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gravity inside a solid sphere
I'm having a hard time setting up a triple integral to find the force of gravity inside a solid sphere. I've done a similar proof in physics before with gravity inside a spherical shell, but it only required a single integral. In this problem the answer must be derived using a triple integral.
Newton's law of gravity:
|\vec{F_{grav}}|= \frac{GmpdV}{r^{2}}
I believe i found a way to set up the triple integral using spherical coordinates on another physics forum thread, but I don't understand how to get the integrand. Can someone please explain the way the intergrand was derived in the following integral?
Homework Statement
I'm having a hard time setting up a triple integral to find the force of gravity inside a solid sphere. I've done a similar proof in physics before with gravity inside a spherical shell, but it only required a single integral. In this problem the answer must be derived using a triple integral.
Homework Equations
Newton's law of gravity:
|\vec{F_{grav}}|= \frac{GmpdV}{r^{2}}
The Attempt at a Solution
I believe i found a way to set up the triple integral using spherical coordinates on another physics forum thread, but I don't understand how to get the integrand. Can someone please explain the way the intergrand was derived in the following integral?
arildno said:And, if you want to prove it mathematically using Newton's general law of gravitation and calculus techniques, here is most of it:
1. In spherical polar coordinates, let the position of a mass particle inside the ball be given by (\hat{r},\theta,\phi) (measured from the C.M)
where \phi is the angle between the vertical and the particle's position vector.
Let the density be constant for all sphere particles and the radius of the sphere R.
2. Consider a test particle P having mass m and position vector r\vec{k}, i.e, a distance r along the "vertical"
3. We need to sum up all forces acting on P from sphere particles, i.e, compute the integral:
\vec{F}=-G\rho{m}\int_{0}^{R}\int_{0}^{\pi}\int_{0}^{2\pi}\frac{\hat{r}^{2}\sin\phi((r-\hat{r}\cos\phi)\vec{k}-\hat{r}(\sin\phi(\cos\theta\vec{i}+\sin\theta\vec{j}))}{(\hat{r}^{2}+r^{2}-2r\hat{r}\cos\phi)^{\frac{3}{2}}}d\theta{d\phi}d\hat{r}
where G is the universal gravitation constant and \rho is the density of sphere particles.
4. It is easy to see that the horizontal plane components vanishes; the \phi-integration is then best handled by integration by parts.
In the \hat{r} integration, take care of whether you have r<\hat{r} or r>\hat{r}
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