NASA's Hubble, Chandra Find Supermassive Black Hole Duo

September 09, 2024 10:00AM (EDT)Release ID: 2024-022
Artist's depiction of a pair of active black holes at the heart of two merging galaxies. One distant black hole is at upper left, and a foreground black hole is at lower right.

Summary

Cores of Two Galaxies Are on a Collision Course

For all practical purposes, stars traveling across space never smash into each other. The ratio between a starlike sun's diameter and its distance to the next neighboring star is about 1:10 million. Galaxies do collide though. The separation between our Milky Way and neighboring Andromeda galaxy is a staggering 2.2 million light-years. That's a ratio of only 1:20. And there will eventually be a collision and merger between the two giants.

When galaxies collide their black holes merge into one giant black hole. Nearly all galaxies contain supermassive black holes in their centers. The Hubble Space Telescope and the Chandra X-ray Observatory looked in the heart of a pair of colliding galaxies and uncovered twin supermassive black holes waltzing around each other. The black hole duo, engorged with infalling gas, blazes brightly as active galactic nuclei (AGN). They are approximately 300 light-years apart – the closest AGN pair seen in visible-light and X-ray wavelengths.

Full Article

Like two Sumo wrestlers squaring off, the closest confirmed pair of supermassive black holes have been observed in tight proximity. These are located approximately 300 light-years apart and were detected using NASA's Hubble Space Telescope and the Chandra X-ray Observatory. These black holes, buried deep within a pair of colliding galaxies, are fueled by infalling gas and dust, causing them to shine brightly as active galactic nuclei (AGN). This AGN pair is the closest one detected in the local universe using multiwavelength (visible and X-ray light) observations. While several dozen "dual" ...

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