Physical Science
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  • Refs.
  • Ch. 1
    • 1.1 - The Scientific Method
    • 1.2 - Measuring
    • 1.3 - The Metric System
    • 1.4 - Unit Analysis
    • 1.5 - Why Measuring is Important!
    • Ch. 1 Summary
  • Ch. 2
    • 2.1 - What Causes Objects to Move?
    • 2.2 - What is a Force?
    • 2.3 Practical Applications of Newton's First Law
    • 2.4 - Equilibrium
    • Ch. 2 Summary
  • Ch. 3
    • 3.1 - Relative Motion
    • 3.2 - Speed
    • 3.3 - Graphing
    • 3.4 - Speed vs. Velocity
    • 3.5 - Acceleration
    • 3.6 - Free Fall
    • Ch. 3 Summary
  • Ch. 4
    • 4.1 Newton's Second Law of Motion
    • 4.2 Mass vs. Weight
    • 4.3 Free Body Diagrams Revisited
    • 4.4 Terminal Velocity
    • 4.5 Pressure
    • 4.6 Newton's Third Law of Motion
    • Chapter 4 Summary
  • Ch. 5
    • 5.1 - Energy
    • 5.2 - Gravitational Potential Energy
    • 5.3 - Kinetic Energy
    • 5.4 - Energy Conversion and Work
    • 5.5 - Riding your bike up a hill
    • 5.6 - Power
    • Chapter 5 Summary
  • Ch. 6
    • 6.1 - Simple Machines Overview
    • 6.2 - Inclined Planes
    • 6.3 - Levers
    • 6.4 - Wheel and Axle
    • 6.5 - Pulleys
    • Chapter 6 Summary
  • Ch. 7
    • Chapter 7 Pre-test
    • 7.1 - History of the Atom
    • 7.2 - Protons, Neutrons, Electrons
    • 7.3 - From Where did all the Elements Come?
    • 7.4 - Atomic Symbols
    • 7.5 - Isotopes
    • 7.6 - Ions
    • 7.7 - Bohr Model Revisited
    • Ch. 7 Summary
  • Ch. 8
    • Chapter 8 Pre test
    • 8.1 - The Periodic Table
    • 8.2 - Periodic Trends
    • Chapter 8 Summary
  • Ch. 9
    • 9.1 - Molecules and Molecular Formulae
    • 9.2 - Lewis Dot Structures
    • 9.3 - Electronegativity
    • 9.4 - Diatomic Molecules
    • 9.5 - Molecular Shapes
    • 9.6 - Polar and Non-polar molecules
    • 9.7 - Properties Due to Polarity
    • Chapter 9 Summary
  • App.
    • App. I - Setup for Lab Reports

5.2 - Gravitational Potential Energy

Picture
If someone held a brick over your head, you would probably be a little nervous, worrying that he may drop it. From experience you know that when released in a gravitational field, objects accelerate down. If the person were to raise the brick higher, you would be even more nervous, anticipating that you would be hurt more.

Why would a falling brick hurt you? What properties does it have that can cause it to apply a force to your head when dropped?

It has mass. One of the most fundamental properties of matter is mass. If the brick were half as massive, you might only be half as nervous. If the brick were made of sponge instead of clay, you would not be nearly as concerned.

It has height. The higher the brick is, the more dangerous it is to you.

It is in a gravitational field. If this brick was held over your head while you were orbiting on the Space Shuttle, you wouldn’t be concerned at all. If you were on the moon, you wouldn’t be as concerned. On Earth, you know that everything is pulled down with a strength of 9.8 N/Kg.

These are the three properties of the brick that determine how hard it will hit you in the head. If any of them are made greater, the “Ouch factor” is greater. If any are made smaller, the “Ouch factor” is less. Gravitational Potential Energy (PE) is deter­mined by the object’s mass (m), its height (h) and the gravitational field strength of the earth (g). It is defined as:


Picture
This is potential energy. Since the brick has not yet fallen, the energy is stored in it. The energy has not been realized yet. It can come out when the brick is dropped. The energy will come out as the motion of the brick as it picks up speed. It will also move and heat the air as it goes down.

Picture
Think of it another, safer way. When you are sledding down a hill you are converting one type of energy into others without any loss, any­where, anytime. At the top of the hill you have gravitational potential energy (PE). As you slide down, that potential turns into motion- your velocity increases. Also as you are slid­ing down, the sled is rubbing against the snow and turning some of that potential into heat. The potential at the beginning is equal to the motion, heat and potential energies at the end.

In terms of Units:
Picture
The Joule is named after James Prescott Joule, an English physicist from the mid 1800’s who was one of the scientists to define the Law of Conservation of Energy.  All energy can be mea­sured in Joules.

Another common unit of energy is the calorie. The calorie is defined as the amount of energy needed to raise the temperature of one gram of water one degree Celsius. There are 4.18 J in one calorie.

Picture

5.2 Sample Problems

5.2 Review Questions
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