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The top documents tagged [stefanboltzmann law]
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stefanboltzmann law
If a star is very hot, the electrons will be freed from the hydrogen atom. (Ionized) Once they are free, they act like particles and emit a continuous.
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9 - Production of Light. Types pf Sources: Continuum (blackbodies, etc.) Emission line (fluorescent lamps, etc.) Emission bands (LEDs, etc.)
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A Star’s Color, Temperature, and Brightness are Related!
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A star’s color, temperature, size, brightness and distance are all related! Ohio University - Lancaster Campus slide 1 of 47 Spring 2009 PSC 100.
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Fy12 astronomy
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Causes Global Warming
13.673 views
Radiation ppt by iit professor
6.174 views
Blackbody ppt
2.501 views
Modeling Of a Bucket Air Cooler by Using Solar Energy
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E2 stellar radiation
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Black Body 2
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Radiation
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