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

The Total Radiant Energy Per Unit Area Normal To The Physics Question

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

Related Questions:

  1. The minimum velocity (in ms⁻¹) with which a car driver must traverse a flat curve
  2. A police jeep is chasing a culprit going on a motorbike.The motorbike crosses
  3. Three capacitors each of capacitance C and of breakdown voltage V are joined in series
  4. If the ionisation energy for the hydrogen atom is 13.6 eV, the energy required
  5. In a thermodynamic system, working substance is ideal gas. Its internal energy

Topics: Properties of Bulk Matter (130)
Subject: Physics (2479)

Important MCQs Based on Medical Entrance Examinations To Improve Your NEET Score

18000+ students are using NEETLab to improve their score. What about you?

Solve Previous Year MCQs, Mock Tests, Topicwise Practice Tests, Identify Weak Topics, Formula Flash cards and much more is available in NEETLab Android App to improve your NEET score.

NEETLab Mobile App

Share this page with your friends

Be the first to comment

Leave a Reply

Your email address will not be published.


*