The temperature of a body is increased from 2727c to 127127c. The radiation emitted by it increases by a factor o
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The radiation is increased by the factor of 81/256. We can solve this from Stephen Boltzman law of radiation, which is,
P is directly proportional to T^4. Where T is in kelvin
P is directly proportional to T^4. Where T is in kelvin
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All objects with a temperature above absolute zero (0 K, -273.15 oC) emit energy in the form of electromagnetic radiation. A blackbody is a theoretical or model body which absorbs all radiation falling on it, reflecting or transmitting none.
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