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Conceptual Physics Notes on Chapter 12 UniversalGravitation.

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Presentation on theme: "Conceptual Physics Notes on Chapter 12 UniversalGravitation."— Presentation transcript:

1 Conceptual Physics Notes on Chapter 12 UniversalGravitation

2 Universal Gravitation Isaac Newton and the falling apple --- Isaac Newton and the falling apple --- Newton was under a apple tree when a apple hit him on the head and he got an idea that changed the world. Newton was under a apple tree when a apple hit him on the head and he got an idea that changed the world. What was his GREAT idea? …. What was his GREAT idea? ….

3 Universal Gravitation Isaac Newton and the falling moon --- Isaac Newton and the falling moon --- Newton compared a falling Newton compared a falling apple to the moon in orbit around the Earth. He said that the moon fell toward the earth as fast as it moved in a straight line - tangential velocity.

4 Universal Gravitation Newton “generalized” Newton “generalized” his moon findings to ALL objects, and said that ALL objects in the universe attract each other. (Law of Universal Gravitation)

5 Universal Gravitation NEWTON’S LAW OF UNIVERSAL GRAVITATION Every object attracts every other object with a force directly proportional to the mass of each object, but decreases as the square of the distance between masses. Every object attracts every other object with a force directly proportional to the mass of each object, but decreases as the square of the distance between masses. F ~ m 1 m 2 F ~ m 1 m 2 d 2 d 2

6 Universal Gravitation We want the force to equal, so we have to add a constant to the equation. We want the force to equal, so we have to add a constant to the equation. G = 6.67 x 10 -11 kg (Note that the force of gravity is very weak) Henry Cavendish measured G 150 years after Newton’s Law listed above and was said to have WEIGHED the world! Henry Cavendish measured G 150 years after Newton’s Law listed above and was said to have WEIGHED the world!

7 Universal Gravitation

8 So the equation becomes: So the equation becomes: F = G m 1 m 2 d 2 d 2

9 Universal Gravitation Inverse-square Law: The brightness of an object decreases dramatically as we move farther from the source. The result is due to a larger "sphere" of influence. Light from a source like a star shines in all directions, to the area of illumination increases with increasing distance so the total brightness thins out.

10 Universal Gravitation

11 EXAMPLES: 3 2 = 9 but 1/3 2 = 1/9 3 2 = 9 but 1/3 2 = 1/9 2d 2 = 4dbut 1/2d 2 = 1/4d 2d 2 = 4dbut 1/2d 2 = 1/4d (Note that as the distance gets LARGER, the overall force gets smaller )


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