M1.4 Dynamics
									
... same horizontal track, collide. The mass of A is 800 kg and the mass of B is m kg. Immediately before the collision the speed of A is 5 ms–1 and the speed of B is 4 ms–1. Immediately after the collision the trucks are joined together and move with the same speed, 1 ms–1. The direction of motion of A ...
                        	... same horizontal track, collide. The mass of A is 800 kg and the mass of B is m kg. Immediately before the collision the speed of A is 5 ms–1 and the speed of B is 4 ms–1. Immediately after the collision the trucks are joined together and move with the same speed, 1 ms–1. The direction of motion of A ...
									Lecture 14ba
									
... Section 8-4: Torque • Newton’s 1st Law (rotational language version): “A rotating body will continue to rotate at a constant angular velocity unless an external TORQUE acts.” • Clearly, to understand this, we need to define the concept of TORQUE. • Newton’s 2nd Law (rotational language version): Al ...
                        	... Section 8-4: Torque • Newton’s 1st Law (rotational language version): “A rotating body will continue to rotate at a constant angular velocity unless an external TORQUE acts.” • Clearly, to understand this, we need to define the concept of TORQUE. • Newton’s 2nd Law (rotational language version): Al ...
									Questions - TTU Physics
									
... b. Derive expressions for the generalized momenta. (Caution! These are NOT simply the mass times a velocity component!). (6 points) c. Write an expression for the Hamiltonian for the system. This is messy, but doable. Go as far as you can on this! (7 points) d. Derive the equations of motion using H ...
                        	... b. Derive expressions for the generalized momenta. (Caution! These are NOT simply the mass times a velocity component!). (6 points) c. Write an expression for the Hamiltonian for the system. This is messy, but doable. Go as far as you can on this! (7 points) d. Derive the equations of motion using H ...
									Solutions for class #1 from Yosunism website Problem 4.
									
... For normal mode oscillations, there is always a symmetric mode where the masses move together as if just one mass. There are three degrees of freedom in this system, and ETS is nice enough to supply the test- taker with two of them. Since the symmetric mode frequency is not listed, choose choice it! ...
                        	... For normal mode oscillations, there is always a symmetric mode where the masses move together as if just one mass. There are three degrees of freedom in this system, and ETS is nice enough to supply the test- taker with two of them. Since the symmetric mode frequency is not listed, choose choice it! ...
									Answers - Dean Baird`s Phyz Home Page
									
... For the moment, each of these words is taboo—you may not use any of them in your responses below until you are specifically asked to do so. This is important! 1. Push down on the table with your hand. a. The table feels the downward push of your hand. What do you feel? ...
                        	... For the moment, each of these words is taboo—you may not use any of them in your responses below until you are specifically asked to do so. This is important! 1. Push down on the table with your hand. a. The table feels the downward push of your hand. What do you feel? ...
									C f dr
									
... Independence of Paths We assume that D is open, which means that for every point P in D there is a disk with center P that lies entirely in D. (So D doesn’t contain any of its boundary points.) In addition, we assume that D is connected: this means that any two points in D can be joined by a path t ...
                        	... Independence of Paths We assume that D is open, which means that for every point P in D there is a disk with center P that lies entirely in D. (So D doesn’t contain any of its boundary points.) In addition, we assume that D is connected: this means that any two points in D can be joined by a path t ...
									UNIT 2
									
... rough oak surface is attached by a light string that passes over a light, frictionless pulley to a hanging 4.0-kg mass, Y, as shown. The magnitude of the force of friction on block X is 24 N. ( = 9.81 m/s2 [down]) Which of the following statements is correct? a. The acceleration of block X to the ri ...
                        	... rough oak surface is attached by a light string that passes over a light, frictionless pulley to a hanging 4.0-kg mass, Y, as shown. The magnitude of the force of friction on block X is 24 N. ( = 9.81 m/s2 [down]) Which of the following statements is correct? a. The acceleration of block X to the ri ...
									8. Newton`s Law Gravitation Rev.nb
									
