Copernicus’s Model  Many scientists believed our Earth was the center of the solar system, this theory is called geocentric  Copernicus first proposed.

Slides:



Advertisements
Similar presentations
Chapter 27.2 Models of the solar system
Advertisements

Chapter 9 & 10 Gravity Pythagoras (550 BC) n Claimed that natural phenomena could be described by mathematics.
Geocentric Model Earth is center of our Solar System
Models of the solar system (Ch.29.1). 1 st model of the solar system Aristotle (300’s BC) said solar system was geocentric.
Models of the Solar System. The observations that you have been making of the Sun, Moon and stars were the same observations made by early scientists.
Models of the Solar System
MODELS OF THE SOLAR SYSTEM. ARISTOTLE Greek philosopher ( BC) He promoted an earth centered called geocentric, model of solar system He said the.
Planets of the Solar System Section 2 Section 2: Models of the Solar System Preview Key Ideas Early Models Kepler’s Laws Newton’s Explanation of Kepler’s.
Solar System Organization Chapters 3 & 4. Forming the Solar System Accretion- the process of building something up gradually by the gathering together.
CHAPTER 2: Gravitation and the Waltz of the Planets.
Bell Ringer 9/8 OPINION QUESTION – How do you believe the solar system was formed?
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 Rise of Astronomy. Ancient Roots: Early Homo-Sapiens.
The History of Astronomy brought to you by: Mr. Youngberg.
Gravitation and the Waltz of the Planets Kepler, Galileo and Newton.
Solar System Overview. Early Ideas  It was assumed that the Sun, planets, and stars orbited a stationary universe  This is known as a “geocentric” model,
Kepler’s Laws of Planetary Motion. Debate on Planet Motions Geocentric or Heliocentric Universe.
Chapter Planetary Motion & Gravitation Nicholas Copernicus (Polish) Pulished Earth-centered model in 1543 Tycho Brahe (Danish) Vowed to be an astronomer.
Chapter 3: Motion of Astronomical Bodies. A bit more on the Celestial Sphere and motions This works OK if we only consider the stars. What happens when.
Early Astronomy 4/21/ b pgs IN: Draw a diagram showing rotation and revolution. Open a book to pg. 486.
FAMOUS ASTRONOMERS  The name "planet" comes from the Greek term π λανήτης (plan ē t ē s), meaning "wanderer".  Came up with geocentric (earth center)
investigated the nature of light, discovering that sunlight is made of light of different colors; the spectrum is, in order from long to short wavelength:
Kepler’s Laws of Planetary Motion. Objectives Describe Kepler’s Laws of Planetary Motion Relate Kepler’s Laws to Newton’s Laws Prove Kepler’s 3 rd law.
Astronomy  Astronomy is the study of the planets and other objects in space.  The “Golden Age of Astronomy” occurred during 600 – 150 B.C. when the ancient.
2.1 History of Astronomy. What is Astronomy?  The branch of science that deals with celestial objects, space, and the physical universe as a whole.
EARTH & SPACE SCIENCE Chapter 27 Planets of the Solar System 27.2 Models of the Solar System.
Ch. 29 Sec. 1 Overview of Solar System. Early Ideas  Humans have watched the sky for thousands of years  Planets change position relative to the stars.
Historical Models of our Solar System Miss Scillieri 6 th Grade.
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.
Chapter 1: The Copernican Revolution. The Motions of the Planets The Birth of Modern Astronomy The Laws of Planetary Motion Newton’s Laws Summary of Chapter.
17-1 Physics I Class 17 Newton’s Theory of Gravitation.
 Everything in outer space  Stars  Planets  Comets  Asteroids & Meteors  Solar System vs Galaxy vs Universe  What’s the difference?  SIZE?!
Developing the Science of Astronomy (Chapter 4). Student Learning Objectives Compare ancient and modern theories of the solar system Apply Kepler’s Laws.
