A University of Utah-led team discovered a \"hypervelocity star\" that is the closest, second-brightest and among the largest of 20 found so far. Speeding at more than 1 million mph, the star may provide clues about the supermassive black hole at the center of our Milky Way and the halo of mysterious \"dark matter\" surrounding the galaxy, astronomers say. <\/p>\n
\"The hypervelocity star tells us a lot about our galaxy - especially its center and the dark matter halo,\" says Zheng Zheng, an assistant professor of physics and astronomy and lead author of the study published recently in Astrophysical Journal Letters by a team of U.S. and Chinese astronomers. <\/p>\n
\"We can't see the dark matter halo, but its gravity acts on the star,\" Zheng says. \"We gain insight from the star's trajectory and velocity, which are affected by gravity from different parts of our galaxy.\" <\/p>\n
In the past decade, astronomers have found about 20 of these odd stars. Hypervelocity stars appear to be remaining pairs of binary stars that once orbited each other and got too close to the supermassive black hole at the galaxy's center. Intense gravity from the black hole - which has the mass of 4 million stars like our sun - captures one star so it orbits the hole closely, and slingshots the other on a trajectory headed beyond the galaxy. <\/p>\n
Zheng and his colleagues discovered the new hypervelocity star while conducting other research into stars with the Large Sky Area Multi-Object Fiber Spectroscopic Telescope, or LAMOST, located at the Xinglong Observing Station of the National Astronomical Observatories of China, about 110 miles northeast of Beijing. LAMOST boasts a 13.1-foot-wide aperture and houses 4,000 optical fibers, which capture \"spectra\" or light-wavelength readings from as many as 4,000 stars at once. A star's spectrum reveals information about its velocity, temperature, luminosity and size. <\/p>\n
LAMOST's main purpose is to study the distribution of stars in the Milky Way, and thus the galaxy's structure. The new hypervelocity star - named LAMOST-HVS1 - stood out because its speed is almost three times the usual star's 500,000-mph pace through space: 1.4 million mph relative to our solar system. Its speed is about 1.1 million mph relative to the speed of the center of the Milky Way. <\/p>\n
Despite being the closest hypervelocity star, it nonetheless is 249 quadrillion miles from Earth. (In U.S. usage, a quadrillion is 1,000,000,000,000,000 miles or 10 to the 15th power, or 1 million billion). <\/p>\n
\"If you're looking at a herd of cows, and one starts going 60 mph, that's telling you something important,\" says Ben Bromley, a University of Utah physics and astronomy professor who was not involved with Zheng's study. \"You may not know at first what that is. But for hypervelocity stars, one of their mysteries is where they come from - and the massive black hole in our galaxy is implicated.\" <\/p>\n
The Down-Low on a Fast and Loose Star A cluster of known hypervelocity stars, including the new one, is located above the disk of our Milky Way galaxy, and their distribution in the sky suggests they originated near the galaxy's center, Zheng says. <\/p>\n
The diameter of the visible part of our spiral-shaped galaxy is at least 100,000 light years, or 588 quadrillion miles. Zheng says that when the halo of dark matter is added, the estimated diameter is roughly 1 million light years, or 5,880 quadrillion miles. <\/p>\n
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Nearest bright 'hypervelocity star' found<\/a><\/p>\n","protected":false},"excerpt":{"rendered":" A University of Utah-led team discovered a \"hypervelocity star\" that is the closest, second-brightest and among the largest of 20 found so far. Speeding at more than 1 million mph, the star may provide clues about the supermassive black hole at the center of our Milky Way and the halo of mysterious \"dark matter\" surrounding the galaxy, astronomers say. \"The hypervelocity star tells us a lot about our galaxy - especially its center and the dark matter halo,\" says Zheng Zheng, an assistant professor of physics and astronomy and lead author of the study published recently in Astrophysical Journal Letters by a team of U.S Continue reading