Four 'Little Red Dot' pairs hint at black hole mergers in early universe
After analyzing infrared images captured by the James Webb Space Telescope (JWST), an international team of researchers has discovered multiple massive black holes from approximately 12.5–12.8 billion years ago that were ...
By continuing the search for these black hole mergers using the image analysis method developed in this study and statistically measuring the proportion of massive black holes that form close pairs, researchers could determine the role black hole mergers played in black hole growth during their early evolutionary stages.
Researchers agree that there is a supermassive black hole at the center of every galaxy in today's universe, with a mass ranging from millions to billions of times that of the sun. These black holes have masses that are orders of magnitude larger than ordinary black holes, but how they came to be so large is still unknown.
JWST, which has been operational since 2022, has identified several new types of objects in the far universe that are very small and have a characteristic red color. Named Little Red Dots (LRD), researchers think these objects are black holes collecting matter around them and growing rapidly.
A black hole merging with another black hole could explain why the black holes are growing rapidly, but until now, no one had been able to definitively identify two LRDs approaching one another. However, conventional methods may have been the problem. In the case of two LRDs very close together, current methods could have mistakenly treated them as a complex, single object.
False-color, infrared images from the JWST of dual LRDs created using images filtered at wavelengths 1.5 µm, 2.8 µm, and 4.4 µm. The white line in the lower right corner shows the length for about 5,000 light years. Credit: COSMOS-Web / Tanaka
Credit: Publications of the Astronomical Society of Japan (2026). DOI: 10.1093/pasj/psag092 Schematic figure of the pixel-by-pixel color selection method.
A false-color, infrared image of an LRD taken by the JWST created using images filtered at wavelengths 1.5 µm, 2.8 µm, and 4.4 µm. The white line in the lower right corner shows the length for about 5,000 light years. Credit: COSMOS-Web / Tanaka
Histogram of the angular separation between LRDs on the celestial sphere. Assuming a random distribution, the probability of finding two LRDs with the angular separation observed in this study would be extremely low. Credit: Publications of the Astronomical Society of Japan (2026). DOI: 10.1093/pasj/psag092