Planets close to the sun are hot, and they are composed mostly of rocky or metallic substances with high boiling points. As planets get farther from the sun they have increasing amounts of the more volatile materials such as hydrogen and methane and ammonia. Gas giants, far from the sun, are made mostly of volatile substances and have relatively little rocky or metallic substances.
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.
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.
True. The length of time that it takes to complete one orbit around the Sun is directly related to the distance of the orbit from the Sun.
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.
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.
It depend on the distance of planet from sun and size of planet. If distance increases the time ie. Year increases
The period will increase. The relationship is given by Kepler's Third Law.
It decreases as the square of the distance.
It increases.
The tidal effect of a body increases as a cube of the distance.
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.
Gravity doesn't change, no matter where you are. One of the characteristics of the forces due to gravity is that they're inversely proportional to the square of the distance between the two masses involved. So as your distance from a planet changes, the mutual forces attracting you and the planet toward each other change in inverse proportion to the square of the distance between you and the center of the planet.
As a planet moves farther from the sun, its period, or the time it takes to complete one orbit, will increase. This is due to the decreasing gravitational force from the sun at greater distances, which results in the planet taking longer to complete its orbit.
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.
In the troposphere, temperature generally decreases as altitude increases. This is due to the decreasing air pressure and the fact that the upper regions of the troposphere are cooler due to their distance from the Earth's surface.
True. The length of time that it takes to complete one orbit around the Sun is directly related to the distance of the orbit from the Sun.
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.