How to use it
- Enter central-body mass in kilograms.
- Enter radius or distance from its center in meters.
- Calculate ideal escape velocity.
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Estimate ideal escape velocity from an entered mass and center-to-center distance.
Escape velocity is represented here by an ideal point-mass Newtonian relationship at an entered radius.
v = √(2GM ÷ r), using G = 6.67430 × 10⁻¹¹ m³/(kg·s²).
An Earth-like mass and mean radius produce an ideal value near 11.19 km/s.
Atmosphere, rotation, propulsion, trajectory and other bodies are excluded. The result is an educational reference, not operational guidance.