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The Protoactive isotope family
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Protoactives are the most useful but most
unstable sub-atomic structures for life in the Universe. Luckily, they are
largely restricted to single structures as core fusion of Protoactives into
"helium" type structures requires extremely high temperatures (over 20 million
degrees Kelvin). As such, Earth is only exposed to single Protoactives,
restricted to unstable Hydro and Helium type structures. |
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Protoactive atomic structures are also
formed in our atmosphere, as well as from major disturbances such as Asteroid
hits. However, Protoactive isotopes are rarer in the lower mass elements than
compared to the higher elements (weakly fused cores via the effects of nature)
that contain high numbers of protoactives. |
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This partly explains the phenomena that
some elements above Calcium (20) tend to have more Neutrons than Protons.
However, because the relative temperatures to form, Protoactives are much
higher than Protons (and impossibly high for our Sun to create Helium
Protoactive cores), Protoactives are in much lower numbers and behave like
unstable Hydrogen atoms. Deuterium is an excellent example of a Protoactive
Isotope. The Protoactive is more than strong enough to pull in two, sometimes
three Neutrons (as in Tritium). |
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