The total radiant energy per unit area, normal to the direction of incidence

The total radiant energy per unit area, normal to the direction of incidence, received at a distance R from the centre of a star of radius r, whose outer surface radiates as a black body at a temperature T K is given by: (where σ is Stefan’s constant)

Options

(a) σr²T⁴ / R²
(b) σr²T⁴ / 4πr²
(c) σr⁴T⁴ / r⁴
(d) 4π σr²T⁴ / R²

Correct Answer:

σr²T⁴ / R²

Explanation:

E = S / S₀ σT⁴ = 4πr² / 4πR² σT⁴
σr²T⁴ / R²

admin:

Related Questions

  1. The resistance of an ammeter is 13Ω and its scale is graduated for a current
  2. Three masses are placed on the x-axis : 300 g at origin, 500 g at x = 40 cm
  3. The instantaneous angular position of a point on a rotating wheel is given by
  4. The velocity of a particle at an instant is 10 ms⁻¹.After 3 s its velocity will become
  5. The dimensions of universal gas constant are