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Escape velocity

Intermediate

Minimum speed to leave a planet without returning.

Key relationv_e = √(2GM/R)

Escape speed v_e = √(2GM/R) is the minimum speed to reach infinity with zero speed left, ignoring air. It follows from ½mv² = GMm/R.

Worked example

Earth 11.2 km/s, Moon 2.4 km/s, Sun 618 km/s.

Common mistake

It's independent of the direction and the object's mass.

In more detail

Escape velocity is the minimum speed needed to leave a planet's gravitational pull without further propulsion. It is v = sqrt(2GM/R) and does not depend on the mass of the escaping object.

Real-world uses

Open the interactive lesson, with simulation and quiz →

Frequently asked questions

Do I need to reach escape velocity to leave Earth?

Only to escape entirely. Rockets can reach orbit at lower speeds.

Does escape velocity depend on direction?

No, for a spherical planet, the minimum escape speed is the same in all directions.

Does a rocket need to keep burning at escape speed?

No. If it reaches escape speed with no further thrust needed, it will coast away, ignoring drag and other bodies.

Related topics in Gravitation & Orbits

Gravitational potential · Field of a spherical shell · Field inside a uniform sphere · Escape velocity of Earth · Orbital velocity · Satellite energy

← All Gravitation & Orbits topics