The rotation of the moon, or the time it takes to rotate on it's axis exactly once, is
27.322 days (rounded), and the moon's orbital period, or the time the moon takes
to complete one full revolution around the Earth, exactly the same. That's why the
Moon appears to always show the same face. We see the same side of the moon
and never get to view the far side from Earth.
what is Saturn's moon Titan's rotational period
Ananke's rotational period is around 45.7 Earth days. It rotates on its axis at a slower rate compared to many other moons in our solar system.
due to a phenomenon called synchronous rotation, where the moon's rotational period is equal to its orbital period. This gravitational interaction causes one side of the moon to always face the planet.
A day on Haumea is very short, since its rotational period is just 3.9155 hours. It takes 284.12 Earth-years (103774 Earth-days) for it to completely orbit the Sun, which means there are 636,081.216 Haumean days in one Haumean year.
Saturn has a sidereal rotational period of 10.57 hours and a rotational velocity of 9.87 km per second. Because of its gaseous composition, it has a varying rotational period at the poles which is about 10 hours 45 minutes.
30048.135 days
what is Saturn's moon Titan's rotational period
Ananke's rotational period is around 45.7 Earth days. It rotates on its axis at a slower rate compared to many other moons in our solar system.
243 days in earth days and no earth years.
Haumea's rotational period is 3.9155 hours.
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.
it3671/4 24 hr
due to a phenomenon called synchronous rotation, where the moon's rotational period is equal to its orbital period. This gravitational interaction causes one side of the moon to always face the planet.
A day on Haumea is very short, since its rotational period is just 3.9155 hours. It takes 284.12 Earth-years (103774 Earth-days) for it to completely orbit the Sun, which means there are 636,081.216 Haumean days in one Haumean year.
Saturn has a sidereal rotational period of 10.57 hours and a rotational velocity of 9.87 km per second. Because of its gaseous composition, it has a varying rotational period at the poles which is about 10 hours 45 minutes.
7.8 hours
The inner planets, such as Mercury, Venus, Earth, and Mars, have shorter rotational periods ranging from about 24 hours to a few days. In comparison, the outer planets, like Jupiter, Saturn, Uranus, and Neptune, have longer rotational periods ranging from around 10 hours to a few days. This difference is mainly due to the size and mass distribution of the planets.