Q1: A cylindrical rod of length h h and diameter d d is placed inside a cubic enclosure of side length L . S denotes the inner surface of the cube. The view-factor FS − S is [GATE ME 2023]
(a) 0
(b) 1
(c) 
(d) 
Ans: (d)

Surface area of centrifugal rod = π d h + 2 π d 2 /4
Or A1 = π (dh + d2/2)
Surface area of cube A2 = 6 x L2
For surface 1 (cylinder), F11= 0
So F12 = 1...(i)
For surface 2(cube)
F21 + F22 = 1
F22 = 1 − F21
F21 = 1 − F22 . . . (ii)
By reciprocity theorem for surface 1 and 2
A1 F12 = A2 F21
F12 = A1/ A2
[F12 = 1 from equation (i)]
So, By equation (ii)
F22 = Fs S = 1- 
Q1: Wien's law is stated as follows: λm T = C, where C is 2898 μmK and λm is the wavelength at which the emissive power of a black body is maximum for a given temperature T. The spectral hemispherical emissivity (ε λ) of a surface is shown in the figure below (1 ˚A = 10− 10 m). The temperature at which the total hemispherical emissivity will be highest is __________ K (round off to the nearest integer). [GATE ME 2022, SET-2]
Ans: (4825 to4835]
From the figure we can say that at 6000 ˚A wavelength total hemispherical emissivity is maximum
λm = 6000 ˚A 0.6 μm
Wein's law
λm T = 2898 μmK
T = 2898/0.6 = 4830K
Note: In this question, we need to find temperature at which total hemispherical emissivity will be highest.
But to calculate total hemispherical emissivity we require additional data like function chart and emissivity value at particular wavelength.
With the use of Wein's law we can find out temperature at which spectral emissivity is highest but in question it is asked temperature for total hemispherical emissivity.
Q2: A flat plate made of cast iron is exposed to a solar flux of 600 W/m2 at an ambient temperature of 25°C. Assume that the entire solar flux is absorbed by the plate. Cast iron has a low temperature absorptivity of 0.21. Use Stefan-Boltzmann constant = 5.669 × 10− 8 W/m 2 − K 4. Neglect all other modes of heat transfer except radiation. Under the aforementioned conditions, the radiation equilibrium temperature of the plate is __________ °C (round off to the nearest integer). [GATE ME 2020, SET-1]
Ans: (210 to 225)
Equilibrium Temperature = TS?
In this it is mentioned that entire flux is absorbed by the plate it means for solar flux absorptivity is 1. Kirchhoff's law α = ε = 0.21
Surface of cast iron and surrounding fluid temperature difference is small due to this we can use Kirchhoff's law At equilibrium condition Energy absorbed = Energy leaving

Ts = 491.34 K
Ts = 218.34 °C
Ts = 218 °C
Q1: A solid sphere of radius 10 mm is placed at the centroid of a hollow cubical enclosure of side length 30 mm. The outer surface of the sphere is denoted by 1 and the inner surface of the cube is denoted by 2. The view factor F22 for radiation heat transfer is ________ (rounded off to two decimal places). [GATE ME 2021,SET-1]
Ans: (0.76 to0.78)
r1 = 10 mm

A2 = 6 x (302)
F12 = 1

Q2: The spectral distribution of radiation from a black body at T1 = 3000 K has a maximum at wavelength λ max. The body cools down to a temperatureT2. If the wavelength corresponding to the maximum of the spectral distribution at T2 is 1.2 times of the original wavelength λ max . then the temperature T2 is ________ K (round off to the nearest integer). [GATE ME 2020, SET-2]
Ans: (2499 to 2501)
From Wien's Displacement law,

Question for GATE Past Year Questions: Radiation
Try yourself:For a glass plate transmissivity and reflectivity are specified as 0.86 and 0.08 respectively, the absorptivity of the glass plate is
[1988]
Explanation
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Question for GATE Past Year Questions: Radiation
Try yourself:A diffuse radiation surface has
[1991]
Explanation
Radiation intensity is independent of angle in diffuse radiation.
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Question for GATE Past Year Questions: Radiation
Try yourself:What is the value of the view factor for two inclined flat plates having common edge of equal length and wlth an angle of 20 degrees?
[2002]
Explanation

= 0.826
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Question for GATE Past Year Questions: Radiation
Try yourself:The following figure was generated from experimental data relating spectral black body emissive power to wave length at the three temperatures T1, T2 and T3( T1 > T2 >T3).

