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Keplerian Orbit Physics

60 FPS

Native Newton-Raphson orbital solver, Keplerian equations, and Hohmann transfer trajectory calculator.

Celestial Mechanics Formulas
1. Kepler's Equation & Solver:
M = E - e · sin(E)
E_{k+1} = E_k - (E_k - e · sin(E_k) - M) / (1 - e · cos(E_k))

Solved iteratively via Newton-Raphson root finding for Eccentric Anomaly E from Mean Anomaly M.

2. True Anomaly ν & Radial Distance r:
r = a(1 - e · cos(E)) = a(1 - e²) / (1 + e · cos(ν))
tan(ν/2) = √((1+e)/(1-e)) · tan(E/2)
3. Vis-Viva Orbital Velocity:
v = √(μ · (2/r - 1/a)),   T = 2π · √(a³ / μ)
4. Hohmann Transfer Delta-v (Δv):
Δv_1 = √(μ/r_1) · (√(2r_2 / (r_1+r_2)) - 1)
Δv_2 = √(μ/r_2) · (1 - √(2r_1 / (r_1+r_2)))
t_trans = π · √((r_1+r_2)³ / (8μ))

Hohmann Transfer

Departure Burn (Δv₁): 2.94 km/s
Arrival Burn (Δv₂): 2.65 km/s
Total Mission Δv: 5.59 km/s
Flight Duration: 259 days
Required Lead Angle: 44.3°

Space Telemetry Feed NORAD #25544

ISS Velocity 27,580 km/h
Altitude 418.5 km
Coordinates 28.4°N, 80.5°W
Inclination 51.64° LEO
Active Body: Earth
Heliocentric Distance (r): 1.000 AU
Orbital Velocity (v): 29.78 km/s
True Anomaly (ν): 0.0°
Orbital Period (T): 365.25 days
Sun (1.0 M☉) Target Orbit Hohmann Ellipse | Pan: Drag • Zoom: Wheel