There is no necessary connection between mass and distance.
The mass of a planet does not affect its orbital speed, for example.
However the "giant planets" are further from the Sun than the less massive "terrestrial planets".
The outer (more massive planets) contain a lot of gases. So, they would surely lose a lot of their mass if they were nearer the Sun.
(In fact, we have found planets called "hot Jupiters" orbiting other stars.
These are Jupiter type planets, but they orbit very close to their star.)
No. The surface gravity of a planet is a product of its size and mass. It has nothing to do with distance from the sun. However, a planet farther away from the sun will experience a weaker pull from the sun's gravity.
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.
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.
No, an object's weight is determined by the gravitational pull of the planet it is on, not its distance from the sun. Objects will weigh the same on a planet close to the sun as they would on a planet farther away.
Yes, its all to do with Kepler's third law of planetary motion, which describes the relationship between the orbital period of the plant and the distance of that planet from the sun. Kepler found that the square of the period, P, is proportional to the cube of the semi-major axis, a (P2 = ka3). The planets orbit the sun in an ellispse, the semi major axis is the `longest radius` within this ellipse. Kepler found that a constant `k` was needed in the equation - this was later found to relate to the mass of the objects. The planets mass is usually a lot less than the star its orbiting, so can often be dropped from the equation.
No. The surface gravity of a planet is a product of its size and mass. It has nothing to do with distance from the sun. However, a planet farther away from the sun will experience a weaker pull from the sun's gravity.
The size of a planet is not related to it's distance from the sun. Planet mass and orbital velocity are factors that determine it's distance from the sun.
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.
No. A planet's gravitational pull is determined by the planet's mass. A planet's orbital speed is determined by the the mass of the Sun and the planet's distance from the Sun.
mass of the planet and the distance from the sun
Yes, its all to do with Kepler's third law of planetary motion, which describes the relationship between the orbital period of the plant and the distance of that planet from the sun. Kepler found that the square of the period, P, is proportional to the cube of the semi-major axis, a (P2 = ka3). k is a constant relating to the mass of the objects.
No, the distance of a planet from the sun is determined more by its orbit and gravitational interactions with other celestial bodies rather than its mass. The mass of a planet does affect its gravity, which in turn influences its orbit, but it is not the sole factor determining its distance from the sun.
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.
No, an object's weight is determined by the gravitational pull of the planet it is on, not its distance from the sun. Objects will weigh the same on a planet close to the sun as they would on a planet farther away.
Yes, its all to do with Kepler's third law of planetary motion, which describes the relationship between the orbital period of the plant and the distance of that planet from the sun. Kepler found that the square of the period, P, is proportional to the cube of the semi-major axis, a (P2 = ka3). The planets orbit the sun in an ellispse, the semi major axis is the `longest radius` within this ellipse. Kepler found that a constant `k` was needed in the equation - this was later found to relate to the mass of the objects. The planets mass is usually a lot less than the star its orbiting, so can often be dropped from the equation.
We do not yet have enough information about the relationship (if any) between the planet's distance from the primary and its mass. Our information on the mass and orbital distances is skewed by method of detection of exoplanets; occultation of the primary by the planet. This method detects very large planets more easily than smaller ones, and depends on us viewing across the orbital plane of the planetary system. Otherwise, we wouldn't see occultations at all.
You can use the formula M = (V^2 * R) / G, where M is the planet's mass, V is the orbital speed, R is the distance from the sun, and G is the gravitational constant. By plugging in the values of V and R, you can calculate the planet's mass.