Aristotle. Aristotle. Plato s Student. Knowledge comes from experience BCE Born in Stagira, in Thrace, near Macedonia.

Similar documents
PHY1033C/HIS3931/IDH 3931 : Discovering Physics: The Universe and Humanity s Place in It Fall Prof. Peter Hirschfeld, Physics

Plato. Plato. Plato and Socrates. The Reality of Ideas

The History of Astronomy

How the Greeks Used Geometry to Understand the Stars

Aristotle on Space. Physics, Book IV

PHYSICS 107. Lecture 1: The Puzzle of Motion. In American universities there are three main types of physics courses for nonspecialists.

Pythagoras. Pythagoras of Samos. Pythagoras and the Pythagoreans. Numbers as the ultimate reality

Bit of Administration.

21 Evolution of the Scientific Method

Natural Questions. About 2000 years ago Greek scientists were confused about motion. and developed a theory of motion

Claudius Ptolemy. Logic at its Best. Mathematical Reasoning. Saving the Heavens

The Copernican Revolution

The Copernican Revolution

Notes on Timaeus M. Baumer

Reserve your right to think, for even to think wrongly is better than not to think at all. To teach superstitions as truth is a most m terrible

Foundations of Astronomy The scientific method-winning or losing?

Newton s First Law of Motion

Newton s Laws Review

Astronomy Notes Chapter 02.notebook April 11, 2014 Pythagoras Aristotle geocentric retrograde motion epicycles deferents Aristarchus, heliocentric

Chapter 3 - Gravity and Motion. Copyright (c) The McGraw-Hill Companies, Inc. Permission required for reproduction or display.

HISTORY OF ASTRONOMY

Lecture 8. Eudoxus and the Avoidance of a Fundamental Conflict

Does it matter what you call an object? Does the public care so much? Were scientists made fun of, but not HP Computer Company?

History of Astronomy. Historical People and Theories

The Scientific Revolution

Making Sense of the Universe (Chapter 4) Why does the Earth go around the Sun? Part, but not all, of Chapter 4

Processes that Shape the Earth

ASTR 2010 Modern Cosmology. Professor: James Green

Galileo Galilei. Trial of Galileo before the papal court

Announcements. l LON-CAPA #1 and Mastering Physics 1+2 due next Tuesday

UNIT 2 The Particulate Nature of Matter

INTRODUCTION TO LOGIC

Humanities 3 V. The Scientific Revolution

What is a Revolution? A Revolution is a complete change, or an overthrow of a government, a social system, etc.

BEFORE YOU READ. Forces and Motion Gravity and Motion STUDY TIP. After you read this section, you should be able to answer these questions:

GRAVITY IS AN ATTRACTIVE FORCE

Motions of the Planets ASTR 2110 Sarazin

The Copernican Revolution

Energy Efficiency, Acoustics & Daylighting in building Prof. B. Bhattacharjee Department of Civil Engineering Indian Institute of Technology, Delhi

Tycho Brahe and Johannes Kepler

Directions: Read each slide

The Philosophy of Physics. Is Space Absolute or Relational?

A tour along the road to modern science

Announcements. Topics To Be Covered in this Lecture

Things to do today. Terminal, Astronomy is Fun. Lecture 24 The Science of Astronomy. Scientific Thinking. After this lecture, please pick up:

The Newtonian Synthesis. Conceptual Physics 11 th Edition. The Universal Law of Gravity. The Universal Law of Gravity. The Newtonian Synthesis

How we do science? The scientific method. A duck s head. The problem is that it is pretty clear that there is not a single method that scientists use.

3 Newton s First Law of Motion Inertia. Forces cause changes in motion.

Tides Unit II: The Bulge Theory of the Tides (3.5 pts)

Please pick up your midterms from front of class

The History and Philosophy of Astronomy

Ptolemy (125 A.D.) Ptolemy s Model. Ptolemy s Equant. Ptolemy s Model. Copernicus Model. Copernicus ( )

PHY1033C/HIS3931/IDH 3931 : Discovering Physics: The Universe and Humanity s Place in It Fall Prof. Peter Hirschfeld, Physics

* Pre-Unit Assessment Solar System 5-PS2-1, MS-ESS1-2, MS-ESS1-3. Earth, Moon, Sun System K-PS3-1, 1-ESS1-1, 1-ESS1-2

Topics for today. Galileo s Physics Newton s philosophy & physics How to test a theory

