| ⇦ |
| ⇨ |
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: - The moment of inertia of a rod about an axis through its centre and perpendicular
- A galvanometer having internal resistance 10Ω requires 0.01 A for a full scale
- A student performs an experiment to determine the Young’s modulus of a wire
- The temperature at which the vapour pressure of a liquid becomes equal to the external
- The ratio of specific charge of an α-particle to that of a proton is
Topics: Properties of Bulk Matter
(130)
Subject: Physics
(2479)
Important MCQs Based on Medical Entrance Examinations To Improve Your NEET Score
- The moment of inertia of a rod about an axis through its centre and perpendicular
- A galvanometer having internal resistance 10Ω requires 0.01 A for a full scale
- A student performs an experiment to determine the Young’s modulus of a wire
- The temperature at which the vapour pressure of a liquid becomes equal to the external
- The ratio of specific charge of an α-particle to that of a proton is
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.
Share this page with your friends

Leave a Reply