- #1
Philosophaie
- 462
- 0
I am learning about General Relativity. The planetary orbits can be calculated with more precision especially Mercury. I am stuck on how to get from the Schwarzschild Metric:
a four variable Differential Equation
to a radius(r,theta,phi,t) and velocity(r,theta,phi,t) of a single planet in an ecliptical orbit around a single sun in a somewhat inertial space.
Any hints or suggestions would be helpful!
a four variable Differential Equation
to a radius(r,theta,phi,t) and velocity(r,theta,phi,t) of a single planet in an ecliptical orbit around a single sun in a somewhat inertial space.
Any hints or suggestions would be helpful!