Protons

Protons are emitted from carbon atoms in solar reactions as hydrogen is converted into helium. 41:8.1

The reciprocal function of the mesotron holds the charged protons and uncharged neutrons together in the nucleus of an atom, ensuring stability and preventing disruption. 42:8.3-4

In Orvonton, introducing over 100 orbital electrons instantly disrupts the central proton, causing the dispersion of electrons and other energies. 42:7.7

A proton may be no larger than an electron, but it weighs almost two thousand times more than an electron and is eighteen hundred times as heavy as an electron. 42:6.7-8 42:7.2

See also

• atoms
• matter

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