An electric kitchen range has a total wall area of m2 and is insulated with a layer of fiberglass cm thick. The inside surface of the fiberglass has a temperature of °C, and its outside surface is at °C. The fiberglass has a thermal conductivity of . What is the heat current through the insulation, assuming it may be treated as a flat slab with an area of m2 ?
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20. Heat and Temperature
Heat Transfer
Problem 72
Textbook Question
Most stars are main-sequence stars, a group of stars for which size, mass, surface temperature, and radiated power are closely related. The sun, for instance, is a yellow main-sequence star with a surface temperature of 5800 K. For a main-sequence star whose mass M is more than twice that of the sun, the total radiated power, relative to the sun, is approximately P/Psun=1.5(M/Msun)3.5. The star Regulus A is a bluish main-sequence star with mass 3.8Msun and radius 3.1Rsun. What is the surface temperature of Regulus A?

1
Step 1: Begin by understanding the Stefan-Boltzmann law, which relates the radiated power of a star to its surface temperature. The formula is P = σA(T^4), where P is the radiated power, σ is the Stefan-Boltzmann constant, A is the surface area of the star, and T is the surface temperature.
Step 2: Calculate the surface area of Regulus A using the formula for the surface area of a sphere, A = 4πR². Since the radius of Regulus A is given as 3.1Rₛᵤₙ, substitute this value into the formula to express the surface area in terms of the sun's radius.
Step 3: Use the given relationship for radiated power relative to the sun, P/Pₛᵤₙ = 1.5(M/Mₛᵤₙ)^3.5, to calculate the radiated power of Regulus A relative to the sun. Substitute the mass of Regulus A (3.8Mₛᵤₙ) into the formula.
Step 4: Combine the Stefan-Boltzmann law and the relative power formula. Express the surface temperature of Regulus A in terms of the sun's surface temperature (Tₛᵤₙ). Use the relationship T = (P / (σA))^(1/4) and substitute the values for P and A calculated in the previous steps.
Step 5: Simplify the expression for the surface temperature of Regulus A, ensuring all terms are expressed relative to the sun's values (Tₛᵤₙ, Rₛᵤₙ, etc.). This will give the surface temperature of Regulus A in terms of Tₛᵤₙ.

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Key Concepts
Here are the essential concepts you must grasp in order to answer the question correctly.
Main-Sequence Stars
Main-sequence stars are a category of stars that are in a stable phase of stellar evolution, where they fuse hydrogen into helium in their cores. Their properties, such as size, mass, surface temperature, and luminosity, are interrelated, following specific relationships defined by stellar models. The sun is a prime example of a main-sequence star, and understanding this category is crucial for analyzing other stars' characteristics.
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Stellar Mass-Luminosity Relation
The mass-luminosity relation describes how the luminosity (or total radiated power) of a star is related to its mass. For main-sequence stars, this relationship can be expressed as P/Pₛᵤₙ = (M/Mₛᵤₙ)³.⁵, indicating that more massive stars emit significantly more energy. This concept is essential for calculating the luminosity of stars like Regulus A based on its mass.
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Surface Temperature and Color
The surface temperature of a star is a critical factor that influences its color and spectral classification. Higher temperatures correspond to bluer stars, while lower temperatures correspond to redder stars. The temperature can be estimated using the Stefan-Boltzmann law, which relates luminosity, radius, and temperature, allowing for the determination of a star's surface temperature based on its luminosity and size.
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