This image shows the elliptical galaxy NGC 4889 in front of hundreds of background galaxies, and deeply embedded within the Coma galaxy cluster. Well-hidden from human eyes, there is a gigantic supermassive black hole at the center of the galaxy. Credit: NASA & ESA
The placid appearance of NGC 4889 can fool the unsuspecting observer. But the elliptical galaxy harbours one of the most supermassive black holes ever discovered. Located ~300 million light-years away in the Coma Cluster, the giant elliptical galaxy NGC 4889, the brightest and largest galaxy in this image has a black hole that is 21 billion times the mass of the Sun. The event horizon has a diameter of ~130 billion kilometres. This is about 15X 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 4 million times that of the Sun and an event horizon just 1/5 the orbit of Mercury.
But the gigantic black hole has stopped feeding on stars and dust, and is 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 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 quasar and 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 find out how and where quasars 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. https://www.spacetelescope.org/news/heic1602/
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