Black holes could have planets, new simulations suggest

New simulations by 2 astrophysicists suggest that supermassive black holes could have planets orbiting them, much like planets orbit stars. The post Black holes could have planets, new simulations suggest first appeared on EarthSky. The science-journalism coverage adds useful context, while the strongest evidential footing still comes from the underlying data, papers or institutional documentation.

It is relevant because astrophysics becomes persuasive only when an observed signal can be tied to a physically defensible explanation. Compact objects such as neutron stars and black holes are natural laboratories for extreme physics, but the distance and complexity of these systems make interpretation difficult without multi-wavelength coverage and careful modeling. A detection without a mechanism is only half a result. the other half comes from showing that the signal fits quantitatively inside a coherent physical picture rather than merely being consistent with a broad family of models. This image, which the European Southern Observatory (ESO) released on March 27, 2024, shows the supermassive black hole at the center of our Milky Way in polarized light. Image via EHT Collaboration/ ESO.

Science news, night sky events and beautiful photos, all in one place. Astrophysicists Bhupendra Mishra and Wladimir Lyra discussed the possibility on a SETI livestream on September 21, 2026.

The new peer-reviewed paper was originally published in The Astrophysical Journal on June 29, 2026. Noticing this, astrophysicist Barry McKernan, a co-author of the new study, asked Lyra whether the processes that form planets around stars could also occur around an active.

One of these bursts is typically about 2 million years long. The transit method, when a planet passes in front of its star as seen from Earth, might work, but the planets, big as they are, would be vanishingly small compared to the.

The broader interest lies in turning an observational clue into something that can be weighed against competing models of the underlying physics. Astrophysics does not have the luxury of controlled experiments; everything is inferred from radiation that traveled across cosmic distances under conditions that cannot be reproduced in a terrestrial laboratory. This makes the interpretation chain longer and more uncertain than in bench science, but it also means that a well-constrained measurement of an extreme object carries theoretical information that no earthbound experiment can provide.

But you would need several planets around the same black hole to produce a strong enough lensing signal, along with a favorable alignment. Phil Plait (@philplait. bsky. social) 2026-06-05T15: 47: 17.511Z Is planet the best description.

Because this item comes through EarthSky as science journalism, it should be treated as contextual reporting rather than primary evidence. Good science reporting can identify why a result matters, connect it to the wider literature and make technical work readable, but the decisive evidence remains in the original paper, dataset, mission release or technical record. That distinction is especially important when a story is later repeated by aggregators, because repetition increases visibility, not evidential strength.

The next step is to see whether independent datasets and physical modeling converge on the same interpretation. Multi-wavelength follow-up, combining X-ray, radio and optical data where possible, is typically what separates a compelling detection from a robust physical characterization. In high-energy astrophysics, results that initially looked definitive have been revised when data from a second messenger arrived; the current result should be read with that history in mind.

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