Thursday, September 7, 2023

4144 - MILKY WAY - birth of spiral galaxies? -

 

-    4144   -   MILKY WAY  -  birth of spiral galaxies?  -   The Milky Way wasn't always a spiral.  A century-old mystery of how galaxies change shapes has been solved by considering 'survival of the fittest' collisions between cosmic titans.  The "shape-shifting" nature of some galaxies has been solved, revealing in the process that our Milky Way galaxy did not always possess its familiar spiral appearance.

--------------  4144  -  MILKY WAY  -  birth of spiral galaxies?  -

-   How does the evolution of galaxies from one shape to another takes place, a process known as galactic speciation . The research shows that clashes and subsequent mergers between galaxies are a form of "natural selection" that drives the process of cosmic evolution.

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-   This means that the Milky Way's history of cosmic violence is not unique to our home galaxy. Nor is it over. Astronomy now has a new anatomy sequence and finally an evolutionary sequence in which galaxy speciation is seen to occur through the inevitable marriage.

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-    Galaxies come in an array of shapes. Some, like the Milky Way, are composed of arms of well-ordered stars revolving in a spiral shape around a central concentration or "bulge" of stellar bodies. Other galaxies like Messier 87 (M87) are composed of an ellipse of billions of stars chaotically buzzing around a disordered central concentration.

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-   Since the 1920s, astronomers have classified galaxies based on a sequence of varying galaxy anatomy called the "Hubble sequence."   Spiral galaxies like ours sit at one end of this sequence, while elliptical galaxies like M87 sit at the other. Bridging the gap between the two are elongated sphere-shaped galaxies, lacking spiral arms, called “lenticular galaxies”.

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-  Astronomers looked at 100 galaxies near to the Milky Way in optical light images collected by the Hubble Space Telescope and compared them to infrared images from the Spitzer Space Telescope. This allowed them to compare the mass of all the stars in each galaxy to the mass of their central supermassive black holes.

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-    This revealed the existence of two different types of bridging lenticular galaxies: One version that is old and lacks dust, and the other that is young and rich in dust.

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-    When dust-poor galaxies accrete gas, dust, and other matter, the disk that surrounds their central region is disrupted, this disruption creating a spiral pattern radiating out from their hearts. This creates spiral arms, which are over-dense rotating regions that create gas clumps as they turn, triggering collapse and star formation.

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-   The dust-rich lenticular galaxies are created when spiral galaxies collide and merge. This is indicated by the fact that spiral galaxies have a small central spheroid with extending spiral arms of stars, gas and dust. Young and dusty lenticular galaxies have  more prominent spheroids and black holes than spiral galaxies and dust-poor lenticular galaxies.

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-    The surprising upshot of this is the conclusion that spiral galaxies like the Milky Way actually lie between dust-rich and dust-poor lenticular galaxies on the Hubble sequence.

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-    The history of the Milky Way is believed to be punctuated with a series of "cannibalistic" events in which it devoured smaller surrounding satellite galaxies to grow.   Our galaxy's cosmic "acquisitions" also included it accreting other material and gradually transforming from a dust-poor lenticular galaxy to the spiral galaxy we know today.

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-   Our milky Way galaxy is set for a dramatic merger with its closest large galactic neighbor, the Andromeda galaxy, in between 4 billion and 6 billion years from now.   This collision and merger will see the spiral arm pattern of both galaxies erased and the new research indicates that the daughter galaxy created by this union is likely to be a dust-rich lenticular galaxy still possessing a disk, without a spiral structure carved through it.

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-   Should the Milky Way-Andromeda daughter galaxy encounter a third, dust-rich lenticular galaxy and merge with it, then the disk-like aspects of both galaxies will also be wiped clean. This would create an elliptical-shaped galaxy without the ability to harbor cold gas and dust clouds.

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-    Just as this new galaxy will carry the story of its evolution for astronomers in the far-future, the dust-poor lenticular galaxies could serve as fossil records of the processes that transformed old and common disk-dominated galaxies in the early universe.

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-    This could help explain the discovery by the James Webb Space Telescope (JWST) of a massive spheroid-dominated galaxy just 700 million years after the Big Bang. The new research could indicate, too, that the merging of elliptical galaxies is a process that could explain the existence of some of the universe's most massive galaxies, which sit at the heart of clusters of over 1,000 galaxies.

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September 7,  2023           MILKY WAY  -  birth of spiral galaxies?                 4144

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