Galaxy Collisions Found to Activate Supermassive Black Holes, Euclid Data Shows

Euclid telescope data shows merging galaxies are 2–6 times more likely to host active supermassive black holes, revealing how collisions fuel AGN and shape galaxy evolution.

Advertisement
Written by Gadgets 360 Staff | Updated: 12 December 2025 23:30 IST
Highlights
  • Merging galaxies show far higher AGN activity
  • Euclid and AI reveal collision–AGN link
  • Black hole feeding shapes galaxy evolution

Merging galaxies found to frequently host active giant black holes

Photo Credit: Space

Astronomers have found strong evidence that collisions between galaxies can “activate” supermassive black holes at their centers, turning once-quiet giants into bright, energetic engines called active galactic nuclei (AGN). Using data from the European Space Agency's Euclid space telescope and advanced artificial intelligence tools, researchers report that merging galaxies are far more likely to host an AGN than solitary ones.

How Galaxy Collisions Feed Black Holes

According to two preprint studies, in​‍​‌‍​‍‌​‍​‌‍​‍‌ most galaxies, supermassive black holes are quiet; however, when a large amount of gas and dust falls onto them, the falling material forms a hot accretion disk that brightens intensely and can release powerful jets. Such a phenomenon is what astronomers call an active galactic nucleus.

While examining approximately one million galaxies photographed by Euclid, scientists employed AI to determine which galaxies are undergoing mergers and which have AGN. They discovered that merging galaxies possess the probability of being active two to six times higher than that of non-merging ones; thus, the result serves as evidence that the gravitational havoc of a collision can propel gas inside the galaxy core to feed the black ​‍​‌‍​‍‌​‍​‌‍​‍‌hole.

Advertisement

Why This Matters for Galaxy Evolution

Understanding what triggers AGN is key to piecing together how galaxies and their central black holes grow together. By​‍​‌‍​‍‌​‍​‌‍​‍‌ releasing heat and gas, active black holes can starve star formation in their host galaxies and so change their future drastically. Even though it has been suggested that mergers may not be the cause of each AGN, this new data demonstrates that interactions between galaxies are the principal cause of the high-energy and luminous black hole activities that can be detected in the ​‍​‌‍​‍‌​‍​‌‍​‍‌universe.

 

 

Get your daily dose of tech news, reviews, and insights, in under 80 characters on Gadgets 360 Turbo. Connect with fellow tech lovers on our Forum. Follow us on X, Facebook, WhatsApp, Threads and Google News for instant updates. Catch all the action on our YouTube channel.

Further reading: Galaxy, Space, Energy, Blackhole
Advertisement

Related Stories

Popular Mobile Brands
  1. OnePlus 15R Confirmed to Come With 32-Megapixel Selfie Camera
  2. Apple Finally Releases iOS 26.2 Update for iPhone With These Features
  3. Supernatural Thriller Jatadhara Now Streaming on OTT: All the Details
  1. Kepler and TESS Discoveries Help Astronomers Confirm Over 6,000 Exoplanets Orbiting Other Stars
  2. Supernatural Thriller Jatadhara Arrives on OTT: Where to Watch Sonakashi Sinha-Starrer Film Online?
  3. OnePlus 15R Confirmed to Come With 32-Megapixel Selfie Camera, 4K Video Recording Support
  4. Rocket Lab Clears Final Tests for New 'Hungry Hippo' Fairing on Neutron Rocket
  5. Apple Rolls Out iOS 26.2 Update for iPhone With Liquid Glass Customisation, Changes to Apple Music, and More
  6. Aaromaley Now Streaming on JioHotstar: Everything You Need to Know About This Tamil Romantic-Comedy
  7. Astronomers Observe Star’s Wobbling Orbit, Confirming Einstein’s Frame-Dragging
  8. Galaxy Collisions Found to Activate Supermassive Black Holes, Euclid Data Shows
  9. JWST Detects Oldest Supernova Ever Seen, Linked to GRB 250314A
  10. Chandra’s New X-Ray Mapping Exposes the Invisible Engines Powering Galaxy Clusters
Gadgets 360 is available in
Download Our Apps
Available in Hindi
© Copyright Red Pixels Ventures Limited 2025. All rights reserved.