A uniform, solid sphere of radius 3 has its center on the origin in the x y z coordinate system. The sphere has 1 unit of mass per unit volume.
Consider a sub-region within the greater sphere. The sub-region is a sphere with radius 1 centered at ( x , y , z ) = ( 2 , 0 , 0 ) .
What is the magnitude of the net gravitational force on the mass within the sub-region?
Note: Universal gravitational constant G = 1 , for simplicity
Hint: I used a triple integral to solve this. It might also be possible to do this with a sextuple integral, but that is much more demanding (and there is a risk of singularities arising at the sub-region boundary). The triple integral avoids the singularities too.
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@Mark Hennings sir. I am not able to understand the first step of your solution. Please can you explain a bit??
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A small volume element d x d y d z is a distance ( x − 2 ) 2 + y 2 + z 2 away from the point ( 2 , 0 , 0 ) , and the line from the volume element to the point ( 2 , 0 , 0 ) makes an angle θ with the x -axis, where cos θ = ( x − 2 ) 2 + y 2 + z 2 x − 2 The gravitational force at the point ( 2 , 0 , 0 ) will (by symmetry) be its component along the x -axis, which is therefore ∭ ( x − 2 ) 2 + y 2 + z 2 G m ρ d x d y d z cos θ and we are done.
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@Mark Hennings sir. Density means mass per unit volume. So why you have multiplied density with mass ?? Can you explain me bit??
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@A Former Brilliant Member – The gravitational force between two objects of masses m 1 and m 2 is r 2 G m 1 m 2 , where r is the distance between them. The small volume element has mass ρ d x d y d z , while the test particle has mass m .
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The force F on the subregion due to the larger region is equal and opposite to the force on the larger region due to the subregion. Since the subregion is spherically symmetric, the gravitational field outside the subregion due to that subregion is equal to that of a point particle of the same mass m as the subregion at the centre of the subregion. This force clearly acts parallel to the x -axis, and so F has magnitude ∣ F ∣ = ∭ ( x − 2 ) 2 + y 2 + z 2 ≥ 1 x 2 + y 2 + z 2 ≤ 9 ( x − 2 ) 2 + y 2 + z 2 G m ρ × ( x − 2 ) 2 + y 2 + z 2 2 − x d x d y d z We are integrating over a volume of revolution, and we have G = ρ = 1 and m = 3 4 π , so that ∣ F ∣ = 3 4 π ∬ ( x − 2 ) 2 + y 2 ≥ 1 x 2 + y 2 ≤ 9 , y ≥ 0 ( ( x − 2 ) 2 + y 2 ) 2 3 2 π y ( 2 − x ) d x d y But then ∣ F ∣ = 3 8 π 2 ∫ − 3 1 ( ∫ 0 9 − x 2 ( ( x − 2 ) 2 + y 2 ) 2 3 y ( 2 − x ) d y ) d x + 3 8 π 2 ∫ 1 3 ( ∫ 1 − ( x − 2 ) 2 9 − x 2 ( ( x − 2 ) 2 + y 2 ) 2 3 y ( 2 − x ) d y ) d x = 3 8 π 2 ∫ − 3 1 [ − ( x − 2 ) 2 + y 2 2 − x ] y = 0 9 − x 2 d x + 3 8 π 2 ∫ 1 1 [ − ( x − 2 ) 2 + y 2 2 − x ] y = 1 − ( x − 2 ) 2 9 − x 2 d x = 3 8 π 2 ∫ − 3 1 { − 1 3 − 4 x 2 − x + 1 } d x + 3 8 π 2 ∫ 1 1 { − 1 3 − 4 x 2 − x + 2 − x } d x = 3 3 2 π 2 − 3 8 π 2 ∫ − 3 3 1 3 − 4 x 2 − x d x = 3 3 2 π 2 − 3 2 π 2 ∫ − 3 3 { 1 3 − 4 x − 1 3 − 4 x 5 } d x = 3 3 2 π 2 − 3 2 π 2 [ − 6 1 ( 1 3 − 4 x ) 2 3 + 2 5 1 3 − 4 x ] − 3 3 = 3 3 2 π 2 − 3 2 π 2 ( − 6 1 + 2 5 + 6 1 2 5 − 2 2 5 ) = 9 3 2 π 2 so a numerical integration is not necessary.