No. The link is between the planet's distance from its star and the period of its orbit.
Doubling the distance reduces the force of gravity to one quarter its original.
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.
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.
Yes, there is a relationship between the mass of a planet and its gravitational field strength. The greater the mass of a planet, the stronger its gravitational field strength will be. Gravity is directly proportional to mass, so planets with more mass will have a stronger gravitational pull.
Newton's law of universal gravitation states that the force of gravity between two objects is directly proportional to the product of their masses and inversely proportional to the square of the distance between their centers. This means that gravity depends on both the mass of the planet and the distance between the planet and the object experiencing the force.
Gravity is the attraction between two or more bodies. It is propotional to their mass and inversely proportional to their distance.
There is something missing from the question. The planet must have a moon. The only way to measure the mass of a planet is by using data about a moon orbiting the planet or data about the path of a spacecraft passing or going into orbit around the planet. If you know the distance to a planet then you can work out the moon's distance from the planet. The planet's mass can then be found. It's a bit of trigonometry and Newton's version of Kepler's Third Law. So that's the reason that it is necessary to know the distance to the planet.
F = G*m(planet)*m(object)/(r^2) where F is the gravitational force G is the gravitational constant m is mass r is the distance between the object and the center of the planet g = G*m(planet)/(r^2) where g is the acceleration due to gravity.
The size of a planet's orbit is primarily determined by its distance from the star it orbits, as well as the planet's mass and the characteristics of the star. The orbiting planet's velocity and gravitational interactions with other bodies in the system also play a role in determining the size of its orbit.
F = (G m1 m2) / (r^2) Where G is the univeral gravitational constant, m1 is the mass of the planet, m2 is the test mass, F is the force acting between the planet and the test mass, and r is the distance between the centroid of the planetary mass and the centroid of the test mass. --------------------------------------------------------------------------------------- Gravity is the force that pulls you to the ground on Earth. The strength of gravity depends on how big the planet you are standing on is (as shown by the formula above). Look in the link below to see how much you would weigh on other planets.
The amount of gravity that something possesses is proportional to its mass and distance between it and another object.
The mass of the planet is all you need to know. That, along with the mass of the other object and the distance between their centers, tells you the strength of the force between them.
The weight of an object on the surface of a planet depends on ...-- The mass of the object.-- The mass of the planet.-- The distance between the center of the object and the centerof the planet, i.e. the planet's radius.
Yes, there is a relationship between a planet's distance from the sun and its surface gravity. The closer a planet is to the sun, the stronger the gravitational pull from the sun, which can affect the planet's own gravity. However, other factors, such as a planet's mass and composition, also play a significant role in determining its surface gravity.
The gravitational force on an object at a standard distance is proportional to the mass of the planet.
A more massive planet is attracted more by the Sun if other things like the distance are equal. The force of gravity on a planet is proportional to the mass of the planet and inversely proportional to the sare of the distance.