David C. answered 01/27/21
Enthusiastic H.S. and College Physics Tutor earning a Ph.D.
Hi Ina,
For this question we would use newton's formula for gravitation:
Fg = GmM/r^2
Where G is the gravitational constant, m is the mass of the falling object, M is the mass of the planet, and r is the distance from the center of the planet. Implementing the formula F=ma we can reduce this down to:
ma = GmM/r2
a=GM/r2
Using g = 9.81 m/s2 to represent the gravitational acceleration of Earth, we can substitute in the size and mass of Venus to get the gravitational acceleration of Venus relative to Earth:
g=GMEarth/rEarth2
aVenus = GMvenus/rVenus2 = G(0.0558 MEarth)/(0.381 rEarth)2 = 0.0558/(0.381)2 * GMEarth/rEarth2
aVenus = 0.0558/(0.381)2 * g = 0.3844 *9.81m/s2 = 3.8 m/s2