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A black dwarf is a theoretical stellar remnant, specifically a white dwarf that has cooled sufficiently to no longer emit significant heat or light. Because the time required for a white dwarf to reach this state is calculated to significantly exceed the current age of the universe (13.79 billion years), no black dwarfs are expected to exist in the…
Formation, Composition & The Sun as a black dwarf
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black dwarf dwarfs white would years temperature mass exist also limit hypothetical sun approximately cooled proton decay take massive longer
| Subject | Predicate | Object | Confidence | Src |
|---|---|---|---|---|
| Black dwarf | Average luminosity | negligible (visual) ≤ 23 kW/m2 (total) | 1.00 | infobox |
| Black dwarf | Mass range | Up to Chandrasekhar limit (non-rotating) | 1.00 | infobox |
| Black dwarf | Temperature | Under 798 K (Draper point) | 1.00 | infobox |
| Black dwarf | Type | Hypothetical class of future stellar remnant | 1.00 | infobox |
| Black dwarf | is a | theoretical stellar remnant | 0.90 | text |
| Black dwarf | related to Formation | What | 0.60 | section |
| Black dwarf | related to Formation | If | 0.60 | section |
| Black dwarf | related to Formation | They | 0.60 | section |
| Black dwarf | related to Formation | Various | 0.60 | section |
| Black dwarf | related to Formation | M0 | 0.60 | section |
| Black dwarf | related to Formation | MDM Observatory's | 0.60 | section |
| Black dwarf | related to The Sun as a black dwarf | Once | 0.60 | section |
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