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The surface temperature of the sun is `T_(0)` and it is at average distance `d` from a planet. The radius of the sun is `R`. The temperature at which planet radiates the energy isA. `T_(0) sqrt((R)/(2d))`B. `T_(0) sqrt((2R)/(d))`C. `T_(0) sqrt((R)/(d))`D. `T_(0) ((R)/(d))^(1//4)` |
Answer» Correct Answer - A `r =` Radius of planet `T_(1)`= Temperature of planet at which energy is radiated Power radiated by Sun, `P=4 pi R^(2)sigma T_(0)^(4)` Energy recived by planet = `(P)/(4 pi d^(2)) xx pi r^(2) = (R^(2)T_(0)^(4)pi r^(2)sigma)/(d^(2))` Energy radiated by planet = `4 pi r^(2)sigma T_(1)^(4)` For thermal equilibrium, `(R^(2)T_(0)^(4)pi r^(2)sigma)/(d^(2)) = 4 pi r^(2)sigma T_(1)^(4)` `R^(2)T_(0)^(4) = 4d^(2)T_(1)^(4)` `T_(1) = T_(0)sqrt((R)/(2d))`. |
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