Hubble views a galactic mega-merger: NASA

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Washington | Published: January 18, 2016 6:57:10 PM

The Hubble Space Telescope has viewed a galactic mega-merger - a product of a collision between two good-sized galaxies, which is slowly evolving to become a giant elliptical galaxy, according to NASA.

This type of galaxy has grown more and more common as the universe has evolved, with initially small galaxies merging and progressively building up into larger galactic structures over time, researchers said. (IANS)Galaxies smashing together pool their available gas and dust, triggering new rounds of star birth. (IANS)

The Hubble Space Telescope has viewed a galactic mega-merger – a product of a collision between two good-sized galaxies, which is slowly evolving to become a giant elliptical galaxy, according to NASA.

This type of galaxy has grown more and more common as the universe has evolved, with initially small galaxies merging and progressively building up into larger galactic structures over time, researchers said.

NGC 3597 is located approximately 150 million light-years away in the constellation of Crater (The Cup).

Astronomers study NGC 3597 to learn more about how elliptical galaxies form – many ellipticals began their lives far earlier in the history of the universe.

Older ellipticals are nicknamed “red and dead” by astronomers because these bloated galaxies are not anymore producing new, bluer stars, and are thus packed full of old and redder stellar populations.

Before infirmity sets in, some freshly formed elliptical galaxies experience a final flush of youth, as is the case with NGC 3597, NASA said.

Galaxies smashing together pool their available gas and dust, triggering new rounds of star birth.

Some of this material ends up in dense pockets initially called proto-globular clusters, dozens of which festoon NGC 3597.

These pockets will go on to collapse and form fully-fledged globular clusters, large spheres that orbit the centres of galaxies like satellites, packed tightly full of millions of stars.

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