As a result, this celestial body becomes absolutely black and human cannot observe it directly (Montgomery, C., Orchiston, W., & Whittingham, 90). In 1915, Einstein Albert, a great physicist, published the Einstein field equations which describes the fundamental interaction of gravitation as a result of spacetime being curved by matter and energy (Einstein Albert, 884). One month later, Karl Schwarzschild, a German physicist, got the accurate solution of Einstein field equations and deduced that if the mass of an object is compressed within small diameter, all matter and energy will be trapped (Yi, 205).
In 1934, Wilhelm Heinrich Walter Baade, a German astronomer, mentioned that when a senescent star with huge mass cannot get enough from nuclear fusion, it is likely to become a black hole due to sufficient gravitation (Yi, 209).
In 1993, Julius Robert Oppenheimer, an American theoretical physicist worked out that if a star that its mass three times the sun without any nuclear fusion, it must be compressed by its gravitation and become a black hole (Yi, …show more content…
During the life cycle of a star, it keeps nuclear fusion all the time to maintain its energy to resist the self-inflicted gravitation. The nuclear fusion starts with hydrogen and then produce other heavy element which makes the mass of star increase. When the mass become larger, the star gain more energy to push up its nuclear fusion to high levels. The heavier the star is, the less life cycle it has. At the end of its life cycle, due to the lack of energy, it cannot create nuclear fusion. Consequently, it will be compressed by self-inflicted gravitation. If the sun start to be compressed, it will become with dwarf, a stellar remnant composed mostly of electron-degenerate matter. However, if the mass of that star is three times the mass of the sun, that star will become black hole (Rincon,