Earth/Moon as seen from Mars. Bit of Administration …. HomeworksHomeworks –Bless, pp. 105-139 –BNSV, pp. 70-83 Observing LabObserving Lab –Nice Work on.

Slides:



Advertisements
Similar presentations
Ch. 2 The Copernican Revolution (Stonehenge, England)
Advertisements

Astronomy 1 – Winter 2011 Lecture 4; January
From Aristotle to Newton
© Sierra College Astronomy Department 1 Renaissance Astronomy.
Copyright © 2010 Pearson Education, Inc. Chapter 1 The Copernican Revolution.
Week 5 Day 1: Announcements. Comments on Mastering Astronomy.
The Origin of Modern Astronomy
Ancient Astronomy Objects in the Sky move in cycles –Stars, Sun, Moon, eclipses, etc. Why did most ancient people care? –Agriculture –Religion Egyptians.
Announcements Solutions to Homework 3 are posted on web site. Test next week: Tuesday, Wednesday, or Thursday (your choice); at testing center; one hour.
History of Astronomy  Motions of the sky caused by and controlled by gods. Big Horn Medicine Wheel Temple at Caracol.
Do our planets move?.
PHY134 Introductory Astronomy More Moving Parts 1.
Chapter 2 The Copernican Revolution. Units of Chapter Ancient Astronomy 2.2 The Geocentric Universe 2.3 The Heliocentric Model of the Solar System.
Galileo, Tycho, and Kepler and Kepler. Galileo’s Experiments ( ) Galileo tried something new – doing experiments! Dropping balls to measure gravity.
ASTRONOMY 161 Introduction to Solar System Astronomy Class 6.
CHAPTER 2: Gravitation and the Waltz of the Planets.
From the ancients to the moderns Nicholas Copernicus (1473–1543) Tycho Brahe (1546–1601) Johannes Kepler (1571–1630)
Web 1 Ancient Theories of Solar System 1.heliocentric theory 2. geocentric theory 3. Aristotle 4. Aristarchus 5. Ptolemy 6. Copernicus 7. Johannes Kepler.
Ancient astronomy Geocentric Heliocentric Mass and Gravity GalileoKepler Newton $ 200 $ 200$200 $ 200 $ 200 $400 $ 400$400 $ 400$400 $600 $ 600$600.
Chapter 2 The Copernican Revolution. Units of Chapter Ancient Astronomy 2.2 The Geocentric Universe 2.3 The Heliocentric Model of the Solar System.
Observing the Solar System. Observers in Ancient Greece noticed that although the stars seemed to move, they stayed in the same position relative to one.
The History of Astronomy brought to you by: Mr. Youngberg.
The Copernican Revolution. Nicolaus Copernicus 1473 – 1543.
The Solar System Copernicus (1473)
Reminders Answering cell phones during class shaves a little off your grade each time. Answering cell phones during class shaves a little off your grade.
The Dead Guys.
History of Astronomy. Our Universe Earth is one of nine planets that orbit the sun The sun is one star in 100 billion stars that make up our galaxy- The.
Goals Explain how accurate observations led to Heliocentric model Explain retrograde motion Describe contributions of Copernicus, Tycho, Galileo, and.
The Origin of Modern Astronomy
Questions What was the first idea of how the universe was structured?
Astronomy The Science that Studies The Universe Ancient Greeks To Isaac Newton.
Survey of the Universe Tom Burbine
For about 1600 years from the time of the ancient Greeks until the 1600’s people believed that the Sun, stars and planets orbited the Earth.
Chapter 2 The Copernican Revolution. Units of Chapter Ancient Astronomy 2.2 The Geocentric Universe 2.3 The Heliocentric Model of the Solar System.
The Copernican revolution. Discussion What is the simplest universe imaginable: one where making predictions about the future would be the easiest thing.
Day 3 Chapter 2 Gravitation and the Motion of the Planets.
Kepler’s Laws of Planetary Motion. Debate on Planet Motions Geocentric or Heliocentric Universe.
Universal Gravitation. Brief Astronomical History A.D Ptolemy Greek Astronomer A.D. Believed in Geo- centrism First to latitude and longitude.
