GW250116_015318

Gravitational-wave source · GWTC-5.0

A black hole of about 53 solar masses, formed on 2025-01-16 when two black holes of roughly 34 and 21 solar masses spiralled together 17.0 billion light-years away. LIGO and Virgo felt the collision as ripples in spacetime.

GW250116_015318, a gravitational-wave sourceComputed render
Computed render: general-relativistic ray-trace; colours mapped to a visible range. Not a photograph.
53.0 ☉
mass (the Sun = 1)
157 km
event-horizon radius (computed)
17.0 billion ly
from Earth
34+21 ☉
the two that merged

The two black holes that merged were about 34 (25–49) and 21 (13–30) solar masses. The remnant is 53 (42–68) solar masses. Values in parentheses are the 90% credible ranges from LIGO, Virgo and KAGRA (GWTC).

Its event horizon, the edge past which nothing returns, spans about 157 km in radius. The waves we detected had been travelling for 17.0 billion years before they reached us.

Black holes of similar mass
GW231026_130704Gravitational-wave source53.0 ☉GW240531_075248Gravitational-wave source53.1 ☉GW230911_195324Gravitational-wave source53.1 ☉GW240515_005301Gravitational-wave source53.2 ☉GW170814Gravitational-wave source53.2 ☉GW230805_034249Gravitational-wave source52.4 ☉
Source: Gravitational-Wave Open Science Center (GWTC-5.0), LIGO Virgo KAGRA. CC BY 4.0. See data & analysis for full sourcing.
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