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Physics 16 Problem Set 8 Solutions
Physics 16 Problem Set 8 Solutions

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Impulse / Momentum Problem Set

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... on it. An object will accelerate if it has a net force acting on it, and the acceleration will be in the direction of the force. In this experiment, a lab cart will be accelerated by a known force, and its acceleration will be measured by a vernier motion detector. The product of the total mass acce ...
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... 56. A hole is drilled to the center of the earth and a ball is dropped into it. When the ball is at the earth's center, compared with their respective values at the earth's surface, A. its mass and weight are the same. B. its mass and weight are both 0. C. its mass is the same and its weight is 0. D ...
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...  The impact force will still react the same.  1. If the impulse is over a long time, then the impact force is small.  Example - a circus net  2. If the impulse is over a short time, then the impact force is large.  Example - a body dumped from a 10 story window ...
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Chapter 4: Newton`s Three Laws of Motion First

a = Vf - Vi t a  = 2d t a  = F m
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... The gravitational force exerted on an astronaut on Earth’s surface is 650 N down. When she is in the International Space Station, is the gravitational force on her (a) larger, (b) exactly the same, (c) smaller, (d) nearly but not exactly zero, or (e) exactly zero? According to Newton’s law of univer ...
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Newton`s Second Law

... The main theory behind this experiment is NŒž›–•˅šGzŒŠ–•‹GsˆžSGžŠGdefines the relationship between force and the acceleration a force produces. uŒž›–•˅šGšŒŠ–•‹G“ˆžGš›ˆ›Œš that the force on an object is directly proportional to its acceleration when the mass is constant. It also states that when f ...
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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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