Holed on

A sphere of uniform mass density ρ \rho and radius a + b a+b has a spherical hole of radius b b drilled a distance a a from its center. The gravitational field is measured at the far side of the hole (at the blue point) and is found to be g 0 . g_0.

What will the field measure at the near side of the hole (at the green point)?

a ( a + b ) g 0 \frac{a}{\left(a+b\right)} g_0 g 0 g_0 a 2 ( a + b ) 2 g 0 \frac{a^2}{\left(a+b\right)^2} g_0 ( a + b ) ( a b ) g 0 \frac{\left(a+b\right)}{\left(a-b\right)} g_0

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5 solutions

Arjen Vreugdenhil
May 29, 2017

Principle : The field of a homogeneous sphere of radius R R at a point at distance d R d \leq R from its center points inward and is proportional to ρ d \rho d , where ρ \rho is the density.

First, consider the field of a solid sphere of radius a + b a + b , without the hole. For the blue point we have d = a + b d = a + b ; for the green point we have d = a b d = a - b ; so we find that g 1 , b l = a + b , g 1 , g n = a b . \vec g_{1,bl} = a + b,\ \ \ \vec g_{1,gn} = a - b. We choose units so that the proportionality constant involving density, G G , and other constant factors is equal to 1. Moreover, the positive direction is chosen toward the center of the large sphere.

Next, consider the field of a solid sphere of radius b b that would fit in the hole. For both points we have d = b d = b , so we get g 2 , b l = b , g 2 , g n = b . \vec g_{2,bl} = b,\ \ \ \vec g_{2,gn} = -b.

Now for the given shape, which at the given points has fields g 0 = g 3 , b l \vec g_0 = \vec g_{3,bl} and g = g 3 , g n \vec g' = \vec g_{3,gn} , respectively. By the superposition principle, if we add the field of this shape and the field of the small sphere together, we should find the field of the large solid sphere. Thus { g 1 , b l = g 2 , b l + g 3 , b l g 1 , g n = g 2 , g n + g 3 , g n { a + b = b + g 0 a b = b + g { g 0 = a g = a \begin{cases} \vec g_{1,bl} = \vec g_{2,bl} + \vec g_{3,bl} \\ \vec g_{1,gn} = \vec g_{2,gn} + \vec g_{3,gn} \end{cases} \longrightarrow \begin{cases} a+b = b + g_0 \\ a-b = -b + g' \end{cases} \longrightarrow \begin{cases} g_0 = a \\ g' = a \end{cases} We see immediately that g = g 0 \boxed{g' = g_0} .

Let P P be a point on the line segment connecting the green and blue points, at distance d d from the center of the large sphere ( a b d a + b a - b \leq d \leq a+b ). Then at point P P , g = g = g 0 g = g' = g_0 . In other words, along this line the gravitational field along this line segment is homogeneous!

Arjen Vreugdenhil - 4 years ago

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We can prove a stronger statement here, that the field is uniform in the entire cavity. This is true regardless of the shape and size of the cavity.

Pranshu Gaba - 4 years ago

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True. The argument is the same, but involves vectors. Let P P be a point in the cavity, with position r \vec r relative to the center of the large sphere, and therefore with position r r 0 \vec r - \vec r_0 with respect to the center r 0 \vec r_0 of the cavity. Then the field at point P P due to the large sphere is proportional to r \vec r , and a sphere filling the cavity would produce field proportional to r r 0 \vec r - \vec r_0 . Therefore the field is actually g r ( r r 0 ) = r 0 \vec g \propto \vec r - (\vec r - \vec r_0) = \vec r_0 independent of the choice of P P , as long as it's inside the cavity.

In other words, spherical cavities create uniform fields!

Arjen Vreugdenhil - 4 years ago

What a beautiful solution, and well-summarized takeaway! Awesome job, Arjen.

Eli Ross Staff - 4 years ago

@Arjen Vreugdenhil Is the field inside cavity always uniform and proportional to distance between their centres if there are 2 or more than 2 cavities?

Nitish Deshpande - 4 years ago

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No. The conclusion that the field inside the cavity is uniform depends essentially on the fact that inside a homogeneous sphere, there is a linear relationship between the gravitational field and the position vector: g r . \vec g \propto -\vec r.

