How to calculate the gravitational field outside of a sphere

In summary, the student attempted to solve a problem involving the gravitational field between a solid sphere and a thin sheet of mass, but did not understand the concepts and ultimately used Gauss's law.
  • #1
Vitani11
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3

Homework Statement


A uniform solid sphere of mass M and radius R is fixed at a distance h above a thin infinite sheet of mass density σ. Obtain the magnitude of the force between the sphere and the sheet.

Homework Equations

The Attempt at a Solution


I've found the gravitational field from the sheet which turned out to be a constant. Now I need the gravitational field of the sphere outside of its radius at a point h. Wouldn't that just be -GM/(R+h)2?
 
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  • #2
I've found the gravitational field from the sheet which turned out to be a constant. Now I need the gravitational field of the sphere outside of its radius at a point h.

Why do you need that? How would you calculate the gravitational force on a body?
 
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  • #3
I don't know. I'm not good at physics at all - a lot of conceptual gaps here. Due to Newtons third law I can say that if I were to find the gravitational field due to the infinite sheet I can just multiply it by the mass of the sphere and then I have it, right? Here is the way I found the gravitational field of the infinite sheet:
∫g⋅dA = -4πGM
g∫dA = -4πGσA
g = -4πGσ

So I can then say the force between the two objects is

F = -4πGσM.

Thoughts?
 
  • #4
Obviously these are vectors.
 
  • #5
Close, but you need to make it clear what you're doing. For example, if you're trying to use Gauss's law for the entire plane, you haven't got a closed surface to integrate over. And the area and mass of the sheet are both infinite, so your first equation can't apply to the whole plane, and it's not clear exactly what you're trying to do when you cancel A from both sides--a procedure that is meaningless when the area is infinite.

The calculation can be done by treating the sheet as a set of elementary masses and adding up the resulting forces, but it needs some familiarity with multivariable integration.
.
 
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  • #6
Okay. So it would be better to not use Gauss law for this because this is not a closed surface? dF= -GMdm/(r2+h2). I changed dm to σ2πrdr so this became ∫dF = -GMσ2π∫r\(r2+h2)dr where the limits are from 0 to infinity. this makes sense to me, but when evaluating an integral a natural log comes up and its limit goes to infinity.
 
  • #7
I changed dm to σ2πrdr so this became ∫dF = -GMσ2π∫r\(r2+h2)dr

You need to take account of the fact that the force from your ring of matter is acting at an angle. By symmetry there are no horizontal forces in the resultant; so what you want is the vertical component of the force you have now--you need another factor of
h/(r2 + h2)1/2
inside the integral.

If need be, you could probably convince yourself about this by taking the vertical component of the force from a single element of your ring and then integrating round the circle.

Incidentally, you've obviously done this without much multivariable integration. I was thinking of the limit of a square plane, rather than a circular one. But of course they both give the same answer in the limit.
 
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  • #8
Solved. Thank you for the help - I'm aware that the horizontal components cancel I just was iffy on how to approach this problem because it seemed a lot more complicated than it is.
 
  • #9
Glad it worked out.

Just for completeness: You can use Gauss's law for this calculation. I don't think I've ever done it that way, but you might find it quicker if you get comfortable with the concepts. It involves constructing a (small) cylindrical closed surface. Look for articles on the Gaussian Pillbox, if you're interested.
 
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1. What is the formula for calculating the gravitational field outside of a sphere?

The formula for calculating the gravitational field outside of a sphere is: Gm/r^2, where G is the gravitational constant, m is the mass of the sphere, and r is the distance from the center of the sphere to the point where the gravitational field is being calculated.

2. How do you determine the direction of the gravitational field outside of a sphere?

The direction of the gravitational field outside of a sphere is always inwards, towards the center of the sphere. This is because the force of gravity is always attractive, pulling objects towards each other.

3. What units are used for the gravitational field outside of a sphere?

The units for the gravitational field outside of a sphere are Newtons per kilogram (N/kg) or meters per second squared (m/s^2). These units represent the strength of the gravitational force per unit mass of an object.

4. Is the gravitational field outside of a sphere affected by the mass of the object?

Yes, the gravitational field outside of a sphere is directly proportional to the mass of the object. This means that as the mass of the object increases, the strength of the gravitational field also increases.

5. How does the distance from the center of the sphere affect the gravitational field outside of the sphere?

The gravitational field outside of a sphere is inversely proportional to the square of the distance from the center of the sphere. This means that as the distance increases, the strength of the gravitational field decreases. This relationship follows the inverse square law.

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