nucleosynthesis

Stellar element creation

Nucleosynthesis is the process by which atomic nuclei form from simpler particles—protons and neutrons.

Most hydrogen and helium originated in the Big Bang.

Heavier elements form inside stars through fusion, and the heaviest elements emerge from supernovae and neutron star collisions.

Carbon nucleosynthesis occurs in red giants.

neutronstar

kilonova

Neutron star merger explosion

uranium · lanthanides · actinides · gravitational waves · ejecta

stellar

red giant

Aged star with cooled, expanded envelope

nuclear

fusion

Joining into unity

thermonuclear · gamma rays · neutrino · resonance

bigbang

primordial

Existing from the start

hydrogen · recombination

elements

helium

Lightest noble gas

  • carbonSixth element, atomic symbol C
  • oxygenElement eight, colorless gas
  • ironElement twenty-six

nitrogen · neon · silicon · magnesium · sulfur · nickel · calcium · argon · chromium · cobalt

explosive

supernova

Exploding massive star

cosmochemistry

presolar grains

Particles predating our star

solar nebula · chondrites

Opposites
nuclear process direction

nucleosynthesisnuclear fission

Atomic core division

radioactive decay · nuclear decay · alpha decay · beta decay · fission

element origin

nucleosynthesischemical bonding

Atoms joining into molecules

Family

nuclear, nucleus, synthesis, nucleon, nuclei, nucleons

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