Simple Surface Integral - Heat Flow on Surface of Star

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Homework Help Overview

The problem involves calculating the rate of heat flow across the surface of a star modeled as a sphere with a given temperature distribution defined by the function u = 1/sqrt(x^2+y^2+z^2). The star has a radius of 5, and the original poster expresses confusion regarding their attempts to solve the surface integral and the resulting values.

Discussion Character

  • Exploratory, Assumption checking, Mathematical reasoning

Approaches and Questions Raised

  • The original poster attempts to evaluate the surface integral using two methods, questioning why their logic leads to an incorrect answer despite following the correct procedures. They also consider whether the surface integral should simply be the product of the surface area and the value of the function u at the surface.

Discussion Status

Participants are exploring the relationship between the function u and the surface integral, with some questioning whether the function f used in the integral is indeed equal to u. There is an ongoing examination of the parameterization and the implications of the radius on the calculations.

Contextual Notes

The original poster mentions receiving the correct answer from someone else but is uncertain about the reasoning behind their own calculations leading to a different result. There is a focus on understanding the assumptions made in the problem setup and the definitions of the variables involved.

wadawalnut
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Homework Statement


I have this problem in an online assignment. Someone told me the answer, so I already got it right, but I don't know why my logic leads me to the wrong answer. The problem:
The temperature u of a star of conductivity 1 is defined by u = \frac{1}{sqrt(x^2+y^2+z^2)}. If the star is a sphere of radius 5, find the rate of heat flow outward across the surface of the star.

Homework Equations


Surface integral: \int \int_S f(x,y,z) * dS
Surface area of sphere = 4\pi r^2
The correct answer is 4\pi

The Attempt at a Solution


I tried this two ways and got the same answer both ways, unfortunately this answer isn't correct.
First method was flat out doing the integral. Firstly, it is clear that u = \frac{1}{| \vec{r} |}. However, the radius on the surface of the sphere is always 5, so u = \frac{1}{5}. If we use the parametrization \vec{r} = (\rho \cos(\theta)\sin(\phi), \rho \sin(\theta) \sin(\phi), \rho \cos(\phi)) And dS is \rho^2 \sin(\phi) d\phi d\theta. Once again, \rho = 5 for every point on the surface of the star. Now we can fill out the surface integral:
\int_0^{\pi} \int_0^{2\pi} \frac{1}{5} * 25\sin(\phi)d\theta d\phi \\<br /> = 5 \int_0^{\pi} \int_0^{2\pi} \sin(\phi) d\theta d\phi \\<br /> = 10\pi \int_0^{\pi} \sin(\phi) d\phi \\<br /> = 10\pi (-\cos(\phi))|_0^{\pi} = 20\pi
I knew that wasn't correct, so I thought of an alternative: At each point on the surface, the value of the function is just \frac{1}{r} = \frac{1}{5}. So shouldn't the surface integral evaluate to the surface area of the sphere multiplied by the function u, and thus \frac{4\pi 5^2}{5} = 20\pi?
It seems like the value doesn't depend on the radius.
Can someone explain this to me?
 
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wadawalnut said:

Homework Statement


I have this problem in an online assignment. Someone told me the answer, so I already got it right, but I don't know why my logic leads me to the wrong answer. The problem:
The temperature u of a star of conductivity 1 is defined by u = \frac{1}{sqrt(x^2+y^2+z^2)}. If the star is a sphere of radius 5, find the rate of heat flow outward across the surface of the star.

Homework Equations


Surface integral: \int \int_S f(x,y,z) * dS
Surface area of sphere = 4\pi r^2
The correct answer is 4\pi

The Attempt at a Solution


I tried this two ways and got the same answer both ways, unfortunately this answer isn't correct.
First method was flat out doing the integral. Firstly, it is clear that u = \frac{1}{| \vec{r} |}. However, the radius on the surface of the sphere is always 5, so u = \frac{1}{5}. If we use the parametrization \vec{r} = (\rho \cos(\theta)\sin(\phi), \rho \sin(\theta) \sin(\phi), \rho \cos(\phi)) And dS is \rho^2 \sin(\phi) d\phi d\theta. Once again, \rho = 5 for every point on the surface of the star. Now we can fill out the surface integral:
\int_0^{\pi} \int_0^{2\pi} \frac{1}{5} * 25\sin(\phi)d\theta d\phi \\<br /> = 5 \int_0^{\pi} \int_0^{2\pi} \sin(\phi) d\theta d\phi \\<br /> = 10\pi \int_0^{\pi} \sin(\phi) d\phi \\<br /> = 10\pi (-\cos(\phi))|_0^{\pi} = 20\pi
I knew that wasn't correct, so I thought of an alternative: At each point on the surface, the value of the function is just \frac{1}{r} = \frac{1}{5}. So shouldn't the surface integral evaluate to the surface area of the sphere multiplied by the function u, and thus \frac{4\pi 5^2}{5} = 20\pi?
It seems like the value doesn't depend on the radius.
Can someone explain this to me?

Your ##u = u(x,y,z)## is the temperature at the point ##(x,y,z)## in the star. How is the rate of heat flow across the star's surface related to the function ##u##? In other words, how is your function ##f(x,y,z)## obtained from the function ##u(x,y,z)##?
 
Last edited:
In general:

$$\iint_S f(x, y, z) \space dS = \iint_D f(\vec r(u, v)) |\vec r_u \times \vec r_v| \space dA$$

For this particular problem we can adapt the notation:

$$\iint_S u(x, y, z) \space dS = \iint_D u(\vec r(\theta, \phi)) |\vec r_{\theta} \times \vec r_{\phi}| \space dA$$

You need to find a suitable ##\vec r(\theta, \phi)##, and project the sphere onto the x-y plane to obtain the region ##D##. Take ##\rho = 5## for the parameterization.
 
Zondrina said:
In general:

$$\iint_S f(x, y, z) \space dS = \iint_D f(\vec r(u, v)) |\vec r_u \times \vec r_v| \space dA$$

For this particular problem we can adapt the notation:

$$\iint_S u(x, y, z) \space dS = \iint_D u(\vec r(\theta, \phi)) |\vec r_{\theta} \times \vec r_{\phi}| \space dA$$

You need to find a suitable ##\vec r(\theta, \phi)##, and project the sphere onto the x-y plane to obtain the region ##D##. Take ##\rho = 5## for the parameterization.

Do we know that ##f = u##? I asked the OP that, but have received no response.
 

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