VISUAL PHYSICS ONLINE THE LANGUAGE OF PHYSICS KINEMATICS

Similar documents
THE LANGUAGE OF PHYSICS:

DO PHYSICS ONLINE. WEB activity: Use the web to find out more about: Aristotle, Copernicus, Kepler, Galileo and Newton.

HSC PHYSICS ONLINE THE LANGUAGE OF PHYSICS: FRAMES OF REFERENCE

VISUAL PHYSICS ONLINE THE LANGUAGE OF PHYSICS SCALAR AND VECTORS

How Astronomers Learnt that The Heavens Are Not Perfect

Newton s Law of Universal Gravitation (attraction between. Gravitation field strength surrounding the Earth g E

Astronomy- The Original Science

SCIENTIFIC REVOLUTION

VISUAL PHYSICS ONLINE

,.~ Readlng ~ What,~,~~ is a geocentric system? Chapter3 J 73

Announcements. Topics To Be Covered in this Lecture

Space Notes Covers Objectives 1 & 2

VISUAL PHYSICS ONLINE KINEMATICS DESCRIBING MOTION

PHYS 160 Astronomy Test #1 Fall 2017 Version B

The Scientific Revolution,

Was Ptolemy Pstupid?

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

VISUAL PHYSICS ONLINE

Intro to Astronomy. Looking at Our Space Neighborhood

Homework #2 is online and is due next Friday! Planetarium shows are getting full. Solar Observing starts Monday!

The Scientific Revolution

THE SCIENTIFIC REVOLUTION

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

Scientific Revolution

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

THE SCIENTIFIC REVOLUTION

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

Introduction To Modern Astronomy I

Day 4: Scientific Ideas Change the World

Force mediated by a field - long range: action at a distance: The attractive or repulsion between two stationary charged objects.

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

Scientific Revolution

Revolution and Enlightenment. The scientific revolution

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

2010 Pearson Education, Inc. Chapter 4 Making Sense of the Universe: Understanding Motion, Energy, and Gravity

2. See FIGURE B. This person in the FIGURE discovered that this planet had phases (name the planet)?

The Scientific Revolution

1 Astronomy: The Original Science

Contents: -Information/Research Packet. - Jumbled Image packet. - Comic book cover page. -Comic book pages. -Example finished comic

MODULE 4.1 ELECTRICITY ELECTRICAL POTENTIAL VISUAL PHYSICS ONLINE. voltage V. electrical potential V potential difference V

Chapter 3 The Science of Astronomy

The Scientific Revolution Learning Target

The History of Astronomy. Theories, People, and Discoveries of the Past

Main Themes: 7/12/2009

VISUAL PHYSICS ONLINE DYNAMICS TYPES OF FORCES FRICTION

Astronomy 1010 Planetary Astronomy Sample Questions for Exam 1

THE SCIENTIST CFE 3293V

MODULE 4.1 ELECTRICITY ELECTRIC CURRENT VISUAL PHYSICS ONLINE CURRENT I

The History of Astronomy. Please pick up your assigned transmitter.

Gravitation Part I. Ptolemy, Copernicus, Galileo, and Kepler

Gravity. Announcement. Topics in Chapter 5. Topics for Today. PHYS 1403 Introduction to Astronomy. Motion. Chapter 5. Exam 1

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

Newton s Laws Review

D. A system of assumptions and principles applicable to a wide range of phenomena that has been repeatedly verified

Models of the Solar System. The Development of Understanding from Ancient Greece to Isaac Newton

Johannes Kepler ( ) German Mathematician and Astronomer Passionately convinced of the rightness of the Copernican view. Set out to prove it!

In this chapter, you will consider the force of gravity:

Name Class Date. Ptolemy alchemy Scientific Revolution

Galileo Educator Network

N = R * f p n e f l f i f c L

MAXIMIZING YOUR PHYSICS EXAMINATION MARKS

Describing motion: Kinematics in two dimension

Claudius Ptolemaeus Second Century AD. Jan 5 7:37 AM

Remember that all physical quantities are measured in units. The unit of force is called the newton (N), where 1 N = (1 kg)(1 m/s 2 ).

Physics : Fall Semester Review Chapter 1-4

Chapter 18: Studying Space Astronomy: The Original Science

Scientific Revolution and the Enlightenment Introduction

Chapter 4. The Laws of Motion

January 19, notes.notebook. Claudius Ptolemaeus Second Century AD. Jan 5 7:37 AM

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

Galileo Galilei. Trial of Galileo before the papal court

Sir Isaac Newton ( )

Welcome to Physics 43!

