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Chapter 11 Questions
Chapter 11 Questions

PHY131H1F  - Class 9
PHY131H1F - Class 9

... • Gravity is always attractive, and acts between any two objects. • Electromagnetism causes repulsion and attraction between charged particles, such as the protons and electrons in matter. This gives rise to almost all of the forces we deal with in PHY131/132: Normal, Tension, etc. • Weak and Strong ...
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newtons laws study guide key
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Law of Inertia
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... “The acceleration of a body is directly proportional to the magnitude of the net force, in the same direction as the net force, and inversely proportional to the mass of the body” * “in the same direction as the net force” ◦ a in the same direction of body’s motion  speed up ◦ a in opposite directi ...
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... not a kind of force but simply a label. When the whirling bucket is at the top of the circle, both gravity and the contact force of the bucket on the water contribute to the centripetal force. When the water is moving at its minimum speed at the top of the swing, the water is in free fall (accelerat ...
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Motion - Cloudfront.net

... 1. Balanced Force – forces on an object that are equal in size and opposite in direction The net force = 0 2. Unbalanced Force – forces on an object that are unequal in size and opposite in direction The net force = the larger force ...
Forces in Mechanical Systems
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Physics 11 Review Qu.. - hrsbstaff.ednet.ns.ca

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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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