Schwarzschild, "Über das Gravitationsfeld einer Kugel aus inkompressibler Flussigkeit nach der Einsteinschen Theorie", Sitzungsberichte der Deutschen Akademie der Wissenschaften zu Berlin, Klasse fur Mathematik, Physik, und Technik (1916) pp 424. Schwarzschild, "Über das Gravitationsfeld eines Massenpunktes nach der Einsteinschen Theorie", Sitzungsberichte der Deutschen Akademie der Wissenschaften zu Berlin, Klasse fur Mathematik, Physik, und Technik (1916) pp 189. Modern General Relativity: Black Holes, Gravitational Waves, and Cosmology. Visible universe, if its density is the critical density, as a hypothetical black hole.Supermassive black hole, which could also either be a static black hole or a rotating black hole.Stellar black hole, which could either be a static black hole or a rotating black hole.Primordial black hole, a hypothetical leftover of the Big Bang.27 million light-years away in the constellation Canes Venatici, beneath. Micro black hole and extra-dimensional black hole Diameter of 4 million miles (6 million km), about four times the diameter of the Sun.The first supermassive black hole featured is that of the dwarf galaxy J1601+3113, with a mass about.
Chandrasekhar limit, a second requirement for black hole formation.This means the largest amount of water you can have without forming a black hole would have a radius of 400 920 754 km (about 2.67 AU). The Schwarzschild radius of a 1012 kg black hole is approximately 148 fm (1.48 × 1013 m), which is much smaller than an atom but larger than an atomic nucleus. R s = 2 G M c 2, įor example, the density of water is 1000 kg/m 3. For a stellar-mass black hole the radius of the event horizon increases by about 3 kilometers for every solar mass that is captured.
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