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A
Hungry Starburst Galaxy
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Messier 61, NGC 4303 Spiral Galaxy RA 12hr 21m 54.95s Dec +04° 28' 24.92" Virgo 55 million light years 6.5×5.5 arc-min 9.7 ESA/Hubble & NASA April 28, 2014 Full Image: G1901 Closeup: G1417 |
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ABOUT THIS IMAGE: This new Hubble picture is the sharpest ever image of the core of spiral galaxy Messier 61. Taken using the High Resolution Channel of Hubble's Advanced Camera for Surveys, the central part of the galaxy is shown in striking detail. Also known as NGC 4303, this galaxy is roughly 100 000 light-years across, comparable in size to our galaxy, the Milky Way. Both Messier 61 and our home galaxy belong to a group of galaxies known as the Virgo Supercluster in the constellation of Virgo (The Virgin) - a group of galaxy clusters containing up to 2000 spiral and elliptical galaxies in total. Messier 61 is a type of galaxy known as a starburst galaxy. Starburst galaxies experience an incredibly high rate of star formation, hungrily using up their reservoir of gas in a very short period of time (in astronomical terms). But this is not the only activity going on within the galaxy; deep at its heart there is thought to be a supermassive black hole that is violently spewing out radiation. Despite
its inclusion in the Messier Catalogue, Messier 61 was actually discovered
by Italian astronomer Barnabus Oriani in 1779. Charles Messier also noticed
this galaxy on the very same day as Oriani, but mistook it for a passing
comet - the comet of 1779. |
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