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Yes, the equation p2 = a3, where p is a planet's orbital period in years and a is the planet's average distance from the Sun in AU. This equation allows us to calculate the mass of a distance object if we can observe another object orbiting it and measure the orbiting object's orbital period and distance.
About 29.5 Earth years.
Semimajor axis of its orbit, the average of the maximum and minimum distance from the Sun. <<>> That's basically the planet's average distance from the Sun.
It takes 10,832 Earth days to complete one orbit around the Sun.
Saturn takes 29.447 years to make one orbit of the sun.
The average rotation period (day) of Saturn is about 10 hours and 30 minutes.
Yes, the equation p2 = a3, where p is a planet's orbital period in years and a is the planet's average distance from the Sun in AU. This equation allows us to calculate the mass of a distance object if we can observe another object orbiting it and measure the orbiting object's orbital period and distance.
It would depend on the star it was orbiting. If it were in our solar system, its orbital period would be little more than 30 years. (Saturn is approximately 9.5 AU from the Sun.)
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Average speed over a period of time = (distance covered in a period of time) divided by (time it took to cover the distance).
About 29.5 Earth years.
The planet must be farther from the star than Earth is from the Sun. According to Kepler's third law, a longer orbital period means that the planet must be farther from its star. In fact you could work out its average distance from the star, using Kepler's law.
distance
A2. There is no maximum orbiting height. Consider for a moment the comets of long return period.
Saturn orbits the Sun once every 29.4571 Earth Years.
Semimajor axis of its orbit, the average of the maximum and minimum distance from the Sun. <<>> That's basically the planet's average distance from the Sun.
Average speed during a period of time =(distance traveled during the time) divided by (length of the time period)