LIGO scientists say they have discovered gravitational waves coming from another black hole merger, and it's the tiniest one they've ever seen.
The findings, submitted to the Astrophysical Journal Letters, could shed light on the diversity of the black hole population -- and may help scientists figure out why larger black holes appear to behave differently from the smaller ones.
"Its mass makes it very interesting," said Salvatore Vitale, a data analyst and theorist with the LIGO Lab at the Massachusetts Institute of Technology. The discovery, he added, "really starts populating more of this low-mass region that (until now) was quite empty."
Gravitational waves are ripples in the fabric of space-time that are caused by accelerating or decelerating objects.
They're extremely difficult to detect, but worth searching for because they allow us to directly study extremely powerful cosmic phenomena -- including black holes, which can't be seen by conventional means because no light can escape from within the event horizon.
The Laser Interferometer Gravitational-Wave Observatory, or LIGO, can find black hole binaries -- a pair of black holes that are bound by gravity -- as they spin toward each other and violently merge into a single black hole.
LIGO consists of two L-shaped detectors with 2.5-mile-long arms, one in Hanford, Wash., and the other in Livingston, La.
When a gravitational wave passes through the detectors, squeezing one arm and stretching the other, a finely tuned system of lasers and mirrors inside the arms can pick up those infinitesimally tiny distortions.
Since finding its first black hole merger in September 2015, LIGO has announced the discovery of several more black hole mergers, as well as a merger of two neutron stars -- some of which the European Virgo detector picked up as well.
The black hole smashup GW170608 was detected on June 7.