Chapter 3 The Science of Astronomy

Slides:



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

From Aristotle to Newton
Gravitation and the Waltz of the Planets
Chapter 1: Origins of Modern Astronomy
Day 4 Chapter 2 part 2 Kepler’s Laws Newton’s Laws
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
Ancient Astronomy Objects in the Sky move in cycles –Stars, Sun, Moon, eclipses, etc. Why did most ancient people care? –Agriculture –Religion Egyptians.
Astronomy 101 Section 020 Lecture 4 Gravitation and the Waltz of the Planets John T. McGraw, Professor Laurel Ladwig, Planetarium Manager.
ASTR100 (Spring 2008) Introduction to Astronomy The Science of Astronomy Prof. D.C. Richardson Sections
Chapter 4 Gravitation and the Waltz of the Planets.
Planetary Motions.
Astronomy Picture of the Day. Question The Moon has a(n) ________ orbit meaning ________. A. synchronous, its orbital period is equal to its rotation.
History of Astronomy  Motions of the sky caused by and controlled by gods. Big Horn Medicine Wheel Temple at Caracol.
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.
FOUNDATIONS OF ASTRONOMY Casey Trout. ANCIENT BELIEFS Ancient cultures learned how to predict the weather, the seasons, time of day, & eclipses In Central.
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)
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.
Chapter 2: The Rise of Astronomy. Ancient Roots: Early Homo-Sapiens.
Chapter 26.2: Observing the Solar System
Today’s topics Orbits Parallax Angular size and physical size Precession Reading sections 1.5, 2.6,
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.
Origin of Modern Astronomy
The History of Astronomy brought to you by: Mr. Youngberg.
History of Astronomy - Part II
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.
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 Origin of Modern Astronomy
Chapter 2 The Copernican Revolution. Units of Chapter Ancient Astronomy 2.2 The Geocentric Universe 2.3 The Heliocentric Model of the Solar System.
Day 3 Chapter 2 Gravitation and the Motion of the Planets.
Gravity. Geocentric vs. Heliocentric Model The Geocentric Model Arguments For: Parallax not seen Almagest says so Fits with “heavenly” perfection Arguments.
Astronomy Picture of the Day Windows on the Universe Simulation: Comets and Retrograde Motion.
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.
Chapter 3c The Science of Astronomy. © 2005 Pearson Education Inc., publishing as Addison-Wesley 3.3 The Copernican Revolution How did Copernicus, Tycho,
Kepler Orbits Last time we saw that this equation describes an ellipse. r min = perihelion (for solar orbits) or perigee r max = aphelion (for solar orbits)
Chapter 2 The Copernican Revolution. Chapter 2 Learning Objectives  Know the differences and similarities between the geocentric and heliocentric models.
Early Astronomy Chapter 22, Section 1.
Notebooks: We had a very BASIC notebook check. For our next notebook check you need to have your cover completed, table of contents filled out, titles.
NATS From the Cosmos to Earth Nicholas Copernicus ( ) - wanted better way to predict planetary positions - adopted Sun-centered planetary.
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.
Chapter 3b The Science of Astronomy. 3.2 Ancient Greek Science Why does modern science trace its roots to the Greeks? How did the Greeks explain planetary.
Mav Mark 11/3/11 When electricity leaves a power plant is it AC or DC, and is it at high voltage or low voltage?
Ch 22 Astronomy. Ancient Greeks 22.1 Early Astronomy  Astronomy is the science that studies the universe. It includes the observation and interpretation.
The Organization of the Solar System and Planetary Motion
How We Know Where They’re Going.  Geocentric Model  Earth is the center of the universe  Philosophy at the time leads to the idea of perfection and.
Our Planet and Solar System. Ancient and Pre-Modern Theories of the Universe/Solar System Aristotle’s theory of four elements Astronomy and Astrology.
Title your notes: Models of the Solar System
Universe Tenth Edition Chapter 4 Gravitation and the Waltz of Planets Roger Freedman Robert Geller William Kaufmann III.
The “Geocentric Model” Aristotle vs. Aristarchus (3 rd century B.C.): Aristotle: Sun, Moon, Planets and Stars rotate around fixed Earth. Ancient Greek.
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.
CHAPTER 2: Gravitation and the Waltz of the Planets.
Gravitation and the Waltz of the Planets
Origin of Modern Astronomy
Introduction To Modern Astronomy II
The Copernican Revolution
THE SCIENCE OF ASTRONOMY Wednesday, February 1, 12.
CHAPTER 27.2: Gravitation and the
Chapter 2 Sections
Presentation transcript:

Chapter 3 The Science of Astronomy

How is modern science rooted in ancient astronomy? Note: fun to discuss the claims that these had to have been made by "ancient astronauts"… Macchu Pichu, Peru: Structures aligned with solstices. © 2014 Pearson Education, Inc.

Cosmogony A cosmogony is theory about Earth’s place in the universe. A geocentric cosmogony is a theory that proposes Earth to be at the center of the universe. A heliocentric cosmogony is a theory that proposes the Sun to be at the center of the universe.