Moon’s Motion: Lunar Month Synodic month: time from one new moon to the next (29.53 days) Sideral month: time it takes the Moon to complete one orbit (27.32.
Theories of Planetary Motion
Chapter 3c The Science of Astronomy. © 2005 Pearson Education Inc., publishing as Addison-Wesley 3.3 The Copernican Revolution How did Copernicus, Tycho,
Chapter 2 The Copernican Revolution. Chapter 2 Learning Objectives  Know the differences and similarities between the geocentric and heliocentric models.
AST 101 Lecture 6 Return to Heliocentrism. What needs explaining Phases of the moon Diurnal motion of the Sun Annual motions of the stars Inferior planets.
Solar System Theory Dr Ward. In The Beginning There Was... ● Celestial Sphere Model (Plato 427 to 347 BC) – Earth at centre – All objects around it placed.
Astronomy: A Beginner’s Guide to the Universe Seventh Edition © 2013 Pearson Education, Inc. The Copernican Revolution Chapter 1 Clickers.
The Origin of Modern Astronomy Chapter 4. The sun, moon, and planets sweep out a beautiful and complex dance across the heavens. Previous chapters have.
C/2002 T7 (LINEAR). Bit of Administration …. HomeworksHomeworks –Due in lecture or by 3:45 on Friday at 6515 Sterling –Error in Question 5: replace ‘3’
Early Astronomy Chapter 22, Section 1.
NATS From the Cosmos to Earth Nicholas Copernicus ( ) - wanted better way to predict planetary positions - adopted Sun-centered planetary.
Daily rise & set of sun, moon, & stars. Daily motion of stars Deductions: 1)Earth spins 2)Spherical shape 3)Moon reflects Sun’s light 4)A coordinate system.
Page 1 FAMOUS ASTRONOMERS. Page 2 ARISTOTLE Proved the Earth is round Worked with Optics Created a "prototype" of the Scientific Method His influence.
Unit 1 Physics Detailed Study 3.1 Chapter 10: Astronomy.
Explaining the Universe. Pioneer and Voyager missions Pioneer 10 and 11 Voyager 1 and 2 Portrait of Solar System.
Quiz #2 Review Giants of Science (Ch. 2), Gravity and Motion (Ch. 3) Light and Atoms (Ch. 4) Thursday 29 September 2011 Also study the Quiz 1 recap notes.
“Intro to Astronomy” §Terms You Need To Know! 1. Astronomy- The study of everything outside of the earth’s atmosphere. 2. Celestial Sphere - Imaginary.
Ch 22 Astronomy. Ancient Greeks 22.1 Early Astronomy  Astronomy is the science that studies the universe. It includes the observation and interpretation.
© 2007 Jones and Bartlett Publishers Chapter thru 2-10 From an Earth-Centered to a Sun-Centered System Courtesy of NASA/JPL-Caltech.
Charting the Heavens: Foundations of Astronomy Learning Goals Describe the Celestial Sphere and how astronomers use angular measurement to locate objects.
Foundations-Copernican Revolution Lecture 3: Newton: Gravity and the Laws of Motion.
The “Geocentric Model” Aristotle vs. Aristarchus (3 rd century B.C.): Aristotle: Sun, Moon, Planets and Stars rotate around fixed Earth. Ancient Greek.
Models of the Solar System. Earliest Astronomers (Before 400 BC) ► Early civilizations (e.g., Maya, Babylonians) observed the heavens for religious and.
1 The Dead Guys. 2 Timeline 3 Ancient Astronomy.
Lecture Outlines Astronomy Today 8th Edition Chaisson/McMillan © 2014 Pearson Education, Inc. Chapter 2.
CHAPTER 2: Gravitation and the Waltz of the Planets.
The Copernican Revolution The Birth of Modern Science.
Ptolemy ( AD ) History of Astronomy - lived in Egypt, at the time a Roman province, where he ruled as a governor - wrote The Almagest, one of.
Astronomy HISTORY OF ASTRONOMY. The scientific method had not been invented yet Most of the ideas of the time were based on Pure Thought The ideas of.
Chatfield Senior High Physics
The Copernican Revolution
CHAPTER 27.2: Gravitation and the
Presentation transcript:

