The radiation emitted by the surface of the Sun emits maximum power at a wavelength of about 500 n m . Assuming the Sun to be a blackbody emitter. If its surface temperature K is given by α ∙ β × 10 γ then fill the value of α + β + γ . (Wie

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The radiation emitted by the surface of the Sun emits maximum power at a wavelength of about 500 n m . Assuming the Sun to be a blackbody emitter. If its surface temperature K is given by α ∙ β × 10 γ then fill the value of α + β + γ . (Wien’s constant is given by 2.898 m m K )

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&#955; = 500 nm , T = b &#955; T = 2 .898 &#160; mm 500 &#160; nm = 5 .8 &#215; 10 3

The radiation emitted by the surface of the Sun emits maximum power at a wavelength of about 500 n m . Assuming the Sun to be a blackbody emitter. If its surface temperature K is given by α ∙ β × 10 γ then fill the value of α + β + γ . (Wien’s constant is given by 2.898 m m K )

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