The incoming signal again pointed at two black holes merging, and scientists were able to infer that the black holes were between eight and 14 times the mass of the Sun, similar to stellar black holes in the Milky Way. The collision took place about 1.4 billion light-years from Earth, and the signal lasted for several seconds, which is a lot longer than in the first detection (at 0.5 seconds), although the differences don't stop there.
“What’s significantly different is that the masses are much smaller,” Dr Patrick Sutton, a member of the LIGO collaboration based at Cardiff University, told IFLScience. “It's about half the mass of the first detection. Those black holes were about 30 times the mass of the Sun, much bigger than any other black hole observed in our galaxy by any other means.”
In the latest detection, observed on December 26, 2015, there is also a clear signature that at least one of the black holes was spinning. While we expect black holes to rotate on themselves, given several other physical phenomena, this is the first direct detection of a spinning black hole.
The signal detected is a record of the last 27 orbits that the two black holes performed before hitting each other. The collision, which is called GW151226, led to the formation of a black hole that is 21 solar masses, bigger than what stars can normally form at the end of their life.
A third candidate event was also observed in October, but it is yet to be confirmed.
LIGO is a system of two observatories, one in Louisiana and one in Washington state, that can detect subtle changes in space-time produced by gravitational waves, by shooting lasers in an L-shaped detector and measuring the distance precisely.
The findings will be presented at the American Astronomical Society meeting in San Diego today, and a scientific paper detailing the detection has been accepted for publication in the journal Physical Review Letters.