(d) Calculate the maximum amount of heat which may be lost per second by radiation from a sphere of 5 cm in diameter at a temperature of 600 K when placed in an enclosure at a temperature of 300 K. Given that, \(\sigma = 5.7 \times 10^{-12} \, \text{watts/cm}^{-2}/(^\circ \text{C})^{-1}\).
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Another Explanation (5): Here's the solution:
The surface area of the sphere is \(4\pi r^2 = 4\pi (2.5)^2 = 25\pi \, \text{cm}^2\).
Using Stefan-Boltzmann's Law, the power radiated is given by:
\(P = \sigma A (T_1^4 - T_2^4)\)
Where:
- \(\sigma = 5.7 \times 10^{-12} \, \text{watts/cm}^2/K^4\)
- \(A = 25\pi \, \text{cm}^2\)
- \(T_1 = 600 \, K\)
- \(T_2 = 300 \, K\)
Substituting the values:
\(P = 5.7 \times 10^{-12} \times 25\pi \times (600^4 - 300^4) \approx 0.71 \, \text{watts}\)
Therefore, the maximum amount of heat lost per second by radiation is approximately 0.71 watts.
Related Questions (Any University/Year)
- (b) State Kirchhoff's law. From Stefan's law derive Newton's law of cooling. [6]
- (h) Calculate the energy radiated per minute from the filament of an incandescent Lamp at 1500 K if the surface area is \(4.5 \times 10^{-5} \, \text{m}^2\) and its relative emittance is \(0.65 \, (\sigma = 5.672 \times 10^{-8} \, \text{W/m}^2\text{K}^4)\).
- (c) What is the wavelength of maximum intensity radiation radiated from a source at temperature \(3000^\circ \text{C}\)? (Wien's constant \(b = 0.288 \, \text{cm} \cdot \text{K}\)).
- (f) Calculate the surface temperature of sun and moon given that \( \lambda_m = 4753 \text{\AA} \) and \( 14 \mu \text{m} \) respectively, \( \lambda_m \) being wavelength of maximum intensity of emission.
- (d) Calculate the maximum amount of heat which may be lost per second by radiation from a sphere of 5 cm in diameter at a temperature of 600 K when is placed in an encloser at a temperature of 300 K. Given that \(\sigma = 5.7 \times 10^{-12} \, \text{watts/cm}^{-2} / (\circ C)^{-4}\).
- (4) The spectral energy curve of sunlight has a maximum at a wavelength of \(4.84 \times 10^{-7} \, \text{m}\). Assuming the Sun to be a black body,
- (xiii) State Stefan-Boltzmann law.
- (b) State and explain Stefan-Boltzmann's law.
- (g) If a black body at temperature 6174 K emits 4700 \text{\AA} with maximum energy; Calculate the temperature at which it will emit a wavelength of \( 1.4 \times 10^{-5} \text{m} \) with maximum energy.
- g) What is Stefan-Boltzmann law?
- (c) A black body at temperature 4980 K emits radiation of wavelength 4000 Å with maximum energy. Calculate the temperature at which it will emit a wavelength of \(1.45 \times 10^{-5} \, \text{cm}\) with maximum energy.
- (b) What is the energy density of the Sun's radiation?
- (k)What is Stefan-Boltzmann law? State Wein's displacement law.
- (c)Calculate the surface temperature of sun and moon given that \( \lambda_m = 4753 \, \text{Å} \) and 14 \(\mu \text{m}\) respectively, \( \lambda_m \) being wavelength at the maximum intensity of emission.
- (g) A black sphere of diameter 4 cm is heated to 400 K when the surrounding temperature is 300 K. What is the rate at which energy is radiated? Given \( \sigma = 6 \times 10^{-8} \, \text{Wm}^{-2} \, \text{K}^{-4} \).
- (d) If a black body at temperature \(6174 \, \text{K}\) emits \(4700 \, \text{Å}\) with maximum energy. Calculate the temperature at which it emits a wavelength of \(1.4 \times 10^{-3} \, \text{m}\) with maximum energy.
- (a) What is the temperature of its emitting surface?
- (j) State Wien’s displacement law.
- b) Derive Wien's law of energy distribution.
- (d) An aluminum foil of relative emittance 0.1 is placed in between two concentric spheres at temperatures 300 K and 200 K respectively. Calculate the temperature of the foil after the steady state is reached. Assume that the spheres are perfect blackbody radiators. Also calculate the rate of energy transfer between one of the spheres and the foil. [\(\sigma = 5.672 \times 10^{-8} \, \text{M.K.S. units}\)]