Verified Solution • 2025–26 Session moderate

QAIPMT-2007-Ph-2353: NEET 2007 Physics - Class 12 AIPMT-2007-Ph-2353 Solution: Assuming the sun to have a spherical outer surface of radius r…

Assuming the sun to have a spherical outer surface of radius r radiating like a black body at temperature t∘Ct^\circ C the power received by a unit surface (normal to the incident rays) at a distance R from the centre of the sun is where σ\sigma is the Stefan's constant. 4πr2σ(t+273)4R2\frac{4\pi r^2 \sigma (t+273)^4}{R^2} 16π2r2σt4R2\frac{16\pi^2 r^2 \sigma t^4}{R^2} r2σ(t+273)4R2\frac{r^2 \sigma (t+273)^4}{R^2} 4πr2σt4R2\frac{4\pi r^2 \sigma t^4}{R^2}

Multiple Choice Options

  • A 6.8 eV
  • B 13.6 eV
  • C 1.7 eV
  • D 3.4 eV.

Step-by-Step Verified Solution

E n = _ 13.6 n 2 E 1 = -13.6 eV E 2 = _ 13.6 2 2 = -3.4 eV Kinetic energy of an electron in the first excited state is K = �E 2 = 3.4 eV.

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