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NGC 6946

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NGC 6946 is a grand design, face-on intermediate spiral galaxy. It features a small, bright nucleus at its center. This galaxy sits in the sky between two northern constellations, Cepheus and Cygnus. It is located approximately 25.2 million light-years from Earth. This distance is about 7.72 megaparsecs. This distance is quite similar to the distance of the M101 galaxy. NGC 6946 is part of the Virgo Supercluster. It is one of many bright spiral galaxies near the Milky Way. However, it sits beyond the confines of our Local Group.

The structure of NGC 6946 is very specific. It is classified as a double-barred spiral galaxy. This means it has two bars of stars within its structure. The inner, smaller bar plays a very important role. It is believed to be responsible for funneling gas into the center of the galaxy. This movement of gas leads to prodigious star formation. Because it creates stars so rapidly, scientists call it an active starburst galaxy. This process of moving gas and creating stars defines its intense activity.

Observing NGC 6946 can be quite difficult for astronomers. The galaxy is heavily obscured by interstellar matter. This happens because the galaxy is located close to the galactic plane of the Milky Way. This matter acts like a veil of dust and gas. Within the spiral arms, there are also strange features. Some regions appear to be devoid of stars and gaseous hydrogen. These empty regions can span up to two kiloparsecs across. There are also two regions of unusual dark lanes of nebulosity visible in the arms.

Many unusual celestial objects exist within this galaxy. One such object is called the 'Red Ellipse.' It is located along one of the northern arms. It looks like a super-bubble or a very large supernova remnant. It may have been formed by an open cluster containing massive stars. Another object is known as 'Hodge's Complex.' This was discovered in 1967. For a long time, it was thought to be a young supergiant cluster. However, in 2017, scientists conjectured it might be an interacting dwarf galaxy. This smaller galaxy is actually superimposed on NGC 6946.

NGC 6946 is famously known as the 'Fireworks Galaxy.' This nickname comes from its high rate of supernovae. A supernova is the massive explosion of a star. Since 1917, astronomers have observed ten supernovae in this galaxy. This rate is about ten times higher than the rate in our Milky Way. This is surprising because the Milky Way has twice as many stars as NGC 6946. As of 2017, NGC 6946 held the record for the most supernovae seen. That record was eventually surpassed by the galaxy NGC 3690.

Several specific supernovae have provided deep insights. In 2004, the explosion SN 2004et was discovered by S. Moretti. This was a Type II-P supernova. This event was special because the progenitor star was identified. The progenitor was a red supergiant in an interacting binary system. It shared its orbit with a blue supergiant. This was only the seventh time such an event was directly identified with its host star. Another event, SN 2017eaw, was found in May 2017. It was also a Type II-P supernova. Its progenitor was a red supergiant with a mass of around 15.

In 2009, a single star provided a truly spectacular sight. This star was a yellow hypergiant. It flared up and became over one million times brighter than the Sun. After this flare, it faded very rapidly. Observations from the Hubble Space Telescope suggest the star did not survive. Scientists believe it formed a black hole, designated N6946-BH1. They can see infrared emission from this position. This light likely comes from debris falling onto the new black hole. This sequence of events shows the violent life cycles occurring within the galaxy.

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