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Chapter 10 - UCF Physics
Chapter 10 - UCF Physics

... Four small spheres are fastened to the corners of a frame of negligible mass lying in the xy plane (Fig. 10.7). Two of the spheres have mass m = 3.1kg and are a distance a = 1.7 m from the origin and the other two have mass M = 1.4 kg and are a distance a = 1.5 m from the origin. (a) If the rotatio ...
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... forces acting on the particles of the system. The forces are not specified as conservative or non-conservative. There is no indication if the forces are constant or not. The only requirement is that the forces must be internal to the system.  This gives a hint about the power of this new model. ...
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AP Physics I Course Syllabus_Student Version

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Chapter4.2 - Department of Physics & Astronomy

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momentum - Sharyland High School

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Chapter 14 - Illinois State University

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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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