Kepler, Newton, and laws of motion

Conceptual Physics Fundamentals. Chapter 3: EQUILIBRIUM AND LINEAR MOTION

Enlightenment and Revolution. Section 1

Practice Test DeAnza College Astronomy 04 Test 1 Spring Quarter 2009

HW Chapter 3 Q 14,15 P 2,7,812,18,24,25. Chapter 3. Motion in the Universe. Dr. Armen Kocharian

Eclipses and Forces. Jan 21, ) Review 2) Eclipses 3) Kepler s Laws 4) Newton s Laws

Physics General Physics. Lecture 3 Newtonian Mechanics. Fall 2016 Semester. Prof. Matthew Jones

2X CLAUDIUS PTOLEMY BIOGRAPHY 780L

1UNIT. The Universe. What do you remember? Key language. Content objectives

Name: Exam 1, 9/30/05

Physics 141 Dynamics 1 Page 1. Dynamics 1

Venus Phases & Newton s Laws

Monday, October 3, 2011

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

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

Free-Body Diagrams: Introduction

Astronomy 1 Fall 2016

Section 5. Objectives

2X CLAUDIUS PTOLEMY BIOGRAPHY 1260L

Chapter 3 The Science of Astronomy. Copyright 2012 Pearson Education, Inc.

Last time we finished Ch. 2

ASTRONOMY CURRICULUM Unit 1: Introduction to Astronomy

Occam s Razor: William of Occam, 1340(!)

2. 4 Base your answer to the question on the time line below and on your knowledge of social studies.

A100 Exploring the Universe: The Invention of Science. Martin D. Weinberg UMass Astronomy

7 Study Guide. Gravitation Vocabulary Review

Chapter 6: Circular Motion, Orbits, and Gravity Tuesday, September 17, :00 PM. Circular Motion. Rotational kinematics

Transcription:

VISUAL PHYSICS ONLINE THE LANGUAGE OF PHYSICS KINEMATICS The objects that make up space are in motion, we move, soccer balls move, the Earth moves, electrons move,.... Motion implies change. The description of the motion of objects is called kinematics. Since the beginning of human time the study of the motions of the heavens has been important. People who had knowledge of the motion of the heavens had power and control over others because they knew about the seasons, eclipses and could make predictions. In ancient cultures, people were very frightened during solar and moon eclipses. 1

Developing theories about the motion of the Sun and planets was very frustrating. Many religions had the Earth at the centre of the Universe. For presenting views opposing the Earth centred Universe one could be burnt alive at the stake. Developing a consistent theory of motion was difficult. Physical theories are not just discovered, they are creations of the human mind and must be invented and not discovered. It is claimed that the study of physics is man s greatest intellectual achievement. Physics is a creative process and physicists build on the best of the past to create new visions of the future. A significant time for science was when Nicholas Copernicus (1473 1543) concluded from experimental data on the motion of the planets, that the Earth revolved around the Sun. Johannes Kepler (1571 1630) could decipher accurately and precisely the paths of the planets and produced mathematical laws accounting for the motion of the planets around the Sun. 2

The work of Galileo Galilei (1564 1642) produced a dramatic change in the way science was to be done. Galileo s ideas overturned the Aristotelian view of the world that had persisted for more than 2000 years. Galileo s genius was that he realized that the world can be described through mathematics and that experimentation and measurement were crucial elements in developing scientific theories where approximation was necessary to limit complexity. 3

Following on from Galileo was Isaac Newton (1642 1727), who developed the underlying theory of the causes of motion (dynamics). He published one of the most famous books of science in 1686, Principia. 4

WEB ACTIVITY / DISCUSSIONS Use the web to find out more about: Aristotle, Copernicus, Kepler, Galileo and Newton. Group discussion: Why did people such as priests who had scientific knowledge of the seasons and astronomy have control over the bulk of the population in their societies? Group discussion: In the period from the 15 th century to the 19 th century in Western Europe there was a dramatic change in social, cultural and technological aspects for people but this did not occur in China, which at the beginning of the 15 th century could be considered to be more advanced socially, culturally and technologically than Europe. Explain why the no change in China compared with the scientific and technological developments that occurred in Western Europe in this 400 year period. 5

Consider the physical situation of a tractor pulling a crate across a paddock as shown in figure 1. Fig. 1. A complex physical situation of a tractor pulling a crate across a paddock. Kinematics is the branch of classical mechanics which describes the motion of objects without consideration of the masses of those objects nor the forces that may have caused the motion. We will use the example of the tractor and crate to develop the necessary scientific language to describe its motion. In studying the motion of objects, you need to use scientific terms carefully as the meaning of words used in Physics often has a different meaning to the way they are used in everyday speech. 6

