White dwarf
node · earth · Galactic
The exposed, cooling core left when a star of up to roughly eight solar masses has shed its envelope. It is typically comparable in mass to the Sun and comparable in size to the Earth, held up not by heat but by electron degeneracy pressure, and it therefore cannot contract as it cools. A white dwarf produces no new energy: it radiates away its residual heat over timescales far longer than the present age of the universe. Its mass is bounded above by the Chandrasekhar limit near 1.4 solar masses. A directly measured initial-to-final mass relation spans progenitors from 0.85 to 7.5 solar masses and is markedly non-linear, so the mapping from birth mass to remnant mass is an empirical result rather than a simple proportionality. Not a place on Earth.
Read in · 1
Evidence · 2
Timeline
No dated observations are stored for this object. Atlas shows what was observed and when — it does not infer a history.
Connections · 3
- Chandrasekhar limitconstrained_by
- Degeneracy pressuredepends_on
- Red giant and asymptotic giant branchderived_from
Assembled narrative · 1
Assembled from 31 blocks · 2 evidence · 27 related
- Story
- The exposed, cooling core left when a star of up to roughly eight solar masses has shed its envelope. It is typically comparable in mass to the Sun and comparable in size to the Earth, held up not by heat but by electron degeneracy pressure, and it therefore cannot contract as it cools. A white dwarf produces no new energy: it radiates away its residual heat over timescales far longer than the present age of the universe. Its mass is bounded above by the Chandrasekhar limit near 1.4 solar masses. A directly measured initial-to-final mass relation spans progenitors from 0.85 to 7.5 solar masses and is markedly non-linear, so the mapping from birth mass to remnant mass is an empirical result rather than a simple proportionality. Not a place on Earth.
- Knowledge
- Degeneracy pressure
- Chandrasekhar limit
- Red giant and asymptotic giant branch
- White dwarf
- Connections
- Chandrasekhar limit
- Degeneracy pressure
- Red giant and asymptotic giant branch
- Sirius B
- Alvan Graham Clark sees Sirius B
- A maximum mass for ideal white dwarfs is published
- Subrahmanyan Chandrasekhar
- Degeneracy pressure
- White dwarf
- A maximum mass for ideal white dwarfs is published
- Chandrasekhar limit
- White dwarf
- Neutron star
- A maximum mass for ideal white dwarfs is published
- A radius is measured for the heaviest known neutron star
- Main sequence (core hydrogen burning)
- Betelgeuse (Alpha Orionis)
- Planetary nebula
- White dwarf
- Betelgeuse fades by more than a magnitude
- Evidence
- Measures the mapping from progenitor mass to white dwarf mass across the stated range and shows it to be markedly non-linear. Journal, volume, article number and arXiv identifier come from ADS and preprint listings via search; the paper was not fetched, and the slope values are not reproduced here.
- Derives an upper mass bound for a body supported by relativistic electron degeneracy. Journal, volume and pages come from an ADS scan listing seen via search; the paper was not fetched, and the statement that its own derived value was about 0.91 solar masses rests on a secondary summary.
Observed changes · 0
No public Signals are attached to this object. Signals show what changed and when it was observed — never a direction or a rank.
Actions
/atlas?object=OBJECT_WHITE_DWARF&experience=OBJECT_WHITE_DWARF