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Time = distance3/2Kepler's 3rd Law of Planetary Motion gives this relationship:The cube of the average distance from the Sun is proportional to the square ofthe period of revolution (year).So: (Distance)3 is proportional to (year)2
The distance a planet is from the Sun relates to the length of the planet's year because it determines the time it takes for the planet to complete one revolution around the Sun. A planet's "year" is the time taken to orbit the Sun once. The further a planet is from the Sun, the further it must travel to complete an orbit. Also, a planet moves more slowly when it is further from the Sun. The mathematical equation for all this is given by Kepler's "Third Law of Planetary Motion". Earth takes about 365.25 days to complete a revolution. So, our year is 365 days with 366 days in a "leap year".
The distance a planet is from the Sun relates to the length of the planet's year because it determines the time it takes for the planet to complete one revolution around the Sun. A planet's "year" is the time taken to orbit the Sun once. The further a planet is from the Sun, the further it must travel to complete an orbit. Also, a planet moves more slowly when it is further from the Sun. The mathematical equation for all this is given by Kepler's "Third Law of Planetary Motion". Earth takes about 365.25 days to complete a revolution. So, our year is 365 days with 366 days in a "leap year".
It's when the earth makes a full rotation around the sun.
distance from a source of light and how long it takes to orbit that source
It depends which planet you are on. On Earth an planetary year is 365 +/- days. On Saturn a single year is almost 30 earth years.
The time it takes for any given planet to make one complete revolution around its sun determines the length of its year.
Depends on where you are (latitude) and the time of year.
Typically, this length of time is called a "year". Each planet's year is a different length than that of the other planets and increases as the planet is further from the Sun.
Time = distance3/2Kepler's 3rd Law of Planetary Motion gives this relationship:The cube of the average distance from the Sun is proportional to the square ofthe period of revolution (year).So: (Distance)3 is proportional to (year)2
The distance a planet is from the Sun relates to the length of the planet's year because it determines the time it takes for the planet to complete one revolution around the Sun. A planet's "year" is the time taken to orbit the Sun once. The further a planet is from the Sun, the further it must travel to complete an orbit. Also, a planet moves more slowly when it is further from the Sun. The mathematical equation for all this is given by Kepler's "Third Law of Planetary Motion". Earth takes about 365.25 days to complete a revolution. So, our year is 365 days with 366 days in a "leap year".
The distance a planet is from the Sun relates to the length of the planet's year because it determines the time it takes for the planet to complete one revolution around the Sun. A planet's "year" is the time taken to orbit the Sun once. The further a planet is from the Sun, the further it must travel to complete an orbit. Also, a planet moves more slowly when it is further from the Sun. The mathematical equation for all this is given by Kepler's "Third Law of Planetary Motion". Earth takes about 365.25 days to complete a revolution. So, our year is 365 days with 366 days in a "leap year".
A planetary year is the amount of time it takes a planet to orbit the Sun. A planetary year on Earth is 365.26 days.
A planetary year is one orbit of a planet around the sun.
The time it takes to go around its solar systems sun.
Mercury is the closest planet to the Sun. According to Kepler's law of planetary motion, the nearer a planet is to the sun, the faster it orbits the Sun.
It's when the earth makes a full rotation around the sun.