However, outside the sphere it becomes g r r 3 . \vec g \propto \frac{-\vec r}{r^3}. If there are two cavities, then being inside one cavity means being outside the other; this introduces an additional term, which is not linear in r \vec r .

Arjen Vreugdenhil - 4 years ago

Why is it that Gauss's Law for Gravity doesn't work for this situation?

Diego Chavez - 3 years, 4 months ago

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It works-- the only question is, how would you apply it to solve this problem?

Arjen Vreugdenhil - 3 years, 4 months ago
Tapas Mazumdar
May 29, 2017

Let the mass of the larger sphere be M M and the mass of the smaller sphere cut out to make the hole be m m .

Given that

ρ = Mass of large sphere Volume of large sphere = M 4 3 π ( a + b ) 3 \rho = \dfrac{\text{Mass of large sphere}}{\text{Volume of large sphere}} = \dfrac{M}{\frac 43 \pi (a+b)^3}

Therefore

m = ρ ( 4 3 π b 3 ) = M 4 3 π ( a + b ) 3 4 3 π b 3 = M ( b a + b ) 3 m = \rho \left( \dfrac 43 \pi b^3 \right) = \dfrac{M}{\frac 43 \pi (a+b)^3} \cdot \dfrac 43 \pi b^3 = M {\left( \dfrac{b}{a+b} \right)}^3

At blue point \color{#3D99F6} \text{ blue point } the gravitational field lines due to both spheres is directed in the same direction. Since the direction is same so let us consider the sense of both gravitational fields to be in positive sense. Thus at the blue point, we have

E large sphere = G M ( a + b ) 2 E small sphere = G m b 2 = G M b ( a + b ) 3 \begin{aligned} & E_{\text{large sphere}} = \dfrac{GM}{(a+b)^2} \\ & E_{\text{small sphere}} = \dfrac{Gm}{b^2} = \dfrac{GMb}{(a+b)^3} \end{aligned}

As the small sphere is 'carved out', so the net field at blue point (by the principle of superposition) is

E net at blue = E large sphere E small sphere = G M ( 1 ( a + b ) 2 b ( a + b ) 3 ) = G M a ( a + b ) 3 E_{\text{net at blue}} = E_{\text{large sphere}} - E_{\text{small sphere}} = GM \left( \dfrac{1}{(a+b)^2} - \dfrac{b}{(a+b)^3} \right) = \dfrac{GMa}{(a+b)^3}

At green point \color{#20A900} \text{ green point } the gravitational field lines due to both spheres is directed in opposite directions. As the direction is opposite so let us consider the gravitational field of larger sphere to be positive while that of the smaller one to be negative. Thus at the green point, we have

E large sphere = G M ( a b ) ( a + b ) 3 E small sphere = G m b 2 = G M b ( a + b ) 3 \begin{aligned} & E_{\text{large sphere}} = \dfrac{GM(a-b)}{(a+b)^3} \\ & E_{\text{small sphere}} = -\dfrac{Gm}{b^2} = -\dfrac{GMb}{(a+b)^3} \end{aligned}

The net field at green point (by the principle of superposition) is

E net at green = E large sphere E small sphere = G M ( a b ( a + b ) 3 + b ( a + b ) 3 ) = G M a ( a + b ) 3 E_{\text{net at green}} = E_{\text{large sphere}} - E_{\text{small sphere}} = GM \left( \dfrac{a-b}{(a+b)^3} + \dfrac{b}{(a+b)^3} \right) = \dfrac{GMa}{(a+b)^3}

We find that

E net at blue = E net at green E_{\text{net at blue}} = E_{\text{net at green}}

Thus we get

E net at green = g 0 E_{\text{net at green}} = \boxed{g_0}

Could you please explain how you derived the gravitational field of the large sphere at the green point? I really can't see how you produced it Thanks.

Utsav Garg - 4 years ago

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The formula for gravitational field inside a sphere of radius R R and mass M M at a distance r r from its center is given by

E = G M r R 3 E = \dfrac{GMr}{R^3}

I am giving the derivation of this formula but for this you need to be familiar with the gravitational equivalent of the Gauss' law.


