Two-phase gas-liquid oxygen is stored in a spherical tank of \(1-m\) diameter, where it is maintained at its normal boiling point. The spherical tank is enclosed by a \(1.6-\mathrm{m}\) diameter concentric spherical surface at \(273 \mathrm{~K}\). Both spherical surfaces have an emissivity of \(0.01\), and the gap between the inner sphere and outer sphere is vacuumed. Assuming that the spherical tank surface has the same temperature as the oxygen, determine the heat transfer rate at the spherical tank surface.

Short Answer

Expert verified
Answer: The heat transfer rate at the spherical tank surface is approximately 13.15 W.

Step by step solution

01

Determine the temperature of the oxygen

The normal boiling point of oxygen is \(90.2 \mathrm{~K}\). Thus, the temperature of the oxygen at its normal boiling point is: \(T_{1} = 90.2 \mathrm{~K}\)
02

Calculate the surface areas of both inner and outer spherical surfaces

We are given the diameters of both the spherical tank (\(1\) m) and the concentric spherical surface (\(1.6\) m), so we can calculate their radii: \(r_{1}=0.5\) m and \(r_{2}=0.8\) m. The surface area of a sphere is given by the formula \(A = 4 \pi r^2\). Therefore, we can find the surface areas for both the inner (spherical tank) and outer (concentric spherical surface) spheres: \(A_{1} = 4 \pi r_{1}^2 = 4 \pi (0.5)^2 = \pi \mathrm{~m}^2\) \(A_{2} = 4 \pi r_{2}^2 = 4 \pi (0.8)^2 = 2.56 \pi \mathrm{~m}^2\)
03

Apply the radiative heat transfer equation

In a vacuum, heat transfer occurs only through radiation. The radiative heat transfer equation is given by: \(q = \dfrac{F_{12}\sigma (T_{1}^4 - T_{2}^4)}{1/\varepsilon_{1} - 1 + (A_{1}/A_{2})(1/\varepsilon_{2} - 1)}\), where \(q\) - heat transfer rate, \(F_{12}\) - view factor between surface 1 and surface 2, which is equal to \(1\) for concentric spheres, \(\sigma\) - Stefan-Boltzmann constant \((5.67 \times 10^{-8} \mathrm{W/m}^2 \mathrm{K}^4)\), \(T_{1}\) - temperature of the inner sphere (temperature of the oxygen), \(T_{2}\) - temperature of the outer sphere (\(273 \mathrm{~K}\)), \(\varepsilon_{1}\) and \(\varepsilon_{2}\) - emissivities of surface 1 (spherical tank) and surface 2 (concentric spherical surface) (\((0.01)\) in both cases), and \(A_{1}\) and \(A_{2}\) - surface areas of surfaces 1 and 2. Plugging the given values into the radiative heat transfer equation: \(q = \dfrac{1 \times (5.67 \times 10^{-8}) \times [(90.2)^4 - (273)^4]}{1/0.01 - 1 + (\pi / 2.56 \pi)(1/0.01 - 1)}\) After calculating, we get: \(q \approx -13.15 \mathrm{~W}\) The negative sign indicates that the heat transfer is happening from the outer sphere to the inner sphere. Therefore, the heat transfer rate at the spherical tank surface is approximately \(13.15 \mathrm{~W}\).

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Most popular questions from this chapter

A 2-m-internal-diameter double-walled spherical tank is used to store iced water at \(0^{\circ} \mathrm{C}\). Each wall is \(0.5 \mathrm{~cm}\) thick, and the \(1.5\)-cm-thick air space between the two walls of the tank is evacuated in order to minimize heat transfer. The surfaces surrounding the evacuated space are polished so that each surface has an emissivity of \(0.15\). The temperature of the outer wall of the tank is measured to be \(20^{\circ} \mathrm{C}\). Assuming the inner wall of the steel tank to be at \(0^{\circ} \mathrm{C}\), determine \((a)\) the rate of heat transfer to the iced water in the tank and \((b)\) the amount of ice at \(0^{\circ} \mathrm{C}\) that melts during a 24-h period.

Two gray surfaces that form an enclosure exchange heat with one another by thermal radiation. Surface 1 has a temperature of \(400 \mathrm{~K}\), an area of \(0.2 \mathrm{~m}^{2}\), and a total emissivity of \(0.4\). Surface 2 has a temperature of \(600 \mathrm{~K}\), an area of \(0.3 \mathrm{~m}^{2}\), and a total emissivity of \(0.6\). If the view factor \(F_{12}\) is \(0.3\), the rate of radiation heat transfer between the two surfaces is (a) \(135 \mathrm{~W}\) (b) \(223 \mathrm{~W}\) (c) \(296 \mathrm{~W}\) (d) \(342 \mathrm{~W}\) (e) \(422 \mathrm{~W}\)

Consider an enclosure consisting of 12 surfaces. How many view factors does this geometry involve? How many of these view factors can be determined by the application of the reciprocity and the summation rules?

13-59 This question deals with steady-state radiation heat transfer between a sphere \(\left(r_{1}=30 \mathrm{~cm}\right)\) and a circular disk \(\left(r_{2}=120 \mathrm{~cm}\right)\), which are separated by a center-to- center distance \(h=60 \mathrm{~cm}\). When the normal to the center of disk passes through the center of the sphere, the radiation view factor is given by $$ F_{12}=0.5\left\\{1-\left[1+\left(\frac{r_{2}}{h}\right)^{2}\right]^{-0.5}\right\\} $$ Surface temperatures of the sphere and the disk are \(600^{\circ} \mathrm{C}\) and \(200^{\circ} \mathrm{C}\), respectively; and their emissivities are \(0.9\) and \(0.5\), respectively. (a) Calculate the view factors \(F_{12}\) and \(F_{21}\). (b) Calculate the net rate of radiation heat exchange between the sphere and the disk. (c) For the given radii and temperatures of the sphere and the disk, the following four possible modifications could increase the net rate of radiation heat exchange: paint each of the two surfaces to alter their emissivities, adjust the distance between them, and provide an (refractory) enclosure. Calculate the net rate of radiation heat exchange between the two bodies if the best values are selected for each of the above modifications.

Why is the radiation analysis of enclosures that consist of black surfaces relatively easy? How is the rate of radiation heat transfer between two surfaces expressed in this case?

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