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In solar radiation, the intensity of radiation is maximum around the wavelength `lambda_(m)`. If R is the radius of the sun and c is the velocity of light, the mass lost by the sum per unit time is proportional toA. `(R^(2))/(lambda^(4)c^(2))`B. `(R^(2))/(lambda^(2)c^(2))`C. `(R^(3))/(lambda^(4)c^(3))`D. `(R^(3))/(lambda^(4)c^(2))` |
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Answer» Correct Answer - A |
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