It is called synchronous rotation when the rotation and orbit take the same amount of time.
well, it just so happens I've done research in this type of stuff in school, and i can remember, and tell you that the 2 planets that have the closest period of rotation are Jupiter and Saturn.
When the moon's period of rotation is equal to its period of revolution, it results in synchronous rotation. This means the same side of the moon always faces the Earth.
When a satelite's rotational period is the same as its orbital period, like our moon, the satelite is tidally locked to the body being orbited. Such a rotation rate is known as a synchronous rotation. The effect is that the same side of the satelite always faces the orbited body.
Synchronous rotation occurs when the moon's orbital period (the time it takes to orbit the Earth) and rotational period (the time it takes to rotate on its axis) are equal. This means that the same side of the moon always faces the Earth.
The period of rotation of Callisto, one of Jupiter's moons, is approximately equal to its orbital period, which is about 16.7 Earth days. This means that Callisto takes about 16.7 days to rotate once on its axis.
Cause us to always see the same "face" of the moon. This is called synchronous rotation.
well, it just so happens I've done research in this type of stuff in school, and i can remember, and tell you that the 2 planets that have the closest period of rotation are Jupiter and Saturn.
They are precisely equal.
Because the time periods of the moon's rotation and revolution are exactly equal.
When the moon's period of rotation is equal to its period of revolution, it results in synchronous rotation. This means the same side of the moon always faces the Earth.
the equal area law.
Most of the large moons in our solar system rotate so that they always show the same side to the planet. This is caused by "tidal forces". The tides have slowed the moons' rotations down until their rotation periods equal their orbital periods. The moons also slow down the planets; our planet is rotating slower and slower. Once again, this affects the rotation. However, since angular momentum MUST be conserved, the Moon also gets farther and farther from our planet, thus affecting its revolution around Earth.
When a satelite's rotational period is the same as its orbital period, like our moon, the satelite is tidally locked to the body being orbited. Such a rotation rate is known as a synchronous rotation. The effect is that the same side of the satelite always faces the orbited body.
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.
How gravity works. But specifically, Kepler's Third Law.
Synchronous rotation occurs when the moon's orbital period (the time it takes to orbit the Earth) and rotational period (the time it takes to rotate on its axis) are equal. This means that the same side of the moon always faces the Earth.
Venus has a rotation period longer than its revolution. It takes about 243 Earth days for Venus to complete one rotation on its axis, while it orbits the Sun in about 225 Earth days. This results in Venus having a longer day (rotation period) than its year (revolution period).