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Brilliant spiral Galaxy hosts two supernovae in past 30 years [PHOTO]

Tibi PuiubyTibi Puiu
August 3, 2012
in Remote sensing, Space
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The European Southern Observatory’s (ESO) Very Large Telescope in Chile is back with yet another stunning gem. This spectacular spiral galaxy has hosted two supernova explosions over the last 30 years, making it particularly interesting. Supernovae are one of the brightest and most energetic events in the Universe.

Spiral Galaxy supernova

The galaxy’s name is NGC 1187, and is located 60 million light years away from Earth , in the constellation Eridanus. The first supernova found in NGC 1187, officially called SN 1982R, was detected in October 1982 at ESO’s La Silla Observatory in Chile’s Atacama Desert. The second one, called SN 2007Y, was spotted by amateur astronomer Berto Monard in South Africa in 2007.

When a star reaches the end of its life, it dies off in a spectacular fashion, exploding with a high energy release. So you can imagine the magnitude of its energy release, consider that the radiated energy during a supernova explosion is comparable to the amount of energy the sun will emit over the entire course of its life. Also, it’s no rare event for a supernova to outshine whole galaxies before fading away during the course of a few years.

The first supernova from NGC 1187 is no longer visible in this image, however the second from 2007 is still visible near the bottom of the image, albeit fainter since it’s well past its climax point. Nevertheless, the spiral galaxy is stunning itself, with or without supernovae.

source MNN. Image credit: ESO.

Tags: spiral galaxysupernovavery large telescope

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Tibi Puiu

Tibi Puiu

Tibi is a science journalist and co-founder of ZME Science. He writes mainly about emerging tech, physics, climate, and space. In his spare time, Tibi likes to make weird music on his computer and groom felines. He has a B.Sc in mechanical engineering and an M.Sc in renewable energy systems.

Related Posts

This Picture of the Week shows a stunning spiral galaxy known as NGC 4945. This little corner of space, near the constellation of Centaurus and over 12 million light-years away, may seem peaceful at first — but NGC 4945 is locked in a violent struggle. At the very centre of nearly every galaxy is a supermassive black hole. Some, like the one at the centre of our own Milky Way, aren’t particularly hungry. But NGC 4945’s supermassive black hole is ravenous, consuming huge amounts of matter — and the MUSE instrument at ESO’s Very Large Telescope (VLT) has caught it playing with its food. This messy eater, contrary to a black hole’s typical all-consuming reputation, is blowing out powerful winds of material. This cone-shaped wind is shown in red in the inset, overlaid on a wider image captured with the MPG/ESO telescope at La Silla. In fact, this wind is moving so fast that it will end up escaping the galaxy altogether, lost to the void of intergalactic space. This is part of a new study that measured how winds move in several nearby galaxies. The MUSE observations show that these incredibly fast winds demonstrate a strange behaviour: they actually speed up far away from the central black hole, accelerating even more on their journey to the galactic outskirts. This process ejects potential star-forming material from a galaxy, suggesting that black holes control the fates of their host galaxies by dampening the stellar birth rate. It also shows that the more powerful black holes impede their own growth by removing the gas and dust they feed on, driving the whole system closer towards a sort of galactic equilibrium. Now, with these new results, we are one step closer to understanding the acceleration mechanism of the winds responsible for shaping the evolution of galaxies, and the history of the universe. Links  Research paper in Nature Astronomy by Marconcini et al. Close-up view of NGC 4945’s nucleus
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