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The Moon's Orbit and Rotation



The Earth with its moon, as seen from space.
Click on image for full size (24K GIF)
Image courtesy of NASA.
All the planets except Venus and Mercury have moons. The Earth's Moon is the fifth largest in the whole solar system, and is bigger than the planet Pluto. Earth's gravity pulls on the Moon and keeps it in orbit. The Moon's orbit is almost a perfect circle, so the Moon is about 384,400 km away all the time. Although the Sun is really much bigger than the Moon, the Moon is much closer, so it appears to be the same size as the Sun in our sky. A total eclipse occurs when the Moon is in the right position to just cover up the Sun.

It takes the Moon about 27 days to go around the Earth once. If you check on the Moon several times during one night, you will notice that it moves relative to the stars around it. As the Moon goes around the Earth, different portions of it are lit up by the Sun, causing lunar phases. It takes the Moon one month to go through all its phases.

Have you ever heard the term the 'far-side' of the Moon? The Earth's gravity produces tidal forces on the Moon. This causes the same side of the moon to always face the Earth. People living on the Earth can never see the 'far-side' of the Moon, unless they go there! Tidal forces cause many of the moons of our solar system to always face their planets.

The Moon's Orbit and Rotation



The Earth with its moon, as seen from space.
Click on image for full size (24K GIF)
Image courtesy of NASA.
The Earth's Moon is the fifth largest in the whole solar system, and is bigger than the planet Pluto. The Moon has a nearly circular orbit (e=0.05) which is tilted about 5° to the plane of the Earth's orbit. Its average distance from the Earth is 384,400 km. The combination of the Moon's size and its distance from the Earth causes the Moon to appear the same size in the sky as the Sun, which is one reason we can have total solar eclipses.

It takes the Moon 27.322 days to go around the Earth once. Because of this motion, the Moon appears to move about 13° against the stars each day, or about one-half degree per hour. If you watch the Moon over the course of several hours one night, you will notice that its position among the stars will change by a few degrees. The changing position of the Moon with respect to the Sun leads to lunar phases.

Have you ever heard the term the 'far-side' of the Moon? Because of the effect on the Moon of tidal forces due to the Earth, the same side of the moon always faces the Earth. In other words, it takes the Moon the same amount of time to rotate around once as it does for the Moon to go around the Earth once. Therefore, Earth-bound observers can never see the 'far-side' of the Moon. Tidal forces cause many of the moons of our solar system to have this type of orbit.

The Moon's Orbit and Rotation



The Earth with its moon, as seen from space.
Click on image for full size (24K GIF)
Image courtesy of NASA.
The Earth's Moon is the fifth largest in the whole solar system, and is bigger than the planet Pluto. The Moon has a nearly circular orbit (e=0.05) which is tilted about 5° to the plane of the Earth's orbit. Its average distance from the Earth is 384,400 km. The combination of the Moon's size and its distance from the Earth causes the Moon to appear the same size in the sky as the Sun, which is one reason we can have total solar eclipses.

The Moon's orbital period is 27.322 days. Because of this motion, the Moon appears to move about 13° against the stars each day, or about half of a degree per hour. If you watch the Moon over the course of several hours one night, you will notice that its position among the stars will change by a few degrees. The changing position of the Moon with respect to the Sun leads to lunar phases.

Have you ever heard the term the 'far-side' of the Moon? Because of the effect on the Moon of tidal forces due to the Earth, the same side of the moon always faces the Earth. The rotation period and the orbital period of the Moon are the same. Therefore, Earth-bound observers can never see the 'far-side' of the Moon. Tidal forces cause many of the moons of our solar system to have this type of orbit.


Last modified prior to September, 2000 by the Windows Team

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