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Examination 1
Examination 1

... a breaking of bonds within the molecules that were reaction to form new bonds and new molecules. The identity of the atoms participating in the reaction remained the same - so in balancing the reaction we always made sure that the number of atoms of each element on both sides of the eqn. was the sam ...
Nuclear Chemistry
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... • Nuclear fission is the splitting of an atomic nucleus. • For fission to occur the uranium 235 or plutonium 239 nucleus must first absorb a neutron. • The nucleus undergoing fission splits into two smaller nuclei and 2 or 3 neutrons and energy is released. • The neutrons may go on to start a chain ...
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... produces an electric charge in the surrounding air can produce fluorescence (glowing)  Nuclear radiation damages most cells.  The source of radiation is the nucleus. NUCLEAR STABILITY:  The nucleus contains protons and neutrons. This poses a problem as the positive protons try to repel each other ...
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... 116. What is the molar mass of aluminum hydroxide? 78.22 g 117. How many moles of sodium sulfate are 35.5 g of sodium sulfate? 0.25 mol 118. How many atoms are in one formula unit of aluminum sulfate? 17 119. Hydrazine (dinitrogen tetrahydride) is used as a liquid rocket fuel. Hydrazine reacts with ...
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Nuclear fusion



In nuclear physics, nuclear fusion is a nuclear reaction in which two or more atomic nuclei come very close and then collide at a very high speed and join to form a new nucleus. During this process, matter is not conserved because some of the matter of the fusing nuclei is converted to photons (energy). Fusion is the process that powers active or ""main sequence"" stars.The fusion of two nuclei with lower masses than Iron-56 (which, along with Nickel-62, has the largest binding energy per nucleon) generally releases energy, while the fusion of nuclei heavier than iron absorbs energy. The opposite is true for the reverse process, nuclear fission. This means that fusion generally occurs for lighter elements only, and likewise, that fission normally occurs only for heavier elements. There are extreme astrophysical events that can lead to short periods of fusion with heavier nuclei. This is the process that gives rise to nucleosynthesis, the creation of the heavy elements during events such as supernova.Following the discovery of quantum tunneling by Friedrich Hund, in 1929 Robert Atkinson and Fritz Houtermans used the measured masses of light elements to predict that large amounts of energy could be released by fusing small nuclei. Building upon the nuclear transmutation experiments by Ernest Rutherford, carried out several years earlier, the laboratory fusion of hydrogen isotopes was first accomplished by Mark Oliphant in 1932. During the remainder of that decade the steps of the main cycle of nuclear fusion in stars were worked out by Hans Bethe. Research into fusion for military purposes began in the early 1940s as part of the Manhattan Project. Fusion was accomplished in 1951 with the Greenhouse Item nuclear test. Nuclear fusion on a large scale in an explosion was first carried out on November 1, 1952, in the Ivy Mike hydrogen bomb test.Research into developing controlled thermonuclear fusion for civil purposes also began in earnest in the 1950s, and it continues to this day. The present article is about the theory of fusion. For details of the quest for controlled fusion and its history, see the article Fusion power.
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