One Each Day Till They Go Away (Part 1)

Classical Mechanics Level pending

There is a circular disk of radius 1 m 1 \text{m} in the x y xy plane, centered on the origin. The disk has a mass density of 1 kg/ m 2 1 \text{kg/ m}^2

The disk explodes into a sort of dust, with each infinitesimal piece of disk having an initial speed v 0 = 10 m/s v_0 = 10 \text{m/s} . The initial motion of each infinitesimal piece is in the direction of a unit vector going from point ( x 0 , y 0 , z 0 ) = ( 1 , 0 , 1 ) (x_0,y_0,z_0) = (-1, 0 , -1) to the respective piece.

After the initial explosion, each piece of disk travels under the influence of gravity, which has a magnitude of 10 m/s 2 10 \text{m/s}^2 and points in the negative z z direction.

Once each piece of disk lands again in the x y xy plane, it remains in that position. What is the moment of inertia of the final mass distribution about the z z axis?

Bonus: Make a plot of the final mass distribution


The answer is 276.2.

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1 solution

Karan Chatrath
Jun 5, 2021

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 ) (r \cos{\theta},r \sin{\theta},0) , where 0 r 1 0 \le r \le 1 and 0 θ 2 π 0 \le \theta \le 2\pi .

The velocity of projection is:

v o = v x o i ^ + v y o j ^ + v z o k ^ \vec{v}_o = v_{xo} \ \hat{i} + v_{yo} \ \hat{j} + v_{zo} \ \hat{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 ^ ) ) \vec{v}_o = v_o \left(\frac{\left(r \cos{\theta} \ \hat{i} + r \sin{\theta} \ \hat{j}\right) - \left( -1 \ \hat{i} + 0 \ \hat{j} -1 \ \hat{k}\right)}{\biggr\lvert \left(r \cos{\theta} \ \hat{i} + r \sin{\theta} \ \hat{j}\right) - \left( -1 \ \hat{i} + 0 \ \hat{j} -1 \ \hat{k}\right) \biggr\rvert} \right)

This leads to:

v x o = 10 ( r cos θ + 1 ) r 2 + 2 r cos θ + 2 v_{xo} = \frac{10(r \cos{\theta}+1)}{r^2 + 2r\cos{\theta} + 2} v y o = 10 r sin θ r 2 + 2 r cos θ + 2 v_{yo} = \frac{10r\sin{\theta}}{r^2 + 2r\cos{\theta} + 2} v z o = 10 r 2 + 2 r cos θ + 2 v_{zo} = \frac{10}{r^2 + 2r\cos{\theta} + 2}

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 ¨ = 10 \ddot{x} = 0 \ ; \ \ddot{y} = 0 \ ; \ \ddot{z} = -10 x ˙ ( 0 ) = v x o ; y ˙ ( 0 ) = v y o ; z ˙ ( 0 ) = v z o \dot{x}(0) = v_{xo} \ ; \ \dot{y}(0) = v_{yo} \ ; \ \dot{z}(0) = v_{zo} x ( 0 ) = r cos θ ; y ( 0 ) = r sin θ ; z ( 0 ) = 0 x(0) = r \cos{\theta} \ ; \ y(0) = r \sin{\theta} \ ; \ 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 x = v_{xo}t + r \cos{\theta} \ ; \ y = v_{yo}t + r \sin{\theta} \ ; \ z = v_{zo}t - 5t^2

Now, the mass element's final position is when its z coordinate becomes zero. This happens at time:

t f = v z o 5 t_f = \frac{v_{zo}}{5}

The final x and y coordinates of the mass element are:

x f = v x o t f + r cos θ x_f = v_{xo}t_f + r \cos{\theta} y f = v y o t f + r sin θ y_f = v_{yo}t_f + r \sin{\theta}

After simplification:

x f = r cos θ + 20 ( r cos θ + 1 ) r 2 + 2 r cos θ + 2 x_f = r \cos{\theta} + \frac{20(r \cos{\theta}+1)}{r^2 + 2r\cos{\theta} + 2} y f = r sin θ + 20 r sin θ r 2 + 2 r cos θ + 2 y_f = r \sin{\theta} + \frac{20r\sin{\theta}}{r^2 + 2r\cos{\theta} + 2}

Now, the mass of the mass element is: d m = σ r d r d θ ; σ = 1 dm = \sigma \ r \ dr \ d\theta \ ; \ \sigma = 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 dI = \left(x_f^2 + y_f^2\right) \ dm

Simplifying:

d I = ( r 2 + 40 r 2 + 40 r cos θ r 2 + 2 r cos θ + 2 + 400 ( r 2 + 2 r cos θ + 1 ) ( r 2 + 2 r cos θ + 2 ) 2 ) r d r d θ dI = \left( r^2 + \frac{40r^2 + 40r\cos{\theta}}{r^2 + 2r\cos{\theta} + 2} + \frac{400\left(r^2 + 2r\cos{\theta} + 1 \right)}{\left(r^2 + 2r\cos{\theta} + 2\right)^2} \right)r \ dr \ d\theta

Finally, the total moment of inertia about the Z axis is:

I = 0 2 π 0 1 ( r 2 + 40 r 2 + 40 r cos θ r 2 + 2 r cos θ + 2 + 400 ( r 2 + 2 r cos θ + 1 ) ( r 2 + 2 r cos θ + 2 ) 2 ) r d r d θ 276.1474 I = \int_{0}^{2\pi} \int_{0}^{1} \left( r^2 + \frac{40r^2 + 40r\cos{\theta}}{r^2 + 2r\cos{\theta} + 2} + \frac{400\left(r^2 + 2r\cos{\theta} + 1 \right)}{\left(r^2 + 2r\cos{\theta} + 2\right)^2} \right)r \ dr \ d\theta \approx 276.1474

The mass distribution is as follows:

r r is varied in steps of 0.04 and θ \theta is varied is steps of π / 50 \pi/50 . The points in red indicate the initial mass distribution which is obviously a unit disk. The points in blue indicate the final mass distribution.

I am worrried about your 886 day streak :).
Well nothing to disappoint I have started working on how to make website.
It will take me only 6-8 months to make a website like Brilliant.
I invite you to upload solutions on my website as you used to upload in Brilliant.


Talulah Riley - 1 week ago

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