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If earths rotation stoped, the moon would be released. |
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| May22-11, 03:14 PM | #18 |
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If earths rotation stoped, the moon would be released.
A glance at Newtons's Law of Universal Gravitation will tell you that gravity is always a two-way street - just as the moon raises tides on earth, so earth must cause tides to sweep across the surface of the moon. These tides are not in water, of course, but in the solid rock of the lunar surface. In an amazing piece of planetary heavy lifting, the moons crust would have been distorted by up to 7 meters!
This giant tidal bulge sweeping across the moon had an interesting effect. As the moon turned beneath the Earth, the rock tide was dragged across its surface, but the rising of the tides isn't instantaneous; it takes time for the surface of the moon to respond to the pull of the earth. During that time, the moon will have rotated a bit, carrying the peak of the rock tide with it. The tidal bulge will therefore not be in perfect alignment with Earth, but slightly ahead of it. Earths gravity acts in the misshapen Moon in such a way that it tries to pull it back into sync; in other words, it works like a giant brake. Over time, this effect, known as Tidal Locking, gradually synchronizes the rotation rate of the moon with its with its orbital period, effectively meaning that the tidal bulge can remain in exactly the same place on the moons surface beneath the Earth and doesn't have to be swept around. The moon is now almost, but not quite, tidally locked to Earth, which means that it takes one month to orbit the earth and one month to rotate around on its axis. So there's no dark side of the moon-the side we can't see gets plenty of sunlight, it's just a side that perpetually faces away from the Earth. The Earth-Moon system is in fact still evolving towards being perfectly tidally locked, and in one interesting consequence of this is that the Moon is gradually drifting further and further away from the Earth at a rate of just under 4 centimeters per year. I hope this helps. |
| May23-11, 02:14 AM | #19 |
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| May23-11, 02:45 AM | #20 |
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| May23-11, 03:16 AM | #21 |
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As for my reasoning: At some point, perhaps when the moon breaks free, it will depart from us at a much faster rate. Unless the drift remains at a constant speed until it does break free, then it must be accelerating away from us even now, if only at a tiny rate of acceleration. |
| May23-11, 03:24 AM | #22 |
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Gravitational potential follows a 1/r law(?).
Why do you suggest that the Moon can "break free"? That is not what is happening at all. |
| May23-11, 03:43 AM | #23 |
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| May23-11, 04:14 AM | #24 |
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| May23-11, 04:32 AM | #25 |
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In classical mechanics, the gravitational potential at a location is equal to the work (energy transferred) per unit mass that is done by the force of gravity as an object moves to that location from a reference location. It is analogous to the electric potential with mass playing the role of charge. By convention, the gravitational potential is defined as zero infinitely far away from any mass. As a result it is negative elsewhere. I think I understand it, but I could be wrong. I'm not sure I understand the "as an object moves" part. Is there a better way of wording it? Why do I suggest the Moon can break free? If it's moving away from us at 4cm/year then at some point won't its own inertia will be stronger than the gravity which keeps it in orbit? Or will it remain in orbit, regardless of distance (at least until some other body pulls it from us)? |
| May23-11, 06:18 AM | #26 |
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"...though even at that, the Earth-Moon system is not expending any energy."
IIRC, the system is losing some energy to tidal friction / turbulence. The Moon's 'retreat' rate seems to have altered when the passage between South America and Antarctica opened, so tides could flow over the sill. Previously, 'retreat' rates seem to have depended on continental grouping, always changing due plate tectonics... Uh, IMHO, the Moon should reach an equilibrium at one of Earth's 'trojan' points -- L4 / L5... |
| May23-11, 07:44 AM | #28 |
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As with many situations, you need to consider the availability of Energy if you want to determine what will happen. In this case, there would never be enough energy available for tho Moon actually to escape. |
| May23-11, 09:58 AM | #29 |
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| May23-11, 10:14 AM | #30 |
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| May23-11, 11:54 AM | #31 |
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Mentor
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The growing consensus is that the Moon formed at about 4 to 6 Earth radii from the center of the Earth from the remnants of a collision between the proto-Earth and a Mars-sized body. That early Moon receded rather quickly from that initial orbit thanks to the huge tidal forces at such short distances. |
| May23-11, 02:10 PM | #32 |
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According to Wiki (YMMV)...
http://en.wikipedia.org/wiki/Tidal_acceleration "The rotational angular momentum of the Earth decreases and consequently the length of the day increases. The net tide raised on Earth by the Moon is dragged ahead of the Moon by Earth's much faster rotation. Tidal friction is required to drag and maintain the bulge ahead of the Moon, and it dissipates the excess energy of the exchange of rotational and orbital energy between the Earth and Moon as heat. If the friction and heat dissipation were not present, the Moon's gravitational force on the tidal bulge would rapidly (within two days) bring the tide back into synchronization with the Moon, and the Moon would no longer recede. Most of the dissipation occurs in a turbulent bottom boundary layer in shallow seas such as the European shelf around the British Isles, the Patagonian shelf off Argentina, and the Bering Sea.[10] "The dissipation of energy by tidal friction averages about 3.75 terawatts, of which 2.5 terawatts are from the principal M2 lunar component and the remainder from other components, both lunar and solar.[11]" And... http://bowie.gsfc.nasa.gov/ggfc/tides/intro.html "The tidal braking in the earth's rotation is actually caused primarily by friction in the oceans, where ``friction'' may refer to any number of physical mechanisms which have yet to be determined definitively. For example, bottom friction, induced by tidal currents flowing across the seabed, various kinds of wave breaking, and scattering of tidal waves into oceanic internal waves are all thought to play a role. For a recent overview of this subject, look up Walter Munk's paper ``Once again: once again--tidal friction,'' published in Progress in Oceanography, vol. 40, pp. 7-36, 1997." Unfortunately, the link to that paper is broken, but Google found... http://champs.cecs.ucf.edu/Library/J...20friction.pdf |
| May23-11, 02:17 PM | #33 |
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Mentor
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While angular momentum is conserved here, mechanical energy is not. As mentioned in the previous post, it is the lossiness of the system that ultimately is the cause of the recession of the Moon and the slowing of the Earth's rotation rate. |
| May23-11, 03:17 PM | #34 |
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