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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Evidence · 1
Timeline
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Connections · 3
- Giant molecular cloudconcerns
- Stellar nucleosynthesisconcerns
- Initial stellar massconcerns
Assembled narrative · 1
Assembled from 32 blocks · 1 evidence · 29 related
- Story
- 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.
- Knowledge
- Initial stellar mass
- Giant molecular cloud
- Stellar nucleosynthesis
- The first stars form from metal-free gas
- Connections
- Giant molecular cloud
- Stellar nucleosynthesis
- Initial stellar mass
- Eagle Nebula (Messier 16) and the Pillars of Creation
- Protostar
- Planetary nebula
- Supernova
- The first stars form from metal-free gas
- The Sun forms and settles onto the main sequence
- Hubble photographs the Pillars of Creation
- Hydrogen fusion: the proton-proton chain and the CNO cycle
- The iron peak in nuclear binding energy
- Rapid neutron capture (the r-process)
- The first stars form from metal-free gas
- B2FH sets out the synthesis of the elements in stars
- A neutron-star merger is detected in gravitational waves and light
- Hydrogen fusion: the proton-proton chain and the CNO cycle
- Main sequence (core hydrogen burning)
- Supernova
- Protostar
- The first stars form from metal-free gas
- SN 1987A: neutrinos from a collapsing core reach Earth
- Evidence
- 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.
Observed changes · 0
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