The gravitational pull of each of the planets in the Solar System
is different and this will affect the velocity that a spacecraft
would need to be travelling to leave the planet’s surface. This
speed, known as the ESCAPE VELOCITY, depends on both the
radius of the planet, and its mass
R
GM
2
G = Gravitational Constant 0.000 000 000 0667
M = Mass of the planet (in kg)
R = Radius of the planet (in m)
DATA
Very small numbers such as:
0.000 000 000 0667
Are not very practical to use in
calculations so we can rewrite it like
this:
0.000 000 000 06 67
6.67 x 10-11
Number between 1 and 10 Power of 10