Earth/Moon as seen from Mars

Bit of Administration …. HomeworksHomeworks –Bless, pp –BNSV, pp Observing LabObserving Lab –Nice Work on Lab 1 ! –Start Lab 2 on Saturday Timing Matters!Timing Matters! 10 minutes every clear night for two weeks10 minutes every clear night for two weeks

M S J S M E Not to scale! V

The Transition to A Heliocentric Cosmology Copernicus1500 ADCopernicus1500 AD –Daily Motion due to Earth Rotation –Solar Motion due to Earth Revolution –Prograde Motion of Moon and Planets due to their Orbital Motion –Retrograde Motion –Maximum Elongations of Mercury and Venus –Stars Very Far Away - No Parallax –Geometric Distances to the Planets PlanetCopernicusModern Mercury Venus Earth Mars Jupiter Saturn Distances Measured in Astronomical Units Distances Measured in Astronomical Units

M S J S M E Not to scale! V

The Transition to A Heliocentric Cosmology Summer Winter Copernicus –Non-Uniform Motion of Sun, Moon and Planets Retained Uniform Circular Motion, thus required Hipparchus’ epicyles!Retained Uniform Circular Motion, thus required Hipparchus’ epicyles! Summer Winter Hipparchus Copernicus1500 ADCopernicus1500 AD –Daily Motion due to Earth Rotation –Solar Motion due to Earth Revolution –Prograde Motion of Moon and Planets due to their Orbital Motion –Retrograde Motion –Maximum Elongations of Mercury and Venus –Stars Very Far Away - No Parallax –Geometric Distances to the Planets

The Transition to A Heliocentric Cosmology Copernicus1500 ADCopernicus1500 AD –Daily Motion due to Earth Rotation –Solar Motion due to Earth Revolution –Prograde Motion of Moon and Planets due to their Orbital Motion –Retrograde Motion –Maximum Elongations of Mercury and Venus –Geometric Distances to the Planets (example for Venus) –Star Very Far Away No observed parallaxNo observed parallax –Non-Uniform Motion of Sun, Moon and Planets In the 1500’s, the Copernican system did not predict positions better than the highly refined Ptolemaic system The Copernicans had no proof - arguments were aesthetic and philosophical

The Triumph of Heliocentric Cosmology Galileo1600 ADGalileo1600 AD –Siderius Nuncius 1610 (Star Messenger) (Star Messenger)

The Triumph of Heliocentric Cosmology Galileo1600 ADGalileo1600 AD –Siderius Nuncius 1610 (Star Messenger) (Star Messenger) –Application of the Telescope Revolutionary impact of new technologyRevolutionary impact of new technology

The Triumph of Heliocentric Cosmology Galileo1600 ADGalileo1600 AD –Siderius Nuncius 1610 (Star Messenger) (Star Messenger) –Moon Craters, mountains, valleysCraters, mountains, valleys –Earth-like, not perfect or celestial

The Triumph of Heliocentric Cosmology Galileo1600 ADGalileo1600 AD –Siderius Nuncius 1610 (Star Messenger) (Star Messenger) –Moon Craters, mountains, valleysCraters, mountains, valleys –Earth-like, not perfect or celestial –Sun SunspotsSunspots RotationRotation

The Triumph of Heliocentric Cosmology Galileo1600 ADGalileo1600 AD –Siderius Nuncius 1610 (Star Messenger) (Star Messenger) –Moon Craters, mountains, valleysCraters, mountains, valleys –Earth-like, not perfect or celestial –Sun SunspotsSunspots RotationRotation –Saturn Not sphericalNot spherical

I discovered another very strange wonder, which I should like to make known to their Highnesses..., keeping it secret, however, until the time when my work is published.... the star of Saturn is not a single star, but is a composite of three, which almost touch each other, never change or move relative to each other, and are arranged in a row along the zodiac, the middle one being three times larger than the lateral ones, and they are situated in this form: oOoI discovered another very strange wonder, which I should like to make known to their Highnesses..., keeping it secret, however, until the time when my work is published.... the star of Saturn is not a single star, but is a composite of three, which almost touch each other, never change or move relative to each other, and are arranged in a row along the zodiac, the middle one being three times larger than the lateral ones, and they are situated in this form: oOo

The Triumph of Heliocentric Cosmology Galileo1600 ADGalileo1600 AD –Siderius Nuncius 1610 (Star Messenger) (Star Messenger) –Moon Craters, mountains, valleysCraters, mountains, valleys –Earth-like, not perfect or celestial –Sun SunspotsSunspots RotationRotation –Saturn Not sphericalNot spherical –Milky Way Knowledge unknown to ancients or naked eyeKnowledge unknown to ancients or naked eye

The Triumph of Heliocentric Cosmology Galileo1600 ADGalileo1600 AD –Siderius Nuncius 1610 (Star Messenger) (Star Messenger) –Moon Craters, mountains, valleysCraters, mountains, valleys –Earth-like, not perfect or celestial –Sun SunspotsSunspots RotationRotation –Saturn Not sphericalNot spherical –Milky Way Knowledge unknown to ancients or naked eyeKnowledge unknown to ancients or naked eye –Jupiter’s Moons Microcosm of Copernican Solar SystemMicrocosm of Copernican Solar System

