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Abstract Radiometers are fun-to-watch novelty items, but they also have a distinguished scientific history, having been studied by James Clerk Maxwell and Albert Einstein. A radiometer has a set of four vanes (like small sails) connected to a spindle that is free to rotate. When the radiometer is placed in bright light, the vanes and spindle start to spin. It looks like a magic trick, but there is a scientific explanation for this weird behavior. In this science fair project, you will experiment with this simple, but fascinating, apparatus and determine how the speed of rotation of the radiometer's vanes varies with the amount of light striking them.Objective Measure the speed of rotation of a radiometer and test how the speed varies as the light intensity varies. Introduction Have you ever seen a radiometer before? A radiometer is made up of a glass bulb that contains a set of vanes on a freely rotating spindle. The vanes are painted black on one side and white or silver on the other side. The spindle and vanes rotate when exposed to light. As the intensity of the light increases, the speed of rotation also increases. In bright sunlight, the vanes can spin at several thousand revolutions per minute (RPMs). There is a difference in temperature between the black and white/silver sides of the vanes, since the black sides absorb more light energy. This temperature difference causes air currents that move the vanes forward, with the black sides of the vanes trailing the white/silver sides. Because a temperature difference is used to create motion, the radiometer is a form of heat engine. Figure 1 shows a radiometer with a slowly rotating spindle.
The radiometer was invented by Sir William Crookes in 1873. Crookes' radiometer is the result of serendipity, the act of making unexpected discoveries when looking for something else. In this case, Crookes was looking for a means to weigh very small amounts of chemicals as part of his research (the research eventually resulted in his discovery of the element thallium). To prevent drafts from affecting his scales, he enclosed them in glass and pumped out the air, creating a partial vacuum. Unexpectedly, the apparatus moved when it was struck by light. He decided to pursue the study of this effect, which he called repulsion resulting from radiation—radiation in this sense being light rays. Crookes' original explanation for the motion of the radiometer was that the light was exerting more pressure on the dark side of each vane than on the light side. But this radiation pressure explanation was ruled out by the discovery that if more of the remaining air molecules were removed from the bulb, creating a better vacuum, the motion ceased. If radiation pressure were the correct explanation, the vanes should have spun faster in a better vacuum, since there would be less resistance from the air molecules. Light can produce a force that will push against an object, but the effect is much too small to make the radiometer move. James Clerk Maxwell and Albert Einstein, two of the most brilliant scientists of modern times, both studied the radiometer. Their work, along with contributions from the scientist Osborne Reynolds, resulted in a description of how the flow of air molecules near the vanes results in a force that propels the vanes forward. The flow of gas molecules depends on the temperature difference between the two sides of the vanes. The temperature difference is created as the dark side absorbs more light energy than the light side. See the links in the Bibliography for more details. The radiometer works only at certain air pressures. At normal pressure, about 1 atmosphere (atm), the air currents are not strong enough to push the vanes against the resistance of the surrounding air. At very low pressure, there are not enough air molecules to form the currents needed to move the vanes forward. The challenge for this science fair project is to determine how fast the radiometer is spinning at a given level of light. To put it more precisely, you want to determine how the number of revolutions per minute (RPMs) vary with the illuminance (illuminance is a measure of the intensity of the incident light). You will use a digital light meter to measure the amount of light near the radiometer. The light meter gives readings of illuminance in a unit called a lux (the plural is also lux). The table below lists illuminance values for some common situations.
The lux, which is the SI-derived (International System of Units) unit of illuminance or illumination, is equal to one lumen per square meter. Lumens measure quantity of light emitted by the light source, whereas lux will tell you how many lumens you need, given the area you are trying to illuminate. The difference between the lux and the lumen is that the lux takes into account the area over which the light is spread. 100 lumens, concentrated into an area of 1 square meter (m2), lights up that square meter with an illuminance of 100 lux. The same 100 lumens, spread out over 10m2, produces a dimmer illuminance of only 10 lux. The rate of rotation (RPMs) will be measured with a digital tachometer. This device counts the number of times per minute that light striking it flickers, or changes brightness. The rate of rotation can be read by using the tachometer to measure the flicker in the radiometer's shadow. Terms, Concepts, and Questions to Start Background Research
Questions
Bibliography
Materials and Equipment
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| Figure 2. An example of an experimental setup for measuring the rate of rotation of the vanes of a radiometer at various levels of light. |
Variations
Credits
David B. Whyte, PhD, Science Buddies
Last edit date: 2011-01-31 12:00:00
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