the planet would have its year shorter
The temperature of a planet generally decreases with increasing distance from the Sun due to the inverse square law of radiation, where the intensity of sunlight diminishes with distance. Additionally, a planet's period of revolution, or orbital period, increases with distance from the Sun as described by Kepler's Third Law, which states that the square of a planet's orbital period is proportional to the cube of its average distance from the Sun. Therefore, planets that are farther from the Sun tend to have longer orbital periods and, on average, cooler temperatures.
The period of revolution (time taken to complete one orbit around the sun) increases with distance from the sun. This relationship is described by Kepler's third law of planetary motion, which states that the square of the period of revolution is proportional to the cube of the average distance from the sun (semi-major axis) for a planet.
It decreases as the square of the distance.
The distance of a planet from the sun affects its orbital period. Generally, the farther a planet is from the sun, the longer its orbital period will be. This relationship is described by Kepler's third law of planetary motion, which states that the square of a planet's orbital period is directly proportional to the cube of its average distance from the sun.
The relationship between the planet's SPEED and its distance from the Sun is given by Kepler's Third Law.From there, it is fairly easy to derive a relationship between the period of revolution, and the distance.
The period will increase. The relationship is given by Kepler's Third Law.
It depend on the distance of planet from sun and size of planet. If distance increases the time ie. Year increases
The temperature of a planet generally decreases with increasing distance from the Sun due to the inverse square law of radiation, where the intensity of sunlight diminishes with distance. Additionally, a planet's period of revolution, or orbital period, increases with distance from the Sun as described by Kepler's Third Law, which states that the square of a planet's orbital period is proportional to the cube of its average distance from the Sun. Therefore, planets that are farther from the Sun tend to have longer orbital periods and, on average, cooler temperatures.
The period of revolution (time taken to complete one orbit around the sun) increases with distance from the sun. This relationship is described by Kepler's third law of planetary motion, which states that the square of the period of revolution is proportional to the cube of the average distance from the sun (semi-major axis) for a planet.
How does a planet's distance from the sun affect its period of revolution?
The orbit time of planets increases as the distance from the sun increases. This relationship is described by Kepler's third law of planetary motion, which states that the square of a planet's orbital period is proportional to the cube of its average distance from the sun.
The time taken to complete an orbit increases as the distance from the sun increases. This relationship is described by Kepler's Third Law of Planetary Motion, which states that the square of the orbital period of a planet is directly proportional to the cube of the semi-major axis of its orbit. This means that planets farther from the sun have longer orbital periods.
If a planet's distance from the sun would increase, its revolutionary path would be extended (because it would have to traverse more distance), ergo increasing its period of revolution. Take an ellipse and enlarge it, then measure the perimeter of each ellipse, the larger one will have a larger perimeter.
This can be answered looking at Kepler's Third Law: "The square of the orbital period of a planet is directly proportional to the cube of the semi-major axis of its orbit." What this means is that as the distance of a planet to the sun increases, this change is directly proportional to the length of it's year.
It decreases as the square of the distance.
The distance of a planet from the sun affects its orbital period. Generally, the farther a planet is from the sun, the longer its orbital period will be. This relationship is described by Kepler's third law of planetary motion, which states that the square of a planet's orbital period is directly proportional to the cube of its average distance from the sun.
The relationship between the planet's SPEED and its distance from the Sun is given by Kepler's Third Law.From there, it is fairly easy to derive a relationship between the period of revolution, and the distance.