There is a circular disk of radius in the plane, centered on the origin. The disk has a mass density of
The disk explodes into a sort of dust, with each infinitesimal piece of disk having an initial speed . The initial motion of each infinitesimal piece is in the direction of a unit vector going from point to the respective piece.
After the initial explosion, each piece of disk travels under the influence of gravity, which has a magnitude of and points in the negative direction.
Once each piece of disk lands again in the plane, it remains in that position. What is the moment of inertia of the final mass distribution about the axis?
Bonus: Make a plot of the final mass distribution
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This recent news comes as a disappointment to me. But I am sure to enjoy this last streak of problems.
Consider an elementary mass being projected from the point ( r cos θ , r sin θ , 0 ) , where 0 ≤ r ≤ 1 and 0 ≤ θ ≤ 2 π .
The velocity of projection is:
v o = v x o i ^ + v y o j ^ + v z o k ^ v o = v o ⎝ ⎜ ⎜ ⎛ ∣ ∣ ∣ ∣ ( r cos θ i ^ + r sin θ j ^ ) − ( − 1 i ^ + 0 j ^ − 1 k ^ ) ∣ ∣ ∣ ∣ ( r cos θ i ^ + r sin θ j ^ ) − ( − 1 i ^ + 0 j ^ − 1 k ^ ) ⎠ ⎟ ⎟ ⎞
This leads to:
v x o = r 2 + 2 r cos θ + 2 1 0 ( r cos θ + 1 ) v y o = r 2 + 2 r cos θ + 2 1 0 r sin θ v z o = r 2 + 2 r cos θ + 2 1 0
Now, as the mass element is projected from the specified point, its motion is governed by the following set of ODEs:
x ¨ = 0 ; y ¨ = 0 ; z ¨ = − 1 0 x ˙ ( 0 ) = v x o ; y ˙ ( 0 ) = v y o ; z ˙ ( 0 ) = v z o x ( 0 ) = r cos θ ; y ( 0 ) = r sin θ ; z ( 0 ) = 0
Solving this system of equations leads to:
x = v x o t + r cos θ ; y = v y o t + r sin θ ; z = v z o t − 5 t 2
Now, the mass element's final position is when its z coordinate becomes zero. This happens at time:
t f = 5 v z o
The final x and y coordinates of the mass element are:
x f = v x o t f + r cos θ y f = v y o t f + r sin θ
After simplification:
x f = r cos θ + r 2 + 2 r cos θ + 2 2 0 ( r cos θ + 1 ) y f = r sin θ + r 2 + 2 r cos θ + 2 2 0 r sin θ
Now, the mass of the mass element is: d m = σ r d r d θ ; σ = 1 . Therefore, the moment of inertia of the mass element about the Z axis when it reaches its final position is:
d I = ( x f 2 + y f 2 ) d m
Simplifying:
d I = ( r 2 + r 2 + 2 r cos θ + 2 4 0 r 2 + 4 0 r cos θ + ( r 2 + 2 r cos θ + 2 ) 2 4 0 0 ( r 2 + 2 r cos θ + 1 ) ) r d r d θ
Finally, the total moment of inertia about the Z axis is:
I = ∫ 0 2 π ∫ 0 1 ( r 2 + r 2 + 2 r cos θ + 2 4 0 r 2 + 4 0 r cos θ + ( r 2 + 2 r cos θ + 2 ) 2 4 0 0 ( r 2 + 2 r cos θ + 1 ) ) r d r d θ ≈ 2 7 6 . 1 4 7 4
The mass distribution is as follows:
r is varied in steps of 0.04 and θ is varied is steps of π / 5 0 . The points in red indicate the initial mass distribution which is obviously a unit disk. The points in blue indicate the final mass distribution.