essentially post-1900 Why 1900? Two radical developments: Relativity & Quantum Mechanics Both changed the way

More information

PHYS 160 Astronomy Test #1 Fall 2017 Version B

PHYS 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 information

Ancient Astronomy. Lectures 5-6. Course website:

Ancient Astronomy. Lectures 5-6. Course website: Ancient Astronomy Lectures 5-6 Course website: www.scs.fsu.edu/~dduke/lectures Lectures 5-6 Almagest Books 9 13 geocentric vs. heliocentric point of view the wandering stars, or planets the two anomalies

More information

ASTRO 6570 Lecture 1

ASTRO 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 information

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

BROCK UNIVERSITY. 1. The observation that the intervals of time between two successive quarter phases of the Moon are very nearly equal implies that BROCK UNIVERSITY Page 1 of 10 Test 1: November 2014 Number of pages: 10 Course: ASTR 1P01, Section 2 Number of students: 961 Examination date: 7 November 2014 Time limit: 50 min Time of Examination: 17:00

More information

Read each slide then use the red or some underlined words to complete the organizer.

Read each slide then use the red or some underlined words to complete the organizer. Read each slide then use the red or some underlined words to complete the organizer. 1B Did it start as a bang! 1B The Expanding Universe A. The Big Bang Theory: Idea that all matter began in an infinitely

More information

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

Claudius Ptolemaeus Second Century AD. Jan 5 7:37 AM Claudius Ptolemaeus Second Century AD Jan 5 7:37 AM Copernicus: The Foundation Nicholas Copernicus (Polish, 1473 1543): Proposed the first modern heliocentric model, motivated by inaccuracies of the Ptolemaic

More information

Lesson 2 - The Copernican Revolution

Lesson 2 - The Copernican Revolution Lesson 2 - The Copernican Revolution READING ASSIGNMENT Chapter 2.1: Ancient Astronomy Chapter 2.2: The Geocentric Universe Chapter 2.3: The Heliocentric Model of the Solar System Discovery 2-1: The Foundations

More information

Origins of Modern Astronomy

Origins of Modern Astronomy PHYS 1411 Introduction to Astronomy Origins of Modern Astronomy Chapter 4 Topics in Chapter 4 Chapter 4 talks about the history of Astronomy and the development of the model of the solar system. Brief

More information

EARTH SCIENCE UNIT 9 -NOTES ASTRONOMY

EARTH SCIENCE UNIT 9 -NOTES ASTRONOMY EARTH SCIENCE UNIT 9 -NOTES ASTRONOMY UNIT 9- ASTRONOMY 2 THE SOLAR SYSTEM I. The Solar System:. a. Celestial Body:. i. Examples:. b. MAIN COMPONENTS/MEMBERS OF THE SOLAR SYSTEM: i. 1. Planets are objects

More information

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

Astronomy. 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 information

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?

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? Physics 107 Ideas of Modern Physics (uw.physics.wisc.edu/~rzchowski/phy107) Main emphasis is Modern Physics: essentially post-1900 Why 1900? Two radical developments: Relativity & Quantum Mechanics Both

More information

Chapter 2 The Copernican Revolution

Chapter 2 The Copernican Revolution Chapter 2 The Copernican Revolution Units of Chapter 2 2.1 Ancient Astronomy 2.2 The Geocentric Universe 2.3 The Heliocentric Model of the Solar System The Foundations of the Copernican Revolution 2.4

More information

Monday, October 3, 2011

Monday, October 3, 2011 We do not ask for what useful purpose the birds do sing, for song is their pleasure since they were created for singing. Similarly, we ought not ask why the human mind troubles to fathom the secrets of

More information

PHYS 155 Introductory Astronomy

PHYS 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 information

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

ASTRONOMY LECTURE NOTES MIDTERM REVIEW. ASTRONOMY LECTURE NOTES Chapter 1 Charting the Heavens ASTRONOMY LECTURE NOTES MIDTERM REVIEW ASTRONOMY LECTURE NOTES Chapter 1 Charting the Heavens How Do We Locate Objects in the Sky? Local-Sky Coordinates versus Celestial-Sphere Coordinates When the sky

