An asteroid/meteor impact is one theory. The truth is that nobody knows for sure, just like the exact origin of the moon is not known for certain.
27.3217 days. This is known as the moon's sidereal rotation period. The time between full moons is longer because the earth is going around the sun.
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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.
A synchronous rotation is when an object's rotation period matches its orbital period, causing the same side of the object to always face its orbiting body. This is commonly seen in moons orbiting larger planets, such as Earth's moon.
Ganymede, one of Jupiter's moons, rotates on its axis once every 7.15 Earth days. This synchronous rotation means that the same side of Ganymede constantly faces Jupiter. The rotation period was determined based on observations made by spacecraft missions like Voyager and Galileo.
The earth's period of rotation is a few minutes short of 24 hours, whereas the moon's period of rotation is a bit over 27 days.
They are precisely equal.
27.3217 days. This is known as the moon's sidereal rotation period. The time between full moons is longer because the earth is going around the sun.
Same as it's orbital period, about 27.32 days.
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how is the crater density used in the relative dating
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.
Because it is two moons wich equal 1.230 days
its the natural flow of of water causes by the earths magnetic field from it rotation which thus interacts with the moons gravitational pull called"TIDES"
Yes as Pluto is the smallest and the last planet in the solar system, it is smaller then the earths moons.
A synchronous rotation is when an object's rotation period matches its orbital period, causing the same side of the object to always face its orbiting body. This is commonly seen in moons orbiting larger planets, such as Earth's moon.
Rotation and Revolution.