About This Chapter
How It Works:
- Identify the lessons in Prentice Hall Conceptual Physics' Universal Gravitation chapter with which you need help.
- Find the corresponding video lessons within this companion course chapter.
- Watch fun videos that cover the universal gravitation topics you need to learn or review.
- Complete the quizzes to test your understanding.
- If you need additional help, rewatch the videos until you've mastered the material or submit a question for one of our instructors.
Students will learn:
- Law of universal gravitation
- Newton's formula for the force of gravity
- Earth's gravitational pull and its applications
- Types, causes and effects of tides
- Schwarzschild black holes and the event horizon
- Big Bang theory and the origin of the universe
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1. Sir Isaac Newton And Astronomy
This lesson will teach you about Newton's laws of motion and universal gravitation as well as why the moon doesn't fly off into space and why it doesn't crash into the Earth.
2. The Law of Universal Gravitation: Definition, Importance & Examples
Gravity is what pulls us toward Earth, but it's also what pulls Earth toward us. This is explained by the law of universal gravitation, which describes how all objects in the universe have this important force between them.
3. Isaac Newton's Formula for the Force of Gravity: Definition & Example
Watch this video lesson and you will see how you can calculate the force of attraction between two objects. Learn why our planets don't spin themselves out of orbit around the sun.
4. Gravitational Pull of the Earth: Definition & Overview
Earth's gravitational pull is often misunderstood, but without it, life on Earth would be impossible. In this lesson, we'll define the gravitational pull and give some examples of how it is used. A quiz is provided to test your understanding.
5. What Are Tides? - Causes & Effects
Tides rise and fall under the influence of the gravitational pull of the moon and sun. Learn about different tides, why they are predictable and their effects on coastal regions of the world.
6. Black Holes: the Event Horizon and Schwarzschild Radius
This lesson describes the event horizon and the Schwarzschild radius, including their implications on the gravitational attraction a black hole exerts on the universe around it.
7. Origins of the Universe: The Big Bang and Expanding & Contracting Universes
Students will learn the origins of the universe, the Big Bang theory, the timeline of the universe, how the universe is still expanding to this day, and what astronomers expect the universe to look like in the future.
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Other chapters within the Prentice Hall Conceptual Physics: Online Textbook Help course
- Chapter 1: About Science
- Chapter 2: Mechanical Equilibrium
- Chapter 3: Newton's First Law of Motion-Inertia
- Chapter 4: Linear Motion
- Chapter 5: Projectile Motion
- Chapter 6: Newton's Second Law of Motion - Force and Acceleration
- Chapter 7: Newton's Third Law of Motion - Action and Reaction
- Chapter 8: Momentum
- Chapter 9: Energy
- Chapter 10: Circular Motion
- Chapter 11: Rotational Equilibrium
- Chapter 12: Rotational Motion
- Chapter 14: Satellite Motion
- Chapter 15: Special Relativity - Space and Time
- Chapter 16: Relativity - Momentum, Mass, Energy, and Gravity
- Chapter 17: The Atomic Nature of Matter
- Chapter 18: Solids
- Chapter 19: Liquids
- Chapter 20: Gases
- Chapter 21: Temperature, Heat, and Expansion
- Chapter 22: Heat Transfer
- Chapter 23: Change of Phase
- Chapter 24: Thermodynamics
- Chapter 25: Vibrations and Waves
- Chapter 26: Sound
- Chapter 27: Light
- Chapter 28: Color
- Chapter 29: Reflection and Refraction
- Chapter 30: Lenses
- Chapter 31: Diffraction and Interference
- Chapter 32: Electrostatics
- Chapter 33: Electric Fields and Potential Energy
- Chapter 34: Electric Current
- Chapter 35: Electric Circuits
- Chapter 36: Magnetism
- Chapter 37: Electromagnetic Induction
- Chapter 38: The Atom and the Quantum
- Chapter 39: The Atomic Nucleus and Radioactivity
- Chapter 40: Nuclear Fission and Fusion