Ellipsoidal Shell Gravity

A massive ellipsoidal shell has the following form:

x 2 4 + y 2 1 + z 2 1 = 1 \frac{x^2}{4} + \frac{y^2}{1} + \frac{z^2}{1} = 1

The shell has σ \sigma units of mass per unit surface area. A point particle of mass m m is positioned at ( x , y , z ) = ( 1 , 0 , 0 ) (x,y,z) = (1,0,0) . The universal gravitational constant is G G .

What is the magnitude of the gravitational force exerted by the shell on the particle?

Details and Assumptions:
1) σ = 1 \sigma = 1
2) m = 1 m = 1
3) G = 1 G = 1 (for simplicity)


The answer is 1.077.

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2 solutions

Karan Chatrath
Jun 13, 2019

Let the position vector of a point on the surface be:

r = x i ^ + y j ^ + z k ^ \vec{r} = x \hat{i} + y \hat{j} + z \hat{k}

The position vector of the point of interest (at which force needs to be computed) is:

r p = 1 i ^ + 0 j ^ + 0 k ^ \vec{r}_p = 1 \hat{i} + 0 \hat{j} + 0 \hat{k}

It is given that the mass per unit area of this ellipsoid is unity. Let us consider a small area element which is a part of the surface. The surface area of this is computed as follows:

z = 1 x 2 4 y 2 z = \sqrt{1 - \frac{x^2}{4} - y^2}

or,

z = f ( x , y ) z = f(x,y)

Which implies: z f ( x , y ) = ϕ = 0 z - f(x,y) = \phi = 0 . The gradient of this expression is:

( ϕ ) = f x i ^ f y j ^ + 1 k ^ \nabla(\phi)= - f_x \hat{i} - f_y \hat{j} + 1 \hat{k}

Where f x f_x and f y f_y are partial derivatives of f ( x , y ) f(x,y) with respect to x x and y y respectively. Therefore, the mass of this element is:

d M = σ ( ϕ ) d y d x dM = \sigma \mid\nabla(\phi)\mid dydx

The gravitational force can be computed by using the inverse square law:

d F = d F x i ^ + d F y j ^ + d F z k ^ d\vec{F} = dF_x \hat{i} + dF_y \hat{j} + dF_z \hat{k}

or:

d F = G ( d M ) m r r p 2 ( r r p r r p ) d\vec{F} = \frac{G(dM)m}{\mid\vec{r} - \vec{r}_p\mid^2}\bigg(\frac{\vec{r} - \vec{r}_p}{\mid\vec{r} - \vec{r}_p\mid}\bigg)

Integrating this over the elliptical region x 2 4 + y 2 = 1 \frac{x^2}{4} + y^2 = 1 , multiplying the answer by 2 (since only the top half of the surface is considered here), and taking the magnitude of the resultant, gives us the answer of 1.085 . This is different from 1.077. I got lucky. Posting this not so detailed solution to know if I made a mistake.

Looks like we did it the exact same way, qualitatively. For my final run, I used Δ x = Δ y = 1 20000 \Delta x = \Delta y = \frac{1}{20 000} for the region in the x y xy plane. That resulted in 400 × 1 0 6 400 \times 10^6 elements for each half of the ellipsoid (top and bottom). I ran it several other times before that with bigger deltas to check for convergence of the result.

Steven Chase - 1 year, 12 months ago

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Okay, so the difference in results is due to numerical reasons as opposed to a conceptual reason. That is reassuring. Thank you

Karan Chatrath - 1 year, 12 months ago

My result is admittedly not perfect, but it should be "good enough" so as not to give false negatives. Our results are only different by seven tenths of one percent, and the Brilliant decimal answer margin is three percent.

Steven Chase - 1 year, 12 months ago

I have a question here. What about Gauss' theorem? According to this theorem, the flux of gravitational field over any closed surface within the shell is -4πG times the mass of the gravitating body enclosed by the surface, which is zero. Where am I going wrong?

A Former Brilliant Member - 1 year, 12 months ago

I agree. The net flux over any closed surface within the shell is zero. But the field need not be zero at each point on that surface.

Steven Chase - 1 year, 12 months ago
Mark Hennings
Jun 13, 2019

Since the ellipsoid is a solid of revolution, the gravitational force at the point ( 1 , 0 , 0 ) (1,0,0) acts along the x x -axis, and has magnitude 0 π 2 cos t 1 ( 2 cos t 1 ) 2 + sin 2 t × G m σ 2 π sin t 4 sin 2 t + cos 2 t d t ( 2 cos t 1 ) 2 + cos 2 t = G m σ 0 π 2 π sin t 1 + 3 sin 2 t ( 2 4 cos t + 3 cos 2 t ) 3 2 d t \int_0^\pi \frac{2\cos t - 1}{\sqrt{(2\cos t - 1)^2 + \sin^2t}} \times \frac{Gm\sigma 2\pi \sin t \sqrt{4\sin^2t + \cos^2t}\,dt}{(2\cos t - 1)^2 + \cos^2t} \; = \; Gm\sigma \int_0^\pi \frac{2\pi \sin t \sqrt{1 + 3\sin^2t}}{(2 -4\cos t + 3\cos^2t)^{\frac32}}\,dt which equals 1.085033 M G σ 1.085033MG\sigma after numerical integration. This makes the answer 1.085033 \boxed{1.085033} .

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