Skip to main content
🔭 Gravitation

Escape Velocity Calculator

Find the speed needed to break free of a planet or star's gravity — v = √(2GM/r) — from its mass and radius. Earth works out to about 11.2 km/s.

v = √(2GM / r)
From mass & radius
Earth ≈ 11.2 km/s
Object mass cancels
100% Free
🔭 Open Full Physics Calculator 📖 Read the Guide

Escape velocity — Quick answer

Escape velocity is the minimum speed to break free of a body's gravity. It depends only on the body's mass and radius.

v = √(2 G M / r) (G = 6.674×10⁻¹¹)
= √(2 g r) using surface gravity g

Worked example: Earth, M = 5.972×10²⁴ kg, r = 6.371×10⁶ m → v ≈ 11,186 m/s (11.2 km/s).

Escape velocity of some bodies

BodyEscape velocityNote
Moon≈ 2.38 km/slight & small
Mars≈ 5.03 km/sintermediate
Earth≈ 11.2 km/sreference

Used for: rocketry, orbital mechanics, astronomy, mission design.

🔭 Escape Velocity Calculator

Enter the body's mass and radius to get escape velocity. (Earth ≈ 5.972e24 kg, 6.371e6 m.)

Escape velocity
In km/s
In km/h
Orbital speed √(GM/r)

⚠️ Use SI units — kilograms and metres — with G = 6.674×10⁻¹¹ to get speed in m/s. Escape velocity is independent of the escaping object's mass, and assumes no atmosphere or further propulsion.

Escape velocity is the minimum launch speed an object needs to break free of a body's gravity and coast away forever, with no further push — given by v = √(2GM/r). It comes from setting the object's kinetic energy equal to the gravitational potential energy holding it down, and remarkably the object's own mass cancels out, so a pebble and a rocket need the same speed. It depends only on the planet's mass M and radius r, which is why Earth's value is a fixed 11.2 km/s while the lighter Moon needs just 2.4.

Reviewed: June 20, 2026 · Author: Naveen P N, Founder — AI Calculator · Verified against: the energy derivation of escape velocity v = √(2GM/r).

The escape velocity equations

Escape velocity
v = √(2 G M / r) (G = 6.674×10⁻¹¹ N·m²/kg²)
Using surface gravity
v = √(2 g r) (since g = GM/r²)
Versus orbital speed
v_escape = √2 × v_orbit · v_orbit = √(GM/r)

Put the mass in kilograms and the radius in metres, multiply by twice the gravitational constant, and take the square root to get metres per second. If you know the surface gravity instead of the mass, the equivalent form v = √(2gr) is handier. Escape velocity is always √2 ≈ 1.414 times the circular orbital speed at the same radius, because escaping needs twice the kinetic energy of orbiting.

Worked example — escaping Earth

Scenario: Earth has mass 5.972×10²⁴ kg and radius 6.371×10⁶ m. What is its escape velocity?

Plug in
v = √(2 × 6.674×10⁻¹¹ × 5.972×10²⁴ / 6.371×10⁶)
Result
v = √(1.251×10⁸) ≈ 11,186 m/s ≈ 11.2 km/s

Earth's escape velocity is about 11.2 km/s — roughly 40,300 km/h. Notice nothing about the escaping object appears in the formula, so this speed is the same for a satellite or a stray atom. Repeat the calculation for the Moon (M = 7.35×10²² kg, r = 1.74×10⁶ m) and you get ≈ 2.38 km/s; for Mars, ≈ 5.03 km/s — both far easier to leave than Earth, which is exactly why low-gravity worlds are attractive launch points.

Frequently Asked Questions

How do you calculate escape velocity?

v = √(2GM/r), G = 6.674×10⁻¹¹. Earth: √(2×6.674e-11×5.972e24/6.371e6) ≈ 11,186 m/s.

What is Earth's escape velocity?

About 11.2 km/s (≈ 40,300 km/h) at the surface, ignoring air resistance.

Does it depend on the object's mass?

No — the object's mass cancels. A pebble and a spaceship need the same 11.2 km/s for Earth.

Moon and Mars escape velocity?

Moon ≈ 2.38 km/s, Mars ≈ 5.03 km/s — both far below Earth's, so easier to launch from.

Escape vs orbital velocity?

Escape is √2 × orbital. Orbit = √(GM/r); escape = √(2GM/r), about 41% faster.

Ready to perform complete calculations?

Use the full AI Calculator suite for gravitation and orbital mechanics with a professional PDF report.

🔭 Open Full Calculator — Free

No registration required · 350+ engineering calculators · PDF report export