The Stefan-Boltzmann law says that the radiation of heat R from an object is directly proportional to

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The Stefan-Boltzmann law says that the radiation of heat R from an object is directly proportional to the fourth power of the kelvin temperature of the object. For a certain object, R = 213.73 at room temperature (293 K). Find R, to the nearest hundredth, if the temperature increases to 335 K.

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College Algebra

ISBN: 978-0134697024

12th edition

Authors: Margaret L. Lial, John Hornsby, David I. Schneider, Callie Daniels

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