Creative Commons License Copyright © Michael Richmond. This work is licensed under a Creative Commons License.

Gravitational potential energy and escape velocity

How much energy does it take to send a spaceship far from the Earth? Let's find out. We'll use a simple model for a spaceship: a big bullet of mass M = 1 kg shot out of a big gun, like this one:


Illustration from Jules Verne's book From the Earth to the Moon.

Things get even more interesting when an adventurer from France declares that if they make the projectile hollow, he will ride inside it!


Illustration from Jules Verne's book From the Earth to the Moon.

Worksheet for this exercise

The bullet starts at the Earth's surface, a distance R1 = 6.37 x 106 meters from the center of the Earth, and then flies to a final distance of R2 = 2 x 6.37 x 106 meters, where it stops momentarily.


The bullet starts at the Earth's surface, a distance R1 = 6.37 x 106 meters from the center of the Earth, and then flies to a final distance of R2 = 11 x 6.37 x 106 meters, where it stops momentarily.


The bullet starts at the Earth's surface, a distance R1 = 6.37 x 106 meters from the center of the Earth, and then flies to a final distance of R2 = 101 x 6.37 x 106 meters, where it stops momentarily.

(Yes, we are ignoring the effect of the Moon's gravitational force ...)


The bullet starts at the Earth's surface, a distance R1 = 6.37 x 106 meters from the center of the Earth, and then flies to a final distance of R2 = 1,001 x 6.37 x 106 meters, where it stops momentarily.


The bullet starts at the Earth's surface, a distance R1 = 6.37 x 106 meters from the center of the Earth, and then flies to a final distance of R2 = 10,001 x 6.37 x 106 meters, where it stops momentarily.

(Yes, we are ignoring the effect of the Sun's gravitational force, and that of the other planets ....)


The bullet starts at the Earth's surface, a distance R1 = 6.37 x 106 meters from the center of the Earth, and then flies to a final distance of R2 = 100,001 x 6.37 x 106 meters, where it stops momentarily.

(Yes, we are ignoring the effect of the Sun's gravitational force, and that of the other planets ....)


The bullet starts at the Earth's surface, a distance R1 = 6.37 x 106 meters from the center of the Earth, and then flies to a final distance of R2 = 1,000,001 x 6.37 x 106 meters, where it stops momentarily.

(Yes, we are ignoring the effect of the Sun's gravitational force, and that of the other planets ....)


Summary of the results



 R1 (km)             R2 (km)        gained GPE (J)    initial speed (m/s)
----------------------------------------------------------------------
6.37x10^6        2 x 6.37x10^6     31.3     million         7,913 

                11 x 6.37x10^6     56.9     million        10,670

               101 x 6.37x10^6     62.0     million        11,135

             1,001 x 6.37x10^6     62.55    million        11,185

            10,001 x 6.37x10^6     62.61    million        11,190

           100,001 x 6.37x10^6     62.616   million        11,190.7

         1,000,001 x 6.37x10^6     62.61626 million        11,190.73

----------------------------------------------------------------------
 

There's a clear pattern: at some point, the bullet gains a VERY large extra distance for just a small increase in initial velocity. Suppose that we make the final distance R2 = infinity. We can use the conservation of energy to find the speed required to keep the bullet going forever:

If we ask the bullet to reach a final distance Rf = ∞ with a final speed vf = 0, then

That allows us to define a special initial speed, the escape velocity from the Earth:

We can finish our table now ....



 R1 (km)             R2 (km)        gained GPE (J)    initial speed (m/s)
----------------------------------------------------------------------
           100,001 x 6.37x10^6     62.616   million        11,190.7

         1,000,001 x 6.37x10^6     62.61626 million        11,190.73

               infinity            62.61633 million        11,190.74
----------------------------------------------------------------------
 

Creative Commons License Copyright © Michael Richmond. This work is licensed under a Creative Commons License.