Spiral Galaxy M83

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This new Hubble image shows the scatterings of bright stars and thick dust that make up spiral galaxy Messier 83 (M83), otherwise known as the Southern Pinwheel Galaxy. One of the largest and closest barred spirals to us, this galaxy is dramatic and mysterious; it has hosted a large number of supernova explosions, and appears to have a double nucleus lurking at its core. M83 is not one to blend into the background. Located some 15 million light-years away in the constellation of Hydra (The Sea Serpent), it is one of the most conspicuous galaxies of its type in our skies. It is a prominent member of a group of galaxies known as the Centaurus A/M83 Group, which also counts dusty Centaurus A and irregular NGC 5253 as members. Spiral galaxies come in a range of types depending on their appearance and structure - for example, how tightly wound their arms are, and the characteristics of the central bulge. Messier 83 has a "bar" of stars slicing through its center, leading to its classification as a barred spiral. The Milky Way also belongs to this category. These bars are thought to act a bit like a funnel, channelling gas inwards towards the galaxy's center. This gas is then used to form new stars and also to feed the galaxy's central black hole, explaining why many barred or intermediate spirals - including M83 - have very active and luminous central regions. However, M83's center is mysterious and unusual; the supermassive black hole at its heart is not alone. This striking spiral displays a phenomenon known as a double nucleus - a feature that has also been spotted in the Andromeda Galaxy, the nearest spiral galaxy to us. This does not mean that M83 contains two central black holes, but that its single supermassive black hole may be ringed by a lopsided disc of stars, which orbits around the black hole and creates the appearance of a dual core. As well as this double nucleus, M83 has hosted quite a few supernova explosions - six in total that we have observed (SN 1923A, SN 1945B, SN 1950B, SN 1957D, SN 1968L, and SN 1983N). This number is matched by only two other galaxies: M61 which also has six, and NGC 6946, which tops the list with nine. As well as these explosions, almost 300 supernova remnants - the older leftovers from exploded stars - have been found within M83, detected using the data that make up this image. These observations are being used to study the life cycle of stars. As well as these old remnants, some 3000 star clusters have been identified in M83, some of which are very young at under 5 million years old.
Image Credit: NASA, ESA, and the Hubble Heritage Team (STScI/AURA)
Acknowledgement: William Blair (Johns Hopkins University)
Image enhancement: Jean-Baptiste Faure