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The first stars form from metal-free gas

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The earliest generation of stars condensed out of gas containing only hydrogen, helium and traces of lithium left by Big Bang nucleosynthesis. With no carbon, oxygen or dust to radiate heat away, that gas could not cool efficiently, and theory predicts the first stars were consequently far more massive than typical stars today. No individual first-generation star has ever been observed; the epoch is constrained indirectly, by the composition of the oldest surviving low-mass stars and by observations of the earliest galaxies. The date is a model-dependent bracket, not a measurement.

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Connections · 3
Assembled narrative · 1

Assembled from 32 blocks · 1 evidence · 29 related

  1. Story
  2. The earliest generation of stars condensed out of gas containing only hydrogen, helium and traces of lithium left by Big Bang nucleosynthesis. With no carbon, oxygen or dust to radiate heat away, that gas could not cool efficiently, and theory predicts the first stars were consequently far more massive than typical stars today. No individual first-generation star has ever been observed; the epoch is constrained indirectly, by the composition of the oldest surviving low-mass stars and by observations of the earliest galaxies. The date is a model-dependent bracket, not a measurement.
  3. Knowledge
  4. Initial stellar mass
  5. Giant molecular cloud
  6. Stellar nucleosynthesis
  7. The first stars form from metal-free gas
  8. Connections
  9. Giant molecular cloud
  10. Stellar nucleosynthesis
  11. Initial stellar mass
  12. Eagle Nebula (Messier 16) and the Pillars of Creation
  13. Protostar
  14. Planetary nebula
  15. Supernova
  16. The first stars form from metal-free gas
  17. The Sun forms and settles onto the main sequence
  18. Hubble photographs the Pillars of Creation
  19. Hydrogen fusion: the proton-proton chain and the CNO cycle
  20. The iron peak in nuclear binding energy
  21. Rapid neutron capture (the r-process)
  22. The first stars form from metal-free gas
  23. B2FH sets out the synthesis of the elements in stars
  24. A neutron-star merger is detected in gravitational waves and light
  25. Hydrogen fusion: the proton-proton chain and the CNO cycle
  26. Main sequence (core hydrogen burning)
  27. Supernova
  28. Protostar
  29. The first stars form from metal-free gas
  30. SN 1987A: neutrinos from a collapsing core reach Earth
  31. Evidence
  32. Establishes stellar nucleosynthesis as the origin of the elements heavier than helium and organises production into distinct nuclear processes including slow and rapid neutron capture. Title, authors, journal, volume and pages were read from ADS and publisher listings via search; the review itself was not fetched, so the internal process taxonomy is described from secondary accounts.
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