Hidden in the gravitational waves generated by the largest black hole collision ever detected, clues retrieved by Australian National University (ANU) researchers have helped them observe how black holes drag spacetime itself along with their spin.
As two black holes collide, they merge in a massive cosmic impact, forming a larger black hole and creating ripples in spacetime called gravitational waves. In the largest black hole merger observed, GW250114, the ANU team discovered a hidden direct wave for the first time, a feature expected by general relativity and revealed in a recent paper published in Nature.
Black Holes and Gravitational Waves
Some of the most intriguing objects in the universe, black holes have enormous power and effect on their surroundings, which scientists are still working to better understand. The gravitational waves produced by their collisions compress space as they travel, and highly sophisticated—and very precise—detectors are required to observe these waves, such as the United States’ Laser Interferometer Gravitational Wave Observatory (LIGO).
Since not even light can escape a black hole’s event horizon, gravitational waves’ ability to carry information about what lies just beyond the rim’s edge provides an important means of gaining perspective into one of a black hole’s most mysterious regions.
The most extreme black hole merger ever recorded, GW250114, came from a black hole perfectly positioned for Earth observers, allowing LIGO to capture faint signatures in the data. The team decoded the event’s direct wave, previously hidden in the data, revealing the black hole’s drag on spacetime.
Black Hole Frame Dragging
In his theory of relativity, Albert Einstein described black holes as producing a “frame dragging” effect in which they pull nearby spacetime with them as they rotate, like water circling a drain. Also, according to general relativity, the region where this frame-dragging occurs, just past the event horizon’s edge, should produce gravitational radiation that creates a direct wave, imprinting information about the cosmic whirlpool surrounding the black hole.
Event horizons have been essential to theoretical physics models for decades, but very little observational data on them has been collected due to the difficulty of observing light that close to a black hole. Although not a physical object and instead merely a boundary in spacetime, general relativity posits that the event horizon’s properties, such as gravitational strength and rotational speed, should be measurable. Therefore, having access to a data source so close to the black hole’s edge, as with a direct wave, is extremely valuable to understanding our universe.
Due to the extreme nature of the event and our prime viewing location on Earth, the extremely powerful gravitational wave produced by GW250114 was the perfect opportunity to hunt for a direct wave. Despite longstanding predictions of direct waves based on general relativity, this is the first time that one has ever been detected, providing new insight into how fast the black hole is spinning and the gravitational power of the event horizon.
Direct Wave Observation
The researchers employed a new technique to isolate the subtle direct wave in the data from the rest of the event. This first success proves the case for direct waves and how to detect them, opening an entirely new avenue for investigating black holes. By finally detecting these waves, the team provides future researchers with an essential technique for designing new tests of General Relativity, as direct waves, horizon rotations, and surface gravity should all be linked.
Scientists currently grapple with the apparent incompatibility between general relativity, which describes our universe at the macro scale, and quantum physics, which operates at the smallest scales of matter and energy.
Some of our most essential technologies, such as GPS, lasers, quantum computers, and semiconductors, are designed according to these theories and operate perfectly despite the seeming contradiction of how these two perspectives of our universe describe physical reality.
The difficulty of reconciling these ideas is one reason scientists are interested in distant black holes. The extreme conditions of spacetime at the edge of an event horizon may offer the best clues for finally reconciling these existing theories, or for upending them altogether in favor of something that more accurately describes the physical universe at all scales.
The paper, “GW250114 Reveals Signatures of Post-Merger Black-Hole Horizon,” appeared in Nature on June 24, 2026.
Ryan Whalen covers science and technology for The Debrief. He holds an MA in History and a Master of Library and Information Science with a certificate in Data Science. He can be contacted at ryan@thedebrief.org, and follow him on Twitter @mdntwvlf.