How to use
Escape velocity is the minimum speed in an ideal Newtonian model to reach infinite distance with zero final kinetic energy from radius r around mass M, without further propulsion or drag.
- Enter body mass.
- Enter distance from its center.
- Calculate escape speed, local gravity and circular-orbit speed.
How it is calculated
vₑ=√(2GM/r); g=GM/r²; vorbit=√(GM/r)
Example
Example: Earth-like M≈5.972×10²⁴ kg and r≈6.371×10⁶ m gives escape speed near 11.19 km/s in this model.
Important notes
This Newtonian calculation ignores atmosphere, body rotation, other bodies and general relativity.
Frequently asked questions
Is continued thrust required?
Not in the ideal model once the required trajectory/speed is achieved.
Orbit speed equals escape speed?
No; escape speed is √2 times circular speed at the same r.
Is r altitude?
No, it is distance from the center.