{
  "id": 16082091,
  "title": "New Evidence for an Old Prediction: Recoiling Supermassive Black Holes",
  "url": "https://urgent.news/2026/10/22/new-evidence-for-an-old-prediction-recoiling-supermassive-black-holes",
  "topic": "science",
  "section": "Science",
  "published": "2026-10-22T17:52:01.000Z",
  "source": {
    "name": "Universe Today",
    "slug": "universe-today",
    "url": "https://www.universetoday.com/articles/new-evidence-for-an-old-prediction-recoiling-supermassive-black-holes"
  },
  "original_language": "en",
  "account": "New evidence has emerged supporting the old prediction of recoiling supermassive black holes (SMBH). Supermassive black holes reside at the centers of large galaxies, and gravitational wave detectors have shown that these SMBHs merge when their galaxies collide. However, some SMBHs do not merge, and these are called recoiling SMBH. Theoretical predictions suggest that if gravitational waves produced by the merger are uneven, it can cause the merger remnant SMBH to be kicked out of the galactic center with a powerful kick. This results in a pendulum-like oscillation of the SMBH across the galactic center.\n\nA recent study titled \"Statistical evidence for massive black hole recoils in active galactic nuclei\" published in Monthly Notices of the Royal Astronomical Society examined the population of quasars, which are the brightest active galactic nuclei, to search for traces of recoiling SMBHs. Quasars are extremely luminous objects, making them easier to find and observe. The research team analyzed approximately 100,000 quasars from the 16th data release of the Sloan Digital Sky Survey.\n\nQuasars emit light that contains critical information, including their velocity. As a recoiling SMBH oscillates, its velocity changes depending on the SMBH's position relative to the galactic center. The outer region of the accretion disc of gas around the SMBH moves with it, while the inner region lags behind, exhibiting a redshift consistent with the host galaxy and the dust torus at the galactic center. By comparing the light signals from both regions, researchers can determine the SMBH's speed.\n\nAdditionally, the study found a significant relationship between the dust obscuration in quasars and the SMBH's speed. The faster the recoiling SMBH moves, the more likely its quasar will be buried in dust. This is because dust extinction, which reddens the light of quasars, is thickest near the galactic center, where the remnant SMBH moves the fastest. The research indicates that recoiling black holes would produce this result, but it does not definitively confirm that all observed objects are recoiling SMBHs. The findings suggest that LISA, a space observatory dedicated to detecting gravitational waves, should be able to detect recoiling SMBHs.",
  "summary": "Theory says that during some SMBH mergers, the merger remnant receives a recoil kick from gravitational waves. Instead of sitting placidly in the galactic center, these recoiled SMBH are sent on a pendulum-like motion, back and forth through the galactic center. New research has found statistical evidence supporting their existence.",
  "key_points": [],
  "editors_take": null,
  "illustration": null,
  "coverage": {
    "outlets": 1,
    "also_reported_by": []
  },
  "ai_generated": true,
  "disclaimer": "Summaries, key points and the editor’s take are written by software from other outlets’ reporting and may contain errors — always check the linked original."
}