The Onset of the Tension between Science and Christianity Galileo and the Church

Isaac Newton & Gravity

Origins and Formation of the Solar System

Introduction to Logic

Gravity - What Goes Up, Must Come Down

PTOLEMY DAY 4 REMAINING BASICS OF THE GEOCENTRIC MODEL PROPOSITION 4: THE EARTH HAS THE RATIO OF A POINT TO THE HEAVENS

T h e H u n t i n g t o n Library, Art Collections, and Botanical Gardens. History of Science School Program

BROCK UNIVERSITY. 1. The observation that the intervals of time between two successive quarter phases of the Moon are very nearly equal implies that

Chapter 3 Laws of Motion

Revolution and Enlightenment. The scientific revolution

ASTRONAUT PUSHES SPACECRAFT

1. Which term describes any object that exists in space? a. celestial object b. star c. planet d. asteroid

Introduction to Astronomy

some center of the Universe (he mentions the Pythagorean central fire ) and that the

Inventors and Scientists: Sir Isaac Newton

SSWH13 The student will examine the intellectual, political, social, and economic factors that changed the world view of Europeans.

Chapter 2 The Copernican Revolution

Atomic Theory. Introducing the Atomic Theory:

Force Concept Inventory

Comprehensive Exam Session III Classical Mechanics Physics Department- Proctor: Dr. Jack Straton (Sun. Jan 11 th, 2015) (3 hours long 1:00 to 4:00 PM)

06. The Aristotelian Tradition

Was Ptolemy Pstupid?

cosmogony geocentric heliocentric How the Greeks modeled the heavens

SCIENTIFIC REVOLUTION

Lecture 5. Zeno s Four Paradoxes of Motion

Laws of Force and Motion

Name: Earth 110 Exploration of the Solar System Assignment 1: Celestial Motions and Forces Due on Tuesday, Jan. 19, 2016

Lecture 17 Ptolemy on the Motion of the Earth

Galileo. Galileo Galilei. Galileo, the young mathematics whiz. Astronomer, Anti-anti. anti-copernican

Go on to the next page.

Lesson 6 Newton s First Law of Motion Inertia

GALILEAN RELATIVITY. Projectile motion. The Principle of Relativity

Conceptual Integrated Science, 2e (Hewitt et al.) Chapter 2 Describing Motion. Multiple-Choice Questions

SIMPLICITY AND COMPLEXITY IN NATURE. The reductionist approach has been VERY successful Why?

On the Heavens (Exerpts)

Living Things. Lower KS2 Learning Objective. Ideas for practice. knowledge

Lecture 30 Descartes on Matter and Motion

Astronomy Lesson 8.1 Astronomy s Movers and Shakers

Final Exam Extra Credit Opportunity

Humanities 3 V. The Scientific Revolution

The Origin of Modern Astronomy. Nicolai Copernicus ( )

Chapter 2. The Rise of Astronomy. Copyright (c) The McGraw-Hill Companies, Inc. Permission required for reproduction or display.

Lecture 9 Copernicus on the Earth s Daily Rotation

Unit 3 Lesson 2 Gravity and the Solar System. Copyright Houghton Mifflin Harcourt Publishing Company

Astronomy: Exploring the Universe

Transcription:

Aristotle Knowledge comes from experience 1 Aristotle 384-322 BCE Born in Stagira, in Thrace, near Macedonia. The Stagirite. Son of Nichomacus, prominent physician. Aristotle was likely trained in medicine. 2 Plato s Student At age 17, Aristotle was sent to study with Plato at the Academy. He became Plato s most important student, remaining at the Academy 20 years, until Plato s death. 3

Aristotle becomes a royal tutor. When Aristotle left the Academy in 347, he settled briefly on islands near the Ionian coast, then accepted an invitation to teach the son of the Macedonian king, Philip II, whose father had been attended by Aristotle s own father. 4 Alexander the Great Aristotle tutored Phillip s son, Alexander, for 5 years until Phillip died and Alexander assumed the throne. Alexander went on to conquer much of the nearby world. 5 The Lyceum In 335 BCE, Aristotle returned to Athens and established his own school, in competition with the Academy. Named the Lyceum, as it was adjacent to the temple to the god Apollo Lykaios. Morning serious lectures Evening public lectures Inclusive curriculum Classification approach Aristotle associated with Alexander After Alexander's death in 323, Aristotle fled Athens to prevent a second sin against philosophy. 6

Aristotle s works What we have as Aristotle s works are about 30 closely written, terse, treatises on a full range of philosophical and scientific topics. These may have been his morning lectures, or even student s notes on those lectures. 7 versus Plato s works In contrast, Plato s surviving works consist of about 20 dramatic dialogues that discuss philosophical issues in a Socratic, dialectical, questioning manner. Aristotle may have written such works as well, but they have not survived. 8 The foundation of western philosophy and science Aristotle s works more than Plato s laid the groundwork for the systematic development of philosophy and the basic framework for the understanding of nature. Logic, empirical evidence, systematic explanation. Sound methodology, wrong conclusions. 9

