This preview has intentionally blurred sections. Sign up to view the full version.View Full Document
Unformatted text preview: 1 Chap 13 Gravitation Note – this is an outline of the lecture, print this and take notes on it in lecture It is not the and take notes on it in lecture. It is not the complete lecture. You should attend lecture to get the complete notes Images taken from Halliday/Resnick/Walker, Fundamentals of Physics, 7 th Edition, John Wiley and Sons Inc., by permission. Hints 19. The gravitational force must provide the centripetal force to stop mass flying off the surface of the star as it rapidly rotates. 33. a) Remember that U = Gm A m / R where R is the separation of the centers of the two masses. Now apply conservation of energy with the final KE and PE being zero. 56. b) Know from Newton’s 2 nd law that F G = mv 2 / r . Use this to find v . Now find the ratio of kinetic energies. Newton's Law of Gravitation /kg N.m 10 6.67 G e) (attractiv 2 2 11- 2 2 1 × = = r m m G F law? 3 s Newton' satisfy this Does rd Newton’s 3 rd law Pull of Apple on Earth = pull of Earth on apple Newton’s 3 rd law...
View Full Document
This note was uploaded on 04/07/2008 for the course PHYS 213 taught by Professor Oshea during the Spring '08 term at Kansas State University.
- Spring '08