Warning: foreach() argument must be of type array|object, bool given in /var/www/html/web/app/themes/studypress-core-theme/template-parts/header/mobile-offcanvas.php on line 20

Consider two black coaxial parallel circular disks of equal diameter \(D\) that are spaced apart by a distance \(L\). The top and bottom disks have uniform temperatures of \(500^{\circ} \mathrm{C}\) and \(520^{\circ} \mathrm{C}\), respectively. Determine the radiation heat transfer coefficient $h_{\text {rad }}\( between the disks if they are spaced apart by \)L=D$.

Short Answer

Expert verified
Question: Calculate the radiation heat transfer coefficient between two coaxial parallel circular disks with equal diameter, uniform temperatures of 500°C and 520°C, and spaced apart by a distance equal to their diameter. Answer: The radiation heat transfer coefficient between the two coaxial parallel circular disks is approximately 21.88 W/m²K.

Step by step solution

01

Convert temperatures to Kelvin

To convert temperatures from Celsius to Kelvin, add 273.15 to the temperature in Celsius: \(T_1 = 500^\circ \mathrm{C} + 273.15 = 773.15 \mathrm{K}\) \(T_2 = 520^\circ \mathrm{C} + 273.15 = 793.15 \mathrm{K}\)
02

Calculate the area of the disks

The area of a circular disk can be calculated using the formula: \(A = \pi r^2\), where \(r\) is the radius of the disk. We are given the diameter of the disks, \(D\), and the radius is half the diameter: \(r = \frac{D}{2}\) So, the area of the disks is: \(A = \pi \left(\frac{D}{2}\right)^2\)
03

Calculate the radiation heat transfer between the disks

The radiation heat transfer between the disks can be calculated using the formula: \(q = \sigma A (T_2^4 - T_1^4)\), where - \(\sigma = 5.67 \times 10^{-8} \, \mathrm{W m^{-2} K^{-4}}\): Stefan-Boltzmann constant Substitute the values of \(A\), \(T_1\), and \(T_2\) in the equation: \(q = 5.67 \times 10^{-8} \times \pi \left(\frac{D}{2}\right)^2 \times \left((793.15 \mathrm{K})^4 - (773.15 \mathrm{K})^4\right)\)
04

Calculate the radiation heat transfer coefficient

Now, we can calculate the radiation heat transfer coefficient (\(h_{\text{rad}}\)) using the formula: \(h_{\text{rad}} = \frac{q}{A(T_2 - T_1)}\) Substitute the values of \(q\), \(A\), \(T_1\), and \(T_2\) in the equation: \(h_{\text{rad}} = \frac{5.67 \times 10^{-8} \times \pi \left(\frac{D}{2}\right)^2 \times \left((793.15 \mathrm{K})^4 - (773.15 \mathrm{K})^4\right)}{\pi \left(\frac{D}{2}\right)^2(793.15 \mathrm{K} - 773.15 \mathrm{K})}\) Simplify the equation: \(h_{\text{rad}} = \frac{5.67 \times 10^{-8} \times ((793.15 \mathrm{K})^4 - (773.15 \mathrm{K})^4)}{20 \mathrm{K}}\) Now, we can compute the radiation heat transfer coefficient: \(h_{\text{rad}} \approx 21.88 \, \mathrm{W m^{-2} K^{-1}}\) The radiation heat transfer coefficient between the two coaxial parallel circular disks is approximately \(21.88 \, \mathrm{W m^{-2} K^{-1}}\).

Unlock Step-by-Step Solutions & Ace Your Exams!

  • Full Textbook Solutions

    Get detailed explanations and key concepts

  • Unlimited Al creation

    Al flashcards, explanations, exams and more...

  • Ads-free access

    To over 500 millions flashcards

  • Money-back guarantee

    We refund you if you fail your exam.

Over 30 million students worldwide already upgrade their learning with Vaia!

One App. One Place for Learning.

All the tools & learning materials you need for study success - in one app.

Get started for free

Most popular questions from this chapter

Radiation shields are commonly used in the design of superinsulations for use in space and cryogenics applications. Write an essay on superinsulations and how they are used in different applications.

Two infinitely long parallel plates of width \(w\) are located at \(w\) distance apart, as shown in Fig. P13-51. The two plates behave as black surfaces, where surface \(A_{1}\) has a temperature of \(700 \mathrm{~K}\) and surface \(A_{2}\) has a temperature of \(300 \mathrm{~K}\). Determine the radiation heat flux between the two surfaces.

Two coaxial parallel disks of equal diameter \(1 \mathrm{~m}\) are originally placed at a distance of \(1 \mathrm{~m}\) apart. If both disks behave as black surfaces, determine the new distance between the disks such that there is a \(75 \%\) reduction in radiation heat transfer rate from the original distance of \(1 \mathrm{~m}\).

A solar collector consists of a horizontal aluminum tube having an outer diameter of \(2.5\) in enclosed in a concentric thin glass tube of diameter $5 \mathrm{in}$. Water is heated as it flows through the tube, and the annular space between the aluminum and the glass tube is filled with air at $0.5 \mathrm{~atm}$ pressure. The pump circulating the water fails during a clear day, and the water temperature in the tube starts rising. The aluminum tube absorbs solar radiation at a rate of \(30 \mathrm{Btu} / \mathrm{h}\) per foot length, and the temperature of the ambient air outside is $75^{\circ} \mathrm{F}$. The emissivities of the tube and the glass cover are 0.9. Taking the effective sky temperature to be \(60^{\circ} \mathrm{F}\), determine the temperature of the aluminum tube when thermal equilibrium is established (i.e., when the rate of heat loss from the tube equals the amount of solar energy gained by the tube).

Explain all the different mechanisms of heat transfer from the human body \((a)\) through the skin and \((b)\) through the lungs.

See all solutions

Recommended explanations on Physics Textbooks

View all explanations

What do you think about this solution?

We value your feedback to improve our textbook solutions.

Study anywhere. Anytime. Across all devices.

Sign-up for free