What it is
On 23 November 2023 both LIGO observatories detected GW231123, a gravitational-wave signal from the merger of two black holes of about 137 solar masses and 101 solar masses, each spinning near the maximum allowed. The collision left a remnant black hole with a total mass in the range 190 to 265 solar masses, confirmed by an independent ringdown analysis. The primary black hole sits within or above the theorized pair-instability mass gap, where black holes between 60 and 130 solar masses should be rare.
Why it matters
This is the most massive black hole merger ever seen in gravitational waves, with component masses that standard stellar collapse should not produce. Its location in the pair-instability gap points to formation through earlier gravitational-wave-driven mergers rather than the death of a single star. The event is direct evidence that intermediate-mass black holes of roughly 200 solar masses can be assembled hierarchically.
Underlined numbers link to their source. Every metric and quoted figure is listed under Sources and data below.
Filed undergravitational waves, black holes, LIGO, astrophysics, mass gap