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The light that the NASA\/ESA Hubble Space Telescope collected to create this\u00a0Picture of the Week\u00a0reached the telescope after a journey of 250 million years. Its source was the\u00a0spiral galaxy\u00a0UGC 11397, which resides in the constellation\u00a0Lyra\u00a0(The Lyre). At first glance, UGC 11397 appears to be an average spiral galaxy: it sports two graceful spiral arms that are illuminated by stars and defined by dark, clumpy clouds of dust.<\/p>\n
What sets UGC 11397 apart from a typical spiral lies at its centre, where a supermassive\u00a0black hole\u00a0containing 174 million times the mass of the Sun is growing. As a black hole ensnares gas, dust, and even entire stars from its vicinity, this doomed matter heats up and puts on a fantastic cosmic light show. Material trapped by the black hole emits light from\u00a0gamma rays to radio waves\u00a0and can brighten and fade without warning. But in some galaxies, including UGC 11397, thick clouds of dust hide much of this energetic activity from view in optical light.\u00a0 Despite this, UGC 11397’s actively growing black hole was revealed through its bright X-ray emission \u2014 high-energy light that can pierce the surrounding dust. This led astronomers to classify it as a Type 2 Seyfert galaxy, a category used for\u00a0active galaxies\u00a0whose central regions are hidden from view in visible light by a doughnut-shaped cloud of dust and gas.<\/p>\n
Using Hubble, researchers will study hundreds of galaxies that, like UGC 11397, harbour a supermassive black hole that is gaining mass. The Hubble observations will help researchers weigh nearby supermassive black holes, understand how black holes grew early in the Universe\u2019s history, and even study how stars form in the extreme environment found at the very centre of a galaxy.<\/p>\n
[Image Description:<\/i>\u00a0A spiral galaxy, seen at an angle that gives it an oval shape. It has two spiral arms that curl out from the centre. They start narrow but broaden out as they wrap around the galaxy before merging into a faint halo. The galaxy\u2019s disc is golden in the centre with a bright core, and pale blue outside that. A swirl of dark dust strands and speckled blue star-forming regions follow the arms through the disc.]<\/p>\n<\/p><\/div>\n<\/p><\/div>\n