Flying Over a Rod

At time t = 0 t = 0 , a particle of mass M = 1 kg M = 1 \text{kg} is launched with the following position and velocity:

( x , y ) = ( 2 , 0 ) m ( x ˙ , y ˙ ) = ( 1.2 , 1.2 ) m/s (x,y) = (-2,0) \, \text{m} \\ (\dot{x}, \dot{y}) = (1.2, 1.2) \, \text{m/s}

There is a rod which spans from ( x , y ) = ( 1 , 0 ) (x,y) = (-1,0) to ( x , y ) = ( 1 , 0 ) (x,y) = (1,0) . The rod is fixed in place, and it has a mass density of 1 kg/m 1 \text{kg/m} .

At what time does the particle reach y = 0 y = 0 again?

Details and Assumptions:
1) The only gravity acting on the particle is from the rod. Gravitational constant G = 1 m 3 kg s 2 G = 1 \frac{\text{m}^3}{\text{kg} \, \text{s}^2}
2) We are interested in the lowest value of t t such that t > 0 t > 0


The answer is 2.77.

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2 solutions

Mark Hennings
Apr 20, 2021

The gravitational potential of the bar, with line mass density λ \lambda , is V ( x , y ) = G 1 1 λ d u ( u x ) 2 + y 2 = G λ [ sinh 1 ( u x y ) ] 1 1 = G λ [ sinh 1 ( 1 x y ) + sinh 1 ( x + 1 y ) ] = G λ ln ( x 1 + ( x 1 ) 2 + y 2 x + 1 + ( x + 1 ) 2 + y 2 ) \begin{aligned} V(x,y) & = \; -G \int_{-1}^1 \frac{\lambda\,du}{\sqrt{(u-x)^2 + y^2}} \; = \; -G\lambda\Big[\sinh^{-1}\left(\tfrac{u-x}{y}\right)\Big]_{-1}^1 \; = \; -G\lambda\left[ \sinh^{-1}\left(\tfrac{1-x}{y}\right) + \sinh^{-1}\left(\tfrac{x+1}{y}\right)\right] \\ & = \; G\lambda \ln\left(\frac{x-1 + \sqrt{(x-1)^2 + y^2}}{x+1 + \sqrt{(x+1)^2 + y^2}}\right) \end{aligned} and the particle will satisfy the equations of motion x ¨ = V x y ¨ = V y \ddot{x} \; = \; -\frac{\partial V}{\partial x} \hspace{2cm} \ddot{y} \; = \; -\frac{\partial V}{\partial y} together with the boundary conditions x ( 0 ) = 2 x(0) = -2 , y ( 0 ) = 0 y(0)=0 , x ˙ ( 0 ) = y ˙ ( 0 ) = 1.2 \dot{x}(0) = \dot{y}(0) = 1.2 .

Manipulating the derivatives of V V so that they are not explicitly singular when y = 0 y=0 , we obtain the equations (with G = 1 G=1 and λ = 1 \lambda=1 ): x ¨ = 1 ( x + 1 ) 2 + y 2 1 ( x 1 ) 2 + y 2 y ¨ = 4 x y ( x + 1 ) 2 + y 2 ( x 1 ) 2 + y 2 [ ( x + 1 ) ( x 1 ) 2 + y 2 + ( x 1 ) ( x + 1 ) 2 + y 2 ] \begin{aligned} \ddot{x} & = \; \frac{1}{\sqrt{(x+1)^2 + y^2}} - \frac{1}{\sqrt{(x-1)^2 + y^2}} \\[2ex] \ddot{y} & = \; -\frac{4xy}{\sqrt{(x+1)^2 + y^2}\,\sqrt{(x-1)^2 + y^2}\,\big[(x+1)\sqrt{(x-1)^2 + y^2} + (x-1)\sqrt{(x+1)^2 + y^2}\big]} \end{aligned} These differential equations can be solved numerically, together with their initial conditions, and we obtain that y = 0 y = 0 when t = 2.7651704558 t = \boxed{2.7651704558} .

Karan Chatrath
Apr 14, 2021

At a general time t t , let the position of the point mass be r P = ( x , y , 0 ) \vec{r}_P = (x,y,0) and consider a rod element of length d p dp near the point r L = ( p , 0 , 0 ) \vec{r}_L = (p,0,0) . Then, applying Newton's law of gravitation, the force on the point mass is:

d F = G M d p ( r L r P ) r L r P 3 d\vec{F} = \frac{GM \ dp \ (\vec{r}_L - \vec{r}_P)}{\lvert \vec{r}_L - \vec{r}_P \rvert^3}

Then:

F = 1 1 G M ( r L r P ) r L r P 3 d p \vec{F} = \int_{-1}^{1} \frac{GM \ (\vec{r}_L - \vec{r}_P)}{\lvert \vec{r}_L - \vec{r}_P \rvert^3} \ dp

Applying Newton's second law, the acceleration vector of the point mass is:

a = ( a x , a y , 0 ) = F M \vec{a} = (a_x,a_y,0) = \frac{\vec{F}}{M}

Finally the resulting system of differential equations governing the motion of the point mass is:

x ¨ = a x ; x ˙ ( 0 ) = 1.2 ; x ( 0 ) = 2 \ddot{x} = a_x \ ; \ \dot{x}(0) = 1.2 \ ; \ x(0)=-2 y ¨ = a y ; y ˙ ( 0 ) = 1.2 ; y ( 0 ) = 0 \ddot{y} = a_y \ ; \ \dot{y}(0) = 1.2 \ ; \ y(0)=0

This problem has been handled numerically as follows:

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% Coded using Octave:
clear all
clc

% Spatial discretization of the rod:
dp     = 1e-3;

% Time step:
dt     = 1e-3;

% Initial conditions:
x(1)   = -2;
y(1)   = 0;
dx(1)  = 1.2;
dy(1)  = 1.2;
t(1)   = 0;

% Time index initialisation:
k      = 1;

% Simulating till the particle hits the ground again:
while y(k) >= 0

    % Initialisation of gravitational force:
    F      = [0;0;0];

    % Position vector of point mass:
    rP     = [x(k);y(k);0];

    % Calculating gravitational force:
    for p = -1:dp:1

        % Position vector of rod element:
        rL       = [p;0;0];

        % Gravitational force on point mass due to rod element:
        dF       = (dp*(rL - rP))/(norm(rL - rP)^3);

        % Numerical integration: gravitational force due to entire rod:
        F        = F + dF;
    end

    % Acceleration components (unit point mass):
    ddx     = F(1);
    ddy     = F(2);

    % Numerical integration: Semi implicit Euler:
    dx(k+1) = dx(k) + ddx*dt;
    dy(k+1) = dy(k) + ddy*dt;

    x(k+1)  = x(k) + dx(k+1)*dt;
    y(k+1)  = y(k) + dy(k+1)*dt;

    t(k+1)  = t(k) + dt;
    k       = k + 1;
end

ANSWER   = t(end)
% ANSWER = 2.761

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