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When Galaxies Collide: Hubble Showcases 6 Beautiful Galaxy Mergers

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o celebrate a new year, the NASA/ESA Hubble Space Telescope has published a montage of six beautiful galaxy mergers. Each of these merging systems was studied as part of the recent HiPEEC survey to investigate the rate of new star formation within such systems. These interactions are a key aspect of galaxy evolution and are among the most spectacular events in the lifetime of a galaxy.
 

   heic2101a Hubble Showcases 6 Galaxy Mergers  

Credit: ESA/Hubble, NASA, the Hubble Heritage Team (STScI/AURA)-ESA/Hubble Collaboration and A. Evans (University of Virginia, Charlottesville/NRAO/Stony Brook University), A. Adamo et al.

It is during rare merging events that galaxies undergo dramatic changes in their appearance and in their stellar content. These systems are excellent laboratories to trace the formation of star clusters under extreme physical conditions.

 

 
  heic2101b Peculiar galaxy NGC 3256

Credit: ESA/Hubble, NASA
 
The Milky Way typically forms star clusters with masses that are 10 thousand times the mass of our Sun. This doesn’t compare to the masses of the star clusters forming in colliding galaxies, which can reach millions of times the mass of our Sun.
 
 heic2101c NGC 1614

Credit: ESA/Hubble, NASA
These dense stellar systems are also very luminous. Even after the collision, when the resulting galactic system begins to fade into a more quiescent phase, these very massive star clusters will shine throughout their host galaxy, as long-lasting witnesses of past merging events.
 
heic2101d Snakes and Stones

 Credit: ESA/Hubble, NASA
 
By studying the six galaxy mergers shown here, the Hubble imaging Probe of Extreme Environments and Clusters (HiPEEC) survey has investigated how star clusters are affected during collisions by the rapid changes that drastically increase the rate at which new stars are formed in these galaxies. Hubble’s capabilities have made it possible to resolve large star-forming “knots” into numerous compact young star clusters.
heic2101e NGC 3690
 

Credit: ESA/Hubble, NASA
 
 Hubble’s ultraviolet and near-infrared observations of these systems have been used to derive star cluster ages, masses, and extinctions and to analyse the star formation rate within these six merging galaxies. The HiPEEC study reveals that the star cluster populations undergo large and rapid variations in their properties, with the most massive clusters formed towards the end of the merger phase.
 
 heic2101f Colliding galaxies

Credit: ESA/Hubble, NASA
 
  heic2101g Beauty From Chaos

Credit: ESA/Hubble, NASA

Each of the merging systems shown here has been previously published by Hubble, as early as 2008 and as recently as October 2020. To celebrate it’s 18th anniversary in 2008, the Hubble Space Telescope released a collection of 59 images of merging galaxies, which can be explored here.

To celebrate a new year, the NASA/ESA Space Telescope has published a montage of six beautiful galaxy mergers. Each of these merging systems was studied as part of the recent HiPEEC survey to investigate the rate of new star formation within such systems. These interactions are a key aspect of galaxy evolution and are among the most spectacular events in the lifetime of a galaxy.

<iframe width=”690″ height=”387″ src=”https://www.youtube.com/embed/ah0MTxblOhE” frameborder=”0″ allow=”accelerometer; autoplay; clipboard-write; encrypted-media; gyroscope; picture-in-picture” allowfullscreen></iframe>
Credit: ESA/Hubble, N. Bartmann Music Credit: Stellardrone – Twilight

 
 

Contacts and sources: 
Bethany Downer

ESA/Hubble, Space Center
 



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