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Fission and fusion are different types of nuclear reactions in which energy is released from the high-powered bonds between particles in the atomic nucleus. The atomic nucleus is most stable when binding energies between particles are strongest. This occurs with iron and nickel. For lighter atomic nuclei, energy can be extracted by combining these nuclei together, a process known as nuclear fusion. For nuclei heavier than those of iron or nickel, energy can be extracted by splitting them apart in a process called nuclear fission.

Because the binding force in the atomic nucleus contains enormous energy, fission and fusion can both provide tons of power, in principle. However, practical considerations make the exploitation of nuclear power more difficult than something as simple as starting a fire. For fission, highly purified feedstock, usually uranium or plutonium isotopes, must be used. Isotopes are favored because their instability makes them easier to break apart. The purification of these isotopes is extremely expensive and requires multimillion-dollar centrifuges.

In fusion, an extremely high threshold energy must be reached to combine atomic nuclei. In nature, the only place where this occurs is in the core of a star. The temperature required is in the millions of degrees. Superheated plasma and the focusing of laser power are two methods to achieve this threshold energy.

Because the matter that serves as the medium of fusion must be so hot, it must be isolated from surrounding matter using powerful magnetic fields or inertial containment. This is the principle behind the Tokamak reactor. Still, fusion requires so much energy that no one has yet built a reactor that produces more than it consumes.

The downsides to fission power include both radioactive byproducts and its association with nuclear weapons and meltdowns. In the last decade or so, nuclear physicistshave developed safer ways of building reactors, including methods for recycling the radioactive byproducts of fission. These advances have caused the US government to begin advocating the construction of nuclear reactors again.

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Monday, January 21, 2008
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Not always. The reason being,  increasing atomic number doesn't always equate to increasing mass is because many atoms don't have a number of neutrons equal to the number of protons. In other words, several isotopes of an element may exist. If a sizeable portion of an element of lower atomic number exists in the form of heavy isotopes, then the mass of that element may (overall) be heavier than that of the next element. If there were no isotopes and all elements had a number of neutrons equal to the number of protons, then atomic mass would be approximately twice the atomic number (approximately because protons and neutrons don't have exactly the same mass... the mass of electrons is so small that it is negligible). Different periodic tables give differing atomic masses because the percentages of isotopes of an element may be considered changed from one publication to another.

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Saturday, November 03, 2007
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The element symbol for oxygen is O and its atomic number is 8. The mass numbers for oxygen must be 8 + 8 = 16; 8 + 9 = 17; 8 + 10 = 18. respectively

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