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Circular Motion - Cloudfront.net
Circular Motion - Cloudfront.net

... Types of Speed Linear speed is the distance traveled per unit of time. • A point on the outer edge of the turntable travels a greater distance in one rotation than a point near the center. • The linear speed is greater on the outer edge of a rotating object than it is closer to the axis. • The speed ...
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Helpful text on "system" problems w/ Newton`s Laws
Helpful text on "system" problems w/ Newton`s Laws

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UNIT04-HO1-Notes and Homework Problems

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Mechanics: Scalars and Vectors

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Dynamic Universe Forces Energy Power 2015 (10.4MB PowerPoint)

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File - singhscience

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Solutions - American Association of Physics Teachers

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The Physics of Phun: Roller Coaster Science

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Chapter 5 - Applications of Newton`s Laws

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The Physics of Phun: Roller Coaster Science
The Physics of Phun: Roller Coaster Science

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Physics - Oak Park Unified School District

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View as Printable PDF

Lesson 1 - SchoolRack
Lesson 1 - SchoolRack

... • Inertia is the tendency of an object to resist a change of motion Newton’s first law of motion states that an object will remain at rest or in constant straight-line motion unless unbalanced forces act on the object. • Newton’s second law of motion states that the acceleration of an object increas ...
Student Text, pp. 184-188
Student Text, pp. 184-188

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Linear acceleration of rolling objects Rotational Motion (cont.) R θ

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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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