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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: - Dimensions [ML⁻¹T⁻¹] are related with
- A mass m moves in a circle on a smooth horizontal plane with velocity v₀
- The threshold frequency for a certain photosensitive metal is ν₀. When it is illuminated
- If the wavelength of incident light falling on a photosensitive material decreases,
- The flux linked with a circuit is given by φ=t³+3t-7. The graph between time
Topics: Properties of Bulk Matter
(130)
Subject: Physics
(2479)
Important MCQs Based on Medical Entrance Examinations To Improve Your NEET Score
- Dimensions [ML⁻¹T⁻¹] are related with
- A mass m moves in a circle on a smooth horizontal plane with velocity v₀
- The threshold frequency for a certain photosensitive metal is ν₀. When it is illuminated
- If the wavelength of incident light falling on a photosensitive material decreases,
- The flux linked with a circuit is given by φ=t³+3t-7. The graph between time
Topics: Properties of Bulk Matter (130)
Subject: Physics (2479)
Important MCQs Based on Medical Entrance Examinations To Improve Your NEET Score
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