The History of Astronomy II September 18, 2009. Taking Care of Business (TCB) Read textbook Unit 12 Read textbook Unit 12 Take Moon observations Take.

Slides:



Advertisements
Similar presentations
Kepler’s laws.
Advertisements

Early Astronomers & Planetary Motion
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.
Do our planets move?.
Models of the Solar System
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)
Ancient astronomy Geocentric Heliocentric Mass and Gravity GalileoKepler Newton $ 200 $ 200$200 $ 200 $ 200 $400 $ 400$400 $ 400$400 $600 $ 600$600.
Today’s topics Orbits Parallax Angular size and physical size Precession Reading sections 1.5, 2.6,
Sun, Moon, Earth, How do they work together to help life survive? Our 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.
Origins of Modern Astronomy
Astronomy 1010-H Planetary Astronomy Fall_2015 Day-11.
Topic: Models of the Universe Key Terms: Geocentric Theory Heliocentric Theory.
Astronomical History Ptolemy expresses geocentric model 127AD
The History of Astronomy Part 4 The Debate Heats Up Tycho and Kepler.
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.
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.
Unit 1 Physics Detailed Study 3.1 Chapter 10: Astronomy.
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.
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.
Kepler’s Laws September 21, Taking Care of Business (TCB) Read textbook Unit 12 Read textbook Unit 12 Take Moon observations Take Moon observations.
THE SOLAR SYSTEM Chapter 24A. Unit Objectives Compare models of the solar system To list and describe the objects in our solar system.
EARTH & SPACE SCIENCE Chapter 27 Planets of the Solar System 27.2 Models of the Solar System.
I. Early History of Astronomy
Astronomy 1010 Planetary Astronomy Fall_2015 Day-13.
Bellwork 1.Who is credited with the revolutionary model of a HELIOCENTRIC solar system? A. Aristotle B. Ptolemy C. Galileo D. Copernicus 2.The planets.
PHYS 155 – Introductory Astronomy observing sessions: - observing sessions: Sunday – Thursday, 9pm, weather permitting
Astronomy and the Renaissance. Lesson Overview  Copernicus and the Sun-Centered Model  Kepler’s Laws of Planetary Motion Chapter 1, Lesson 2.
CHAPTER 2: Gravitation and the Waltz of the Planets.
© 2017 Pearson Education, Inc.
Motion of the Moon.
Bellwork Who is credited with the revolutionary model of a HELIOCENTRIC solar system? A. Aristotle B. Ptolemy C. Galileo D. Copernicus The planets loop.
Day 4 Gravitation and the Motion of the Planets
Observing the Solar System
Gravitation and the Waltz of the Planets
Motion of the sun Motion of the moon Motion of the stars
Renaissance Astronomy
Chapter 4 Test Study Guide
MODELS OF THE SOLAR SYSTEM
Brahe & Kepler The Final Battle Yay!!! Yay!!! Geocentric
Chatfield Senior High Physics
Astronomy in the Middle Ages to the Modern Era
Science Starter Answer the following in your notebook: 1. When is the Earth closest to the Sun? 2. Does the speed of the Earth’s revolution change? 3.
Introduction To Modern Astronomy II
22.1 Early Astronomy.
History of Astronomy.
Renaissance Astronomy
Giants of Science Part Two Tycho Brahe & Johannes Kepler
What is the universe Part 2 Motion in Space
Origins of Modern Astronomy
The Copernican Revolution
Chapter 3 Analyzing Scales and Motions of the Universe
Kepler’s Laws.
The Laws of Planetary Motion
The History of Astronomy
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.
LESSON 12: KEPLER’S LAWS OF PLANETARY MOTION
Lesson 2 Models of the Universe
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.
CHAPTER 27.2: Gravitation and the
Part 1: Historical Models
EARTH SCIENCE MRS. DAVIS
The History of Astronomy
History of Modern Astronomy
Early Ideas.
Presentation transcript:

The History of Astronomy II September 18, 2009

Taking Care of Business (TCB) Read textbook Unit 12 Read textbook Unit 12 Take Moon observations Take Moon observations 6 Observations due September 28 6 Observations due September 28 Test #1 – September 18 to September 21 Test #1 – September 18 to September 21 Sept 16 class – last day of test material Sept 16 class – last day of test material Reserve your test date/time ASAP Reserve your test date/time ASAP InQsit instructions on Blackboard InQsit instructions on Blackboard

