Kepler, Galileo & Scientific Revolution

Slides:



Advertisements
Similar presentations
Kepler’s laws.
Advertisements

The Geocentric Theory vs. The Heliocentric Theory
From Aristotle to Newton
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
Astronomy Picture of the Day. Question The Moon has a(n) ________ orbit meaning ________. A. synchronous, its orbital period is equal to its rotation.
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.
Galileo. Activity Ptolemy vs Copernicus Ptolemy’s Explanation of Mars’ retrograde motionPtolemy’s Explanation of Mars’ retrograde motion.
Kepler  Galileo and Newton
Galileo ( ) An Italian scientist, Galileo was renowned for his contributions to physics, astronomy, and scientific philosophy. He is regarded as.
A New Order in Science and Politics. The seventeenth century saw a wave of new thinking about human knowledge, our place in the world, and our place in.
Chapter 2 The Copernican Revolution. Chapter 2 Learning Objectives  Know the differences and similarities between the geocentric and heliocentric models.
The History of Astronomy Part 5 The Debate Concludes Copernicus is Confirmed A Whole New awareness of the Universe.
Analyzing Observing Results Measured Sun’s position at 11:15 am on Fri March 8, 2013: meter stick cast 1.12m shadow  tangent of angle is 1/1.12  angle.
Galileo. Science vs Religion? Historian of science Colin Russell: ‘The common belief that…the actual relations between religion and science over the last.
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.
Galileo Galilei. Early Years Born 15 Feb in Pisa Born 15 Feb in Pisa Educated in Camaldolese Monastery Educated in Camaldolese Monastery Father.
Galileo Galilei – The Experimentalist Did experiments (falling bodies) rather than studying Aristotle Major Works Siderius Nuntius (1610) Dialogue concerning.
Title your notes: Models of the Solar System
Ancient Greeks Early Astronomy  Astronomy is the science that studies the universe. It includes the observation and interpretation of celestial bodies.
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 162 Class 31 Understanding Planetary Motion Use experimental observations (made prior to telescopes) to understand motion of the planets. Period is.
EARLY ASTRONOMERS. Aristotle 3384 BC- 322 BC GGreek Philosopher BBelieved in a geocentric model of the universe EEarth was the center and planets.
Models of the Universe. Throughout history we have looked at the stars and wondered about the universe.
Starter 1.What is astronomy? 2.The movement around the sun is ______. 3.The movement around an axis is____. 4.Compare and contrast global warming and greenhouse.
Observing the Solar System / Earth in Space Chapters 19 & 20 Sections 1 & 2.
CHAPTER 2: Gravitation and the Waltz of the Planets.
Unit 2 Lesson 1 Historical Models of the Solar System
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.
© 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.
Models of the Universe.
From Aristotle to Newton
Tycho Brahe – The Data Taker
Chapter 4 Test Study Guide
Origin of Modern Astronomy
Week 3 Notes Observing the Solar System
Talkin’ bout a Revolution
Physics 229 Week 2 Lab this week: 1. The Winter Sky
Haydn’s The Creation.
Astronomy in the Middle Ages to the Modern Era
Origin of Modern Astronomy
Astronomy Earth Science.
The History of Astronomy
Ch. 22: Astronomers Mr. Litaker 11/10/2018.
Scientific Revolution Scientists
The Copernican Revolution
The Scientific Revolution.
Chapter 3 Analyzing Scales and Motions of the Universe
Origin of Modern Astronomy
Earth’s Role as a Body in Space
The Geocentric Theory vs. The Heliocentric Theory
Kepler.
The Scientific Revolution.
LESSON 12: KEPLER’S LAWS OF PLANETARY MOTION
Kepler’s Laws of Planetary Motion
CHAPTER 27.2: Gravitation and the
I see, I think, I wonder The Scientific Revolution.
Mountains on the Moon Galileo observed the mountains of the Moon with his telescope Estimated their elevation correctly.
Solar Eclipses.
Geocentric Model Earth Centered
Chapter 2 Sections
The Scientific Revolution
The History of Astronomy
The Origin of Modern Astronomy
Presentation transcript:

Kepler, Galileo & Scientific Revolution

Kepler’s First Law: Orbit Shape The orbits of the planets are ellipses, with the Sun at one focus Orbits turn out not to be circles nor eccentric circles but ellipses (which can be made with string and thumbtacks as shown) The sun is at one focus (not the center). A foreshortened circle 2

a = “semimajor axis”; e = “eccentricity” Ellipses a = “semimajor axis”; e = “eccentricity” Orbits of most planets are nearly circular and have small e (Mercury and Pluto most notable exceptions) 3

Kepler’s Second Law: Motion in Time An imaginary line connecting the Sun to any planet sweeps out equal areas of the ellipse in equal times conservation of angular momentum: same effect makes skaters speed up when they draw in their arms 4