Which is the geocentric cosmogony and which is the heliocentric cosmogony? geocentric (Earth-centered) heliocentric (Sun-centered)

Planets were often called wandering stars because they seem to move from one constellation to the next.

Planets Known in Ancient Times Mercury difficult to see; always close to Sun in sky Venus very bright when visible; morning or evening “star” Mars noticeably red Jupiter very bright Saturn moderately bright This slide explains what students can see of planets in the sky.

What was once so mysterious about planetary motion in our sky? Planets usually move slightly eastward from night to night relative to the stars. But sometimes they go westward relative to the stars for a few weeks: apparent retrograde motion. The diagram at left shows Jupiter’s path with apparent retrograde motion in 2004-5. The photo composite shows Mars at 5-8 day intervals during the latter half of 2003.

We see apparent retrograde motion when we pass by a planet in its orbit. We also recommend that you encourage students to try the apparent retrograde motion demonstration shown in the book in Figure 2.33a, since seeing it for themselves really helps remove the mystery…

Explaining Apparent Retrograde Motion Easy for us to explain: occurs when we “lap” another planet (or when Mercury or Venus laps us). But very difficult to explain if you think that Earth is the center of the universe! In fact, ancients considered but rejected the correct explanation.

Why did the ancient Greeks reject the real explanation for planetary motion? Their inability to observe stellar parallax was a major factor.

Scientists use parallax to measure distances.

The Greeks knew that the lack of observable parallax could mean one of two things: Stars are so far away that stellar parallax is too small to notice with the naked eye. Earth does not orbit the Sun; it is the center of the universe. With rare exceptions such as Aristarchus, the Greeks rejected the correct explanation (1) because they did not think the stars could be that far away. Thus, the stage was set for the long, historical showdown between Earth-centered and Sun-centered systems. In fact, the nearest stars have parallax angles less than 1 arcsecond, far below what the naked eye can see. Indeed, we CAN detect parallax today, offering direct proof that Earth really does go around the Sun…

Ancient Science The ancient Greeks were the first to seek to explain nature by means of logic and geometry, and not resort to supernatural explanations. We must not forget that besides the Greeks, there were many cultures that contributed to the advancement of science and astronomy. Egyptian and Mayan measurements of time. Polynesian navigation. Chinese and Islamic astronomers, to mention a few! While astronomy and astrology both grew out of the same source, astrology cannot stand up to the rigors of modern science.

Our mathematical and scientific heritage originated with the civilizations of the Middle East.

The Greeks advanced the concept of Science, and moved away from superstition and mythology. For 700 years, the Greeks postulated such ideas as the Earth is a sphere, that the elements are composed of basic bits, called atoms, and that planets existed and circled in the heavens. Aristotle argued for a Earth-centered universe. Eratosthenes accurately estimated the circumference of the Earth. Around 150 AD, Ptolemy put forth the first published work detailing a geocentric model of the Universe.

Special Topic: Eratosthenes Measures Earth (c. 240 B.C.) Measurements: Syene to Alexandria distance ≈ 5000 stadia angle = 7° Calculate circumference of Earth: 7/360  (circum. Earth) = 5000 stadia  circum. Earth = 5000  360/7 stadia ≈ 250,000 stadia This slide based on the special topic box to show Eratosthenes calculation. Compare to modern value (≈ 40,100 km): Greek stadium ≈ 1/6 km  250,000 stadia ≈ 42,000 km

The most sophisticated geocentric model was that of Ptolemy (A. D The most sophisticated geocentric model was that of Ptolemy (A.D. 100-170) — the Ptolemaic model: Sufficiently accurate to remain in use for 1,500 years. Arabic translation of Ptolemy’s work named Almagest (“the greatest compilation”) Ptolemy

The Copernican Revolution Copernicus devised the first comprehensive heliocentric cosmology to successfully explain retrograde motion

sidereal period is the time it takes a planet to orbit the Sun once. synodic period is the time that elapses between two successive identical configurations as seen from Earth (e.g., time from opposition to opposition)

Tycho Brahe measured distances using parallax that disproved ancient ideas about the heavens A supernova in 1572 was shown to exist in the distant heavens; this troubled scholars who previously thought the heavens were unchanging. He showed that comets were objects that occurred in the region of the planets, not in Earth’s atmosphere.

Compiled the most accurate (one arcminute) naked eye measurements ever made of planetary positions. Still could not detect stellar parallax, and thus still thought Earth must be at center of solar system (but recognized that other planets go around Sun). Hired Kepler, who used Tycho’s observations to discover the truth about planetary motion. Remind students that one arcminute is equivalent to the width of a fingernail at arm’s length… Tycho Brahe (1546-1601)

Kepler first tried to match Tycho’s observations with circular orbits But an 8-arcminute discrepancy led him eventually to ellipses. “If I had believed that we could ignore these eight minutes [of arc], I would have patched up my hypothesis accordingly. But, since it was not permissible to ignore, those eight minutes pointed the road to a complete reformation in astronomy.” Kepler quote offers a good opportunity to talk about the nature of science, and how failure to match observations should force a change in hour hypotheses. Johannes Kepler (1571-1630)

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

The distance between the two foci impact the eccentricity of the ellipse’s shape.

