A galaxy with two hearts

Jan 09, 2014
This new Hubble image shows the scatterings of bright stars and thick dust that make up spiral galaxy Messier 83, 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. Credit: NASA, ESA, and the Hubble Heritage Team (STScI/AURA) Acknowledgement: William Blair (Johns Hopkins University)

This new Hubble image shows the spiral galaxy Messier 83, 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 is thought to have a double nucleus lurking at its core.

Messier 83 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 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 centre, 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 centre. This gas is then used to form new stars and also to feed the galaxy's central black hole, explaining why many barred spirals—including Messier 83—have very active and luminous central regions.

However, Messier 83's centre is mysterious and unusual; the 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 Messier 83 contains two central , 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 [1].

As well as this double nucleus, Messier 83 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: Messier 61 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 Messier 83, 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 Messier 83, some of which are very young at under 5 million years old.

This mosaic image uses observations taken by Hubble's Wide Field Camera 3. It shows the galaxy in full, with dark dust lanes, fiery red patches of gas, and bright blue patches of recent star formation speckled across the spiralling arms. Although it looks sprawling, Messier 83 is just under half of the size of the Milky Way.

This new image is being released today, 9 January 2014, at the 223rd meeting of the American Astronomical Society in Washington, DC, USA.

Explore further: We're not alone—but the universe may be less crowded than we think

More information: [1] This central region is a very bizarre place. Neither of the two components making up the double nucleus are actually aligned with the galaxies kinematic centre—the region inferred to be the central part of Messier 83 from the motions of the stars within the galaxy. The "second nucleus" is not seen directly, but is detected by studying how mass within the galaxy is distributed.

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not rated yet Jan 09, 2014
The 'bars' are illusory. The stellar/gas denstity distributions throughout the galaxy are driven by gravity, angular momentum, and radiation pressure. Gravity insures Keplerian orbits of the stars and gas clouds around the galactic center, conservation of angular momenum in stellar interactions imposes the rotating disk structure, and radiation pressure compresses the gases to the point that stellar ignition can occur. The 'bars' occur because of the angular velocities varies with the distance from the center with an 'inflection point' where the propagation of pressure waves matches the orbital velocity.
5 / 5 (2) Jan 09, 2014
M 83 is not only unusual for its double nucleus and large number of observed supernovae, but the galaxy also displays an extended region of neutral hydrogen(HI) and stellar emission far beyond the optical disk:



M 83 is among a small number of galaxies that are known to exhibit star formation as well as abundant HI reservoirs well beyond the optical disk of the galaxy. Extended disks in isolated, undisturbed galaxies like M 83 may be common in the universe.

In addition to the extended disk, a stellar tidal stream from a disrupted dwarf galaxy has been observed associated with M 83: http://arxiv.org/.../0308142
1 / 5 (2) Jan 10, 2014
The stellar/gas denstity distributions throughout the galaxy are driven by gravity, angular momentum, and radiation pressure.

That's the hypothesis, but of course for it to work correctly you need to invent 5 times more matter than what is observed.To be sure, these are plasma processes that drive galaxies not this comparatively weak gravitational force.


Note that the PC version even explain the "double heart" observed above, oh and the presence of the HI clouds. The accuracy of the plasma model is unavoidable, well except those who can't see the obvious.
Captain Stumpy
5 / 5 (1) Jan 29, 2014
To be sure, these are plasma processes that drive galaxies not this comparatively weak gravitational force

this is speculation based upon the publications of pseudo-science crackpot sites and they contain no validity within the scope of modern cosmological physics as there is no proof other than the claims made by the author.

if there is a legitimate claim to your supposition, i would recommend posting valid reputable links to legitimate scientific studies from physicists and cosmologists and not engineers, as your EU site does not take into consideration much of the information required for a honest assessment of astrophysics based upon the claims of other prominent astrophysicists in the field


the standard model is more effective at representing the stellar/gas density distributions than your CRACKPOT EU site
5 / 5 (1) Feb 04, 2014
The 'bars' are illusory.

That's true of the arms but I thought it was suspected that the stars in the bar remained in it as a permanent feature.

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