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:

Slides:



Advertisements
Similar presentations
Astronomy Notes to Accompany the Text
Advertisements

FINISH COPYING THIS INTO YOUR NOTES
Early Astronomers & Planetary Motion
From Aristotle to Newton
Famous Astronomers. Ptolemy Thought the Earth was at the center of the universe and that the other planets revolved around it (GEOcentric model) Thought.
Goals Explain how accurate observations led to Heliocentric model Review contributions of Galileo and Kepler Explain Kepler’s Laws Explain Newton’s laws.
Week 5 Day 1: Announcements. Comments on Mastering Astronomy.
The Origin of Modern Astronomy
Newton’s Law of Universal Gravitation By: Heather Britton.
Chapter 4 Gravitation and the Waltz of the Planets.
Feb. 2, 2011 NEWS: Exoplanets from Kepler.
Early Models of the Universe. Pythagoreans (500 B.C.) Believed the stars, planets, sun, and moon were attached to crystalline spheres which rotated around.
Do our planets move?.
Chapter 2 The Copernican Revolution. Units of Chapter Ancient Astronomy 2.2 The Geocentric Universe 2.3 The Heliocentric Model of the Solar System.
Gravitation and the Waltz of the Planets Chapter Four.
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.
Early Astronomers and their Ideas
Galileo, Tycho, and Kepler and Kepler. Galileo’s Experiments ( ) Galileo tried something new – doing experiments! Dropping balls to measure gravity.
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.
CHAPTER 2: Gravitation and the Waltz of the Planets.
Section 7–3: Motion in Space
Ancient astronomy Geocentric Heliocentric Mass and Gravity GalileoKepler Newton $ 200 $ 200$200 $ 200 $ 200 $400 $ 400$400 $ 400$400 $600 $ 600$600.
Acceleration - rate of change of velocity (speed or direction), occurs any time an unbalanced force is applied.
Chapter 2 The Copernican Revolution. Units of Chapter Ancient Astronomy 2.2 The Geocentric Universe 2.3 The Heliocentric Model of the Solar System.
Chapter 2.
The History of Astronomy brought to you by: Mr. Youngberg.
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.
Gravitation and the Waltz of the Planets Kepler, Galileo and Newton.
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 Solar System Observing the Solar System Guide For Reading How do the heliocentric and geocentric description of the solar system differ? What did.
Astronomy The Science that Studies The Universe Ancient Greeks To Isaac Newton.
The Copernican revolution. Discussion What is the simplest universe imaginable: one where making predictions about the future would be the easiest thing.
Universal Gravitation. Brief Astronomical History A.D Ptolemy Greek Astronomer A.D. Believed in Geo- centrism First to latitude and longitude.
Chapter Planetary Motion & Gravitation Nicholas Copernicus (Polish) Pulished Earth-centered model in 1543 Tycho Brahe (Danish) Vowed to be an astronomer.
In 1543 Copernicus published On the Revolutions of the Heavenly Spheres in which he proposed that Earth and the other planets orbit the sun in perfect.
In this chapter you will:  Learn the nature of gravitational force.  Relate Kepler’s laws of planetary motion to Newton's laws of motion.  Describe.
© 2013 Pearson Education, Inc. Astronomy: A Beginner’s Guide to the Universe Seventh Edition © 2013 Pearson Education, Inc. Chapter 1 Lecture The Copernican.
Chapter 2 The Copernican Revolution. Chapter 2 Learning Objectives  Know the differences and similarities between the geocentric and heliocentric models.
EARTH & SPACE SCIENCE Chapter 27 Planets of the Solar System 27.2 Models of the Solar System.
Early Astronomy Chapter 22, Section 1.
Chapter 22 Section 1 Early Astronomers Aristotle Copernicus Kepler GalileiNewton.
Models of the Solar System
The Copernican Revolution
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.
Astronomy- The Original Science
FAMOUS ASTRONOMERS  Believed in geocentric universe  earth was the center  used circular orbits with epicycles  was supported by the church for.
Astronomy Chapter Astronomy People in ancient cultures used the seasonal cycles to determine when they should plant and harvest crops. They built.
 Astronomy- the study of the universe  Year- the time required for the Earth to orbit once around the sun  Month- a division of the year that is based.
Ch 22 Astronomy. Ancient Greeks 22.1 Early Astronomy  Astronomy is the science that studies the universe. It includes the observation and interpretation.
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 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
Chapter 1 The Copernican Revolution. The planets’ motions Wanderers among the stars Retrograde motion.
History of Astronomy How have ideas about the solar system and our place in it changed over time? How have ideas about the solar system and our place.
THE SOLAR SYSTEM Chapter 24A. Unit Objectives Compare models of the solar system To list and describe the objects in our solar system.
I.Astronomer Ideas A.The Greeks thought Earth was a rotating dome- celestial sphere. B.Geocentric system- Earth at the center of the revolving planets.
Lecture Outlines Astronomy Today 8th Edition Chaisson/McMillan © 2014 Pearson Education, Inc. Chapter 2.
Bell Ringer What celestial body is at the center of our solar system? What is celestial body or bodies has the farthest orbit in our solar system? What.
Modern Day Astronomers (sort of) The New Guys. The Astronomers Copernicus Galileo Tycho Brahe Johannes Kepler Sir Isaac Newton.
Topic: Early Astronomy PSSA: D/S8.A.2.2. Objective: TLW explain how the discoveries of early astronomers has changed mankind’s understanding of.
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.
Gravity Newton’s Law of Gravitation Gravitational Fields.
Ancient Greeks Early Astronomy  Astronomy is the science that studies the universe. It includes the observation and interpretation of celestial bodies.
© 2017 Pearson Education, Inc.
Formation of the Solar System
Origin of Modern Astronomy
Presentation transcript:

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: red, orange, yellow, green, blue, indigo, violet developed a reflecting telescope Newton's Law of Gravitation describes the gravitational attraction between objects; the force of their gravitational attraction (F) depends only on their masses and the distance between them, according to the formula F = Gm 1 m 2 / r 2. The universal gravitational constant (abbreviated G) is the constant of proportionality in Newton's equation; G is a fundamental constant of nature that determines the strength of the force of the gravitational interaction between objects Reflecting telescope gravity

constructed the first complete astronomical telescope discovered that the moon, shining with reflected light, had an uneven, mountainous surface discovered the four largest satellites of Jupiter, the first satellites of a planet other than Earth to be detected observed and studied the oval shape of Saturn and phases of venus His investigations confirmed his acceptance of the Copernican theory of the solar system Galileo’s recordings of Venus's phases Galileo’s recordings of Jupiter’s moons

First to correctly explain planetary motion, thereby, becoming founder of celestial mechanics and the first "natural laws" in the modern sense; being universal, verifiable, precise. The First Law: The orbit of a planet/comet about the Sun is an ellipse with the Sun's center of mass at one focus The Second Law: A line joining a planet/comet and the Sun sweeps out equal areas in equal intervals of time The third law: The squares of the periodic times are to each other as the cubes of the mean distances. Second Law First law

Copernicus thought that the planets orbited the Sun, and that the Moon orbited Earth. The Sun, in the center of the universe, did not move, nor did the stars. Ptolemy thought that all celestial objects — including the planets, Sun, Moon, and stars — orbited Earth. Earth, in the center of the universe, did not move at all.