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Treat the surface of the sun as a perfect blackbody at a temperature of 5800K. According to Planck's distribution law, how many photons are emitted by the sun in the high-energy end of the visible spectrum (around 380nm) for every photon emitted in the low-energy end (around 680nm)?

Treat the surface of the sun as a perfect blackbody at a temperature of 5800K. According to Planck's distribution law, how many photons are emitted by the sun in the high-energy end of the visible spectrum (around 380nm) for every photon emitted in the low-energy end (around 680nm)?

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Question 4 Treat the surface of the sun as a perfect blackbody at a temperature of 5800K. According to Planck's distribution law, how manyphotons are emitted by the sun in the high-energy end of the visible spectrum (around 380nm) for every photon emitted in the low-energy end (around 680nm)?
Transcribed Image Text:Question 4 Treat the surface of the sun as a perfect blackbody at a temperature of 5800K. According to Planck's distribution law, how manyphotons are emitted by the sun in the high-energy end of the visible spectrum (around 380nm) for every photon emitted in the low-energy end (around 680nm)?
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