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isotope of beryllium
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Beryllium-10 (10Be) is a radioactive isotope of beryllium.
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A very unstable isotope of beryllium, 8Be, undergoes emission with a half-life of 0.07 3 10215 s (0.07 fs).
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This isotope of beryllium has a nuclear halo that consists of four clustered neutrons; this allows it to be easily separated intact in the high-speed collision with the carbon target.
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Cosmogenic isotopes of aluminium, beryllium, chlorine, iodine and neon, formed by spallation of terrestrial elements under cosmic ray bombardment, have been detected on Earth.
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The beryllium isotope record measures solar energy output, independent of volcanic blocking.
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Beryllium can then fuse with helium to form an isotope of carbon that is stable.
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Researchers know this because when cosmic rays hit the atmosphere, they produce an isotope of beryllium, 10Be, which is preserved in polar ice.
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Of the 26 monoisotopic elements (those with only a single stable isotope), all but one have an odd atomic number, and all but one has an even number of neutrons — the single exception to both rules being beryllium.
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In their samples, they found an excess of beryllium-10 (10Be), an isotope produced by cosmic rays and atoms of nitrogen and oxygen.
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A partial list of radionuclides not found on Earth, but for which decay products are present: Notable isotopes with shorter lives still being produced on Earth include: Manganese-53 and beryllium-10 are produced by cosmic ray spallation on dust in the upper atmosphere.
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Cosmic-ray intensity can be estimated from the proxy record of the isotopes beryllium-10, carbon-14, and chlorine-36 deposited in various strata, isotopes which are thought to derive either from the original cosmic-ray source, or as a result of collisions in interstellar space.
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Two examples of isotopes that emit neutrons are beryllium-13 (decaying to beryllium-12 with a mean life 2.7×10−21 s) and helium-5 (helium-4, 7×10−22 s).
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Actually, more than one type of beryllium was formed, and one of these was an isotope with an atomic weight of 8. It was very radioactive and lasted barely one ten-thousand-billionth of a second, after which it disintegrated, producing two helium nuclei again.
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The physical link between low sunspot activity and cooling temperatures has not been established, but the coincidence of the Maunder Minimum with the deepest trough of the Little Ice Age is suggestive of such a connection.[2] The Spörer Minimum has also been identified with a significant cooling period near the beginning of the Little Ice Age. Other indicators of low solar activity during this period are levels of the isotopes carbon-14 and beryllium-10.[3]
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The physical link between low sunspot activity and cooling temperatures has not been established, but the coincidence of the Maunder Minimum with the deepest trough of the Little Ice Age is suggestive of such a connection.[2] The Spörer Minimum has also been identified with a significant cooling period near the beginning of the Little Ice Age. Other indicators of low solar activity during this period are levels of the isotopes carbon-14 and beryllium-10.[3]
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Of the 26 "monoisotopic" elements that have only a single stable isotope, all but one have an odd atomic number — the single exception being beryllium.
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Both of the natural isotopes have an unexpectedly low nuclear binding energy per nucleon (~5.3 MeV) when compared with the adjacent lighter and heavier elements, helium (~7.1 MeV) and beryllium (~6.5 MeV).
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Similarly, Lockwood 2007 compared neutron monitor measurements, Beryllium 10 and Carbon 14 isotopes (both proxies for cosmic radiation) as well as several other measures of solar activity and concluded "the observed rapid rise in global mean temperatures seen after 1985 cannot be ascribed to solar variability, whichever of the mechanism is invoked and no matter how much the solar variation is amplified."
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