The language you will learn can be used to describe the motion of galaxies, stars, planets, comets, satellites, rockets, golf balls, cars, microscopic objects, and so on. Principles, laws, theories and models will be given to help us understand the physical world surrounding us and to make predictions using mathematical models. MODELS AND REAL-LIFE SITUATIONS We will often develop simple models that are not necessarily a good approximation to the real world but none the less can be quite useful. A physicist is a person who can take a complex situation and begin to understand its working by first creating a simple model which ignores many aspects of the real situation, but by doing this, they can start to develop an understanding of the situation. 7

In our tractor / crate example to simplify the situation we could make the following simplification and/or approximations: The mass of the rope connecting the tractor and crate can be ignored. The crate is pulled along a frictionless surface. A constant force is applied to the crate by the rope connecting the tractor to the crate. Ignore the physical dimensions of the crate and tractor and treat them as point particles. An object or sets of objects can be classified as a System. Identifying the System of interest and focusing our attention on the System makes it easy to apply the appropriate physical principles. To improve your physics ability throughout this course it is essential that you learn how to visualise and simplify a physical situation. Often a starting point to answering an examination question is to draw a scientific but simple diagram of the physical situation. People who are good at physics do this automatically. Those that struggle with physics and think it is a hard subject do so because they can t visualise and then draw an appropriate annotated diagram of the situation as part of their answer. 8

Fig. 2A. The System is the crate and is shown as a dot in a scientific annotated diagram. To identify the System a circle is often drawn around the object or objects. Fig. 2B. The System is the tractor and is shown as a dot in a scientific annotated diagram. Fig. 2C. The System is the tractor and crate and is shown as a dot in a scientific annotated diagram. 9

PHYSICAL QUANTITIES Physical quantities like mass where a single number gives a measurement of the quantity and add together as simple numbers are called scalar quantities. Other examples of scalar quantities include time, temperature, volume, density, energy, work, power and electric charge. Physical quantities that require for their complete specification a positive scalar quantity (magnitude) and a direction are called vector quantities. Examples of vector quantities include displacement, velocity, acceleration, force, momentum, electric fields and magnetic fields. Physical quantities are represented by symbols and often the symbol contains a subscript. Subscripts are usually numbers and / or letters but also words can be used. The symbol m can be used for the physical quantity and the subscript used to identify the System Mass of tractor Mass of crate m tractor m crate Mass of System (tractor and crate) mcrate mtractor 10

A vector quantity is written as a bold symbol or a small arrow above the symbol. Often a curved line draw under the symbol is used when the vector is hand written. It is most important that you develop the skill of using appropriate symbols with subscripts to identify physical quantities. Events A useful idea in describing the motion of a System is to use the term Event. For example, to say that the System is located at position (x, y) at time t defines an Event. Event 1: At 2:00 pm the tractor was at the northern end of the paddock. t1 2 : 00 pm x1 0 m y1 100 m Event 2: At 5:00 pm the tractor was at the centre of the paddock. t2 5 : 00 pm x2 0 m y2 0 m 11

The symbol t gives the time, symbol x gives the X position of the tractor and gives y the Y position. The subscript identifies the instance (Event) when the measurements of the location of the tractor were made. So, subscripts are used to identify the System or Event. Double subscript may be used to define a System and Event or the relative values and their interpretation depend upon the physical situation. When using double subscripts, you need to be very careful of their meaning s QP position of tractor at point Q relative to the position P s A1 displacement of particle A at the time of Event 1 s A2 displacement of particle A at the time of Event 2 F AB force of System B acting on System A 12

Units A unit must always be attached to a physical quantity. You must know the S.I. units for all physical quantities that you encounter during your Physics course. You should possess the necessary skills to change one set of units to another. Physical quantities should be written in the following format Review: Significant Figures Change of unit Convert 37.6 km.h -1 to? m.s -1 1 km = 10 3 m 1 h = 3.6x10 3 s 1 km.h -1 = 10 3 / (3.6x10 3 ) m.s -1 = (1/3.6) m.s -1 37.6 km.h -1 = (37.6/3.6) m.s -1 = 10.4 m.s -1 answer written to 3 significant figures Review: Change of Unit 13

You should watch a Korean historical drama (YouTube) Jang Youngil The drama is about the life of a real 15 th century scientist, Jang Youngsil (Jang Yeong-Sil). The drama gives an excellent account of the conflicts between science, technology, politics, society, superstition, and culture. The rich could control the poor by keeping them ignorant and uneducated. It is well worth your while to watch the many episodes taking note of the struggles of scientists and people who had independent thoughts from the ruling classes. The drama goes a long way to explain why there were very few scientific and technological advanced in the eastern cultures since the 15 th century until the intervention of the western powers in the 19 th century. VISUAL PHYSICS ONLINE If you have any feedback, comments, suggestions or corrections please email: Ian Cooper School of Physics University of Sydney ian.cooper@sydney.edu.au 14