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Why does the Same Side of the Moon Always Face the Earth? |
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The same side of the moon always faces the Earth. The "dark side" of the moon is not actually dark — it gets cycles of day and night just like most places on Earth — it is just so named because we never see it. The "far side of the moon" is a more correct term. The reason that one side of the moon is never visible from the Earth is because the moon spins once on its axis in precisely the same amount of time it takes to revolve around the Earth. If its rate of rotation were slightly different than its rate of revolution, we would eventually be exposed to the entire surface of the moon. However, these two intervals have been equal for all of recorded history, and probably for millions of years or longer. This otherwise bizarre phenomenon can be explained in terms of a subtle effect generated by gravitation and friction — tidal locking. Through their mutual gravitational attraction, the Earth and the moon create tidal bulges on each other. One bulge faces in the direction of the other body, and one faces away. These bulges generate heat through the friction of rock rubbing against itself. Over time, they siphon energy away from the rotational momentum of both bodies, producing a breaking effect. Because the Earth's mass dominates the Earth-Moon system, the moon experiences the greater braking effect. Over time, the moon's rotation has progressively slowed until the rate of rotation matches the rate at which the tidal bulge moves around the body. Today, lunar tidal bulges are located at a constant position with respect to the rotation of the moon, meaning a sort of equilibrium has been reached. The Earth's rate of rotation slows over time due to moon-created tidal forces, but the braking effect is much smaller -- in order to be synchronized perfectly with the moon, the Earth would need to rotate only once per lunar cycle, or about every 29.5 days. Then the moon would always be in the same place in the sky, and visible from only one side of the Earth, but this is not the case. In certain planetary systems, like that of dwarf planet Pluto and its satellite Charon, both bodies are tidally locked to one another.
Written by
Michael Anissimov |
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