More information

Space Notes Covers Objectives 1 & 2

Space Notes Covers Objectives 1 & 2 Space Notes Covers Objectives 1 & 2 Space Introduction Space Introduction Video Celestial Bodies Refers to a natural object out in space 1) Stars 2) Comets 3) Moons 4) Planets 5) Asteroids Constellations

More information

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

The History of Astronomy. Please pick up your assigned transmitter. The History of Astronomy Please pick up your assigned transmitter. When did mankind first become interested in the science of astronomy? 1. With the advent of modern computer technology (mid-20 th century)

More information

Benefit of astronomy to ancient cultures

Benefit of astronomy to ancient cultures Benefit of astronomy to ancient cultures Usefulness as a tool to predict the weather (seasons) Usefulness as a tool to tell time (sundials) Central Africa (6500 B.C.) Alignments Many ancient cultures built

More information

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

3) 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 information

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

1) 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 information

ASTR 1010 Spring 2016 Study Notes Dr. Magnani

ASTR 1010 Spring 2016 Study Notes Dr. Magnani The Copernican Revolution ASTR 1010 Spring 2016 Study Notes Dr. Magnani The Copernican Revolution is basically how the West intellectually transitioned from the Ptolemaic geocentric model of the Universe

More information

He was a Polish astronomer in the XV and XVI century. He was born in 1473 in Torun and he died in 1543 when he was 70 years old.

He was a Polish astronomer in the XV and XVI century. He was born in 1473 in Torun and he died in 1543 when he was 70 years old. Ptolomeo He lived in Rome around 100 AC, where he developed his model of the solar system which had a very important impact on the science because it could explain the motions of heavenly bodies and it

More information

A100 Exploring the Universe: The Rise of Science. Martin D. Weinberg UMass Astronomy

A100 Exploring the Universe: The Rise of Science. Martin D. Weinberg UMass Astronomy A100 Exploring the Universe: The Rise of Science Martin D. Weinberg UMass Astronomy weinberg@astro.umass.edu September 11, 2012 Read: Chap 3 09/11/12 slide 1 Problem Set #1 due this afternoon at 5pm! Read:

More information

Copernican Revolution 15 Jan. Copernican Revolution: questions on reading assignment

Copernican Revolution 15 Jan. Copernican Revolution: questions on reading assignment Copernican Revolution 15 Jan Final exam is Wed, May 6 th, not 5 th. Questions on reading Motion of the sun & planets Ptolemy s Almagest Copernicus de Revolutionibus Orbium Caelestium, (Concerning Revolutions

More information

Tuesday: Special epochs of the universe (recombination, nucleosynthesis, inflation) Wednesday: Structure formation

Tuesday: Special epochs of the universe (recombination, nucleosynthesis, inflation) Wednesday: Structure formation Introduction to Cosmology Professor Barbara Ryden Department of Astronomy The Ohio State University ICTP Summer School on Cosmology 2016 June 6 Today: Observational evidence for the standard model of cosmology

More information

Cultural Evolution, II

Cultural Evolution, II Cultural Evolution, II Evolution of Concept of Universe Interest part of f c Requires the following: 1. Understand the size and nature of Universe 2. Understand place in Universe (not the center) 3. Optimistic

More information

ASTR : Stars & Galaxies (Spring 2019)... Study Guide for Midterm 1

ASTR : Stars & Galaxies (Spring 2019)... Study Guide for Midterm 1 ASTR-1200-01: Stars & Galaxies (Spring 2019)........................ Study Guide for Midterm 1 The first midterm exam for ASTR-1200 takes place in class on Wednesday, February 13, 2019. The exam covers

More information

Model Universe Including Pressure

Model Universe Including Pressure Model Universe Including Pressure The conservation of mass within the expanding shell was described by R 3 ( t ) ρ ( t ) = ρ 0 We now assume an Universe filled with a fluid (dust) of uniform density ρ,

More information

Planets & The Origin of Science

Planets & The Origin of Science Planets & The Origin of Science Reading: Chapter 2 Required: Guided Discovery (p.44-47) Required: Astro. Toolbox 2-1 Optional: Astro. Toolbox 2-2, 2-3 Next Homework Due. Sept. 26 Office Hours: Monday,

