Resource: Inverse Square Law
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HTML Interactive
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This animation, originally created for a KET distance learning physics course, explains the mathematical formula for the Inverse Square Law by demonstrating how the brightness of light changes with the distance from a source in one, two, and three dimensions. This animation can be viewed in segments or as a whole.
Teachers' Domain, Inverse Square Law, published September 2, 2008, retrieved on ,
http://www.teachersdomain.org/resource/ket08.sci.phys.mfw.ketinverse/
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Have you ever noticed that light from a flashlight seems much brighter when it shines on something nearby than when focused on something far away? Maybe you’ve also noticed that when you use spray paint the thickness of the coat is related to how close you hold the can to the wall. These effects are due to a physical property known as the Inverse Square Law, which states that the strength of a given physical quantity is inversely proportional to the distance from the source squared or I → 1/d2 (I=Intensity). Inversely proportional means that as distance increases, intensity decreases.
The most well-known story about the Inverse Square Law comes from one of the most famous stories in all of science—Sir Isaac Newton and the apple. According to the story, Newton was trying to understand the planetary motion of the heavens when an apple fell from a tree, hit him on the head, and let loose a stream of ideas that would change physics forever. Newton wondered how the gravity that caused the apple to fall was related to the gravity that acted on much more distant objects like the Moon. He made some calculations and found that the Moon was falling toward Earth with an acceleration that was 3,600 times smaller than the apple’s acceleration. He knew the Moon was about 60 times as far from Earth's center as the falling apple was. Newton realized the inverse square of the distance was correlated to the change in the effects of gravity, 1/602 = 1/3600. Newton also saw that because he was squaring the inverse distance, the relationship was non-linear. For example, a satellite half as far away as the Moon experiences gravity at 1/302 = 1/900, not 1/1800. Note that the distance is one-half the distance to the Moon, yet the intensity is four times as strong as the intensity at the Moon—not twice as strong as you might expect.
The Inverse Square Law applies to anything that radiates in all directions. Gravity obviously follows this law because our spherical planet tugs on objects all across Earth's surface. The light intensity from a bulb, the radiation escaping a brick of Uranium, the force on an electron in an electric field, and the screeching sounds of a passing ambulance are all under the command of the Inverse Square Law. From a far distance these things seem to be weak—a faint light on your face or the subtle sounds of the sirens. But as you get closer to the emanating source, the effect grows larger, and the closer you get, the more rapidly the effect increases.
Source: "Inverse Square Law"
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