The conclusion in that the measurements are
[2005]
Explanation
Wien's displacement law is not satisfied, i.e., λmax T = C
which tells lower λmax for higher temperature.
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Question for GATE Past Year Questions: Radiation
Try yourself:For an opaque surface, the absorptivity (α), transmissivity (τ) and reflectivity (ρ) are related by the equation
[2012]
Explanation
α + τ + ρ = 1
for opaque surface, τ = 0
∴ α + ρ = 1
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Question for GATE Past Year Questions: Radiation
Try yourself:The radiative heat transfer rate per unit area (W/m2) between two plane parallel gray surfaces (emissivity = 0.9) maintained at 400 K and 300 K is (σ = Stefan Boltzmann constant = 5.67 × 10-8 W/m2K4)
[1993]
Explanation
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Question for GATE Past Year Questions: Radiation
Try yourself:A plate having 10 cm2 area each side is hanging in the middle of a room of 100 m2 total surface area. The plate temperature and emissivity are respectively 800 K and 0.6. The temperature and emissivity valute for the surfaces of the room are 300 K and 0.3 respectively. Boltzmann's constant σ = 5.67 × 10-8 W/m2K4. The total heat loss from the two surfaces of the plate is
[2003]
Explanation
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Question for GATE Past Year Questions: Radiation
Try yourself:A100 W electric bulb was switched on in a 2.5 m × 3 m × 3 m size thermally insulated room having a temperature of 20°C. The room temperature at the end of 24 hours will be
[2006]
Explanation
Heat generated by bulb = 100 × 24 × 60 × 60 Joule.
∴ Heat dissipated = r × V × Cv × (T - 20)
⇒ 100 × 24 × 60 × 60 = 1.24 × 9 × 2.5 × 3 × Cv (T – 20)
⇒ T = 450º
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Question for GATE Past Year Questions: Radiation
Try yourself:Radiative heat transfer is intercepted between the inner surfaces of two very large isothermal parallel metal plates. While the upper plate (designated as plate 1) is a black surface and is the warmer one being maintained at 727°C, the lower plate (plate 2) is a diffuse and gray surface with an emissivity of 0.7 and is kept at 227°C. Assume that the surfaces are sufficiently large to form a two-surface enclosure and steady-state conditions to exist. Stefan-Boltzmann constant is given as 5.67 × 10–8 W/m2K4.
The irradiation (in kW/m2) for the plate (plate 1) is
[2009]
Explanation
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Question for GATE Past Year Questions: Radiation
Try yourself:Radiative heat transfer is intercepted between the inner surfaces of two very large isothermal parallel metal plates. While the upper plate (designated as plate 1) is a black surface and is the warmer one being maintained at 727°C, the lower plate (plate 2) is a diffuse and gray surface with an emissivity of 0.7 and is kept at 227°C. Assume that the surfaces are sufficiently large to form a two-surface enclosure and steady-state conditions to exist. Stefan-Boltzmann constant is given as 5.67 × 10–8 W/m2K4.
If plate 1 is also a diffuse and gray surface with an emissivity value of 0.8, the net radiatibn heat exchange (in kW/m2) between plate 1 and plate 2 is
[2009]
Explanation
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Question for GATE Past Year Questions: Radiation
Try yourself:Two larged if fuse gray parallel plates, separated by a small distance, have surface temperature of 400 K and 300 K. If the emissivities of the surfaces are 0.8 and the Stefan-Boltzmann constant is 5.67 × 10–8 W/ m2K4, the net radiation heat exchange rate in kW/m2 between the two plates is
[2013]
Explanation
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Question for GATE Past Year Questions: Radiation
Try yourself:The total emissive power of a surface is 500 W/ m2 at temperature T1 and 1200 W/m2 at emperature T2, where the temperature are in Kelvin. Assuming the emissivity of the surface to be constant, the ratio of the temperature T1/T2 is
[2015]
Explanation
Emissive power ∝ T4
⇒ 
∴ 
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Question for GATE Past Year Questions: Radiation
Try yourself:The emissive power of a blackbody is P. If its absolute temperature is doubled, the emissive power becomes
[2017]
Explanation
Eb = σ T4