Chapter 29 The Solar System Ch Models of the Solar System.
Kepler’s Laws What they tell us, and where they come from.
Kepler’s Laws of planetary motion Newton’s law of universal gravitation Free fall acceleration on surface of a planet Satellite motion Lecture 13: Universal.
MODELS OF THE SOLAR SYSTEM Chap. 29, Sect. 1 OBJECTIVES: SWBAT… 1. Compare the models of the universe developed by Ptolemy and Copernicus. 2. Summarize.
Models of the Solar System
PHYS 2010 Nathalie Hoffmann University of Utah
NEXT Gravity and the Solar System Properties of Planets Gas Giants Terrestrial Planets Word!
Chapter 1 The Copernican Revolution. The planets’ motions Wanderers among the stars Retrograde motion.
A New View of the Universe Topic. Essential Question How did the view of the universe change during the Scientific Revolution? Essential Question.
THE SOLAR SYSTEM Chapter 24A. Unit Objectives Compare models of the solar system To list and describe the objects in our solar system.
Section Orbital Motion of Satellites and Kepler’s Laws
KEPLER’S LAWS OF PLANETARY MOTION Objective: I will summarize Kepler’s three laws of planetary motion. 11/10/15.
Modern Day Astronomers (sort of) The New Guys. The Astronomers Copernicus Galileo Tycho Brahe Johannes Kepler Sir Isaac Newton.
Historical Models of our Solar System and Kepler’s Laws of Planetary Motion.
Models of the Solar System Ch 27.2 Page 691 Early models  Around 2,000 years ago, Aristotle suggested the earth- centered or geocentric model of the.
EARTH & SPACE SCIENCE Chapter 27 Planets of the Solar System 27.2 Models of the Solar System.
Simple Harmonic Motion Universal Gravitation 1. Simple Harmonic Motion Vibration about an equilibrium position with a restoring force that is proportional.
History of Astronomy The guys with their eyes on the skies.
 Compare the models of the universe developed by Ptolemy and Copernicus.  Summarize Kepler’s three laws of planetary motion.  Describe how Newton explained.
Aristotle suggested an Earth-centered, or geocentric, model of the solar system. In this model, the sun, the stars, an the planets revolved around Earth.
Formation of the Solar System
Kepler’s 3 Laws of planetary motion
Kepler’s Laws of Motion
MODELS OF THE SOLAR SYSTEM
Section 2: Models of the Solar System
Kepler and Planetary Motion
Models of the Solar System
Section 2: Models of the Solar System
The Laws of Planetary Motion
LESSON 12: KEPLER’S LAWS OF PLANETARY MOTION
Gravitational Fields, Circular Orbits and Kepler
Aim: How do we compute Eccentricity?
EARTH SCIENCE MRS. DAVIS
Gravitational Fields, Circular Orbits and Kepler’s Laws
THE EARTH, THE MOON & THE SUN
Bell Work: What is the center of the Universe?
Presentation transcript:

Copernicus’s Model  Many scientists believed our Earth was the center of the solar system, this theory is called geocentric  Copernicus first proposed our solar system was heliocentric – suncentered

Geocentric vs. Heliocentric  Geocentric  Heliocentric

Kepler’s Laws 1 st law- Law of Ellipses 2 nd law- Law of Equal Areas 3 rd law- Law of Periods

Law of Ellipses- The orbit of every planet is an ellipse (oval shape) with the Sun at one of the two foci.orbit planetellipsefoci

Law of Equal Areas- A line joining a planet and the Sun sweeps out equal areas during equal intervals of time.line

Law of Periods- The square of the orbital period of a planet is directly proportional to the cube of the semi-major axis of its orbit. (measures how long on avg. it takes for the planet to make it around the sun).square orbital period proportional cubesemi-major axis

Newton’s Applications of Kepler’s Laws  Newton explained why the planets move.  He created his own laws which explained why the planets keep moving around the sun.  He theorized that “gravity” and “inertia” caused the planets to keep moving