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📚 College Physics 2e
Chapters ▾
1 Introduction: The Nature of Science and Physics2 Kinematics3 Two-Dimensional Kinematics4 Dynamics: Force and Newton's Laws of Motion5 Further Applications of Newton's Laws: Friction, Drag, and Elasticity6 Uniform Circular Motion and Gravitation7 Work, Energy, and Energy Resources8 Linear Momentum and Collisions9 Statics and Torque10 Rotational Motion and Angular Momentum11 Fluid Statics12 Fluid Dynamics and Its Biological and Medical Applications13 Temperature, Kinetic Theory, and the Gas Laws14 Heat and Heat Transfer Methods15 Thermodynamics16 Oscillatory Motion and Waves17 Physics of Hearing18 Electric Charge and Electric Field19 Electric Potential and Electric Field20 Electric Current, Resistance, and Ohm's Law21 Circuits and DC Instruments22 Magnetism23 Electromagnetic Induction, AC Circuits, and Electrical Technologies24 Electromagnetic Waves25 Geometric Optics26 Vision and Optical Instruments27 Wave Optics28 Special Relativity29 Quantum Physics30 Atomic Physics31 Radioactivity and Nuclear Physics32 Medical Applications of Nuclear Physics33 Particle Physics34 Frontiers of Physics

Chapter 7: Work, Energy, and Energy Resources

A field with four wind turbines and the Sun setting in the background.
Figure 7.1 How many forms of energy can you identify in this photograph of a wind farm in Iowa?How many forms of energy can you identify in this photograph of a wind farm in Iowa? (credit: Jürgen from Sandesneben, Germany, Wikimedia Commons)

Energy plays an essential role both in everyday events and in scientific phenomena. You can no doubt name many forms of energy, from that provided by our foods, to the energy we use to run our cars, to the sunlight that warms us on the beach. You can also cite examples of what people call energy that may not be scientific, such as someone having an energetic personality. Not only does energy have many interesting forms, it is involved in almost all phenomena, and is one of the most important concepts of physics. What makes it even more important is that the total amount of energy in the universe is constant. Energy can change forms, but it cannot appear from nothing or disappear without a trace. Energy is thus one of a handful of physical quantities that we say is conserved.

Adapted from College Physics 2e by OpenStax (openstax.org), licensed under CC BY-NC-SA 4.0. Changes were made. License: CC-BY-NC-SA-4.0.