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Lecture series from Conceptual Physics, 8th Ed.

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Presentation on theme: "Lecture series from Conceptual Physics, 8th Ed."— Presentation transcript:

1 Lecture series from Conceptual Physics, 8th Ed.

2 Copernicus, Brahe, and Kepler p142
Used Brahe’s data to develop mathematical models of the motions of the planets. Thought he would gather some data before shooting off his mouth about his heliocentric ideas. Which was probably a good idea seeing as how his nose had already been cut off in a duel. (He was rich and threw really gnarly parties so he got away with a lot.) Speculated that the sun was the center of the solar system.

3 Kepler’s Laws p143 First he translated Brahe’s data from Earth based reference to what would be seen by a stationary observer outside the solar system. His laws of planetary motion are: 1. Planets move in ellipses. 2. The “equal areas” thing. 3. T2 proportional to R3 Fantastic stuff, but he didn’t know about gravity, didn’t apply “inertia”, didn’t know why ellipses… BUT, he was right because he had good data.

4 Newton’s Law of Universal Gravitation p144
-knew that inertia kept the planets moving. -the force acting on the planets caused them to curve. -from looking at Kepler’s stuff, he knew the force emanated from the sun. (He deduced gravity.) -he also deduced that the forced decreased with the square of the distance. -the apple thing reminded him that gravity acts between masses and therefore objects in orbit are falling around their primaries. Here it is gang!! Gm1m2 Fg = d2

5 The Universal Gravitational Constant, G p145
F d2 G = = 6.67x10-11 Nm2/kg2 m1m2 An interesting example: How much does the earth mass? Imagine an object on the surface of the earth. From F=Gmemo/d2 mog = Gmemo/d2 g d2 (9.8) (6.4x106)2 So, me = = = 6.0x1024kg G (6.67x10-11)

6 Gravity and Distance: The Inverse-Square Law p147
Weight decreases as person climbs.

7 Weight and Weightlessness p149
Fig Your weight equals the force with which you press against the floor.

8 More Weightlessness Both people are in a gravitational field. In fact. Gravity does not produce weight! The floor produces weight.

9 Ocean Tides p150 Equal forces to the right means Jell-O ball stays spherical. Forces shown here cause left side to lag behind. The left side is further from moon and is not pulled as strongly toward moon.

10 More on Tides F = G m m / d2 This planet has bigger tides because “delta” F is greater. Smaller “delta” F means smaller tides. “Delta” F refers to the difference in forces at the front and back of the planet.

11 Spring tides: Neap tides:
The earth’s tilt means that this person has a lower high tide than this person. Tides in the Earth and the atmosphere work the same way.

12 Tides on the Moon p154 Why does the moon always face us?
The key thing is that the moon acts like a pendulum. This part of the moon swings back and forth trying to line up with the Earth.

13 The Gravitational Field Inside a Planet p155
First, the outside field lines: Now, the inside: Last, the in and the out -side

14 Einstein’s Theory of Gravitation p157
Albert says that the moon is NOT pulled to the Earth. The moon curves because the surface it travels on is tilted toward the Earth.

15 Black Holes p157 Their gravitational field is so strong that even light can not escape! Because of F=Gmm/d2 When the star collapses to ½ its radius, Supy’s weight quadruples. When the star crushes its matter to a few hundred kilometers, that may be the last we see of it. A collapsing star with Superman standing on its surface. Things orbit it and spiral inward. Only gravity, charge and angular momentum remain.

16 Universal Gravitation p 159
As far out as we can see, matter seems to obey Newton’s law of gravitation: F=Gmm/d2. Neptune and Pluto were discovered by using the law. The activities of distant galaxies seem to obey the law. BUT, the universe is expanding too fast!! To be continued.


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