Simple Harmonic Motion and Gravitation: Solving for r(t)

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Homework Help Overview

The discussion revolves around a problem connecting gravitation and simple harmonic motion, specifically analyzing the motion of a mass dropped through a hole drilled through the Earth. The original poster seeks to demonstrate that this motion is simple harmonic and to derive a formula for r(t).

Discussion Character

  • Exploratory, Conceptual clarification, Mathematical reasoning

Approaches and Questions Raised

  • The original poster begins with the equation for simple harmonic motion and attempts to derive the angular frequency, questioning how to express it as a function of time. Another participant introduces Newton's law of gravitation and discusses the mass below the particle as a function of r, leading to a differential equation that suggests a harmonic solution. The original poster seeks clarification on the terminology used regarding the "harmonic solution."

Discussion Status

The conversation is active, with participants exploring different aspects of the problem. One participant has provided a mathematical framework that leads to a harmonic solution, while another is seeking clarification on the conceptual meaning of this solution. There is no explicit consensus yet, but the discussion is productive and focused on understanding the underlying principles.

Contextual Notes

Participants are working under the assumption of a frictionless environment and a constant mass density for the Earth. The original poster is navigating the complexities of deriving the angular frequency while trying to maintain the relationship between distance from the center and time.

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I'm working on a problem on relating gravitation and simple harmonic motion. The idea is that a mass dropped in a hole drilled through the Earth will oscillate (no friction, etc).

The question asks this:
"Show that the motion of the mass is simple harmonic motion and find a formula for r(t)"

So, I'm starting with the basic r(t) equation for simple harmonic motion, r(t) = Acos(wt) where A is the total radius of the Earth (the amplitude), t is the time and w is the angular frequency. My problem is that any attempt to find an angular frequency seems to involve dictating the distance from the center, r, which is what I'm trying to find as a function of time.

The best I've been able to come up with is w = sqrt(k/m) where k is the "gravitational spring constant" involving (4/3)pi * p * R * G, R being the radius that I'm trying to find.

How should I find w in this case?
 
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First, considerer Newtons gravitation law:

F = \frac{-GmM}{r^{2}};

where the minus sign indicates that the force is attractive. Now consider a body moving through the center of the Earth, at a distance r(t) from the center. Suppose that the Earth has constant mass density \rho. Tha total mass "below" (e.g, that will effectively exerct a resultant force uppon) the particle located at position r(t) (supposing that r(t) is always smaller than the outter radius of the Earth) will be clearly a function of r of the form:

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

Plugging that formulae on Newton's gravitation law and writing F = ma we have:

a = \frac{-4 G \rho \pi r^{3}}{3 r^{2}} = \frac{-4 G \rho \pi r}{3};

Then, writing a = \frac{d^{2}r}{dt^{2}}, we get:

\frac{d^{2}r}{dt^{2}} = \frac{-4 G \rho \pi r}{3};

Solving for r (which should be easy enough) you get the harmonic solution and, furthermore, the angular frequency of oscilation.
 
Quiablo -

Thanks for your reply, it's very helpful. One question: When you say "the harmonic solution", what does that mean conceptually? I follow the math, but I'm a little fuzzy on the terminology.
 
I just wanted to mean that you will get, as a solution to the differential equation, a harmonic function of the form A cos(Bx), as you said it should be. You can right solutions of the exponential form also, complex exponentials, but that won't help you much in this case.

The general solution to the the second order diff equation:

\frac{d^{2}r}{dt^{2}} = -C r

where C substitutes the group of multiplying constants, can be written in the form:

r(t) = A_{1} cos (Bt) + A_{2} sin (Bt)

or equivalently:

r(t) = A_{3} cos (Bt + \phi );

Where A1, A2, A3, B and \phi are all constats, to be determined by the initial conditions of the problem (except for B, which will be determined directly by C, which is known by looking at the orignal equation).
 

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