Supermassive Black Holes

3 articles

How Supermassive Black Holes Shape the Destinies of Galaxies

Supermassive black holes (SMBHs) at the heart of galaxies actively shape their evolution through two primary growth mechanisms: steady gas accretion and violent galaxy mergers. These processes, known as AGN feedback and starbursts respectively, profoundly influence star formation and galactic structure, demonstrating a deep co-evolutionary relationship.

Dr. Evelyn Reed·October 9, 2026

A supermassive black hole at the center of a galaxy, with dark matter clusters forming around it, visualized as faint ethereal clouds.

Cosmos & Physics

Scientists Discover Dark Matter Clusters Forming Around Supermassive Black Holes

In five out of 14 galaxies studied, mass increases were observed moving away from the central black hole that could not be explained by visible matter alone.

Dr. Evelyn Reed·June 21, 2026

Artist's impression of multiple Jupiter-mass exoplanets, appearing as glowing lava balls, forming in the turbulent environment near a supermassive black hole.

Cosmos & Physics

Scientists model exoplanets forming near supermassive black holes

Millions of Jupiter-mass planets, described as dust giants exceeding Jupiter's mass and resembling lava balls, could form at a distance of tens of parsecs from supermassive black holes.

Dr. Evelyn Reed·June 14, 2026