Solid hemisphere center of mass in spherical coordinates

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Homework Help Overview

The discussion revolves around finding the center of mass of a solid hemisphere with constant density using spherical coordinates. Participants are examining the setup and calculations involved in the center of mass formula.

Discussion Character

  • Exploratory, Mathematical reasoning, Assumption checking

Approaches and Questions Raised

  • The original poster attempts to compute the center of mass using an integral approach but encounters unexpected results. Some participants question the derivation of the center of mass equation and the completeness of the integral setup.

Discussion Status

Participants are actively engaging with the problem, raising questions about the integral's formulation and the assumptions made regarding the density and volume. There is a recognition of the need to clarify the vector nature of the position in the context of the integral.

Contextual Notes

Some participants note potential missing terms in the integral related to the Jacobian and the representation of the position vector in spherical coordinates. The discussion reflects on the implications of symmetry in the problem setup.

Ledamien
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Hello,

I am struggling with what was supposed to be the simplest calc problem in spherical coordinates. I am trying to fid the center of mass of a solid hemisphere with a constant density, and I get a weird result.
First, I compute the mass, then apply the center of mass formula. I divide both and voila, obviously wrong result. What is wrong here?

Cm = 1 / M \int \rho r^3 sin \theta dr d\theta d\varphi

M = ρ V → 1/M = 1/ρV

V = 2 \pi R^3 / 3

Cm = 3/ (2 \pi R^3) \int r^3 sin \theta dr d\theta d\varphi

Integrated over:
r → 0 to R
\theta → 0 to \pi/2
\varphi → 0 to 2 \pi

Cm = 3/ (2 \pi R^3) * \pi R^4 / 2
Cm = 3R / 4

So, what do I do wrong?
 
Last edited:
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How did you derive your equation for the Cm?
 
Ledamien said:
\int \rho r^3 sin \theta dr d\theta d\varphi
Isn't there a trig term missing in that integral? There should be one from the Jacobian and another for the fact that you're interested in the displacement in only one Cartesian coordinate.
 
1/M \sum mi ri
1/M\int \rho(r) r dV - this is a volume integral.
1/M\int [\rho(r) r] r^2 dr sin \theta) d\theta d\varphi - this is a volume integral in spherical coordinates.
My idea was that a simple volume integral for a hemisphere, going from 0 to r, 0 to \pi/2 and 0 to 2\pi would be sufficient. As the density is constant I can pull it out of the integral, and \rho/M is simply 1/V, one over the total volume - the same integral but with r^2 instead of r^3. I seem to be missing a 1/2 somewhere, but where?
 
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Ledamien said:
1/M \sum mi ri
1/M\int \rho(r) r dV - this is a volume integral.
What exactly does ri stand for in the first line? What is the appropriate formula to replace it in the second?
 
ri is the vector position of a mass in some direction. I know that by symmetry it should be on the z axis. Should I multiply the whole thing be z hat in spherical (cos\theta - sin\theta). That does not make much sense, and it does not work.
 
Ledamien said:
ri is the vector position of a mass in some direction.
Yes, it's a vector. But you have replaced it by r, the magnitude of the vector. You cannot do that because in the integral the components of the vector in the x and y directions would cancel.
Should I multiply the whole thing be z hat in spherical (cos\theta - sin\theta). That does not make much sense, and it does not work.
Multiplying by sin or cos of theta (depending on which way it's measured) makes sense to me.
 
OK I got it, I skipped a step:
Cm = 1/V\int r (r hat) dV
As I know it's on the z axis:
Cm = 1/V\int z (z hat) dV

z = r cos\theta
dV = r^2 sin\thetadr d\theta d\varphi

Cm = 1/V\intr cos\theta (z hat) r^2 sin\thetadr d\theta d\varphi

I can pull out z hat from the integral.

With V = (2\piR^3)/3, this gives me 3R/8 (z hat).

Well, that was silly...

Thank you guys for your help.
 
Last edited:

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