Two concentric spheres of diameters \(15 \mathrm{~cm}\) and \(25 \mathrm{~cm}\) are separated by air at \(1 \mathrm{~atm}\) pressure. The surface temperatures of the two spheres enclosing the air are \(T_{1}=350 \mathrm{~K}\) and \(T_{2}=\) \(275 \mathrm{~K}\), respectively. Determine the rate of heat transfer from the inner sphere to the outer sphere by natural convection.

Short Answer

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Question: Determine the rate of heat transfer from the inner sphere to the outer sphere by natural convection, given the surface temperatures of the two concentric spheres with diameters of 15 cm and 25 cm are 350 K and 275 K, respectively, and the air pressure between them is 0.1 MPa. Answer: To calculate the rate of heat transfer from the inner sphere to the outer sphere by natural convection, follow these steps: 1. Calculate the radius of both spheres: r1 = 0.075 m, r2 = 0.125 m 2. Determine the mean film temperature and air properties at this temperature: T_film = 312.5 K 3. Calculate the Grashof (Gr) and Prandtl (Pr) numbers: Gr = (g * β * (T1 - T2) * (r2 - r1)^3) / ν^2, Pr = (μ * c_p) / k 4. Determine the Nusselt number: Nu = 0.154 * (Gr * Pr)^(1/5) 5. Calculate the convective heat transfer coefficient: h = (Nu * k) / (r2 - r1) 6. Determine the rate of heat transfer: Q = 4π * r1 * r2 * h * (T1 - T2) After calculating all the values, you will get the rate of heat transfer from the inner sphere to the outer sphere by natural convection.

Step by step solution

01

Calculate the radius of both spheres

Given the diameters, we can calculate the radii of the spheres: - Radius of sphere 1, \(r_1 = \frac{d_1}{2} = \frac{15\mathrm{~cm}}{2} = 7.5\mathrm{~cm} = 0.075\mathrm{~m}\) - Radius of sphere 2, \(r_2 = \frac{d_2}{2} = \frac{25\mathrm{~cm}}{2} = 12.5\mathrm{~cm} = 0.125\mathrm{~m}\)
02

Determine the mean film temperature and air properties at this temperature

To find the mean film temperature, we average the surface temperatures of the two spheres: $$ T_{film} = \frac{T_1 + T_2}{2} = \frac{350\mathrm{~K} + 275\mathrm{~K}}{2} = 312.5\mathrm{~K} $$ At this temperature, we can determine the properties of air using air property tables or correlations. The properties we'll need are the dynamic viscosity (\(\mu\)), thermal conductivity (\(k\)), thermal expansion coefficient (\(\beta\)), and specific heat (\(c_p\)).
03

Calculate the Grashof (Gr) and Prandtl (Pr) numbers

The Grashof number is a dimensionless number that characterizes the flow's buoyancy forces relative to viscous forces. The Prandtl number is a dimensionless number that characterizes the relative importance of momentum and thermal diffusion in convective heat transfer. $$Gr = \frac{g\beta(T_1 - T_2)(r_2 - r_1)^3}{\nu^2}$$ $$Pr = \frac{\mu c_p}{k}$$ where \(g\) is the acceleration due to gravity (\(9.81\mathrm{~m/s^2}\)), \(\nu\) is the kinematic viscosity (\(\nu = \frac{\mu}{\rho}\)), and \(\rho\) is the density of air.
04

Determine the Nusselt number

To find the Nusselt number (\(Nu\)), we use the correlation for natural convection between concentric spheres: $$Nu = 0.154 \times (Gr \times Pr)^{1/5}$$
05

Calculate the convective heat transfer coefficient

The convective heat transfer coefficient (\(h\)) can be calculated using the Nusselt number through: $$h = \frac{Nu \times k}{r_2 - r_1}$$
06

Determine the rate of heat transfer

Finally, we can calculate the rate of heat transfer (\(Q\)) using the convective heat transfer coefficient and the temperature difference between the surfaces of the spheres: $$Q = 4\pi r_1 r_2 h(T_1 - T_2)$$ After calculating all the values, we will get the rate of heat transfer from the inner sphere to the outer sphere by natural convection.

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Most popular questions from this chapter

Under what conditions does natural convection enhance forced convection, and under what conditions does it hurt forced convection?

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