Born in the hot cores of massive stars, this nitrogen atom formed through proton and alpha captures during hydrogen and helium burning and related shell burning phases. Later ejected by supernova.
Stellar processes set elemental abundance available to planets.
Dispersal through the Interstellar Medium [2]
Molecular clouds, dust grains, and ice chemistry.
later
›
The atom joined interstellar gas and ices, then condensed into a molecular cloud and protoplanetary disk that formed planets and planetesimals.
Interstellar chemistry and collapse determine element partitioning into planets.
Arrival on Early Earth — Accretion and Outgassing [3]
N2 is fixed biologically and abiotically, nitrified, assimilated, and returned via ammonification and denitrification; microbes drive most transformations.
Human activity alters fluxes through fertilizers and emissions.
Fixed nitrogen flows into soils and aquatic systems, is taken up by producers, passed through food webs, and recycled by decomposers.
An atom can pass through multiple living systems over time.
Into the Fungus — Uptake and Assimilation by Mycelium [6][7]
Saprotrophic and mycorrhizal strategies for nitrogen acquisition.
now
›
Fungi absorb inorganic and organic nitrogen; enzymes free amino acids and ammonium which mycelium transports to build proteins and nucleic acids in the fruiting body.
The atom becomes part of mushroom biomass.
The Big Picture — Cosmic to Living Connections [3][4]
How stellar origins and Earth cycles connect to life.
relevance
›
This atom's story links stellar element synthesis, planetary redistribution, and biological recycling, showing why Earth can support life and how cycles are sensitive to human influence.
Takeaway: life is made from ancient stardust.
References (APA)
Britannica, T. Editors of Encyclopaedia. (2025). Stellar nucleosynthesis. Encyclopaedia Britannica. https://www.britannica.com/science/stellar-nucleosynthesis
Fogel, M. L. (2015). Nitrogen in extraterrestrial environments and interstellar medium. Elements, 11(6), 423-431.
Li, Y., et al. (2024). The origin and evolution of Earth's nitrogen. National Science Review, 11(6), nwae201. https://doi.org/10.1093/nsr/nwae201