“Dynamics by Hibbeler,” Dr. S. Nasseri, MET Department, SPSU 1 RECTILINEAR KINEMATICS: ERRATIC MOTION Today’s Objectives: Students will be able to: Determine.
Chapter 8 GravitationNEW
RECTILINEAR KINEMATICS: ERRATIC MOTION (Section 12.3) Today’s Objectives: Students will be able to determine position, velocity, and acceleration of a.
W = F x d
7.1. 7.2 7.3 7.4 W = F x d W = F x 0 = 0 7.5 Power = work / time PE KE PE = mgh KE = ½ mv 2.
Excitation of Supernova Remnants by Twisting of the Neutron Star Dipole Magnetic Flux
LOM Assignment
University Physics: Mechanics
2 Excitation of Supernova Remnants by Twisting of the Neutron Star Dipole Magnetic Flux Stirling Colgate, LANL with Hui Li, LANL & Ken Fowler, UC Berkley,