Kepler’s Second Law: A line joining a planet and the Sun sweeps out equal areas in equal intervals of time.

Kepler’s Third Law: The square of a planet’s sidereal period is proportional to the cube of the length of its orbit’s semimajor axis (p2=a3).

Italian scientist Galileo made discoveries that strongly supported a heliocentric cosmology

Galileo’s telescope revealed phases of Venus which could only occur IF Venus orbits the Sun.

Galileo’s telescope revealed that Jupiter had moons which orbited Jupiter instead of Earth.

Galileo was formally vindicated by the Church in 1992. The Catholic Church ordered Galileo to recant his claim that Earth orbits the Sun in 1633. His book on the subject was removed from the Church’s index of banned books in 1824. Galileo was formally vindicated by the Church in 1992. The scientific case was essentially settled, but the story was more complex in his own time as politics intervened…

Isaac Newton formulated three laws that describe fundamental properties of physical reality

Newton’s Three Laws of Motion A body remains at rest or moves in a straight line at a constant speed unless acted upon by an unbalanced outside force. Force = mass x acceleration Whenever one body exerts a force on a second body, the second body exerts an equal and opposite force on the first body.

Newton’s description of gravity accounts for Kepler’s laws Newton’s universal law of gravitation states: Two bodies attract each other with a force that is directly proportional to the square of the distance between them. This law mathematically proves Kepler’s Third Law (p2=a3). This law describes various orbits objects can take when moving near the Sun. This law can be used to predict when comets, such as Halley’s comet, will pass near Earth.

Video Early Astronomers

An introduction to the scientific method, skepticism, hoaxes & hokum Science vs. Myth An introduction to the scientific method, skepticism, hoaxes & hokum

The Scientific Method Observing the Universe led to the scientific method. As astronomers sought to explain the patterns of the motion of the planets, they developed a methodology that set science apart from pseudo-science. Science: The discovery of natural explanations for what we observe and measure in the natural world, and can experiment on in the laboratory. It is an amazing realization that the Universe is knowable! Our understanding of nature is growing exponentially. There is much we don’t know, but we no longer accept that it can’t be known. In time, we will learn more, and we will fill in the gaps in our knowledge. We no longer need to invent explanations, through the application of the Scientific Method, we know that if it can be explained it will be explained in time.

The Scientific Method The scientific method can be used to predict how physical systems will behave. Scientists first create a scientific theory, based on mathematical models or observation. Then scientists make predictions using this theory. Scientists then perform experiments and make observations that either agree with their theory or disprove it. Scientific theories are based on independent and verifiable testing, not on personal belief systems.

Remember The Scientific Method --- Observation and Experiments are used to Support or Reject a Theory

Not Scientific How can we tell? 1. Some is clearly made up. 2. Images on the moon are presumed to be pyramids, without more than a grainy picture and an elaborate “pyramid scheme” has been concocted. Occam’s Razor says the most likely explanation is the simpler one, as long as it agrees with all the evidence. We don’t choose an explanation that makes us happy or fits our preconceived ideas, if another theory is better. Peer review helps to remove this type of bias.

Pseudoscience Pseudoscience includes astrology, myths and belief systems that cannot be confirmed or disproven by science. There is insufficient evidence to “prove” UFOs or ghosts or demons exist. There is no scientific theory that can be applied and tested. As soon as we have measurable/testable evidence for one of these, we can apply the scientific method.

Video Carl Sagan on Astrology

Science & Common Sense Science explains natural phenomena with formulae that are tested and superior to non-scientific answers. But, scientific answers do not always agree with “Midwestern Common Sense”. Why? We have a lot of experience with the world we live in, but we don’t have experience being the size of an atom, or as massive as a star or as fast as a light beam. Quantum Mechanics is incredibly accurate at making predictions, yet it is hard to reconcile with our common sense. Just because something doesn’t agree with our gut instinct doesn’t mean we should reject it out of hand. Example: A child has a hard time understanding the law of gravity. When told that people live on the other side of the world, and the world is shaped like a beach ball, the small child might wonder why the people don’t just fall off the Earth! Our common sense is biased towards our experiences. 46

Video Michael Shermer on Cognitive Biases Perception Test

Conclusions Do you understand the scientific method, and how astronomy contributed to its development and human history? Read the handouts and consider examples of pseudoscience and why they are rejected by the scientific method. Think of the arguments made by people to justify their non-scientific beliefs. Can you use Carl Sagan’s “Baloney Detection” to recognize them? [Bring an example to our next class.] Consider your place in the cosmos. Do you have a good perspective of the scale of the universe? The size of atoms, planets, stars, galaxies and the vast distances between them? Consider the 13.7 billion year history of the cosmos. Think of how that history fits onto the Cosmic Calendar, and how short a span of time humans have existed. Do you understand how looking farther out in space allows us to look farther back in time? 48

References www.badastronomy.com www.randi.org www.skeptic.org www.scicop.org www.badastronomy.com/bad/misc/astrology.html Carl Sagan’s “The Demon Haunted World: Science as a Candle in the Dark”, ISBN 978-0345409461. 49