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Forces - Lincoln Park High School
Forces - Lincoln Park High School

... Second law: The acceleration a of a body is parallel and directly proportional to the net force F and inversely proportional to the mass m, i.e., F = ma. Third law: The mutual forces of action and reaction between two bodies are equal, opposite and collinear. ...
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Test Review Slides - University of Mount Union

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... Robots are programmed to move with vectors. A robot must be told exactly how far to go and in which direction for every step of a trip. A trip of many steps is communicated to the robot as series of vectors. A maildelivery robot needs to get from where it is to the mail bin on the map. Find a sequen ...
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... ► Hooke’s Law: The displacement of a spring from its unstretched position is proportional the force applied. ► The slope of a force vs. displacement graph is equal to the spring constant. ► The area under a force vs. displacement graph is equal to the work done to compress or stretch a spring. ...
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... 1-Dimensional Finite Elements 1. Stiffness and Load Vector Formulations for mechanical, heat transfer and fluid flow problems. The system equation to be solved can be written in matrix form as: [K] {D} = {q} Where [K] is traditional known as the ‘stiffness’ or ‘coefficient’ matrix (conductance matr ...
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... The force of the sun is always towards the sun Which is perpendicular to the direction the plants travel (not quite a circle – but don’t consider that here) ...
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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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