Your mass does not change. Your weight, however, changes in proportion to the gravity of each planet.
.The atomic mass increases
Density of a planet = (Planet's mass) divided by (Planet's volume)
Venus is the planet closest in mass to Earth, with a mass about 81% that of Earth.
No, the mass of a planet and its size are not the same. Mass refers to the amount of matter in an object, while size refers to the physical dimensions of the object. A planet's mass is determined by the total amount of material it contains, while its size is a measure of its physical dimensions.
Yes, the mass of a planet affects its orbital period according to Kepler's third law of planetary motion. The heavier the planet, the longer its orbital period will be. This is because a more massive planet exerts a stronger gravitational force, causing it to move more slowly around its star.
The gravitational acceleration inside a planet is determined by its mass and radius. It generally decreases as you move towards the center of the planet due to the increasing mass above you.
Gravity depends largely on mass, the bigger the planet the greater the gravity should be
It increases
.The atomic mass increases
The more distant the orbit, the longer the year.
A planet that falls into a black hole would get completely destroyed. Its mass would be added to the mass of the black hole.
Mass stays the same while weight reduces because the gravity is weaker at distance.
The mass of the object remains the same since it is a measure of the amount of matter in an object, but the weight changes because weight is dependent on gravity, which varies from planet to planet. If the gravitational force on the new planet is different than on Earth, the weight of the object will be different.
in what direction do sand dunes move
Density of a planet = (Planet's mass) divided by (Planet's volume)
Venus is the planet closest in mass to Earth, with a mass about 81% that of Earth.
If the object doesn't move to another planet while you double its mass,its weight will also double.