Protons are emitted from carbon atoms in solar reactions as hydrogen is converted into helium. [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. [2] In Orvonton, introducing over 100 orbital electrons instantly disrupts the central proton, causing the dispersion of electrons and other energies. [3]
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. [4]
See also: UB 42:3.5.