<Table> <Tr> <Td> Part of a series of articles about </Td> </Tr> <Tr> <Th> General relativity </Th> </Tr> <Tr> <Td> G μ ν + Λ g μ ν = 8 π G c 4 T μ ν (\ displaystyle G_ (\ mu \ nu) + \ Lambda g_ (\ mu \ nu) = (8 \ pi G \ over c ^ (4)) T_ (\ mu \ nu)) </Td> </Tr> <Tr> <Td> <Ul> <Li> <Ul> <Li> Introduction </Li> <Li> History </Li> </Ul> </Li> <Li> Mathematical formulation </Li> <Li> <Ul> <Li> Tests </Li> </Ul> </Li> </Ul> </Td> </Tr> <Tr> <Td> Fundamental concepts (show) <Ul> <Li> Principle of relativity </Li> <Li> Theory of relativity </Li> <Li> Frame of reference </Li> <Li> Inertial frame of reference </Li> <Li> Rest frame </Li> <Li> Center - of - momentum frame </Li> <Li> Equivalence principle </Li> <Li> Mass--energy equivalence </Li> <Li> Special relativity </Li> <Li> Doubly special relativity </Li> <Li> de Sitter invariant special relativity </Li> <Li> World line </Li> <Li> Riemannian geometry </Li> </Ul> </Td> </Tr> <Tr> <Td> Phenomena (hide) <Table> <Tr> <Td> <Ul> <Li> Gravitoelectromagnetism </Li> <Li> Kepler problem </Li> <Li> Gravity </Li> <Li> Gravitational field </Li> <Li> Gravity well </Li> <Li> Gravitational lensing </Li> <Li> Gravitational waves </Li> <Li> Gravitational redshift </Li> <Li> Redshift </Li> <Li> Blueshift </Li> <Li> Time dilation </Li> <Li> Gravitational time dilation </Li> <Li> Shapiro time delay </Li> <Li> Gravitational potential </Li> <Li> Gravitational compression </Li> <Li> Gravitational collapse </Li> <Li> Frame - dragging </Li> <Li> Geodetic effect </Li> <Li> Gravitational singularity </Li> <Li> Event horizon </Li> <Li> Naked singularity </Li> <Li> Black hole </Li> <Li> White hole </Li> </Ul> </Td> </Tr> <Tr> <Th> Spacetime </Th> </Tr> <Tr> <Td> <Ul> <Li> Space </Li> <Li> Time </Li> <Li> Spacetime diagrams </Li> <Li> Minkowski spacetime </Li> <Li> Closed timelike curve (CTC) </Li> <Li> Wormhole <Ul> <Li> Ellis wormhole </Li> </Ul> </Li> </Ul> </Td> </Tr> </Table> </Td> </Tr> <Tr> <Td> <Ul> <Li> Equations </Li> <Li> Formalisms </Li> </Ul> (show) <Table> <Tr> <Th> Equations </Th> </Tr> <Tr> <Td> <Ul> <Li> Linearized gravity </Li> <Li> Einstein field equations </Li> <Li> Friedmann </Li> <Li> Geodesics </Li> <Li> Mathisson--Papapetrou--Dixon </Li> <Li> Hamilton--Jacobi--Einstein </Li> <Li> Curvature invariant (general relativity) </Li> <Li> Lorentzian manifold </Li> </Ul> </Td> </Tr> <Tr> <Th> Formalisms </Th> </Tr> <Tr> <Td> <Ul> <Li> ADM </Li> <Li> BSSN </Li> <Li> Post-Newtonian </Li> </Ul> </Td> </Tr> <Tr> <Th> Advanced theory </Th> </Tr> <Tr> <Td> <Ul> <Li> Kaluza--Klein theory </Li> <Li> Quantum gravity </Li> <Li> Supergravity </Li> </Ul> </Td> </Tr> </Table> </Td> </Tr> <Tr> <Td> Solutions (show) <Ul> <Li> Schwarzschild (interior) </Li> <Li> Reissner--Nordström </Li> <Li> Gödel </Li> <Li> Kerr </Li> <Li> Kerr--Newman </Li> <Li> Kasner </Li> <Li> Lemaître--Tolman </Li> <Li> Taub - NUT </Li> <Li> Milne </Li> <Li> Robertson--Walker </Li> <Li> pp - wave </Li> <Li> van Stockum dust </Li> <Li> Weyl − Lewis − Papapetrou </Li> <Li> Vacuum solution (general relativity) </Li> <Li> Vacuum solution </Li> </Ul> </Td> </Tr> <Tr> <Td> Scientists (show) <Ul> <Li> Einstein </Li> <Li> Lorentz </Li> <Li> Hilbert </Li> <Li> Poincaré </Li> <Li> Schwarzschild </Li> <Li> de Sitter </Li> <Li> Reissner </Li> <Li> Nordström </Li> <Li> Weyl </Li> <Li> Eddington </Li> <Li> Friedman </Li> <Li> Milne </Li> <Li> Zwicky </Li> <Li> Lemaître </Li> <Li> Gödel </Li> <Li> Wheeler </Li> <Li> Robertson </Li> <Li> Bardeen </Li> <Li> Walker </Li> <Li> Kerr </Li> <Li> Chandrasekhar </Li> <Li> Ehlers </Li> <Li> Penrose </Li> <Li> Hawking </Li> <Li> Raychaudhuri </Li> <Li> Taylor </Li> <Li> Hulse </Li> <Li> van Stockum </Li> <Li> Taub </Li> <Li> Newman </Li> <Li> Yau </Li> <Li> Thorne </Li> <Li> others </Li> </Ul> </Td> </Tr> <Tr> <Td> <Ul> <Li> </Li> <Li> </Li> <Li> </Li> </Ul> </Td> </Tr> </Table> <Tr> <Td> Part of a series of articles about </Td> </Tr> <Tr> <Th> General relativity </Th> </Tr>

Where is the event horizon of a black hole located