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Chapter 2
Chapter 2

... Newton’s First Law of Motion: A body continues in a state of rest or uniform motion in a straight line unless made to change that state by forces acting on it ...
F r i c t i o n - Southgate Community School District
F r i c t i o n - Southgate Community School District

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Worksheet #4 over Unit 6 reading: Determining the Net Force

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Also except answer if student derive for particular two bodies.

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Physics Chapter 1-3 Review

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Unit 2 Laws of Motion

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... Work might also be done on an object to raise it to a higher height. In this case, the work done is the force opposing gravity times the distance it rises. We can get this energy back by releasing the object and allowing it to fall. Try it once right now. The amount of energy an object has because o ...
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... – Newton’s First Law • Newton’s first law of motion states that: – Any object that is at rest or any object in uniform motion will remain at rest or in uniform motion unless acted upon by a non-zero net force » Uniform motion means that the object is not accelerating » So, the object is not changing ...
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... that is equally strong, so the two forces cancel, leaving no net force. Example 3: A hockey puck slides on ice at constant velocity. What is the net force acting on the puck? ...
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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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