It looks like you're using an Ad Blocker.
Please white-list or disable AboveTopSecret.com in your ad-blocking tool.
Thank you.
Some features of ATS will be disabled while you continue to use an ad-blocker.
A supermassive black hole — with the mass 21 billion times that of our own sun — has been found at the heart of a distant galaxy.
NGC 4889 is an elliptical galaxy. Rather than being the galaxy most people think of, elliptical galaxies look like they have no real structure, with their collection of stars looking more like blobs in space.
The galaxy is about 300 million light years away, in the heart of a galaxy cluster known as the Coma Cluster. The black hole has an event horizon — a location where not even light can escape — with diameter of 130 billion km. That’s approximately the distance between the sun and Neptune, the last planet in our solar system. Comparatively, the black hole at the heart of our galaxy has an event horizon about one-fifth the orbit of Mercury, the closest planet to the sun and a mass of about four million times that of the sun.
Astronomers believe that the black hole is no longer gobbling up matter. In fact, they believe that stars have begun to form in the surrounding region.
Hidden from human eyes is a supermassive black hole within this elliptical galaxy, NGC 4889.
The placid appearance of NGC 4889 can fool the unsuspecting observer. But the elliptical galaxy, pictured in this new image from the NASA/ESA Hubble Space Telescope, harbours a dark secret. At its heart lurks one of the most massive black holes ever discovered.
Located about 300 million light-years away in the Coma Cluster, the giant elliptical galaxy NGC 4889, the brightest and largest galaxy in this image, is home to a record-breaking supermassive black hole. Twenty-one billion times the mass of the Sun, this black hole has an event horizon - the surface at which even light cannot escape its gravitational grasp - with a diameter of approximately 130 billion kilometres. This is about 15 times the diameter of Neptune's orbit from the Sun. By comparison, the supermassive black hole at the centre of our galaxy, the Milky Way, is believed to have a mass about four million times that of the Sun and an event horizon just one fifth the orbit of Mercury.
But the time when NGC 4889's black hole was swallowing stars and devouring dust is past. Astronomers believe that the gigantic black hole has stopped feeding, and is currently resting after feasting on NGC 4889's cosmic cuisine. The environment within the galaxy is now so peaceful that stars are forming from its remaining gas and orbiting undisturbed around the black hole.
When it was active, NGC 4889's supermassive black hole was fuelled by the process of hot accretion. When galactic material—such as gas, dust and other debris—slowly fell inwards towards the black hole, it accumulated and formed an accretion disc. Orbiting the black hole, this spinning disc of material was accelerated by the black hole's immense gravitational pull and heated to millions of degrees. This heated material also expelled gigantic and very energetic jets. During its active period, astronomers would have classified NGC 4889 as a quasarand the disc around the supermassive black hole would have emitted up to a thousand times the energy output of the Milky Way.
The accretion disc sustained the supermassive black hole's appetite until the nearby supply of galactic material was exhausted. Now, napping quietly as it waits for its next celestial snack, the supermassive black hole is dormant. However its existence allows astronomers to further their knowledge of how and where quasars, these still mysterious and elusive objects, formed in the early days of the Universe.
Although it is impossible to directly observe a black hole—as light cannot escape its gravitational pull—its mass can be indirectly determined. Using instruments on the Keck II Observatory and Gemini North Telescope, astronomers measured the velocity of the stars moving around NGC 4889's centre. These velocities—which depend on the mass of the object they orbit—revealed the immense mass of the supermassive black hole.
Is this something newly discovered about BH's not pulling in matter? You would think of that size there would be a mass gravitational pull inwards, but as reported it is not doing this. I wonder why?
originally posted by: boncho
a reply to: Skywatcher2011
Is this something newly discovered about BH's not pulling in matter? You would think of that size there would be a mass gravitational pull inwards, but as reported it is not doing this. I wonder why?
It's not new at all. There are black holes or super massive black holes at the centre of every galaxy. Eventually they find equilibrium with everything around them.
originally posted by: Thecakeisalie
a reply to: Skywatcher2011
Awesome alright.
Elliptical galaxies are about to get a lot more popular methinks after the discovery of gravy waves (you heard it hear first ATS) as Elliptical galaxies are older and so are their stars. If I may put on my tinfoil hat for a second the size of a black hole could determine the shape of a galaxy.