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The outer surface of a spacecraft in space has an emissivity of \(0.8\) and a solar absorptivity of \(0.3\). If solar radiation is incident on the spacecraft at a rate of \(950 \mathrm{~W} / \mathrm{m}^{2}\), determine the surface temperature of the spacecraft when the radiation emitted equals the solar energy absorbed.

Short Answer

Expert verified
Answer: The surface temperature of the spacecraft when the absorbed radiation equals emitted radiation is 293.2 K.

Step by step solution

01

Define Given Variables

The given information tells us about the emissivity (\(\epsilon\)), solar absorptivity (\(\alpha\)), and solar radiation \(G_{S}\): \(\epsilon = 0.8\) \(\alpha = 0.3\) \(G_{S} = 950 \mathrm{~W} / \mathrm{m}^{2}\)
02

Calculate the Solar Energy Absorbed

To find the solar energy absorbed by the spacecraft, we multiply the solar radiation by the solar absorptivity: \(Q_{absorbed} = \alpha G_{S} \Rightarrow Q_{absorbed} = 0.3 \cdot 950 \mathrm{~W} / \mathrm{m}^{2}\) \(Q_{absorbed} = 285 \mathrm{~W} / \mathrm{m}^{2}\)
03

Use the Stefan-Boltzmann Law

According to the Stefan-Boltzmann Law, the power emitted by the spacecraft's surface due to radiation is given by: \(Q_{emitted} = \epsilon \sigma A T^{4}\) where \(\epsilon\) is the emissivity, \(\sigma\) is the Stefan-Boltzmann constant (\(5.67 \times 10^{-8} \mathrm{W} / \mathrm{m}^{2} \mathrm{K}^{4}\)), \(A\) is the surface area, and \(T\) is the surface temperature of the spacecraft in Kelvin. To find the point where \(Q_{emitted} = Q_{absorbed}\), we can set these two equal: \(\epsilon \sigma A T^{4} = Q_{absorbed}\) Since we're interested in the temperature \(T\), we can isolate that variable: \(T^{4} = \frac{Q_{absorbed}}{\epsilon \sigma A}\)
04

Calculate the Surface Temperature

Since the surface area, \(A\), cancels out on both sides of the equation, we are left with: \(T^{4} = \frac{285 \mathrm{~W} / \mathrm{m}^{2}}{0.8 (5.67 \times 10^{-8} \mathrm{W} / \mathrm{m}^{2} \mathrm{K}^{4})}\) \(T^{4} = 79336.2\) Now, take the fourth root of this result: \(T = \sqrt[4]{79336.2} = 293.2 \mathrm{K}\) The surface temperature of the spacecraft when the absorbed radiation equals emitted radiation is \(293.2 \mathrm{K}\).

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Most popular questions from this chapter

Can a medium involve \((a)\) conduction and convection, (b) conduction and radiation, or (c) convection and radiation simultaneously? Give examples for the "yes" answers.

A person's head can be approximated as a \(25-\mathrm{cm}\) diameter sphere at \(35^{\circ} \mathrm{C}\) with an emissivity of \(0.95\). Heat is lost from the head to the surrounding air at \(25^{\circ} \mathrm{C}\) by convection with a heat transfer coefficient of $11 \mathrm{~W} / \mathrm{m}^{2} \cdot \mathrm{K}\( and by radiation to the surrounding surfaces at \)10^{\circ} \mathrm{C}$. Disregarding the neck, determine the total rate of heat loss from the head. (a) \(22 \mathrm{~W}\) (b) \(27 \mathrm{~W}\) (c) \(49 \mathrm{~W}\) (d) \(172 \mathrm{~W}\) (e) \(249 \mathrm{~W}\)

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Water enters a pipe at \(20^{\circ} \mathrm{C}\) at a rate of $0.25 \mathrm{~kg} / \mathrm{s}\( and is heated to \)60^{\circ} \mathrm{C}$. The rate of heat transfer to the water is (a) \(10 \mathrm{~kW}\) (b) \(20.9 \mathrm{~kW}\) (c) \(41.8 \mathrm{~kW}\) (d) \(62.7 \mathrm{~kW}\) (e) \(167.2 \mathrm{~kW}\)

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