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The intensity or brightness of light as a function of the distance from the light source follows an inverse square relationship. ... Notice that as the distance increases, the light must spread out over a larger surface and the surface brightness decreases in accordance with a “one over r squared” relationship.
The apparent brightness of a star is proportional to 1 divided by its distance squared. That is, if you took a star and moved it twice as far away, it would appear 1/4 as bright; if you moved it four times the distance, it would appear 1/16 as bright. The reason this happens is simple.
The apparent brightness of a star is proportional to 1 divided by its distance squared. That is, if you took a star and moved it twice as far away, it would appear 1/4 as bright; if you moved it four times the distance, it would appear 1/16 as bright. The reason this happens is simple.
Apparent brightness is thus measured in watts per square meter. For instance, the apparent brightness of the Sun is b = 1370 watts/meter2. That is, if you had a perfectly efficient solar panel one meter on a side, if you held it perpendicular to the Sun's rays, it would generate 1370 watts of electricity.
The main technique to measure the distance to a star is from its parallax (if you want to know as to what it is, please write back). If the star is a variable star (its brightness changes periodically), then one can use the period of the variation to determine the distance to the star.
The luminosity of a star, on the other hand, is the amount of light it emits from its surface. The difference between luminosity and apparent brightness depends on distance. ... To think of this another way, given two light sources with the same luminosity, the closer light source will appear brighter.
The luminosity of a star, on the other hand, is the amount of light it emits from its surface. The difference between luminosity and apparent brightness depends on distance. ... To think of this another way, given two light sources with the same luminosity, the closer light source will appear brighter.
This relates the Apparent Brightness of a star (or other light source) to its Luminosity (Intrinsic Brightness) through the Inverse Square Law of Brightness: At a particular Luminosity, the more distant an object is, the fainter its apparent brightness becomes as the square of the distance.
The luminosity of the streetlamp is L = 1000 W = 103 W. The brightness is b = 0.000001 W/m2 = 10-6 = W/m2. So the distance is given by d2 = (103 W)/(4 Pi x 10-6 W/m2). Since 4 Pi is approximately 10, this is d2 = (103 /(10 x 10-6)) m2.
Intensity is a general word signifying the forcefulness or power of any energy. In the case of luminosity it is associated only with the intensity of light's brightness.
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