Answered

Find the best answers to your questions at Westonci.ca, where experts and enthusiasts provide accurate, reliable information. Connect with a community of experts ready to provide precise solutions to your questions quickly and accurately. Explore comprehensive solutions to your questions from knowledgeable professionals across various fields on our platform.

The Stefan-Boltzmann Law relates the energy flux coming from a blackbody (such as a star) to its:
a) wavelength where maximum energy is emitted
b) temperature
c) overall color
d) atomic ground state
e) none of the above


Sagot :

The Stefan-Boltzmann Law links a blackbody's (like a star's) energy flux to its (b) temperature.

The Stefan-Boltzmann law states that a surface's overall radiant heat output is inversely correlated with its absolute temperature.

The power radiated from a black body is described by the Stefan-Boltzmann law in terms of its temperature. In particular, the Stefan-Boltzmann rule states that the black-body radiant emittance, also known as the total energy radiated per unit surface area across all wavelengths per unit time, is precisely proportional to the fourth power of the black body's thermodynamic temperature T.

To know more about Stefan-Boltzmann Law, refer to this link:

https://brainly.com/question/23278418

#SPJ4