Force of gravity equals mass of planet times mass of other times the constant (G) that makes the units work all divided by the distance from one to the other AND the other to one (turns out to be distance squared). F=GxM1xM2/(DxD)
Due to the gravity force which vary according to the mass of each planet.
Gravity depends largely on mass, the bigger the planet the greater the gravity should be
Its mass. More mass=more gravity Also the distance from the planet's center to its surface, i.e. its radius.
No. The strength of surface gravity on a planet depends on its size and mass.
It would depend on the mass of the planets. The surface gravity of a planet is directly proportional to its mass and inversely proportional to the square of its radius. If two planets have the same mass but different sizes, the smaller planet will have stronger gravity because the surface is closer to the center of mass. Conversely, if two planets are of the same size, the one with more mass will have stronger gravity. Since larger planets usually have more mass than smaller ones they usually have stronger gravity, though not always.
The larger the planet mass, the bigger force of gravity it has.
Gravity is directly proportional to mass.
No, because the mass of Venus does not vary.
It doesn't
It doesn't
It doesn't
Objects have a gravitational pull proportional to their mass.
The gravitational force on an object at a standard distance is proportional to the mass of the planet.
Objects have a gravitational pull proportional to their mass.
The gravity of a planet is directly proportional to its mass, and inversely proportional to the square of the distance from the center of mass. For the gravity on the surface of the planet, the distance is just the planet's radius. Thus, if a planet has three times the mass, it has three times the gravity. If you are three times as far away, the gravity decreases by a factor of nine.
The gravitational force on an object at a standard distance is proportional to the mass of the planet.
The gravitational force on an object at a standard distance is proportional to the mass of the planet.