Light from an ideal spherical blackbody 15.0 cm in diameteris analyzed by using a diffraction grating that has 3850 lines/cm.When you shine this light through the grating, you observe that thepeak-intensity wavelength forms a first-order bright fringe at +-14.4from the central bright fringe. (a) What is the temperature of the blackbody?(b) How long will it take this sphere to radiate 12.0 MJ of energyat constant temperature?
Light from an ideal spherical blackbody 15.0 cm in diameteris analyzed by using a diffraction grating that has 3850 lines/cm.When you shine this light through the grating, you observe that thepeak-intensity wavelength forms a first-order bright fringe at +-14.4from the central bright fringe. (a) What is the temperature of the blackbody?(b) How long will it take this sphere to radiate 12.0 MJ of energyat constant temperature?
Principles of Heat Transfer (Activate Learning with these NEW titles from Engineering!)
8th Edition
ISBN:9781305387102
Author:Kreith, Frank; Manglik, Raj M.
Publisher:Kreith, Frank; Manglik, Raj M.
Chapter1: Basic Modes Of Heat Transfer
Section: Chapter Questions
Problem 1.24P: Two large parallel plates with surface conditions approximating those of a blackbody are maintained...
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Light from an ideal spherical blackbody 15.0 cm in diameter
is analyzed by using a diffraction grating that has 3850 lines/cm.
When you shine this light through the grating, you observe that the
peak-intensity wavelength forms a first-order bright fringe at +-14.4
from the central bright fringe. (a) What is the temperature of the blackbody?
(b) How long will it take this sphere to radiate 12.0 MJ of energy
at constant temperature?
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