The Triumph of Heliocentric Cosmology Galileo1600 ADGalileo1600 AD –Siderius Nuncius 1610 (Star Messenger) (Star Messenger) –Moon Craters, mountains, valleysCraters, mountains, valleys –Earth-like, not perfect or celestial –Sun SunspotsSunspots RotationRotation –Milky Way Knowledge unknown to ancients or naked eyeKnowledge unknown to ancients or naked eye –Jupiter’s Moons Microcosm of Copernican Solar SystemMicrocosm of Copernican Solar System

The Triumph of Heliocentric Cosmology Galileo1600 ADGalileo1600 AD –Siderius Nuncius 1610 (Star Messenger) (Star Messenger) –Moon Craters, mountains, valleysCraters, mountains, valleys –Earth-like, not perfect or celestial –Sun SunspotsSunspots RotationRotation –Saturn Not sphericalNot spherical –Milky Way Knowledge unknown to ancients or naked eyeKnowledge unknown to ancients or naked eye –Jupiter’s Moons Microcosm of Copernican Solar SystemMicrocosm of Copernican Solar System –Phases of Venus Unexplainable in Ptolemaic SystemUnexplainable in Ptolemaic System

VenusPhases Ptolemy Copernicus

The Earth would be seen to have phases from a life form on A) Mercury A) Mercury B) Mars B) Mars C) The Sun C) The Sun D) No planet in the Solar System D) No planet in the Solar SystemConcepTest!

Earth/Moon as seen from Mars

The Triumph of Heliocentric Cosmology Galileo1600 ADGalileo1600 AD –Siderius Nuncius 1610 (Star Messenger) (Star Messenger) Galileo too did not abandon Uniform Circular Motion, and did not embrace his contemporary Kepler Galileo’s Problems with the Church were Self-Generated A Dialog Concerning the Two Chief Worlds

The Triumph of Heliocentric Cosmology Tycho Brahe1575 ADTycho Brahe1575 AD –Finest observer since Hipparchus Discovered Nova Stella (“new star”)Discovered Nova Stella (“new star”) –Changes in the heavens Showed Comet to be 6x further than MoonShowed Comet to be 6x further than Moon –Not atmospheric –“Shattered the crystalline spheres” Couldn’t Detect Stellar ParallaxCouldn’t Detect Stellar Parallax –Rejected Copernicus! Made Extensive Precise MeasurementsMade Extensive Precise Measurements of Planetary Positions of Planetary Positions

The Triumph of Heliocentric Cosmology Tycho Brahe1575 ADTycho Brahe1575 AD –Finest observer since Hipparchus Discovered Nova Stella (“new star”)Discovered Nova Stella (“new star”) –Changes in the heavens Showed Comet to be 6x further than MoonShowed Comet to be 6x further than Moon –Not atmospheric –“Shattered the crystalline spheres” Couldn’t Detect Stellar ParallaxCouldn’t Detect Stellar Parallax –Rejected Copernicus! Made Extensive Precise MeasurementsMade Extensive Precise Measurements of Planetary Positions of Planetary Positions Did not abandon Uniform Circular MotionDid not abandon Uniform Circular Motion

The Triumph of Heliocentric Cosmology Kepler1600 ADKepler1600 AD –Primacy of (Tycho Brahe’s) observations –Physical machine that mimics the skies precisely

Kepler’s Three Laws of Planetary Motion 1.The Orbits of the Planets are Ellipses with the Sun at One Focus

Which of the following orbits has the smallest eccentricity? A)B) C) D) All have the same eccentricity.ConcepTest!

Which of the following orbits has the smallest semi-major axis? A)B) C) D) All have the same semi-major axis.ConcepTest!

The Orbits of the Planets are Ellipses with the Sun at One Focus

Kepler’s Three Laws of Planetary Motion 2.The Line Joining The Sun and A Planet Sweeps Out Equal Areas in Equal Times 30 days

The Line Joining The Sun and A Planet Sweeps Out Equal Areas in Equal Times

Kepler’s Three Laws of Planetary Motion 3.The Square of a Planet’s Period (P in Years) Equals the Cube of the Semi-Major Axis of its Orbit (A in AU) P 2 = A 3

A 1