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Statements (19)
| Predicate | Object |
|---|---|
| gptkbp:instanceOf |
astrophysical concept
|
| gptkbp:appliesTo |
gptkb:white_dwarf_stars
|
| gptkbp:describes |
maximum mass of a stable white dwarf star
|
| gptkbp:discoveredBy |
gptkb:Subrahmanyan_Chandrasekhar
|
| gptkbp:exceededBy |
leads to supernova or neutron star formation
|
| gptkbp:field |
astrophysics
|
| gptkbp:hasUnit |
solar mass
|
| https://www.w3.org/2000/01/rdf-schema#label |
Chandrasekhar limit
|
| gptkbp:namedAfter |
gptkb:Subrahmanyan_Chandrasekhar
|
| gptkbp:relatedTo |
stellar evolution
white dwarf supernova degeneracy pressure electron degeneracy |
| gptkbp:significance |
determines fate of stars after nuclear fuel exhaustion
|
| gptkbp:valuation |
approximately 1.4 solar masses
|
| gptkbp:yearProposed |
1930
|
| gptkbp:bfsParent |
gptkb:Tolman–Oppenheimer–Volkoff_limit
|
| gptkbp:bfsLayer |
4
|