Speeding at 1 million mph, it probes black hole and dark matter
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.
This is an astrophysicist-artist's conception of a hypervelocity star speeding away from the visible part of a spiral galaxy like our Milky Way and into the invisible halo of mysterious "dark matter" that surrounds the galaxy's visible portions. University of Utah researcher Zheng Zheng and colleagues in the US and China discovered the closest bright hypervelocity star yet found.
Credit: Ben Bromley, University of Utah.
"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.
"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."
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.
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.
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.
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).
"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."
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.
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.
Scientists know dark matter halos surround galaxies because the way their gravity affects the motion of a galaxy's visible stars and gas clouds. Researchers say only about 5 percent of the universe is made of visible matter, 27 percent is invisible and yet-unidentified dark matter and 68 percent is even more mysterious dark energy, responsible for accelerating the expansion of the universe. By traveling through the dark matter halo, the new hypervelocity star's speed and trajectory can reveal something about the mysterious halo.
Our solar system is roughly 26,000 light years or 153 quadrillion miles from the center of the galaxy – more than halfway out from the center of the visible disk.
By comparison, the new hypervelocity star is about 62,000 light years or 364 quadrillion miles from the galactic center, beyond as well as above the galaxy's visible disk. It is about 42,400 light years from Earth, or about 249 quadrillion miles away.
As far as that is – the star has a magnitude of about 13, or 630 times fainter than stars that barely can be seen with the naked eye – it nevertheless "is the nearest, second-brightest, and one of the three most massive hypervelocity stars discovered so far," Zheng says.
It is nine times more massive than our sun, which makes it very similar to another hypervelocity star known as HE 0437-5439, discovered in 2005, and both are smaller than HD 271791, which was discovered in 2008 and is 11 times more massive than the sun. As seen from Earth, only HD 271791 is brighter than LAMOST-HVS1, Zheng says.
The newly discovered hypervelocity star also outshines our own sun: It is four times hotter and about 3,400 times brighter (if viewed from the same distance). But compared with our 4.6-billion-year-old sun, the newly discovered LAMOST–HVS1 is a youngster born only 32 million years ago, based on its speed and position, Zheng says.
Is there any chance that the supermassive black hole might hurl a hypervelocity star in Earth's direction one day? Not really, Zheng says. First, astrophysicists estimate only one hypervelocity star is launched every 100,000 years. Second, possible trajectories of stars near the supermassive black hole don't forebode any danger, should any of them become a hypervelocity star in the future.
Collaborating Institutions and Funding
Zheng conducted the study with researchers from Rensselaer Polytechnic Institute, Troy, N.Y.; National Optical Astronomy Observatory, Tucson, Ariz.; National Astronomical Observatories, Chinese Academy of Sciences, Beijing and Nanjing; Spitzer Science Center, Pasadena, Calif.; University of California Observatories-Lick Observatory, University of California, Santa Cruz; Georgia State University, Atlanta; Fermi National Accelerator Laboratory, Batavia, Ill.; and University of Science and Technology of China, Hefei.
The study was funded by the U.S. National Science Foundation and the National Development and Reform Commission of China.
University of Utah Communications
75 Fort Douglas Boulevard, Salt Lake City, UT 84113
801-581-6773 fax: 801-585-3350
Lee J. Siegel | Eurek Alert!
Tiny Drops of Early Universe 'Perfect' Fluid
02.09.2015 | Brookhaven National Laboratory
02.09.2015 | European Southern Observatory ESO
China's Loess Plateau was formed by wind alternately depositing dust or removing dust over the last 2.6 million years, according to a new report from University of Arizona geoscientists. The study is the first to explain how the steep-fronted plateau formed.
China's Loess Plateau was formed by wind alternately depositing dust or removing dust over the last 2.6 million years, according to a new report from...
The leaves of the lotus flower, and other natural surfaces that repel water and dirt, have been the model for many types of engineered liquid-repelling surfaces. As slippery as these surfaces are, however, tiny water droplets still stick to them. Now, Penn State researchers have developed nano/micro-textured, highly slippery surfaces able to outperform these naturally inspired coatings, particularly when the water is a vapor or tiny droplets.
Enhancing the mobility of liquid droplets on rough surfaces could improve condensation heat transfer for power-plant heat exchangers, create more efficient...
Longer, more severe, and hotter droughts and a myriad of other threats, including diseases and more extensive and severe wildfires, are threatening to transform some of the world's temperate forests, a new study published in Science has found. Without informed management, some forests could convert to shrublands or grasslands within the coming decades.
"While we have been trying to manage for resilience of 20th century conditions, we realize now that we must prepare for transformations and attempt to ease...
A University of Oklahoma astrophysicist and his Chinese collaborator have found two supermassive black holes in Markarian 231, the nearest quasar to Earth, using observations from NASA's Hubble Space Telescope.
The discovery of two supermassive black holes--one larger one and a second, smaller one--are evidence of a binary black hole and suggests that supermassive...
A team of European researchers have developed a model to simulate the impact of tsunamis generated by earthquakes and applied it to the Eastern Mediterranean. The results show how tsunami waves could hit and inundate coastal areas in southern Italy and Greece. The study is published today (27 August) in Ocean Science, an open access journal of the European Geosciences Union (EGU).
Though not as frequent as in the Pacific and Indian oceans, tsunamis also occur in the Mediterranean, mainly due to earthquakes generated when the African...
20.08.2015 | Event News
20.08.2015 | Event News
19.08.2015 | Event News
02.09.2015 | Physics and Astronomy
02.09.2015 | Life Sciences
02.09.2015 | Awards Funding