This depends on the mass of the planet (and sun or star that it orbits around) and the distance between the two. See Kepler's laws of planetary motion.
A planet's orbital radius directly affects its orbital period through Kepler's third law of planetary motion. The farther a planet is from the star it orbits, the longer its orbital period will be, assuming all other factors remain constant. This relationship is expressed mathematically as T^2 ∝ r^3, where T is the orbital period and r is the orbital radius.
Jupiter's orbital period is only 1.53% less than1/7 the orbital period of Uranus.
Not at all. The only thing that sets the orbital period is the semimajor axis, which is the average of the maximum and minimum distances from the Sun.
Orbital information. You need to know the size of the "semi-major axis". Then you can calculate the orbital period, using Kepler's Third Law.
A planets period or revolution, the time taken to orbit its star, is dependant on its mass, the stars mass and the distance between the two. See Kepler's laws of planetary motion for further information.
Makemake's orbital period is 309.88 years or 113,183 days
A planet's orbital period is related to its distance from the Sun by Kepler's third law, which states that the square of the orbital period is proportional to the cube of the semi-major axis of the orbit. For an orbital period of 3 million years, the planet would need to be located at a distance of approximately 367 AU from the Sun.
The time it takes for a planet to orbit the sun is known as its orbital period. The order of planets from shortest to longest orbital period is: Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, and Neptune. Mercury has the shortest orbital period of about 88 Earth days, while Neptune has the longest orbital period of about 165 Earth years.
The orbital characteristics of the planets in our solar system include their elliptical orbits, which vary in shape and size. Most planets orbit the Sun in a plane known as the ecliptic, with a slight tilt. The distance from the Sun affects their orbital period; for instance, Mercury has a short orbital period of about 88 Earth days, while Neptune takes about 165 Earth years to complete one orbit. Additionally, the planets generally move in the same direction around the Sun, with their orbits becoming more circular as the distance from the Sun increases.
As it increases, the orbital speed increases, and the period (time to complete an orbit) decreases, which is why Mercury has the shortest year, and Neptune the slowest orbital speed.
They are farther away and have larger orbital periods.
The planets rotation does not really relate to the orbital period. Some planets like Mercury and Venus and Mars orbit the sun in a short time, but take a long time to rotate on their axis, Earth is the exception, where a collision with the moon many years ago may have caused its days to be a lot shorter than the other rocky planets. Saturn and Jupiter rotate fairly quickly on their axis.