Consider a smaller sphere with radius r r whose center coincides with that of the original sphere, knowing the value of mass density of the original sphere ρ = M 4 3 π R 3 \rho = \dfrac{M}{\frac 43 \pi R^3} , we see that the mass of this sphere is

m = ρ ( 4 3 π r 3 ) = M r 3 R 3 m = \rho \left( \dfrac 43 \pi r^3 \right) = M \dfrac{r^3}{R^3}

By the Gauss' law

Φ = E d S = 4 π G m \Phi = \oint E \cdot dS = - 4 \pi G m

where E E is uniform and d S \oint dS gives the surface area of the smaller sphere which is nothing but 4 π r 2 4 \pi r^2 . Thus we have

Note: We consider m m here instead of M M because Gauss' law takes the mass within the Gaussian surface and not outside it.

E ( 4 π r 2 ) = 4 π G M r 3 R 3 E (4 \pi r^2) = - 4 \pi G M \dfrac{r^3}{R^3}

which gives

E = G M r R 3 E = - \dfrac{GMr}{R^3}

Note: The negative sign shows that gravitational field is directed towards the center of the sphere.

Tapas Mazumdar - 4 years ago

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Thanks this was quite helpful

Utsav Garg - 4 years ago

I thought you could calculate gravitational field with /(Gm/r^2/). Clearly Gm is a constant, and r is the distance from the center of mass. The only way the two equations can be equal is if a and b are equidistant from the center of mass, which they clearly are not. Can someone explain where I went wrong?

Alex Li - 4 years ago

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Ahh, your formula is not correct. The formula G m r 2 \frac{Gm}{r^2} is applicable for a uniform sphere at any point outside the sphere. But, here we've considered a point inside the sphere where the gravitational field is given by, E = 4 π G ρ r 3 E= \frac{4 \pi G \rho r}{3} .

Rohit Gupta - 4 years ago
Ujjwal Rane
May 31, 2017

Gravitational field at the surface of a solid sphere of mass M, radius R and density ρ \rho is given by g = G M R 2 = G 4 / 3 π R 3 ρ R 2 = G 4 π R ρ 3 g = G\frac{M}{R^2} = G\frac{4/3 \pi R^3 \rho}{R^2} = G\frac{4 \pi R \rho}{3} We will use this general form repeatedly now.

The hole can be treated as having density ρ -\rho or a sphere that produces a 'repulsive' field! Moreover, since at the given points both the fields, have the same line of action, they can be added or subtracted algebraically.

At the blue point net field = G 4 π ( a + b ) ρ 3 G 4 π b ρ 3 = G 4 π a ρ 3 = g 0 G\frac{4 \pi (a+b) \rho}{3} - G\frac{4 \pi b \rho}{3} = G\frac{4 \pi a \rho}{3} = g_0

At the green point net field = G 4 π ( a b ) ρ 3 + G 4 π b ρ 3 = G 4 π a ρ 3 = g 0 G\frac{4 \pi (a-b) \rho}{3} + G\frac{4 \pi b \rho}{3} = G\frac{4 \pi a \rho}{3} = g_0

You have used the formula for the field at the surface of a sphere. What about the field at a point inside the sphere?

Rohit Gupta - 4 years ago

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You are right! At the green point, we indeed need the formula for field inside the sphere. But for a solid sphere of uniform density, only the concentric 'sub-sphere' between the green point and the center is going to exert any force. The field equation remains the same as that of a surface of a sphere. Only the radius need to be changed to (a-b). That is the formula used at the green point.

Ujjwal Rane - 4 years ago

A simpler way would be to notice that the gravitational field must be constant( UNIFORM!) inside the cavity ( it is a pretty standard result, in both gravitation and electrostatics, so I skip the proof; which is easily obtained from simple vector laws), and is given as 4 / 3 π G ρ r 4/3\pi G\rho\vec{r} , where r \vec{r} is the position vector of the center of cavity wrt the center of sphere. Clearly, it is independent of the position of any arbitrary point inside the cavity. Hence the result.

Abdelhamid Saadi
May 29, 2017

The idea of the solution is the actual field can be calculated by the difference between the field of a sphere without hole and field of a sphere with same density filling the hole.

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