Need help solving a differential equation for orbit.

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SUMMARY

The discussion focuses on solving a differential equation related to planetary motion using Newtonian mechanics. The gravitational force is defined by the equation F=-GMm/r^2, leading to the second-order differential equation (d^2x/dt^2)+GM/x^2=0. Initial conditions provided are x(0)=a, x'(0)=b, and x''(0)=c. The solution involves multiplying the equation of motion by v=dx/dt, integrating to derive the conservation of energy, and addressing the complexities of both 1-dimensional and 2-dimensional problems.

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  • Understanding of Newton's laws of motion
  • Familiarity with differential equations
  • Knowledge of gravitational force equations
  • Basic calculus, including integration techniques
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  • Learn about conservation of energy in gravitational systems
  • Explore the use of polar coordinates in solving 2-dimensional motion problems
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Students and professionals in physics, astrophysics, and engineering who are interested in orbital mechanics and solving differential equations related to motion under gravitational forces.

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I want to be able to map the position of a planet given initial position, velocity, and acceleration.

I know the equation for Gravitational force (Newtonian) is: F=-GMm/r^2

Using Newtons second law this gives: m(d^2x/dt^2)=-GMm/x^2

Then simple Algebra yields: (d^2x/dt^2)+GM/x^2=0

I understand you need initial conditions to solve this problem, so I'm going to say that
x(0)=a
x'(0)=b
x''(0)=c
Thank you very much to anyone who helps me out with this!
 
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Multiply the equation of motion by v=dx/dt and integrate.
This will lead you to the conservation of energy:

v²/2 - GM/x = Constant = b²/2 - GM/a

Solve for v = dx/t, and integrate once more.
(here you have a difficulty: there are two solutions)

I assumed you were asked to solve the 1-dimensional problem, not the more realistic 2-d problem.
 
If you want to solve the 2d problem, you should work whit polar coordinates.
Also you are giving more initial conditions that you need.
 

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