Kepler’s Third Law: Relating Orbits The square of a planet’s orbital period is proportional to the cube of its orbital semi-major axis: P 2  a3 Jupiter: 53 / 122 = 125/144 ~ 1 a P Planet Semi-Major Axis Orbital Period Eccentricity ____ P2/a3 Mercury 0.387 0.241 0.206 1.002 Venus 0.723 0.615 0.007 1.001 Earth 1.000 1.000 0.017 1.000 Mars 1.524 1.881 0.093 1.000 Jupiter 5.203 11.86 0.048 0.999 Saturn 9.539 29.46 0.056 1.000 Uranus 19.19 84.01 0.046 0.999 Neptune 30.06 164.8 0.010 1.000 Pluto 39.53 248.6 0.248 1.001 (A.U.) (Earth years) more distant planets move more slowly and have longer "years". Kepler can determine ratio of sizes of the planets' orbits but not the actual sizes; this is because he uses orbit of Earth as baseline for triangulation. If we know the size of one planet's orbit, we can find the rest. Earth's orbit (1 AU)=93 million mi=150 million km=8 light minutes. Nowadays determined by radar ("radio detection and ranging") bounced off Venus. 5

The Baroque Setting In the 1600s church through counter-reformation (Council of Trent 1545-1563) much stricter G. BRUNO (Italian; 1548) proposes that the Sun is just one star out of an infinite number  burned at the stake for heresy 1600 30 Years War (1618-1648) between religions New inventions: telescope, air pump, etc.

Galileo Galilei – The Experimentalist Did experiments (falling bodies) rather than studying Aristotle Major Works Siderius Nuntius (1610) Dialogue concerning the Two Chief World Systems (1632) The latter discusses Copernicus vs Ptolemy ban by Church (1633) revoked by pope 1992 Quotable: “The book of the universe is written in the language of mathematics.” (1564–1642) Telescope invented in Holland in 1608 (HANS LIPPERSHEY) 1616 Galileo ordered to treat Copernicanism as hypothetical 1633 Galileo condemned to permanent house arrest (despite papers giving permission to publish hypothetically) 1992 Vatican acknowledges error after 359 years Galileo's contributions put science firmly on the basis of observation. Argued that the Church should not make scientific positions as articles of faith nor should biblical arguments be applied to science Wrote in Italian rather than Latin

The Scientific Method Systematized by Francis Bacon, Descartes and Galileo in the 17th century Not the only way of knowing, but a very successful one A method to yield conclusions that are independent of the individual Conclusions are based on observation Turtle story (Bertrand Russell?)

Galileo’s Telescopes Galileo’s first telescope was 3x magnifying his last one 32 x

Galileo Galilei (1564–1642) Astronomical observations that contradict Aristotle: Observed mountains on the Moon, suggesting that the Earth is not unique Sunspots; suggests that celestial bodies are not perfect and can change Observed four moons of Jupiter; showed that not all bodies orbit Earth Telescope invented in Holland in 1608 (HANS LIPPERSHEY) 1616 Galileo ordered to treat Copernicanism as hypothetical 1633 Galileo condemned to permanent house arrest (despite papers giving permission to publish hypothetically) 1992 Vatican acknowledges error after 359 years Galileo's contributions put science firmly on the basis of observation. Argued that the Church should not make scientific positions as articles of faith nor should biblical arguments be applied to science Wrote in Italian rather than Latin Observed phases of Venus (and correlation of apparent size and phase); evidence that Venus orbits the Sun Also observed the rings of Saturn that the Milky Way is made of stars

The Starry Messenger Revealing great, unusual, and remarkable spectacles, opening these to the consideration of every man, and especially of philosophers and astronomers; As observed by Galileo Galilei, gentleman of Florence, Professor of Mathematics in the University of Padua With the aid of a Spyglass recently invented by him In the surface of the moon, in innumerable fixed stars, in nebulae, and above all: In four planets, swiftly revolving about Jupiter at differing distances and periods, and known to no none before the Author recently perceived them and decided that they should be named THE MEDICEAN STARS Venice, 1610

Galileo’s Journal on the Discovery of Jupiter’s Moons

Sometimes sees 2,3,4 objects, sometimes left, sometimes right of Jupiter

Sunspots YouTube Video of sketches from the year 1612

Sunspots (Video) Rotation of the Sun

Rotation Period of the Sun Sunspot moves about ¾=75% of diameter in 8 days rotation period roughly 8*2*4/3=21 days (Correct: 26 days)

Debate over Sunspots Who saw them first? Scheiner vs Galileo Neither! What are the sunspots? Could they be clouds across the sun or inner planets transiting the Sun to save Aristotle? No! Appear to move with the sun, no parallax, show appearance like dots painted on a rotating ball