Graphical labs · Numerical simulation
Schwarzschild orbits
Timelike geodesic + precession
d²u/dφ² + u = M/L² + 3Mu² (u=1/r) · G=c=1 · timelike, equatorial
Periapsis a(1−e) must stay > 2M. Precession is the GR 3Mu² term.
- r / M
- 16.8000
- φ (rad)
- 0
- L
- 4.00000
- V²(r)
- 0.930893
- Δω_analytic / rev
- 1.87000
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