What is the Force Generated by a Non-Elliptical Orbit Planet?

Tom1
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Homework Statement



A planet around a star has an orbit that is not exactly an ellipse. In addition to the dominant Fo \alpha r^-2 term due to gravity from the central star, the planet seems to be responding to a slight additional force which has the form F1 \alpha r^-\alpha where \alpha is some constant.


Homework Equations



Included in 1.

The Attempt at a Solution



Where do I begin?
 
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I have no idea since I don't know what you're supposed to be doing.
 
Sorry, part of this seems to have been cut off.

Assuming there is a slight background density of material with spherically symmetric density p1 falling off as p1 (alpha) r^-B

Find the value of B in terms of alpha
 
Can anyone help me get started please? I don't understand this at all and it's due soon.
 
Near as I can tell you want to assume there is a mass distribution with density rho(r)=p1*(r/r0)^(-B). Now you want to figure out the radial dependence of the force it generates. Compute total mass as a function of r, M(r). Use that to calculate the force.
 
To solve this, I first used the units to work out that a= m* a/m, i.e. t=z/λ. This would allow you to determine the time duration within an interval section by section and then add this to the previous ones to obtain the age of the respective layer. However, this would require a constant thickness per year for each interval. However, since this is most likely not the case, my next consideration was that the age must be the integral of a 1/λ(z) function, which I cannot model.
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