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

  • Thread starter Thread starter authgeek
  • Start date Start date
  • Tags Tags
    Gravitation Shm
Click For Summary
SUMMARY

The discussion focuses on deriving the formula for r(t) in the context of simple harmonic motion (SHM) related to gravitational forces acting on a mass dropped through a hole in the Earth. The initial equation for SHM is r(t) = Acos(wt), where A represents the Earth's radius and w is the angular frequency. The angular frequency is derived from Newton's law of gravitation, leading to the expression w = sqrt(k/m), where k is defined as the gravitational spring constant. The resulting differential equation, d²r/dt² = -4Gρπr/3, confirms that the motion is indeed simple harmonic.

PREREQUISITES
  • Understanding of simple harmonic motion (SHM) principles
  • Familiarity with Newton's law of gravitation
  • Basic knowledge of differential equations
  • Concept of gravitational spring constant
NEXT STEPS
  • Explore the derivation of the gravitational spring constant in detail
  • Learn about solving second-order differential equations
  • Investigate the relationship between mass density and gravitational forces
  • Study the implications of oscillatory motion in gravitational fields
USEFUL FOR

Students and professionals in physics, particularly those studying mechanics and gravitational systems, as well as educators looking to explain the principles of simple harmonic motion in a gravitational context.

authgeek
Messages
7
Reaction score
0
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?
 
Physics news on Phys.org
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).
 

Similar threads

  • · Replies 11 ·
Replies
11
Views
2K
  • · Replies 1 ·
Replies
1
Views
1K
  • · Replies 3 ·
Replies
3
Views
2K
  • · Replies 51 ·
2
Replies
51
Views
4K
  • · Replies 1 ·
Replies
1
Views
2K
  • · Replies 1 ·
Replies
1
Views
2K
  • · Replies 10 ·
Replies
10
Views
4K
Replies
16
Views
2K
Replies
25
Views
4K
  • · Replies 3 ·
Replies
3
Views
6K