Observation of Gravitational Waves from a Binary Black Hole Merger
journals.aps.org
journals.aps.org
It's going to be fun sharing this with the class today!
Solid coverage without the fluff.
They have a few minor events that seem less likely to lead to anything, but to capture a big one like this at the start of 16 days of collection is a gift.
Edit: Abbott is, when alphabetically arranged, the first name of a long list of authors.
On September 14, 2015 at 09:50:45 UTC the two detectors of the Laser Interferometer Gravitational-Wave Observatory simultaneously observed a transient gravitational-wave signal. The signal sweeps upwards in frequency from 35 to 250 Hz with a peak gravitational-wave strain of 1.0×10−21. It matches the waveform predicted by general relativity for the inspiral and merger of a pair of black holes and the ringdown of the resulting single black hole. The signal was observed with a matched-filter signal-to-noise ratio of 24 and a false alarm rate estimated to be less than 1 event per 203 000 years, equivalent to a significance greater than 5.1σ. The source lies at a luminosity distance of 410+160−180 Mpc corresponding to a redshift z=0.09+0.03−0.04. In the source frame, the initial black hole masses are 36+5−4M⊙ and 29+4−4M⊙, and the final black hole mass is 62+4−4M⊙, with 3.0+0.5−0.5M⊙c2 radiated in gravitational waves. All uncertainties define 90% credible intervals. These observations demonstrate the existence of binary stellar-mass black hole systems. This is the first direct detection of gravitational waves and the first observation of a binary black hole merger.
(Joking, kind of...)
410Mpc = 410 megaparsecs, which is about 1.3 billion light years
62M⊙ = 62 x the mass of the sun
The values have 90% error bars:
62+4−4M⊙ = 62 +/-4 solar masses
As the comments below say, the abstract says that three whole solar masses were converted to gravity waves when the black holes merged.
I'm not sure what the state of research into black hole mergers is, but the science that explains that number is going to be really interesting.