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Precalculus Module 4, Topic B, Lesson 10: Teacher
Precalculus Module 4, Topic B, Lesson 10: Teacher

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... as particles and define the two cars as the system. This is an isolated system, so its total momentum is conserved in the collision. The cars stick together, so this is a perfectly inelastic collision. FIGURE 9.23 shows a visual overview. We’ve chosen to let the 2.0 ´ 104 kg car (car 1) start ...
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physics - North Stonington Public Schools

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... energy, energy can't just disappear. When work is done on a toy train, the energy supplied is converted into kinetic energy (and some internal energy when friction is taken into account), yet a suitcase placed on a luggage rack is obviously stationary. So where has the energy gone? This question may ...
Copyright © 2010 Pearson Canada Inc., Toronto, Ontario. All rights
Copyright © 2010 Pearson Canada Inc., Toronto, Ontario. All rights

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AP Test Free Response Questions

10. Center of Mass A) Overview B) Systems of Particles and the
10. Center of Mass A) Overview B) Systems of Particles and the

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Classical central-force problem



In classical mechanics, the central-force problem is to determine the motion of a particle under the influence of a single central force. A central force is a force that points from the particle directly towards (or directly away from) a fixed point in space, the center, and whose magnitude only depends on the distance of the object to the center. In many important cases, the problem can be solved analytically, i.e., in terms of well-studied functions such as trigonometric functions.The solution of this problem is important to classical physics, since many naturally occurring forces are central. Examples include gravity and electromagnetism as described by Newton's law of universal gravitation and Coulomb's law, respectively. The problem is also important because some more complicated problems in classical physics (such as the two-body problem with forces along the line connecting the two bodies) can be reduced to a central-force problem. Finally, the solution to the central-force problem often makes a good initial approximation of the true motion, as in calculating the motion of the planets in the Solar System.
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