... gravity is described by Newton's Law of gravitation or the modification called General Relativity due to Einstein. The electromagnetic force will be studied next semester and it involves the electric force which you know of as static electricity and the magnetic force which is involved in the operat ...
                        	... gravity is described by Newton's Law of gravitation or the modification called General Relativity due to Einstein. The electromagnetic force will be studied next semester and it involves the electric force which you know of as static electricity and the magnetic force which is involved in the operat ...
									Slides - Powerpoint - University of Toronto Physics
									
... • Similarly, since FG = GMm/r2, the force on the ocean further from the moon will be less, so it will accelerate less than the rest of the Earth, remaining behind, forming a bulge. • In general, tidal effects tend to stretch objects both toward and away from the object causing the tides. ...
                        	... • Similarly, since FG = GMm/r2, the force on the ocean further from the moon will be less, so it will accelerate less than the rest of the Earth, remaining behind, forming a bulge. • In general, tidal effects tend to stretch objects both toward and away from the object causing the tides. ...
									Slides - PDF - University of Toronto Physics
									
... • They contain important ideas and questions from your reading. • Due to time constraints, I was probably not able to show all the slides during class. • They are all posted here for completeness. ...
                        	... • They contain important ideas and questions from your reading. • Due to time constraints, I was probably not able to show all the slides during class. • They are all posted here for completeness. ...
									Motion - ILM.COM.PK
									
... If acceleration due to gravity is the same for all objects, regardless of mass, then all objects should fall at the same rate. Does a leaf fall as fast as an acorn? ...
                        	... If acceleration due to gravity is the same for all objects, regardless of mass, then all objects should fall at the same rate. Does a leaf fall as fast as an acorn? ...
									Physics 231 Topic 8: Gravitation Wade Fisher October 24-26 2012
									
... space if it weren’t for gravity providing the centripetal force. MSU Physics 231 Fall 2012 ...
                        	... space if it weren’t for gravity providing the centripetal force. MSU Physics 231 Fall 2012 ...
									Newton`s 3rd Law
									
... A common misconception is that a rocket is propelled by the impact of exhaust gases against the atmosphere. In fact, in the early 1900s before the advent of rockets, many people thought that sending a rocket to the moon was impossible because of the absence of an atmosphere for the rocket to push a ...
                        	... A common misconception is that a rocket is propelled by the impact of exhaust gases against the atmosphere. In fact, in the early 1900s before the advent of rockets, many people thought that sending a rocket to the moon was impossible because of the absence of an atmosphere for the rocket to push a ...
Newton's theorem of revolving orbits
In classical mechanics, Newton's theorem of revolving orbits identifies the type of central force needed to multiply the angular speed of a particle by a factor k without affecting its radial motion (Figures 1 and 2). Newton applied his theorem to understanding the overall rotation of orbits (apsidal precession, Figure 3) that is observed for the Moon and planets. The term ""radial motion"" signifies the motion towards or away from the center of force, whereas the angular motion is perpendicular to the radial motion.Isaac Newton derived this theorem in Propositions 43–45 of Book I of his Philosophiæ Naturalis Principia Mathematica, first published in 1687. In Proposition 43, he showed that the added force must be a central force, one whose magnitude depends only upon the distance r between the particle and a point fixed in space (the center). In Proposition 44, he derived a formula for the force, showing that it was an inverse-cube force, one that varies as the inverse cube of r. In Proposition 45 Newton extended his theorem to arbitrary central forces by assuming that the particle moved in nearly circular orbit.As noted by astrophysicist Subrahmanyan Chandrasekhar in his 1995 commentary on Newton's Principia, this theorem remained largely unknown and undeveloped for over three centuries. Since 1997, the theorem has been studied by Donald Lynden-Bell and collaborators. Its first exact extension came in 2000 with the work of Mahomed and Vawda.