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o a first approximation the sun is an ideal blackbody emitter of light, at a temperature T = 5 7 7 0 . K (
o a first approximation the sun is an ideal blackbody emitter of light, at a temperature T
K Figure The diameter of the sun is D x m
a What are the values for lambda max and Mtotal, the peak emission wavelength in nm and total
intensity of emitted light in Jms for the sun?To a first approximation the sun is an ideal blackbody emitter of light, at a temperature
Figure The diameter of the sun is
a What are the values for and the peak emission wavelength in and total
intensity of emitted light in for the sun?
b What is the total rate of at which energy is emitted by the sun
c What fraction of the energy emitted by the sun falls in the visible region of the
spectrum Note: you will have to find the value for the appropriate
integral, approximately. Use the rectangle rule. I would recommend dividing
the integral into two parts, from to and from to
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