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Orbit with time-varying mass

  1. Feb 17, 2012 #1
    1. The problem statement, all variables and given/known data
    An approach to the problem of finding how orbital radius changes with solar mass is to solve the radial equation of motion for a gravitational force that has an explicit time dependence based on the assumed rate of mass loss. Show by numerically solving this equation of motion that one gets the result D proportional to 1/M.


    2. Relevant equations

    I'm not entirely sure what equation of motion the question requires. We can equate the gravitational force with the centripetal force,

    mv2/D = GMm/D2

    but I'm unsure as to how to include the time-dependent solar mass.

    I think we can assume the changes in mass per orbit are small and uniform.


    3. The attempt at a solution


    I tried replacing the constant mass M in the above equation with M(t) and differentiating with respect to t, and using the angular momentum to express v in terms of D, but it's not really getting me anywhere.

    Any advice on how to approach this problem would be greatly appreciated. :D
    Thanks!
     
  2. jcsd
  3. Feb 17, 2012 #2

    tiny-tim

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    welcome to pf!

    hi fizzwhiz! welcome to pf! :wink:

    i think they mean, what happens to the same planet as the solar mass changes?

    so v won't be constant, but the angular momentum of the planet will :smile:
     
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