Hubble Views the Core of Spiral Galaxy Messier 61

New Hubble Image of Spiral Galaxy Messier 61

Messier 61, or NGC 4303, spans about 100,000 light-years, similar to our Milky Way. Both are part of the Virgo Supercluster in the constellation Virgo, a collection of up to 2000 galaxies. Credit: ESA/Hubble & NASA, Acknowledgement: Det58

This newly released Hubble image shows spiral galaxy Messier 61, also known as NGC 4303.

This new Hubble picture is the sharpest ever image of the core of the 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 Milky Way galaxy. 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 Catalog, 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.

A version of this image was submitted to the Hubble’s Hidden Treasures image processing competition by Flickr user Det58.


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