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Question for GATE Past Year Questions: Radiation
Try yourself:The peak wavelength of radiation emitted by a black body at a temperature of 2000 K is 1.45 μm. If the peak wavelength of emitted radiation changes to 2.90 μm , then the temperature (in K) of the black body is
[2018]
Explanation
From wein’s displacement law
λmax T = constant

T2 = 1000 K
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Question for GATE Past Year Questions: Radiation
Try yourself:For the circular tube of equal length and diameter shown in figure below, the view factor F13 is 0.17. The view factor F12 in this case will be
[2001]
Explanation

and 
F13 = 0.17,
F11 = 0,
F11 + F12 + F13 = 1
∴ F12 = 1 – F13
= 1 – 0 – 17 = 0.83
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Question for GATE Past Year Questions: Radiation
Try yourself:A solid cylinder (surface 2) is located at the centre of a hollow sphere (surface 1). The diameter of the sphere is 1 m, while the cylinder has a diameter and length of 0.5 m each.'The radiation configuration factor F11 is
[2005]
Explanation
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Question for GATE Past Year Questions: Radiation
Try yourself:A hollow enclosure is formed between two inf initely long concentric cylinders of radii 1 m and 2 m, respectively. Radiative heat exchange takes place between the inner surface of the larger cylinder (surface-2) and the outer surface of the smaller cylinder (surface-1). The radiating surface are diffuse and the medium in the enclosure is non- participating. The fraction of the thermal radiation leaving the larger surface and striking itself is
[2008]
Explanation
F 11 + F 12 = 1
F 21 + F 22 = 1
F 11 = 0 due to concave surface
F 12 = 1
Now A 1 F 12 = A 2 F 21
⇒ 
⇒ F12 = 1
∴ 
F 21 = 0.5
F 22 = 1 – F 21 = 0.5
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Question for GATE Past Year Questions: Radiation
Try yourself:Consider two infinitely long thin concentric tubes of circular cross section as shown in figure. If D1 and D2 are the diameters of the inner and outer tubes respectively, then the view factor F22 is given by
[2012]
Explanation
F22 = 1 – F21

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Question for GATE Past Year Questions: Radiation
Try yourself:A solid sphere of radius r1 = 20 mm is placed concentrically inside a hollow sphere of radius r2 = 30 mm as shown in the figure.

The view factor F21 for radiation heat transfer is
[2014]
Explanation
F 11 + F 12 =1, here F 11 = 0
∴ F 12 = 1

Now from reciprocating law
A 1 F 12 = A 2 F 21

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Question for GATE Past Year Questions: Radiation
Try yourself:A solid sphere 1 of radius r is placed inside a hollow, closed hemispherical surface 2 of radius 4r. The shape factor F is,
[2015]
Explanation
f11 + f12 = 1
∴ f12 = 1
f21 A2 = f12 A1
∴ 
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Question for GATE Past Year Questions: Radiation
Try yourself:Consider the radiation heat exchange inside an annulus between two very long concentric cylinders. The radius of the outer cylinder is R0 and that of the inner cylinder is Ri. The radiation view factor of the outer cylinder onto itself is
[2016]
Explanation
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Question for GATE Past Year Questions: Radiation
Try yourself:Sphere 1 with a diameter of 0.1 m is completely enclosed by another sphere 2 of diameter 0.4 m.The view factor F12 is
[2019]
Explanation

F11 = 0
F12 = 1
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Question for GATE Past Year Questions: Radiation
Try yourself:Two infinite parallel plates are placed at a certain distance apart. An infinite radiation shield is inserted between the plates without touching any of them to reduce heat exchange between the plates. Assume that the emissivities of plates and radiation shield are equal. The ratio of the net heat exchange between the plates with and without the shield is
[2014]
Explanation

here, n = 1
∴ 
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