Disk winds turn on when a black hole is gobbling material nearly as fast as it can. As light from the disk moves through the winds, some of it is absorbed by material in the wind. Hubble’s ultraviolet instruments detect the particle winds coming off accretion disks from stellar-mass black holes. Five billion years from now when the Sun runs out of the available nuclear fuel in its core, it will end its life as a white dwarf. Our sun, for example, is not massive enough to become a black hole. Only stars with very large masses can become black holes. Black holes created by supernovas can be about five to 50 times the mass of the Sun. If the core remaining after the supernova is very massive, gravity completely collapses the core into a black hole with infinite density. This collapse may also cause a supernova, or an exploding star, that blasts the outer parts of the star into space.
Stellar black holes form when the center of a very massive, dying star collapses in upon itself. Around a supermassive black hole in the center of a galaxy, the swirling disk is made not only of gas but also of stars. Around a stellar black hole, this matter is composed of gas. Matter swirling around a black hole heats up and emits radiation that can be detected. Material falling into a black hole forms a disk, similar to a whirlpool in a bathtub drain. Although we can’t see a black hole, the material around it is visible. Four Successful Women Behind the Hubble Space Telescope's AchievementsĪ black hole is a region of space packed with so much matter that its own gravity prevents anything from escaping - even a ray of light.Characterizing Planets Around Other Stars.Measuring the Universe's Expansion Rate.
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