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For 1 Joule tidal energy harvested
Quote from: hamdani yusufFor 1 Joule tidal energy harvestedThere is a huge amount of tidal energy involved in daily flexing the solid Earth, and dragging the world's oceans across their ocean floors.If we harvested 1 Joule (or 1 TJ) of this energy, it would make an insignificant change in the amount of energy lost to tides every day.
In order for an object to reach a higher and therefore longer orbit its velocity must increase by some amount to get out of its current orbit. The new orbit will require a lower velocity than the original one. So it has to slow down again.
According to my calculations, the Moon gains about 3.826 x 10^18 joules from the Earth due to tidal action every year. It gains 7.564 x 10^18 joules of gravitational potential energy due to the increase in distance from the Earth (3.82 centimeters per year) and loses 3.738 x 10^18 joules of kinetic energy due to the slowing of its orbital speed. That assumes I didn't make any kind of calculation error. The Moon has been doing this for billions of years and will continue to do it for hundreds of millions of years yet. Of course, the rate has varied in the past (it would have taken energy from the Earth at a much faster rate in the distant past when it was much closer to the Earth). In the future, that rate will slow down. The rotational kinetic energy of the Earth is 2.138 x 10^29 joules. It's pretty safe to conclude that nothing humans could do in the immediate future would come remotely close to exhausting such a resource.
Thanks for your effort. Can you share your calculation?
Did you calculate based on earth-moon barycenter? IMO, when the moon is moving away from earth, it also means that the earth is moving away from the barycenter too, which makes total potential energy of the system increase.
Quote from: JeffreyHIn order for an object to reach a higher and therefore longer orbit its velocity must increase by some amount to get out of its current orbit. The new orbit will require a lower velocity than the original one. So it has to slow down again. This imagines that the effect of tides is the same as firing a rocket motor for a short time.If you are in a circular orbit around Earth, and wish to reach a higher circular orbit around Earth using a chemical rocket, you:- fire the rocket for a short time, putting you into an elliptical orbit whose highest point above Earth is the altitude of the new orbit you want.- On this elliptical orbit, you start moving farther from the Earth; your velocity away from the Earth declines towards zero due to gravitational attraction to the Earth.- when you reach the maximum altitude of this elliptical orbit, and are about to fall back to Earth, you fire your rocket again, for a short time, to give you the (lower) velocity you need to stay in orbit at this higher altitude.- As the comment says, this involves (two) bursts of acceleration, plus a period of coasting in zero-g, when you slow down again.- You feel "jerk" at the start and end of the rocket burns (and because rockets are chaotic, you feel some high-frequency jerk during the burn, which does not affect your altitude).However, tidal effects on the Moon are continuous, rather than in short bursts, and so you would not feel any measurable jerk.
Quote from: hamdani yusuf on 21/05/2017 04:51:59Thanks for your effort. Can you share your calculation?I found an equation that predicted orbital velocity based on the distance a satellite is from a planet and the planet's mass. The equation is: orbital velocity (m/s) = square root ((gravitational constant x mass of the planet (kg)) / orbital radius (m)).The orbital velocity I calculated for the Moon's semi-major axis of 384,399,000 meters was 1,018.20824493 meters per second. Then I used Newton's kinetic energy equation to calculate how much kinetic energy the Moon (with a mass of 7.342 x 10^22 kilograms) would have at that velocity. The equation is: kinetic energy (J) = 0.5 x mass (kg) x (velocity (m/s))^2. The result was 38,059,020,182,894,347,263,576,879,000 joules.Then I repeated the calculations with the Moon being 3.82 centimeters further out (384,399,000.0382 meters), resulting in an orbital velocity of 1,018.20824488 meters per second and a kinetic energy of 38,059,020,179,156,504,796,530,624,000 joules. I subtracted the two to get a kinetic energy decrease of 3,737,842,467,046,255,000 joules per year.For the gravitational potential energy, I likewise used the required equation as found by Google. The equation is: gravitational potential energy (J) = (-(gravitational constant) x (mass of Earth (kg)) x (mass of Moon (kg))) / orbital radius (m). First I calculated the potential energy for the Moon at 384,399,000 meters from Earth and then calculated it for the Moon at 384,399,000.0382 meters from Earth. The first result was 76,118,040,365,661,721,284,394,600,402 joules and the second was 76,118,040,358,097,421,841,161,601,579 joules. I subtracted the two to get an increase of 7,564,299,443,232,998,823 joules of gravitational potential energy. I then subtracted the kinetic energy from the potential energy to get 3,826,456,976,186,743,823 joules.
There's an easier way. The total orbital energy can be found by:E= -GMm/2awhere a is the semimajor axis. By using 3.987e14 for GM (we actually know this product more accurately than we know either G or the mass of the Earth) and calling it U, you can find the energy difference by-Um/2 (1/a1-1/a2)For your given Moon mass, this works out to 3,783,812,701,003,630,000 Joules.
Surely the 38.2mm per year of extra separation would not be constant and would increase year on year.... therefore the amount of energy that holds the moon in place would need to increase but as it is decreasing because of all the wave farms, the rate of change of yearly position would also increase, of course this ignores any external forces that may reduce that distance impacts from meteorites for instance ...
Teach us more in this field. After reading on here, we can learn more in this topic.
Quote from: Horence on 22/05/2017 10:32:53Teach us more in this field. After reading on here, we can learn more in this topic.I´m glad you enjoy learning ... But watch out: I´m afraid many things said here may be erroneous. But discussion bring light! (literally translated from Spanish).I can´t actually see how tidal harvesting on Earth could increase our Moon´s speed… Locally harvested energy is a small part of the energy acquired by water (certainly thanks to Moon´s pull … and Sun´s), which if not harvested would be wasted mainly as friction heat. How could that “tele-affect" the Moon?Our planet tides do affect it, making days a little longer after eons. Similarly, when the Moon was first forming (much closer to Earth than now) , on Moon there were tides of molten lava, and that made Moon´s days longer and longer with time.That said, as far as I can understand the reason of Moon´s distance slow increase is related to Earth tides, but independently of any possible harvesting.Moon related high tide doesn´t happen when moon is exactly over considered meridian, but with some delay. That´s because the top of the tidal bulge can´t catch up with below moon meridian, due to the high linear velocity of sea surface because of earth rotation (40,000 km/24h at the equator), and it always is some angular distance East to the meridian below Moon.Although main component of attraction between moon and C.G. of the tidal bulge is vertical, a relatively tiny tangential component does exist. Naturally, in both senses (Newton´s 3rd Law). That is why Moon´s tangential velocity, slowly but surely, increases.It´s a kind of “chainless" hammer throwing effect, without releasing non existing chain ...
...These turbines will add a bit of extra tidal drag. The present tidal bulge position is determined by a balance between the Earth trying to drag the bulge with it and the Moon trying to align it with itself. The extra drag will cause the tidal bulge to be dragged by the rotating Earth just a bit more ahead of the Moon. This in turn, causes it pull forward on the Moon a little more, increasing the rate at which the Moon gains orbital energy.