Heat Transfer MCQ’s – Stefan- Boltzman Law

1 - Question

The Stefan-Boltzmann constant has units of
a) kcal/m2 hr K4
b) kcal/m hr K4
c) kcal/hr K4
d) kcal/m2 K4
View Answer Answer: a
Explanation: According to Stefan-Boltzmann law, q = α A T4.



2 - Question

According to Stefan-Boltzmann law of thermal radiation
a) q = α A T
b) q = α A T4
c) q = α A T3
d) q = α A T5
View Answer Answer: b
Explanation: α is Stefan-Boltzmann constant whose value is 5.67 * 10 -8 W/m2 K4.



3 - Question

Calculate the radiant flux density from a black surface at 400 degree Celsius?
a) 1631.7 W/m2
b) 31.7 W/m2
c) 631.7 W/m2
d) 11631.7 W/m2
View Answer Answer: d
Explanation: E = σ T4 = 5.67 * 10 –8 (400 + 273)4 = 11631.7 W/m2.



4 - Question

If the emitted radiant energy is to be doubled, to what temperature surface of black body needs to be raised? Take radiant flux density as 11631.7 W/m 2.
a) 894.4 K
b) 200.4 K
c) 800.3 K
d) 600.4 K
View Answer Answer: d
Explanation: 2(11631.7) = 5.67 * 10 –8 T 4.



5 - Question

A furnace having inside temperature of 2250 has a glass circular viewing of 6 cm diameter. If the transmissivity of glass is 0.08, make calculations for the heat loss from the glass window due to radiation
a) 234.54 W
b) 652.32 W
c) 328.53 W
d) 762.32 W
View Answer Answer: c
Explanation: Q = σ A T4 (t) = 328.53 W.



6 - Question

The value of radiation coefficient or the Stefan-Boltzmann constant is
a) 5.67 * 10 -8 W/m2 K4
b) 5.67 * 10 -7 W/m2 K4
c) 5.67 * 10 -6 W/m2 K4
d) 5.67 * 10 -5 W/m2 K4
View Answer Answer: a
Explanation: q = α A T4.



7 - Question

Measurements were made of the monochromatic absorptivity and monochromatic hemispherical irradiation incident on an opaque surface, and the variation of these parameters with wavelength may be approximated by the result shown below. Determine the total hemispherical absorptivity


a) 0.557
b) 0.667
c) 0.777
d) 0.887
View Answer Answer: b
Explanation: Incident flux = 800(8 – 2) – 4800 W/m2. Absorptivity = 3200/4800 = 0.667.



8 - Question

What is the wavelength band for Ultraviolet rays?
a) 1 * 10 -6 to 3.9 * 10 -1 micron meter
b) 1 * 10 -4 to 3.9 * 10 -1 micron meter
c) 2 * 10 -3 to 3.9 * 10 -1 micron meter
d) 1 * 10 -2 to 3.9 * 10 -1 micron meter
View Answer Answer: d
Explanation: This is the maximum and minimum wavelength for Ultraviolet rays.



9 - Question

A black body of total area 0.045 m2 is completely enclosed in a space bounded by 5 cm thick walls. The walls have a surface area 0.5 m 2 and thermal conductivity 1.07 W/ m K. If the inner surface of the enveloping wall is to be maintained at 215 degree Celsius and the outer wall surface at 30 degree Celsius, calculate the temperature of the black body
a) 547.3 K
b) 287.4 K
c) 955.9 K
d) 222.2 K
View Answer Answer: c
Explanation: Q r = σ A (T b4 – Tw4), Q c = k A d t/δ = 1979.5 W. So temperature of black body is 955.9 K.



10 - Question

What is the wavelength band for solar radiation?
a) 1 * 10 -1 to 3 micron meter
b) 1 * 10 -1 to 2 micron meter
c) 1 * 10 -1 to 1 micron meter
d) 1 * 10 -1 to 10 micron meter
View Answer nswer: a
Explanation: This is the maximum and minimum wavelength for solar radiation.

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