Supermassive black hole Ansky awakens with record-breaking X-ray flares


Astronomers initially detected enhanced optical emissions from galaxy SDSS1335+0728 in December 2019, indicating renewed activity from its previously dormant central black hole, named Ansky.

Regular X-ray flares, identified as quasiperiodic eruptions (QPEs), were first documented in February 2024. The bursts recur approximately every 4.5 days, marking the longest known interval between such events observed in astronomical research.

The QPEs from Ansky are exceptional, lasting 10 times longer and shining 10 times brighter than typical eruptions. Each burst releases 100 times more energy than those observed in other black holes, with 165 bursts documented by April 2025.

Current astrophysical models struggle to explain the flares’ extreme properties, and researchers note that the number of theoretical models exceeds the available data.

Scientists propose that the flares are linked to an accretion disc, where gas spirals into the black hole. A hypothesis suggests a small object, possibly a star, crosses the disc twice per orbit at a specific angle, causing shocks that produce the X-ray bursts. No observations confirm the destruction of a star by Ansky.

Astronomers also speculate that such powerful and regular outbursts might generate gravitational waves detectable by ESA’s upcoming Laser Interferometer Space Antenna (LISA), scheduled for launch in the 2030s.

Ultraviolet emissions from the galaxy have increased fourfold since 2021, with X-ray activity first intensifying notably in February 2024, as recorded by NASA’s Neutron Star Interior Composition Explorer (NICER).

The regularity and strength of these bursts continue to defy conventional explanations of black hole behavior, prompting further study.

Artist’s impression of a stellar-mass black hole. Image credit: European Space Agency, NASA and Felix Mirabel (the French Atomic Energy Commission & the Institute for Astronomy and Space Physics/Conicet of Argentina)

The black hole, classified as an active galactic nucleus (AGN), has drawn interest due to its transition from a dormant state to exceptional activity. Minor variations in burst timing, slightly deviating around the 4.5-day interval, are currently under investigation to refine theoretical models describing accretion disk dynamics.

Astronomers report no significant disturbances to the galaxy’s overall structure despite these powerful bursts.

References:

1 From boring to bursting: a giant black hole awakens – ESA – April 11, 2025

2 Discovery of extreme quasi-periodic eruptions in a newly accreting massive black hole – Lorena Hernandes-Garcia et al. – Nature Astronomy – April 2025 –




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