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121 lines
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ÜÜÜÜÜÜÜÜÜÜÜÜÜ ÜÜÜ ÜÜÜÜ
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ÜÛÛÛÛÛÛÛÛßÛßßßßßÛÛÜ ÜÜßßßßÜÜÜÜ ÜÛÜ ÜÛÛÛÛÛÛÛÛÜÜÜÜÜÛßß ßÛÛ
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ßÛÛÛÛÛÛÛÛÛÛÛÛÛÛÜ ßÛÛ ÜÛÛÛÜÛÛÜÜÜ ßÛÛÛÛÜ ßÛÛÛÛÛÛÛÜÛÛÜÜÜÛÛÝ Ûß
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ßßßÛÛÛÛÛÛÛÛÛÛÜ ÞÝ ÛÛÛÛÛÛÛÛÛÛÛßßÛÜÞÛÛÛ ÛÛÛÛÛÜ ßßÛÛÛÞß
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Mo.iMP ÜÛÛÜ ßÛÛÛÛÛÛÛÝÛ ÞÛÛÛÛÛÛÛÛÛ ÞÛÛÛÛ ÞÛÛÛÛÛÝ ßÛß
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ÜÛÛÛÛÛÛÛ ÛÛÛÛÛÛÛÛÝ ÞÛÛÛÛÛÛÛÛÝ ÛÛÛ ÛÛÛÛÛÛ
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ÜÛÛÛÛÛÛÛÝ ÞÛÛÛÛÛÛÛÛ ÞÛÛÛÛÛÛÛÛ ß ÞÛÛÛÛÛÛÜ ÜÛ
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ÜÛÛÛÛÛÛÛÝ ÛÛÛÛÛÛÛÛ ÛÛÛÛÛÛÛÛÝ ÞÞÛÛÛÛÛÛÛÛÛß
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ÜÛßÛÛÛÛÛÛ ÜÜ ÛÛÛÛÛÛÛÛÝ ÛÛÞÛÛÛÛÛÝ ÞÛÛÛÛÛÛßß
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ÜÛßÛÛÛÛÛÛÜÛÛÛÛÜÞÛÛÛÛÛÛÛÛ ÞÛ ßÛÛÛÛÛ Ü ÛÝÛÛÛÛÛ Ü
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ÜÛ ÞÛÛÛÛÛÛÛÛÛÛß ÛÛÛÛÛÛÛÛÛ ßÛÜ ßÛÛÛÜÜ ÜÜÛÛÛß ÞÛ ÞÛÛÛÝ ÜÜÛÛ
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ÛÛ ÛÛÛÛÛÛÛÛß ÛÛÛÛÛÛÛÛÛÛÜ ßÛÜ ßßÛÛÛÛÛÛÛÛÛß ÜÜÜß ÛÛÛÛÜÜÜÜÜÜÜÛÛÛÛÛß
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ßÛÜ ÜÛÛÛß ßÛÛÛÛÛÛÛÛÛÛÜ ßßÜÜ ßßÜÛÛßß ßÛÛÜ ßßßÛßÛÛÛÛÛÛÛßß
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ßßßßß ßßÛÛß ßßßßß ßßßßßßßßßßßßß
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ARRoGANT CoURiERS WiTH ESSaYS
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Grade Level: Type of Work Subject/Topic is on:
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[ ]6-8 [ ]Class Notes [Essay on Fusion Energy ]
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[x]9-10 [ ]Cliff Notes [ ]
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[ ]11-12 [x]Essay/Report [ ]
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[ ]College [ ]Misc [ ]
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Dizzed: 11/94 # of Words:868 School: ? State: ?
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ÄÄÄÄÄÄÄÄÄ>ÄÄÄÄÄÄÄÄÄ>ÄÄÄÄÄÄÄÄÄ>Chop Here>ÄÄÄÄÄÄÄÄÄ>ÄÄÄÄÄÄÄÄÄ>ÄÄÄÄÄÄÄÄÄ>ÄÄÄÄÄÄÄÄÄ
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A fusion reaction is one in which two atomic nuclei merge to form a
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heavier nucleus. this is the process that happens in in the stars. In
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average stars, like the sun, the process of fusion is converting hydrogen
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nuclei (or protons) into helium nuclei. There is an enormous amount of
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kinetic energy and gamma rays released in this process that heat the star's
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interior, and this realease is what maintains it at the extreamly high
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temperatures (greater than 10 million K) required to continue the fusion.
