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This course has recently been updated.  To view the archived version of the course, please go here.

Introduction to Mechanics

Purpose of Course  showclose

Physics 101 is the first course in the Introduction to Physics sequence. In general, the quest of physics is to develop descriptions of the natural world that correspond  closely to actual observations.  Given this definition, the story behind everything in the universe is  one of physics.  In practice,  the field of physics is more often limited to the discovery and refinement of the basic laws that underlie the behavior of matter and energy.  While biology is founded upon physics, in practice, the study of biology generally assumes that the present understanding of physical laws is accurate.  Chemistry is more closely dependent on physics and   assumes that physical laws provide accurate predictions.  Engineering, for the most part, is applied physics. In this course, we will study physics from the ground up, learning the basic principles of physical laws, their application to the behavior of objects, and the use of the scientific method in driving advances in this knowledge.  This first course of the three-course series (the subsequent courses in the series are Introduction to Electromagnetism and Introduction to Modern Physics) will cover the area of physics known as classical mechanics. Classical mechanics is the study of motion based on the physics of Galileo Galilei and Isaac Newton. While mathematics is the language of physics, you will only need to be familiar with high school level algebra, geometry, and trigonometry.  The small amount of additional math and calculus that we need will be developed during the course.

Course Information  showclose

Welcome to PHYS101.  General information on this course and its requirements can be found below.

Primary Resources: This course is comprised of a range of different free online materials.  However, the course makes primary use of the following resources:
  • Massachusetts Institute of Technology: Professor Walter Lewin’s Physics I: Classical Mechanics Video Lectures
  • The textbook to accompany this course is OpenStax College’s College Physics.You may find it helpful to download the PDF version and save  the PDF file as it will be used throughout the entire course. Problems will be assigned from this text. These are extremely important as they will be similar to those on the final exams. Solutions to the problem sets  are available, but it is important that you make every effort to solve the problems before looking at the solutions. Getting the answers is not what is important.  It is more important that you understand how to go about finding the answers in a systematic way. The Student Solutions Manual for College Physics can be found here under Learning Resources.
  • Additional  problems will be assigned from Calculus-Based Physicsby Jeffery W. Schnick. Please feel free to browse this text, but our use of the text will only be for problemsand their solutions. Although there will be no readings assigned from this text, it may be useful to look at the appropriate sections of the text when working the problems, particularly if you get stuck.
  • University of Toronto: Professor David Harrison’s “Physics Flash Animations”
Requirements for Completion: In order to complete this course, you will need to work through each unit and all of its readings and lectures.  You will also need to complete: 
  • The Final Exam
Note that you will only receive an official grade on your Final Exam.  However, in order to adequately prepare for this exam, you will need to work through the problems assigned throughout the course.

In order to “pass” this course, you will need to earn a 70% or higher on the Final Exam. Your score on the exam will be tabulated as soon as you complete it.  If you do not pass the exam, you may take it again.

Time Commitment: This course should take you a total of about 130 hours to complete.  Each unit includes a “time advisory” that lists the amount of time you are expected to spend on it and each of its subunits.  These should help you plan your time accordingly.  It may be useful to take a look at these time advisories and to determine how much time you have over the next few weeks to complete each unit, and then to set goals for yourself.  For example, Unit 1 should take approximately 6.75 hours.  Perhaps you can sit with your calendar and decide to complete subunit 1.1 (a total of 3.75 hours) on Monday night and subunit 1.2 (a total of 3 hours) on Tuesday night.  Unit 2 should take you 13.25 hours to complete. Perhaps you can schedule time to complete subunit 2.1 (a total of 4 hours) on Wednesday  night; subunit 2.2 (a total of 2.75 hours) on Thursday night; etc.

Tips/Suggestions: Take comprehensive notes as you complete the resources in this course.  It may also help to keep the problems you solve in one notebook for easy reference.  These notes will serve as a useful review as you prepare and study for the Final Exam.

Good luck to you in this undertaking you are about to embark on.Upon successful completion of this course, the student will be able to:

Learning Outcomes  showclose

Upon successful completion of this course, the student will be able to:
  • Explain the difference between a theory and a law.
  • Identify the values of the most common metric prefixes.
  • Compare and contrast distance and displacement.
  • Define and distinguish between vector and scalar physical quantities.
  • Solve 1-dinentional kinematics problems.
  • Describe the effects of gravity on an object’s motion.
  • Add and subtract vectors.
  • Separately analyze the horizontal and vertical motions in projectile problems.
  • Determine the net force on an object.
  • Use Newton's second law of motion to analyze dynamic problems.
  • Solve problems involving springs.
  • Compare and contrast the physical properties associated with linear motion and rotational motion.
  • State Newton's law of gravity in words.
  • Solve problems involving planets and satellites.
  • Define the work done on an object by a force.
  • Describe the relationship between work done and the change in kinetic energy.
  • Describe the concept of potential energy and how it relates to work.
  • Solve dynamics problems using conservation of energy.
  • Describe the distinction between renewable and non-renewable energy sources.
  • State Newton's 2nd law in terms of momentum.
  • Use conservation of momentum to solve collision problems.
  • Define the conditions necessary for a rigid body to be in equilibrium.
  • Solve statics problems.
  • Solve kinematics and dynamic problems involving rotational motion.
  • Compare and contrast the dynamics of linear and rotational motion.
  • Apply energy concepts to rotational motion.

Course Requirements  showclose

In order to take this course, you must:
 
√    Have access to a computer.
 
√    Have continuous broadband Internet access.
 
√    Have the ability/permission to install plug-ins or software (e.g., Adobe Reader or Flash).
 
√    Have the ability to download and save files and documents to a computer.
 
√    Have the ability to open Microsoft files and documents (.doc, .ppt, .xls, etc.).
 
√    Have competency in the English language.
 
√    Have read the Saylor Student Handbook.

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