Saturday, 29 February 2020

homework and exercises - Free fall in non-uniform field


Imagine I'm a space-diver, with mass m1, 500 miles above the Earth's surface at xi. I want to calculate my position, velocity, and acceleration as a function of time, accounting for the Earth's non-uniform gravitational field, and neglecting air resistance. I've done some basic calculations, and am confused by the answer I get; it seems to imply no acceleration as a function of time, if I start off at rest. Purely Newtonian regime. Here, I imagine I'm falling purely along the x-axis:


Conservation of energy: (Earth mass m2, diver mass m1)


12m1˙x2=Gm2m1x


Square root and integrating:


x(t)xix1/2dx=t0(2Gm2)1/2dt


This gives the solution


x(t)=(32(2Gm2)1/2t+x3/2i)2/3



However, my problem with this is that it seems to imply that the velocity scales:


˙xt1/3,


but if I start off at rest at t = 0, it seems that my velocity will not increase, but decrease with time? What am I doing wrong here? Is there something wrong with my assumption that I can simply place myself at xi with zero velocity? One would expect the diver's velocity to increase as a function of time, and for the gravitational field (since it will be stronger as I get closer to the surface of the Earth).


This should be straightforward, but I'm missing something?



Answer



Your mistake is in your conservation energy equation. The way you wrote it is valid only when falling from infinity, from rest. The correct is: dE=dK+dU=0, that is mvdv=Kx2dx, where KGm1m2. Integrating from (xi,vi) to (x,v) we get 12m(v2v2i)=K(1x1xi). This is the correct equation which you have to start with. Now v=dxdt=±v2i+2Km(1x1xi). Assuming vi=0 and integrating again from (t=0,xi) to (t,x) we obtain t=x(t)xidx2Km(1x1xi), where I am using the minus sign because the axis is oriented upwards. To solve this integral you use the substitution x=xisin2θ, t=2mx3iKθ(x)π2sin2θdθ, where θ(x)=arcsinxxi. Therefore, t=mx3i2K[π2arcsinxxi12sin(2arcsinxxi)]. However this equation cannot be solved for x.


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