28 days, but to be exact 27.321582 days
the orbital period of Saturn in earth years are 89years
The answer depends on what the ordinality is based on: distance from the sun/orbital period distance from the earth brightness in our night sky size/mass number of moons when discovered when visited (fly past) by a spacecraft Each one of these will probably generate a different ordinal number.
That appears to the orbital period of Earth around the Sun, but I think the digits past 365.25 are not correct.
It's a shorter way of saying "menstrual period" as opposed to other kinds of periods, such as orbital periods, periods of time, etc. The etymology of the word is something along the lines of "Interval, season, time, circuit" etc.
270 days = 0.73973 ordinary calendar year 0.72770 calendar leap year 0.73924 earth orbital period
Neptune has 13 known moons and an orbital period of about 60190 Earth days.
For moons to have an orbital resonance, there must be at least two moons orbiting the planet. Orbital resonance occurs when the orbital periods of the moons are related by a ratio of two small integers, such as 1:2 or 2:3.
Same as it's orbital period, about 27.32 days.
Uranus has an orbital period of about 84 Earth years, or approximately 30,687 Earth days. It takes Uranus this long to complete one orbit around the sun.
The moon's orbital period is approximately 27.3 days.
Io is the Galilean Moon that has the fastest revolution around Jupiter, completing one orbit in about 1.8 Earth days. Due to its close proximity to Jupiter, Io experiences strong tidal forces which contribute to its rapid orbit.
16 moons
The orbital period of Mars is equal to about 1.88 Earth years.
No the moon doesn't have orbitals.
The orbital speeds of Jupiter's Galilean moons are significantly faster than Earth's moon. For example, Io, the innermost moon, has an average orbital speed of about 17.3 km/s, whereas Earth's moon has an average orbital speed of about 1 km/s. This difference is because Jupiter's stronger gravitational pull causes its moons to orbit at higher speeds.
A state of `synchronous rotation`. Its where the rotational period of the moon is equal to orbital rotation period about Earth, one face of the moon will always appear to face earth. In our moons case this is due to tidal locking.
A very pronounced ring systemGreater distance from the SunSaturn has at least 62 moons, 53 of which have formal namesA longer orbital period