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This process has been making the stars go for billions of years has
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clear potential as a power source on earth. Once we have started the
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reaction, Fusion requires no energy and realeases energy in a great
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surplus. It also has no environmental problems and causes no pollutions
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whatsoever.
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The problems with fusion are the molecules of hydrogen that are
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supposed to be fused, electro-statically repel each other at a great force.
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The only way to create the conditions where the it is possible to force
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these atoms together and override their repulsion is through enormous heat,
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this method is called thermonuclear.
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Even though fusion reasearch still needs a lot of time, there has been
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some progress in discovering how we can use this. The two fusion reactions
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that are the most promising both involve the heavier isotopes of hydrogen:
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1) deuterium (composed of one proton and one neutron) Deuterium occurs
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naturally as a minor constituent in all hydrogen-containing materials--such
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as water--in quantities sufficient to meet all the energy needs of
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societies for many billions of years.
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2) tritium (composed of one proton and two neutrons). Tritium can be
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bred from lithium by a neutron-induced reaction in a blanket that could
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conceivably surround a fusion reactor. The western United States contains
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large lithium deposits in the salts of dry lake beds, and much larger
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quantities are dissolved in the sea.
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Scientists are trying different combonations of these nuecli to make
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fusion. The reaction that occurs with the greatest probability and at the
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lowest temperatures involves the fusing of a deuterium nucleus with a
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tritium nucleus to form a helium (He4) nucleus and a neutron. The products
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contain 17.6 million electron volts of released kinetic energy, this is
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great--except it's only in theory.
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Now the only thing to figure out is how can someone can get the
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deuterium nuecleus and the tritium nuecleus to fuse. The other objective
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is to create an energy source that you can get more energy out of than you
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put into.
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The first method tried was to use a charged particle accelerator to
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bombard a solid or gaseous tritium target with energetic deuterium nuclei.
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This technique consumes power rather than producing it, however, because
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most of the accelerated nuclei lose their enegy traveling like this.
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Another idea proposed in 1990 involved Tritium within metal bars that
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was put into a tank of dueterium in water. When energy was put into this
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tank something in the tritium bars forced dueterium out of the water and a
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chemical reaction fused the materials. Unfortunaltely, the was again a net
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energy loss, and only a small amount of extra heat was produced.
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Another approach to fusion, pursued since about 1974, is
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termedinertial confinement. Its aim is to compress a solid pellet of
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frozen deuterium and tritium to very high temperatures and densities in a
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process analogous to what occurs in a thermonuclear (hydrogen) bomb. The
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compression is accomplished by bombarding the pellet from all sides,
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simultaneously, with an intense pulse of LASER light, ions, or electrons.
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In 1988 it was learned that the U.S. government, which secretly had been
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using underground nuclear tests in Nevada to study inertial -confinement
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fusion, had achieved such fusion in 1986 by this means, unfortunately it
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only lasted less than a second.
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After trying these methods, most scientists now agree that the only
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way there is a net energy gain obtained is by mimicking the Sun, and
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producing starlike thermonuclear conditions.
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The goal of fusion--in effect, to make and hold a small star--is so
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daunting as to be widely considered the supreme technological challenge yet
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undertaken.
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In addition to an almost inexhaustible fuel supply, fusion has other
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attractive features:
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it is environmentally benign; the resulting ash is harmless helium and
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hydrogen; and the afterheat in the reactor structure would be much less
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than in a fission reactor and would be distributed through a greater
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thermal mass. In addition, because fusion is not a chain reaction, it
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cannot run out of control, and any tampering to the process would cause the
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plasma (the energy involved in the process) to extinguish itself. It would
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also be far more difficult to produce nuclear-weapons materials
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surreptitiously at a fusion plant than at a fission plant; because no
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fissionable material should ordinarily be present at a fusion plant.
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Present levels of support for research are aimed at building the first
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demonstration fusion plant in about the year 2024. This year is based on
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the amount nessesary for fusion reasearch and the very small amount of
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money given to fusion to this reasearch by most governments. If spending
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increases this year will most likely move out of our life times.
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