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mcese 104 structural dynamics
mcese 104 structural dynamics

Help Section - AdvancedPlacementPhysicsC
Help Section - AdvancedPlacementPhysicsC

... the statics of rigid bodies. The situation described on the first slide is static as long as the man is not more than one-third of the way up the ladder, because there is no motion. Therefore, the conditions for static equilibrium apply to the situation. What are the static equilibrium conditions? ...
mcese 104 structural dynamics
mcese 104 structural dynamics

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... • You have probably used the word momentum tossed out in everyday life – but not necessarily 100% correctly. • With a neighbor discuss where you have heard momentum talked about, and try to figure out from that what the average person probably thinks momentum means. ...
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... My friend Zodork comes from another planet. In fact, his home planet has two suns. In other words, Zodork's world is situated in a binary star system. Each of the two stars in this system has a mass M. Each star moves in a circle of radius R in such a fashion that the other star is always situated e ...
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one-body diagrams and contact forces
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Prep 1 - Physics | Oregon State University
Prep 1 - Physics | Oregon State University

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Lec12
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... the flow of air through a jet engine. The principle of impulse and momentum is applied to a system S of particles during a time interval Dt, including particles which enter the system at A during that time interval and those (of the same mass Dm) which leave the system at B. The system formed by 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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