 
                        
                            
                                AI-created image
                            
                        
                    Statements (22)
| Predicate | Object | 
|---|---|
| gptkbp:instanceOf | gptkb:astrophysical_concept | 
| gptkbp:alsoKnownAs | gptkb:Eddington_luminosity | 
| gptkbp:appliesTo | stars accreting black holes accreting neutron stars | 
| gptkbp:c | speed of light | 
| gptkbp:describes | maximum luminosity a star can achieve | 
| gptkbp:determines | balance between radiation pressure and gravitational force | 
| gptkbp:field | astrophysics | 
| gptkbp:firstDescribed | 1926 | 
| gptkbp:form | L_Edd = (4πGMc)/κ | 
| gptkbp:G | gravitational constant | 
| gptkbp:hasUnit | watts | 
| gptkbp:namedAfter | gptkb:Arthur_Eddington | 
| gptkbp:relatedTo | affects growth of supermassive black holes influences stellar evolution limits accretion rates | 
| gptkbp:κ | opacity of the material | 
| gptkbp:מטה | mass of the object | 
| gptkbp:bfsParent | gptkb:Arthur_Eddington | 
| gptkbp:bfsLayer | 4 | 
| https://www.w3.org/2000/01/rdf-schema#label | Eddington limit |