
2003 The McGraw-Hill Companies, Inc. All rights reserved. 14
... be described. Result obtained are also applicable to a system of rigidly connected particles, i.e., a rigid body. ...
... be described. Result obtained are also applicable to a system of rigidly connected particles, i.e., a rigid body. ...
C-Circular-Kinematics-Dynamics-Unit
... By the end of the unit, students will be able to… 1. distinguish between circular (“translational;” “tangential”) and rotational motion. 2. perform measurements and calculations involving period and frequency of rotating objects and objects moving in circular motion. 3. analyze the angular displacem ...
... By the end of the unit, students will be able to… 1. distinguish between circular (“translational;” “tangential”) and rotational motion. 2. perform measurements and calculations involving period and frequency of rotating objects and objects moving in circular motion. 3. analyze the angular displacem ...
Chapter 5
... 4. A free particle that has a mass of 10-19 kg is initially at rest. At some point it is accelerated by a force. After the particle travels 10 m, it has a speed of 103 m/s. What is the magnitude of the accelerating force? Hint 1/Comment: Newton's second law of motion states that an object with mass ...
... 4. A free particle that has a mass of 10-19 kg is initially at rest. At some point it is accelerated by a force. After the particle travels 10 m, it has a speed of 103 m/s. What is the magnitude of the accelerating force? Hint 1/Comment: Newton's second law of motion states that an object with mass ...
Chap. 13: Gravitation
... The starship Enterprise (mass m) is investigating a new star of mass M1, and is holding position a distance Y from the star. There is another star of mass M2 a distance Y from the first along a line perpendicular to that connecting the Enterprise with the first star. Suppose the Enterprise experienc ...
... The starship Enterprise (mass m) is investigating a new star of mass M1, and is holding position a distance Y from the star. There is another star of mass M2 a distance Y from the first along a line perpendicular to that connecting the Enterprise with the first star. Suppose the Enterprise experienc ...
pp\momentum - Dr. Robert MacKay
... Conservation of Momentum Collisions Explosions Elastic Collisions ...
... Conservation of Momentum Collisions Explosions Elastic Collisions ...
Tuesday, Oct. 28, 2014
... For a solid sphere as shown in the figure, calculate the linear speed of the CM at the bottom of the hill and the magnitude of linear acceleration of the CM. Solve this problem using Newton’s second law, the dynamic method. ...
... For a solid sphere as shown in the figure, calculate the linear speed of the CM at the bottom of the hill and the magnitude of linear acceleration of the CM. Solve this problem using Newton’s second law, the dynamic method. ...
Unit 1: The Chemistry of Life.docx
... mass of the planet are given. Use Newton's Universal Law and Newton's Second Law of Motion to express weight and other mathematical concepts for any location in the universe. Determine mass from weight or weight from mass where a value for the acceleration due to gravity is known Draw a free-body di ...
... mass of the planet are given. Use Newton's Universal Law and Newton's Second Law of Motion to express weight and other mathematical concepts for any location in the universe. Determine mass from weight or weight from mass where a value for the acceleration due to gravity is known Draw a free-body di ...
Lec9
... Which leads to an expression for the gravitational potential energy defined purely as a scalar of the inverse distance away from the source. ...
... Which leads to an expression for the gravitational potential energy defined purely as a scalar of the inverse distance away from the source. ...
Physics
... When a tetherball is whirling around the pole, the net force is directed (A) toward the top of the pole (B) toward the ground (C) horizontally away from the pole (D) horizontally toward the pole You are standing in a bus that makes a sharp left turn. Which of the following is true? (A) you lean to t ...
... When a tetherball is whirling around the pole, the net force is directed (A) toward the top of the pole (B) toward the ground (C) horizontally away from the pole (D) horizontally toward the pole You are standing in a bus that makes a sharp left turn. Which of the following is true? (A) you lean to t ...
Modified Newtonian dynamics

In physics, modified Newtonian dynamics (MOND) is a theory that proposes a modification of Newton's laws to account for observed properties of galaxies. Created in 1983 by Israeli physicist Mordehai Milgrom, the theory's original motivation was to explain the fact that the velocities of stars in galaxies were observed to be larger than expected based on Newtonian mechanics. Milgrom noted that this discrepancy could be resolved if the gravitational force experienced by a star in the outer regions of a galaxy was proportional to the square of its centripetal acceleration (as opposed to the centripetal acceleration itself, as in Newton's Second Law), or alternatively if gravitational force came to vary inversely with radius (as opposed to the inverse square of the radius, as in Newton's Law of Gravity). In MOND, violation of Newton's Laws occurs at extremely small accelerations, characteristic of galaxies yet far below anything typically encountered in the Solar System or on Earth.MOND is an example of a class of theories known as modified gravity, and is an alternative to the hypothesis that the dynamics of galaxies are determined by massive, invisible dark matter halos. Since Milgrom's original proposal, MOND has successfully predicted a variety of galactic phenomena that are difficult to understand from a dark matter perspective. However, MOND and its generalisations do not adequately account for observed properties of galaxy clusters, and no satisfactory cosmological model has been constructed from the theory.