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Workshop module 5
Workshop module 5

... endangering anyone’s life. While the clients are busy jumping from a bridge (using the older cords), the owner (M = 100 kg) is attached to a 10 meter length of the new cord and slowly lowered until he is hanging motionlessly. At that time it is noted that the cord has stretched to a new length of 20 ...
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Chapter 3 Notes
Chapter 3 Notes

... harder to start moving?  The only way to change mass is to physically change the object. Ex: cutting off your arm ...
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Monday, Oct. 6, 2008

... observations for a long time. The data people collected, however, have not been explained until Newton has discovered the law of gravitation. Every particle in the Universe attracts every other particle with a force that is directly proportional to the product of their masses and inversely proportio ...
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... Note that the mass and the weight of an object are two different quantities!! Weight of an object is the magnitude of the gravitational force exerted on the object. Not an inherent property of an object!!! Weight will change if you measure on the Earth or on the moon but the mass won’t!! Monday, Sep ...
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Kepler Orbits for Binary Systems

Universal Laws of Motion - www .alexandria .k12 .mn .us
Universal Laws of Motion - www .alexandria .k12 .mn .us

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phys1443-fall07

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Name: Newton`s First Law of Motion: The Law of Inertia “An object at

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... This acceleration toward the centre of the circle is called the centripetal acceleration. This centripetal is Latin for centre seeking. Since we have acceleration we must also have a force that is causing that acceleration, we call this force: centripetal force. Often we mistake, centripetal force w ...
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Chapter 5, Part II

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... pulley fixed at the top of the wedge. The face on which A moves is smooth. The face on which B moves is rough. The coefficient of friction between B and this face is . Particle A is held at rest with the string taut. The string lies in the same vertical plane as lines of greatest slope on each plan ...
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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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