The benchmark for the understanding of nature The standard view of the world for 2,000 years. To understand the development of science it is necessary first to grasp Aristotle s methods and his conclusions about nature. 10 Empiricism First, Aristotle grounds all knowledge on experience. This is unlike Plato for whom knowledge came only when the philosopher escaped from the world of sense perception, which could mislead. Reality, for Aristotle, was the world around us, not the objects of the mind, which could be just fantasy. 11 Aristotle, the biologist Students at the Lyceum collected specimens, dissected, and classified them. Analysis of life forms arose from examination of many real examples. Similarly every subject was examined and classified. 12

Contrasting World Views A basic division in how the world is understood: Plato (pointing up) true knowledge comes from contemplating the abstract ideas. Aristotle (pointing down) true knowledge comes from close examination of the world around. Plato and Aristotle from Raphael s School of Athens. 13 Contrasting World Views, 2 The ideal form, an example: For Plato, a geometric object, e.g. a triangle, circle, cube, etc. The true object exists only in the mind. Actual representations are only approximate. For Aristotle, an animal or plant species, e.g. roses, trout, human beings, etc. The species is what all the instances of it have in common. 14 Logic The way to knowledge beyond what is presented to the senses. Based upon Parmenides principle of the excluded middle. A statement is either true or false. Therefore, if it can be shown that a statement is not true, it must be false. If valid reasoning leads to a false conclusion, one of the premises must be false. 15

Syllogisms The key component of Aristotelian logic is the syllogism. Typical format: Major premise a general truth, or observation Minor premise a particular fact, or specific observation Conclusion an inference implied by the two premises together 16 Syllogisms, 2 The classic example of the syllogism: Major premise: All men are mortal. Minor premise: Socrates is a man. Conclusion: Socrates is mortal. In other words, what applies to all members of a group applies to each and every member. 17 Syllogisms and Logic Aristotle worked out the forms of valid reasoning from premises. The principle is to combine known truths and deduce new knowledge that must be true if the premises are true. The method is sound. 18

However The conclusions from syllogistic reasoning must be true only if the premises are true. Very often, Aristotle reasoned correctly from faulty generalizations and produced impressively argued, but nevertheless false, conclusions. As Plato noted, the senses can deceive. 19 The Four Causes A cause for Aristotle is a factor that partly determines a result. Aristotle identified four causes as the explanation for anything (or event) that is. How and why something came to be is understood by examining its four causes. 20 The Four Causes, 2 The causes are: The Material Cause basically the stuff out of which anything is made. The Formal Cause the form, size, and shape of the thing. The Efficient Cause what put the material into the form it is in. The Final Cause the purpose of the thing. 21

The Four Causes, 3 An example: The causes of a knife. Material: The metal, e.g. iron, steel. Formal: The shape of a knife sharp edge, long shaft, pointed end, rounded handle, etc. Efficient: The tool maker that fashioned it. Final: To cut or slice. 22 The Four Causes, 4 Man-made things are easy enough to classify, but natural objects become more difficult. What is the efficient cause of a tree? What is the final cause of a rain shower? Or a human being? What is the material cause of a thunderclap? The formal cause of sunlight? 23 The Four Causes, 5 For Aristotle, the most important cause was the final cause, that for which the thing exists. Anything is explained only by understanding its purpose. Examples: a chair, a blackboard, a piece of chalk, a shoe. Or, a planet, a drought, a mountain, a leopard. 24

Aristotle s logical analysis applied From the logical tools developed by Aristotle, and the careful observations made and generalized, Aristotle built a complete system that explained the world as it is. His system shows the power of reasoning and the dangers of premature generalizations. 25 Aristotle s Cosmos Classification: There are two different parts of the world. There is the world all around, where things come and go; are born, live, and die; and motions start and stop. There is the world up in the sky, where things happen over and over again: the sun rises and sets, the seasons reoccur, the planets repeat cycles. 26 The Sub-Lunar World The world around us includes the Earth itself, the seas, the atmosphere, and of course fire. It extends up to the moon, the first heavenly body. 27

