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A white dwarf is a very dense type of star: in an Earth-sized volume, it packs a mass that is comparable to the Sun. A white dwarf radiates light from residual heat and eventual crystallization, not from nuclear fusion. Stars like the Sun, whose mass is not high enough to collapse into a neutron star or black hole, are expected to become white dwarf…
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white dwarf dwarfs star mass stars type binary core carbon may temperature hydrogen known also helium surface material energy fusion
| Subject | Predicate | Object | Confidence | Src |
|---|---|---|---|---|
| White dwarf | Average luminosity | 0.01-0.0001 L☉ | 1.00 | infobox |
| White dwarf | Mass range | Up to 1.44 M☉ | 1.00 | infobox |
| White dwarf | Temperature | 4000–40000+ K | 1.00 | infobox |
| White dwarf | Type | Class of stellar remnant. | 1.00 | infobox |
| White dwarf | is a | very dense type of star | 0.90 | text |
| neutron stars | instance of | surpassed only by other compact stars | 0.80 | text |
| the hypothetical quark stars.At these densities the nuclei within the star are much closer than nuclei in ordinary matter | instance of | surpassed only by other compact stars | 0.80 | text |
| iron falling to its core where it accumulates | instance of | The matter processed in the failed detonation is re-accreted by the white dwarf with the heaviest elements | 0.80 | text |
| tidal interaction | instance of | phenomena in binary systems | 0.80 | text |
| star | instance of | phenomena in binary systems | 0.80 | text |
| White dwarf | related to Atmosphere and spectra | Although | 0.60 | section |
| White dwarf | related to Atmosphere and spectra | The | 0.60 | section |
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