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Nuclear physics
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smaller atoms than iron because the binding energy per nucleon peaks around iron (56 nucleons). Since the creation of heavier nuclei by fusion requires energyCompton wavelength (1,627 words) [view diff] exact match in snippet view article find links to article
{fm}}^{2},} which is roughly the same as the cross-sectional area of an iron-56 nucleus. For gauge bosons, the Compton wavelength sets the effective rangeStar (16,417 words) [view diff] exact match in snippet view article find links to article
silicon-burning process that results in the production of the stable isotope iron-56. Any further fusion would be an endothermic process that consumes energyPair-instability supernova (2,104 words) [view diff] exact match in snippet view article find links to article
has a half-life of 77 days and then further decays to the stable isotope iron-56 (see Supernova nucleosynthesis). For the hypernova SN 2006gy, studies indicateOreo O's (904 words) [view diff] no match in snippet view article find links to article
Quantity %DV† Vitamin A equiv. 2% 15 μg Vitamin C 28% 25 mg Minerals Quantity %DV† Calcium 0% 1 mg Iron 56% 10 mg Potassium 2% 49.41 mg Sodium 6% 128.25 mgChemical element (10,055 words) [view diff] exact match in snippet view article find links to article
to iron are made in large stars in the process of becoming supernovas. Iron-56 is particularly common, since it is the most stable nuclide that can easily2010 Michigan gubernatorial election (2,394 words) [view diff] no match in snippet view article find links to article
2% 13,269 25.9% 4,754 1.9% 358 Iosco 61.5% 5,943 35.5% 3,435 3.0% 287 Iron 56.0% 2,516 40.6% 1,825 3.4% 154 Isabella 61.7% 9,865 36.1% 5,776 2.2% 345Supernova (21,940 words) [view diff] exact match in snippet view article find links to article
is generated by the radioactive decay of nickel-56 through cobalt-56 to iron-56. The peak luminosity of the light curve is extremely consistent acrossAbiogenesis (21,073 words) [view diff] exact match in snippet view article find links to article
formation through stellar nucleosynthesis proceeds to its most stable element Iron-56. Heavier elements were formed during supernovae at the end of a stars lifecycleType II supernova (4,792 words) [view diff] exact match in snippet view article find links to article
nickel-56 is produced, which decays radioactively into cobalt-56 and then iron-56 over the course of a few months. As iron and nickel have the highest bindingAnomalon (1,128 words) [view diff] no match in snippet view article find links to article
like cosmic rays. Further studies were carried out with Oxygen 16 and Iron 56, and these experiments also showed the same short tracks. In order forDC Trident (945 words) [view diff] no match in snippet view article find links to article
Iron 392.5 DC Trident 350 Aqua Centurions 344 Ranomi Kromowidjojo ( Team Iron) 56 pts 26–27 October (Match 4) Budapest Danube Arena Cali Condors 610.5 TeamStockholm during the early Vasa era (1,649 words) [view diff] no match in snippet view article find links to article
controlled national trade. The most important export items at this time was iron (56%), butter (11%), train oil (10%), and salmon (6%) (export of copper was2020 International Swimming League (113 words) [view diff] no match in snippet view article find links to article
49 Alia Atkinson London Roar 1:02.66 Budapest SF 2 Hüseyin Emre Sakçı Iron 56.51 Lilly King Cali Condors 1:03.29 Budapest F Adam Peaty London Roar 55Titus Pankey (1,516 words) [view diff] exact match in snippet view article find links to article
half-life followed by cobalt-56 decaying more slowly decaying to stable iron-56 with a 77 day half-life. This is the first example of the now-acceptedCentral nervous system effects from radiation exposure during spaceflight (9,537 words) [view diff] exact match in snippet view article find links to article
(July 2000). "Spatial learning and memory deficits induced by exposure to iron-56-particle radiation". Radiation Research. 154 (1): 28–33. Bibcode:2000RadR