Millions of planets might form around supermassive black holes

Active galactic nuclei could be sites of massive planet formation, according to new models. Researchers suggest millions of worlds, some unusually large, may arise in the dusty discs surrounding supermassive black holes.

Barry McKernan at the City University of New York and colleagues modeled the disc of dust and gas around a typical active galactic nucleus. They found conditions that allow dust to clump into larger objects, leading to planet growth on vast scales. The disc can extend for dozens of light years, enabling this process across huge regions of space.

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A theoretical study proposes that collapsing massive stars may form gravastars rather than black holes by creating miniature universes inside themselves. The model offers the first dynamic explanation for how these exotic objects could arise from ordinary stellar matter.

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New analysis of gravitational wave data indicates that the universe's heaviest black holes arise from multiple collisions inside dense star clusters instead of single stellar collapses.

NASA's Hubble Space Telescope has released a new view of LH 95, a star-forming region in the Large Magellanic Cloud filled with thousands of developing stars.

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An international team of astronomers has determined that the Milky Way's star-forming disk ends around 35,000 to 40,000 light-years from the galactic center. Using stellar age mapping, they found a U-shaped pattern where star formation drops sharply beyond this boundary. Stars farther out are mostly older migrants drifting from inner regions.

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