An object falling through a drilled hole through the earth

AI Thread Summary
An object dropped through a drilled hole in the Earth reaches its maximum velocity at the center and decelerates on the return trip, assuming no air drag. The discussion explores the mathematical modeling of this motion, particularly the changing acceleration due to gravitational forces as the object descends. Participants debate the effects of Earth's rotation and the implications of a hypothetical scenario where two individuals jump simultaneously from opposite sides of the Earth. They conclude that, under ideal conditions, both would emerge at the opposite points, but real-world factors like drag and non-uniform density complicate the situation. Ultimately, the conversation highlights the principles of simple harmonic motion in this context.
Matt Jacques
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A hole is drilled through the Earth so an object can be dropped into the hole, its greatest velocity is at the center of Earth and decelerates on its way back on the other side. Then continues indefinitely provided there is no air drag.

How would one find the velocity at any given point, I have DE next semester, but we did some first order ones, so I would think it is something like:

V^2 = 2A?Y*

*Ball dropped from rest so Vo is zero

A is the acceleration caused from the earth, but it would constantly be changing, wouldn't that be an unknown derivative?

V^2 = 2?R(dg/dr)

I attempted to solve it, I got:

V = sqrt((Gm/R)/ln(2R))

which doesn't make sense...
 
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Are you allowed to make the approximation that the Earth is a sphere? Then use the fact that the force at a given radius is as if all the mass that is within that radius is concentrated at the centre. Can you assume that the Earth has uniform mass density? Then the acceleration at radius r is -rg/R, where R is the Earth's radius. This gives you the same equation as that of a spring, or simple pendulum (i.e. "simple harmonic motion"), and you probably already know how to solve it.
 
The simplest solution is the most elusive. Thanks :)
 
You need to take into account that the M term from GMm/r only applies to the mass 'beneath' you.
 
Originally posted by enigma
You need to take into account that the M term from GMm/r only applies to the mass 'beneath' you.

So if one enters a shaft from Europe say, then what effects a body 'Falling' that has nothing below its feet?

If there were an hypothetical 'Gap' in the Earth from say United Kingdom>>> Sidney Australia, and if there were two test subjects located at the Surface points A (UK) and B (Aussie) who coincide their leaps, does the aussie emerge at point A (UK)and the limey at point B (Aussie)?..or is there another factor due to the situation, and both test subjects come to a rest at the mid-point in shaft, eventually ending up orbiting each other due to the Radial Gravitational effects of the surrounding Earth?
 
Originally posted by ranyart
So if one enters a shaft from Europe say, then what effects a body 'Falling' that has nothing below its feet?

Sorry, I should have made myself more clear.

By putting 'beneath' in quotes, I meant that:

If you build an imaginary cut beneath you, so that you're 'standing' on a smaller sub-sphere of the Earth, that smaller sub-sphere is the part whos gravity affects you. The remaining hollowed-out sphere 'above' you sums to zero force when you integrate the gravitational force over the entire thing.

(or at least, so I've been told. That's one integration I have never actually calculated, to be honest)
 
If there were an hypothetical 'Gap' in the Earth from say United Kingdom>>> Sidney Australia, and if there were two test subjects located at the Surface points A (UK) and B (Aussie) who coincide their leaps, does the aussie emerge at point A (UK)and the limey at point B (Aussie)?..or is there another factor due to the situation, and both test subjects come to a rest at the mid-point in shaft, eventually ending up orbiting each other due to the Radial Gravitational effects of the surrounding Earth?

As long as you assume that the Earth isn't rotating, they'll end up at the other side. Their maximum speed in the center will be smaller than it would be if the force acting on them throughout the descent was the same as the force acting on them at the surface.

If the Earth is rotating, then coriolis forces would cause our intreppid bungee jumpers to wind up eating hot magma not very far down.
 
OK, if we assume a few things:

The Earth is spherical and of uniform density

Friction, drag, the corolis force (this can be ignored by placing the hole through the poles) are ignored.

We know:

a = \frac{GM}{r^2}

Though I won't prove it, as enigma says for a given r you only need consider the mass of the sphere with the radius r, which as I've assumed a spherical Earth with uniform density is given by:

M = \frac{4}{3}\pi r^2 \rho

if we substitute this into the first equation we get:

a = \frac{4}{3} \pi \rho Gr

As the other terms are constant it is clear that the accelration is directly proportional to the displacement from the Earth's centre which means that we should immediately recognise that the object dropped down Matt's hole has simple harmonic motion, whose accelration and velocity is given by the following equations:
v = \omega \sqrt{r_0^2-r^2}

a = -\omega^2 r

\inline{r_0} is the amplitude ort maximum displacemnt which in this case is equal the radius of the Earth and we can see that \inline{\omega}, the angular frequency is equal to \inline{-\sqrt{(\frac{4}{3} \pi \rho Gr})}

we can now get the equation for the velocity:

v = -\sqrt{(\frac{4}{3} \pi \rho Gr)(r_0^2 - r^2)}

As a final note I'll say that obviusly drag and frction can't be ignored and would actually make this into a dampened simple harmonic oscillator, another factor that can't be ignored is the fact that the Earth is not of uniform density and a better approximation is to consider the mass uniformly distrubuted inside the lower mantle and the core and ignore the differing gravity as you move through the upper mantle and crust.
 
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jcsd: Your formulas are more complicated than need be. Your factor
\inline{{4\over3}\pi\rho Gr} is simply \inline{{GM_0r\over r_0^3}} where \inline{M_0} is the Earth's mass. But we already know what this acceleration is at \inline{r=r_0}; it is \inline{g}. Hence

a={4\over 3}\pi\rho Gr=g{r\over r_0}

and this considerably simplifies the calculation. I gave this expression in my first post. Did you miss it?

So frequency is

\omega=\sqrt{g/r_0},

and the final formula for velocity is

v = -\sqrt{\frac{g}{r_0}(r_0^2 - r^2)}.

(BTW, you have an extra factor of \inline{r} under your square root.)
 
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  • #10
[moderator butting in]
Good to see you guys using both the display-mode and inline-mode tex so well! Please let me know if you have any comments, complaints, or suggestions about the tex system.
[/moderater butting in]

- Warren
 
  • #11
krab: I only noticed yor post after I'd posted. I derived the equations as I was writing out my post, I thought that they would probably simplify, but I admit I was too lazy to do it.

The r exponent was a typo, I had to edit the post about four times to get rid of all the typing errors in the latex code, though the inline text worked just fine and it looks better than I thought it would.
 
  • #12
Yea. Thanks Warren, the \inline thing works nicely. I found out about it by comparing jcsd's post to mine. I've now edited my post to make use of it.
 
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