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Cornell Notes Topic/Objective: Physics / Newton`s Laws Name
Cornell Notes Topic/Objective: Physics / Newton`s Laws Name

... Inertia is the tendency of an object to resist a change in its motion. All objects have inertia, whether they are stationary or moving. Inertia explains Newton’s first law of motion, which states that an object at rest will remain at rest and an object in motion will stay in motion unless it is acte ...
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... contact with another stable object. Gravity Force: The force with which the earth, moon, or other massively large object attracts another object towards itself. Gravity will always be a force acting on an object. Air Resistance: A special type of frictional force that acts upon objects as they trave ...
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... does all rotational motion. We call rotational momentum angular momentum as it is mass moving in a circular motion. Thus angular momentum (L) is made up of a mass (m) and angular velocity (). However instead of mass we now talk about rotational inertia (). Hence we get the formula: ...
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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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