Generation and Corruption The Sublunar world is the world of life. Everything in it came into being, had a period of existence, and died. Even motions started and stopped. Even objects that did not appear to have a life span were subject to this process: Rocks, mountains, etc., came into being and passed away, though over very long periods. 28 The Material of the Sublunar World Aristotle accepted the popular four elements of Empedocles as the material of the sublunar world: Earth, Air, Fire, Water. Everything in the sublunar world is made up of these elements, in different combinations. 29 Natural Place The elements all have a natural place in the sublunar world Earth and water are heavy and so their natural place is at the centre of the world. Fire and air are light and their natural place is at the outer edge of the sublunar world. Note: Light does not mean less heavy. 30

Natural Motion When unobstructed, the elements strive to reach their natural place. This is called natural motion, and requires no further explanation. Earth is heavier than water, so it will push past water seeking the centre. Fire is lighter than air, so it pushes further outward. 31 The Sublunar World 32 Forced Motion Objects on Earth are not always in their natural place, nor do they only have natural motion. They may be forced to move unnaturally, by, for example, being pushed or pulled. Or an object may be prevented from going to its natural place by being held back. 33

Everyday Forced Motions A heavy object may be pulled or pushed to a new location. When it is no longer being forced, it stops. If it is pushed off a cliff, it will resume its natural motion downward, seeking its natural place. A light object, e.g. a vessel containing air, may be pushed under water If released will assume its natural motion upward. 34 The Problem with Logic Aristotle s view of the world is complete and consistent. It is based on direct observation, and logical analysis. When something cannot be observed (e.g. a cause), Aristotle endeavours to discover what it must be, by reasoning from what he has already determined. 35 Not so obvious forced motions The weakness of Aristotle s view of the cosmos is revealed most clearly in his analysis of forced motions. Aristotle believed that an object would only move unnaturally, if it was pushed or pulled i.e. was in direct contact with the cause of motion. 36

What about something thrown or shot? Consider a rock being hurled, or an arrow shot from a bow. The motion of the object fits Aristotle s analysis, only so long as it is in contact with the cause of motion the throwing arm or the bowstring. 37 Why does the object move through the air? According to Aristotle, the object resumes its natural motion (i.e. straight down) as soon as it is no longer in contact with whatever was forcing it. But this is obviously not so; it keeps going. 38 Aristotle s Answer: Since the world is full (no empty spaces anywhere), a rock or arrow flying through the air must be pushing the air out of the way as it flies. That air has to go somewhere. It goes behind the moving object and continues to push it forward. 39

Antiperistasis This is the principle of antiperistasis against remaining in the same place. 40 The weakest point in Aristotle s physics Aristotle s antiperistasis argument was the most obviously contrived explanation in his physics. It attracted the attention of later philosophers almost immediately as a problem. 41 The Super-Lunar World The heavens were obviously different. Motions there repeated over and over again. Generation and corruption did not apply. Heavenly objects seemed to always be there. What needed explaining were the cycles. 42

Natural Motion in the Super-Lunar World In the sublunar world, objects moved to their natural place (and then stopped). In the superlunar world, they cycled. Therefore natural motion in the superlunar world must be circular. The circle moves, but stays in the same place. 43 The Material of the Super-Lunar World The materials of the sublunar world have built in tendencies to go to their natural places. Therefore the material of the superlunar world must be different. 44 The Quintessence There are no forced motions or contrary tendencies in the heavens, so there is only one material there. It is an additional and different element. Aristotle called it the Fifth Element. In Latin, that is the Quintessence. 45

The Crystalline Element The heavens must be full (no empty space), but they look like they are empty. Solution: The fifth element must be invisible, like glass, except for the few bits that show up, the planets and the stars. 46 The Problem of the Planets, again All the natural motions of the fifth element are circular. Since there are no forced motions, everything in the heavens must be moving in combinations of circular motions. 47 Eudoxian Spheres Aristotle adopted the scheme of Eudoxus with spherical shells nested inside each other, all turning different ways. But with a difference: Eudoxus was happy to describe the motions geometrically. Aristotle required a cause of motion. 48

Solution: More spheres Eudoxus thought 27 spheres were enough to account for the motions of the celestial sphere and the seven planets (which include the sun and moon). But their motions were independent. Aristotle required that motion be communicated from one to another. He needed 55 spheres in total. 49 The Unmoved Mover The ultimate cause of motion in the universe is what turns the celestial sphere. The celestial sphere rubs up against the spheres of Saturn, which rub up against Jupiter, etc. That ultimate cause is the Unmoved Mover. 50 The Aristotelian Cosmos An illustration from an edition of Aristotle s On the Heavens, published in 1519. 51

A Philosophy for 2000 Years Aristotle s scheme provided a logically consistent explanation for the motions of the heavens and life on Earth. It combined most of the preconceptions of his time into a grand system. His view remained the standard conception for nearly 2000 years. 52