Parallax Review A star located 25 parsecs from the Sun has a parallax angle of A star located 25 parsecs from the Sun has a parallax angle of A. 25 arcseconds A. 25 arcseconds B. 50 arcseconds B. 50 arcseconds C arcseconds C arcseconds D arcseconds D arcseconds E. None of the above E. None of the above 1/25= 1/d 1/25= 1/d

Review Question What is the distance to a star (in parsecs) that has a parallax angle of 0.1 arcseconds? What is the distance to a star (in parsecs) that has a parallax angle of 0.1 arcseconds? a) 0.01 a) 0.01 b) 0.1 b) 0.1 c) 1 c) 1 d) 10 d) 10 e) 100 e) 100 1/  = 1/0.1 1/  = 1/0.1

Ptolemy Earth-centered system Earth-centered system Earth located slightly off the center of orbiting circles Earth located slightly off the center of orbiting circles Ptolemaic model was inconsistent over many years Ptolemaic model was inconsistent over many years Epicycles adds to prove his method, instead it’s too complicated Epicycles adds to prove his method, instead it’s too complicated Geocentric Method Geocentric Method Ptolemy – 100 – 170 A.D.

Ptolemy’s Geocentric Model

Ptolemy’s Epicycles Epicycle Deferent Earth

Ptolemy’s Epicycles

Where is retrograde motion occurring? Planet’s Path

Ptolemy’s Epicycles Where is retrograde motion? Planet’s Path

Astronomy Revolution Idea of an Earth- centered system held to be true for close to 2000 years Idea of an Earth- centered system held to be true for close to 2000 years Believed that there must be a simpler explanation of the Solar System Believed that there must be a simpler explanation of the Solar System Usually true when it is the simplest Usually true when it is the simplest Placed the Sun at the center Placed the Sun at the center Heliocentric system Heliocentric system Nicholas Copernicus –

Discussion Why was the Copernican model not widely accepted at first? Why was the Copernican model not widely accepted at first?

Tycho Brahe Great interest in observing the motions of the sky Great interest in observing the motions of the sky Noticed that positions of planets were not accurate compared to available tables Noticed that positions of planets were not accurate compared to available tables Did his own detailed observations to mark positions Did his own detailed observations to mark positions Discovered a “new star” Discovered a “new star” Supernova Supernova Brahe –

Kepler Wanted to accurately match the observations of Mars – off by as much as 8 arcminutes Wanted to accurately match the observations of Mars – off by as much as 8 arcminutes Developed a new model that did not rely on circles, but instead used ellipses Developed a new model that did not rely on circles, but instead used ellipses Kepler’s 3 Laws of Motion Kepler’s 3 Laws of Motion Johannes Kepler –

Kepler’s First Law The orbit of each planet about the Sun is an ellipse with the Sun at one focus The orbit of each planet about the Sun is an ellipse with the Sun at one focus

Kepler’s Second Law As a planet moves around its orbit, it sweeps out equal areas in equal times As a planet moves around its orbit, it sweeps out equal areas in equal times To do this, a planet must move slower at aphelion (point furthest from sun) than it does at perihelion (point closest to the sun: fastest) To do this, a planet must move slower at aphelion (point furthest from sun) than it does at perihelion (point closest to the sun: fastest)

Post Tutorial Question During which part of the planet’s orbit (A, B, C, or D) would the planet move with the greatest speed? During which part of the planet’s orbit (A, B, C, or D) would the planet move with the greatest speed?

Post Tutorial Question During how many portions of the planet’s orbit (A, B, C and D) would the planet be speeding up the entire time? During how many portions of the planet’s orbit (A, B, C and D) would the planet be speeding up the entire time? a. Only during one of the portions shown. a. Only during one of the portions shown. b. During two of the portions shown. b. During two of the portions shown. c. During three of the portions shown. c. During three of the portions shown. d. During four of the portions shown. d. During four of the portions shown. e. None of the above. e. None of the above.

Post Tutorial Question According to Kepler’s Second Law, during which one of the portion of the planets orbit “B”, “C”, or “D”, would the planet take the same amount of time as it took for the portion of the orbit identified with letter “A”? If you think all the portions of the orbit take the same amount of time, answer “E”. According to Kepler’s Second Law, during which one of the portion of the planets orbit “B”, “C”, or “D”, would the planet take the same amount of time as it took for the portion of the orbit identified with letter “A”? If you think all the portions of the orbit take the same amount of time, answer “E”.