Calculating Centre of Mass for Northern Hemisphere Using Spherical Coordinates

In summary, the conversation discusses how to calculate the z-component of the centre of mass for a northern hemisphere with constant density using spherical coordinates. The equations for calculating the centre of mass and mass are provided, and there is a question about the limits of integration for \theta. The correct limits are determined to be [0,π/2] for both calculations.
  • #1
Ted123
446
0

Homework Statement



Calculate the z-component of the centre of mass for a northern hemisphere of radius [itex]R[/itex] with constant density [itex]\rho_0 > 0[/itex] using spherical coordinates [itex](r,\theta, \varphi )[/itex] defined by:

[itex]x(r,\theta, \varphi) = r\sin\theta\cos\varphi \;\;\;\;\;\;0 \leq r < \infty[/itex]
[itex]y(r,\theta, \varphi) = r\sin\theta\sin\varphi \;\;\;\;\;\;\, 0 \leq \theta \leq \pi[/itex]
[itex]z(r,\theta, \varphi) = r\cos\theta \;\;\;\;\;\;\;\;\;\;\;\;\;\; 0 \leq \varphi < 2\pi[/itex]

Homework Equations



For a solid with density [itex]\rho (\bf{r})[/itex] occupying a region [itex]\cal{R}[/itex],

[itex] z_{cm} = \frac{1}{M} \iiint_{\cal{R}} z \rho (\bf{r})\;dV[/itex]

where [itex]M= \iiint_{\cal{R}} \rho (\bf{r})\;dV[/itex]

The Attempt at a Solution



I have the solution but I'm wondering why the limits of [itex]\theta[/itex] is [itex][0,\pi /2][/itex] for calculating M then it changes to [itex][0,\pi][/itex] when calculating [itex]z_{cm}[/itex] ?

[itex]M = \iiint _{\cal{R}} \rho_0\;dV = \int_0^R dr \int_0^{\frac{\pi}{2}} d\theta \int_0^{2\pi} d\varphi \; r^2\sin\theta = \frac{2\pi}{3}R^3 \rho_0[/itex].

[itex]Mz_{cm} = \iiint _{\cal{R}} z \rho_0\;dV = \int_0^R dr \int_0^{\pi} d\theta \int_0^{2\pi} d\varphi \; r\cos\theta r^2\sin\theta = M \frac{3}{8} R[/itex].
 
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  • #2
have tried carrying through the integration? i think it should be pi/2 as well...
 
  • #3
Hi Ted123! :wink:

It's wrong …

it must be [0,π/2] for both. :smile:
 

Related to Calculating Centre of Mass for Northern Hemisphere Using Spherical Coordinates

What are spherical coordinates and how are they used?

Spherical coordinates are a coordinate system used to locate points in three-dimensional space. They are particularly useful for describing the positions of objects in space and for solving problems in physics and mathematics. Spherical coordinates consist of a radius, an azimuth angle, and an elevation angle.

What is the difference between spherical coordinates and Cartesian coordinates?

The main difference between spherical coordinates and Cartesian coordinates is the way they measure distance and angles. Spherical coordinates use a radial distance, an azimuth angle, and an elevation angle, while Cartesian coordinates use three orthogonal axes (x, y, and z) to locate a point in space.

What are the advantages of using spherical coordinates?

Spherical coordinates have several advantages, including their ability to describe the positions of objects in space accurately, their usefulness for solving problems in physics and mathematics, and their ability to simplify certain mathematical equations.

How do you convert spherical coordinates to Cartesian coordinates?

To convert spherical coordinates to Cartesian coordinates, you can use the following equations:
x = r * sin(θ) * cos(φ)
y = r * sin(θ) * sin(φ)
z = r * cos(θ)
Where r is the radial distance, θ is the azimuth angle, and φ is the elevation angle.

What are some real-world applications of spherical coordinates?

Spherical coordinates have many real-world applications, such as in navigation systems, satellite communication, and astronomy. They are also commonly used in physics and mathematics to solve problems involving three-dimensional space and spherical objects.

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