Return to Table of Contents C HAPTER . 10 Static Equilibrium Giant sequoias up to 100 m high stand in static equilibrium. I n the last chapter we saw how rotation can result…

1.LETTERdoi:10.1038/nature12917A millisecond pulsar in a stellar triple system S. M. Ransom1, I. H. Stairs2, A. M. Archibald3,4, J. W. T. Hessels3,5, D. L. Kaplan6,7, M.…

Slide 1 6. Centripetal force F = ma 1 Slide 2 Example: A stone of mass m sits at the bottom of a bucket. A string is attached to the bucket and the whole thing is made to…

Slide 1 Chapter 12 Gravitation Slide 2 Theories of Gravity Newton’s Einstein’s Slide 3 Newton’s Law of Gravitation any two particles m 1, m 2 attract each other F g…

PHYS 1443 â Section 001 Lecture #13 Thursday, June 22, 2006 Dr. Jaehoon Yu CM and the Center of Gravity Fundamentals on Rotational Motion Rotational Kinematics Relationship…

Gravitation In galaxy M31, one very similar to our own, there is almost certainly a super massive black hole at the center. This very massive object supplies an enormous…

PHYS 1441 â Section 004 Lecture #15 Wednesday, Mar. 24, 2004 Dr. Jaehoon Yu Center of Mass (CM) CM of a group of particles Fundamentals on Rotation Rotational Kinematics…

PHYS 1443 â Section 001 Lecture #13 Thursday, June 21, 2007 Dr. Jaehoon Yu Fundamentals of Rotational Motions Rotational Kinematics Relationship between angular and linear…

PHYSICS 231 Lecture 35: interference & sound Remco Zegers Question hours:Monday 9:15-10:15 Helproom example A pendulum with a length of 4 m and a swinging mass of 1 kg…