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Oscillatory Motion
Oscillatory Motion

... Our goal this semester is to understand how sound waves travel through the water so that we may exploit them to prosecute a target. We will start with simple models and increase complexity as we go. This course is meant to be directly applicable for the war-fighter. To begin with lets go back to our ...
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1201 lab 6 - U of M Physics

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... Method #1: Select a series of masses that give a usable range of displacements. The smallest mass must be much greater than the mass of the spring to fulfill the massless spring assumption. The largest mass should not pull the spring past its elastic limit (about 60 cm). Beyond that point you will d ...
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... Atoms are extremely tiny. Even though the air is full of oxygen and nitrogen molecules, you cannot see them. We know a lot about atoms and molecules, and this knowledge is invaluable when explaining the properties of substances. But, how do we measure atoms? The scale of atomic size means that chemi ...
Slide 1
Slide 1

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N-body problem

In physics, the n-body problem is the problem of predicting the individual motions of a group of celestial objects interacting with each other gravitationally. Solving this problem has been motivated by the desire to understand the motions of the Sun, Moon, planets and the visible stars. In the 20th century, understanding the dynamics of globular cluster star systems became an important n-body problem. The n-body problem in general relativity is considerably more difficult to solve.The classical physical problem can be informally stated as: given the quasi-steady orbital properties (instantaneous position, velocity and time) of a group of celestial bodies, predict their interactive forces; and consequently, predict their true orbital motions for all future times.To this purpose the two-body problem has been completely solved and is discussed below; as is the famous restricted 3-Body Problem.
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