anubis01
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Homework Statement
Find Hamiltons canonical equations for a satellite of mass m moving about a star of mass M at the origin. Consider motion in a plane, using polar coordinates r,\theta.
Repeat the process using cartesian coordinates x,y from the start.
Homework Equations
H=T+V
The Attempt at a Solution
I did both questions but I'm not exactly sure if I defined the kinetic and potential energies correctly for each case. For polar coordinates I found T=m/2 * (r\dot{}2 +r2 \theta\dot{}2) and potential energy V=V(r)
For cartessian coordinates I found the Kinetic T=m/2(x\dot{}2)
and potential energy V=\frac{-GMm}{\sqrt{x^2+y^2}}.
So if anyone can confirm if I set up the kinetic and potential energy equations correctly that would be great.
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