This post is focused on the **escape velocity derivation **to get its

**formula**. Now, what is escape velocity?

**Escape velocity is defined as the minimum velocity with which if an object is thrown from the surface of the earth or any other planet or satellite then the object defeats the gravitational attraction working on it and can go beyond this attraction.**

This is to be noted that this concept of escape velocity is not only applicable to the earth but also it is equally applicable for all other planets and satellites.

But the value of this velocity would be different for them. As we derive the formula of this escape velocity, this point will get clearer.

## Escape velocity Derivation – derive formula as √(2gR)

**Escape velocity derivation**:

We will derive the equations using the following

*:*

**condition**

*The initial kinetic energy of the object would at least equalize the amount of work done to send the same object from the surface of the earth to infinite distance.*

Let’s find the amount of work done first.

**Work Done to send the object from the surface of the earth to infinite distance**

Say mass of the earth is M and its radius is R.

If an object of mass m is positioned at a distance x from the center of the earth, then the Force of **Gravitational Attraction** on the object is expressed as

F = (G M m)/x²

Now if this object is moved a small distance dx against this gravitational force, along the line of action of the same gravitational force then the **work** done is

W = F dx= ((G M m)/x²) dx

So to get the expression of the work done to send the object from the surface of the earth to infinite distance, we need to integrate the above expression with 2 limits, R and infinity. [ R representing the lower limit as it’s the distance of the surface of the earth from its centre]

By integrating with lower limit R and upper limit infinity:

W= ∫((G M m)/x²)dx = (GMm)/R ………………….. (1)

**Initial Kinetic Energy**

Now if the escape velocity of earth is V, then the initial kinetic energy(KE) of the object would be = ½ .m.V^{2} …………. (2)

**Getting the expressions now**

If this initial KE (equation 2) can at least equalize the work done (in eqn 1), then the object can really escape the earth’s gravitation.

So equalizing equation 1 and 2,

**½ .m.V ^{2} = (GMm)/R**

V^{2} = (2GM)/R

Escape Velocity**V = √( 2GM/R) ……… (3) [formula 1]**

As the expression of the acceleration due to gravity on the earth’s surface is **g = (GM)/R^2**

[for this equation read this: acceleration due to gravity]

i.e., **g.R ^{2} = GM**,

therefore we can rewrite equation number 3 as follows:

**V = [ (2 g R ^{2}) / R ]^{(1/2)} = (2gR)^{(1/2)} = √(2gR)**

**Escape Velocity**

V**=√(2gR)**…………** (4) [formula 2]**

**It’s to be noted that this velocity doesn’t depend on the mass of the object which is being thrown.**

But this esc. velocity certainly depends on the mass and the radius of the planet or satellite or star from where the object is being thrown.(see equation 3 above)

2 Equations are derived from this *escape velocity of the earth derivation* process. They are:

**V = √( 2GM/R)V= √(2gR)**

**Esc. Velocity is √2 times of Orbital velocity for nearby orbits**

For an orbit which is pretty close to the earth, we can ignore the height above the surface and can consider only the radius of the earth as the distance between the satellite and the earth’s center. For this scenario, we get an equation for orbital speed

**V _{orbital} = √(gR) **

**[ to find this derivation please refer to our post: Orbital Velocity]**

Whereas as found, ** V _{escape} = √(2gR)**

Very clearly it’s visible that **the Escape velocity is √2 times of Orbital velocity for nearby orbits.**

**Value of the earth’s Escape Velocity**

We know the value of g on the surface of the earth. It’s 9.8 m/s^2.

The radius of the earth (R) is 6400 Km = 6.4 X 10^6 meter.

So from these data, we get the **escape velocity of the earth** from equation 4 above:

**Escape Velocity of earth** =V = √(2 X 9.8 X 6.4 X 10^6) m/s =11200 m/s =**11.2 km/s = 7 mile/second**

So if an object is thrown upwards with a velocity of 11.2 Km/Second from the earth’s surface, it will be able to escape i.e. go beyond the gravitational field of the earth.

**Escape Velocity for moon and Jupiter**

Escape Value of the moon: 2.38 km/sec

and that of Jupiter: 59.5 km/sec

Suggested Reading:

**Orbital Velocity**

**Universal Law of Gravitation**

Anupam M is a Graduate Engineer (Electronics & Communication Engineering, National Institute of Technology -NIT Graduate) who has 2 decades of hardcore experience in Information Technology and Engineering. He is an avid Blogger who writes a couple of blogs of different niches. He loves to teach High School Physics and utilizes his knowledge to write informative blog posts on related topics. Anupam M is the founder and author of PhysicsTeacher.in Blog.