Loading…
Loading contentLoading…
Loading contentThe production of the light elements — hydrogen, helium, and traces of lithium — in the first few minutes of the Universe.
For about three minutes the Universe was hot and dense enough for nuclear fusion, forging roughly 75% hydrogen and 25% helium by mass, plus a trace of lithium and deuterium. The predicted abundances match observations remarkably well, providing one of the strongest confirmations of the hot Big Bang.
Facts on this topic will be cited from these primary and reference sources.
Mission data, planetary science, space telescopes, and public-domain imagery.
Most NASA-produced imagery is in the public domain; individual items are checked for usage terms before publication.