This is actually quite common. The reason is that a Moon around a planet will rotate slower and slower (due to tidal forces), until it always shows its planet the same side. At the same time, the planet - for example, our Earth - will rotate slower and slower, until it will show the Moon the same size. This assumes there is a single Moon, as in the case of Earth. However, since the planet has a larger mass, and thus a higher rotational momentum, it will take the planet longer to slow down. In the case of Earth/Moon, the Moon has already slowed down as far as it can; Earth will slow down, to always show the Moon the same side, some time in the future.
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.
Makemake's orbital period is 309.88 years or 113,183 days
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.
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 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.
Phobos is tidally locked; its rotational period and orbital period are the same (a little under 7 hours 40 minutes).
Phobos is tidally locked; its rotational period and orbital period are the same (a little under 7 hours 40 minutes).
Among the planets and dwarf planets, Neptune takes the longest to complete one revolution around the Sun, taking about 165 Earth years. Among dwarf planets, Eris has an even longer orbital period, taking approximately 557 Earth years to complete one revolution. Thus, Eris holds the record for the longest orbital period in our solar system.
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.