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cse โ€ข paper_1 โ€ข electrodynamics

[UPSC CSE 1990] Black Body Radiation (Q492, 20M)

Define solar constant and say which of the values 1.34\text{ W/m}^2, 1.34 \times 10^3\text{ W/m}^2, 1.34 \times 10^5\text{ W/m}^2 is valid for it. Calculate the total energy radiated by the sun in one second and hence the decrease in its mass per second.

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