More information

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

Astronomy Notes Chapter 02.notebook April 11, 2014 Pythagoras Aristotle geocentric retrograde motion epicycles deferents Aristarchus, heliocentric Around 2500 years ago, Pythagoras began to use math to describe the world around him. Around 200 years later, Aristotle stated that the Universe is understandable and is governed by regular laws. Most

More information

Observational Cosmology

Observational Cosmology Observational Cosmology Prof Simon Driver Simon.Driver@icrar.org 1. An Expanding Universe 2. The Hot Big Bang 3. The Microwave Background 4. Building a model geometry 5. Building a model dynamics 6. The

More information

2.1 Basics of the Relativistic Cosmology: Global Geometry and the Dynamics of the Universe Part I

2.1 Basics of the Relativistic Cosmology: Global Geometry and the Dynamics of the Universe Part I 1 2.1 Basics of the Relativistic Cosmology: Global Geometry and the Dynamics of the Universe Part I 2 Special Relativity (1905) A fundamental change in viewing the physical space and time, now unified

More information

The Early Universe: A Journey into the Past

The Early Universe: A Journey into the Past The Early Universe A Journey into the Past Texas A&M University March 16, 2006 Outline Galileo and falling bodies Galileo Galilei: all bodies fall at the same speed force needed to accelerate a body is

More information

The Early Universe: A Journey into the Past

The Early Universe: A Journey into the Past Gravity: Einstein s General Theory of Relativity The Early Universe A Journey into the Past Texas A&M University March 16, 2006 Outline Gravity: Einstein s General Theory of Relativity Galileo and falling

More information

AS1001: Galaxies and Cosmology

AS1001: Galaxies and Cosmology AS1001: Galaxies and Cosmology Keith Horne kdh1@st-and.ac.uk http://www-star.st-and.ac.uk/~kdh1/eg/eg.html Text: Kutner Astronomy:A Physical Perspective Chapters 17-21 Cosmology Today Blah Title Current

More information

Astronomy 1143 Final Exam Review Answers

Astronomy 1143 Final Exam Review Answers Astronomy 1143 Final Exam Review Answers Prof. Pradhan April 24, 2015 What is Science? 1. Explain the difference between astronomy and astrology. 2. What number is the metric system based around? What

More information

ASTR 200 : Lecture 27. Expansion and large scale structure

ASTR 200 : Lecture 27. Expansion and large scale structure ASTR 200 : Lecture 27 Expansion and large scale structure 1 A preference for recession In 1912, american astronomer Vesto Slipher began painstakingly acquiring spectra of `spiral nebulae' and was the first

More information

Alan Mortimer PhD. Ideas of Modern Physics

Alan Mortimer PhD. Ideas of Modern Physics Alan Mortimer PhD Ideas of Modern Physics Introductory Remarks Lecture Series Outline 1. Foundations of Modern Physics 2. A Window on the Modern World Electromagnetism & Relativity 3. Quantum Physics and

More information

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

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 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 geocentric model for understanding the universe to a

More information

1 Astronomy: The Original Science

1 Astronomy: The Original Science CHAPTER 18 1 Astronomy: The Original Science SECTION Studying Space BEFORE YOU READ After you read this section, you should be able to answer these questions: How do astronomers define a day, a month,

More information

Paradigm Shifts in Cosmology

Paradigm Shifts in Cosmology FEATURE Principal Investigator Naoshi Sugiyama Research Area Astrophysics Paradigm Shifts in Cosmology The paradigm shift as put forward by Thomas Kuhn means revolutionary changes in the normative concepts

More information

Astronomy Today. Eighth edition. Eric Chaisson Steve McMillan

Astronomy Today. Eighth edition. Eric Chaisson Steve McMillan Global edition Astronomy Today Eighth edition Eric Chaisson Steve McMillan The Distance Scale ~1 Gpc Velocity L Distance Hubble s law Supernovae ~200 Mpc Time Tully-Fisher ~25 Mpc ~10,000 pc Time Variable

More information