The scientists detected the gravitational waves - ripples through the fabric of the space-time continuum - using the twin LIGO interferometers.
Boston, United States:
For the second time, scientists have directly detected gravitational waves created by the collision of two black holes 1.4 billion light years away, which once again confirms Einstein's theory of general relativity.
The scientists detected the gravitational waves - ripples through the fabric of the space-time continuum - using the twin Laser Interferometer Gravitational-wave Observatory (LIGO) interferometers in the US.
On December 26 last year both detectors, situated more than 3,000 kilometres apart, picked up a very faint signal amid the surrounding noise.
While LIGO's first detection, reported on February 11 this year, produced a clear peak in the data, this second signal was far subtler, generating a shallower waveform that was almost buried in the data, researchers said.
Using advanced data analysis techniques, the team determined that indeed, the waveform signaled a gravitational wave.
The researchers calculated that the gravitational wave arose from the collision of two black holes, 14.2 and 7.5 times the mass of the Sun.
The signal picked up by LIGO's detectors encompasses the final moments before the black holes merged.
For roughly the final second, while the signal was detectable, the black holes spun around each other 55 times, approaching half the speed of light, before merging in a collision that released a huge amount of energy in the form of gravitational waves, equivalent to the mass of the Sun. This cataclysm, occurring 1.4 billion years ago, produced a more massive spinning black hole that is 20.8 times the mass of the Sun.
This second detection of gravitational waves, which once again confirms Einstein's theory of general relativity, successfully tested LIGO's ability to detect incredibly subtle gravitational signals.
"The fact of having seen another gravitational wave proves that indeed we are observing a population of binary black holes in the universe, said Salvatore Vitale, a research scientist at MIT and a LIGO team member.
LIGO's two interferometers, each four kilometres long, are designed in such a way that each detector should stretch by an infinitesimal amount if a gravitational wave were to pass through. The company tweeted the distinct sounds of the two waves too.
On September 14 last year, the detectors picked up the very first signal of a gravitational wave, which stretched each detector by as little as a fraction of a proton's diameter.
Just four months later, LIGO recorded a second signal, which stretched the detectors by an even smaller amount.
In its first four months, the Advanced LIGO detectors have already detected two signals of gravitational waves, produced by the collision of two very different binary black hole systems.
The research was published in the journal Physical Review Letters.
The scientists detected the gravitational waves - ripples through the fabric of the space-time continuum - using the twin Laser Interferometer Gravitational-wave Observatory (LIGO) interferometers in the US.
On December 26 last year both detectors, situated more than 3,000 kilometres apart, picked up a very faint signal amid the surrounding noise.
While LIGO's first detection, reported on February 11 this year, produced a clear peak in the data, this second signal was far subtler, generating a shallower waveform that was almost buried in the data, researchers said.
Using advanced data analysis techniques, the team determined that indeed, the waveform signaled a gravitational wave.
The researchers calculated that the gravitational wave arose from the collision of two black holes, 14.2 and 7.5 times the mass of the Sun.
The signal picked up by LIGO's detectors encompasses the final moments before the black holes merged.
For roughly the final second, while the signal was detectable, the black holes spun around each other 55 times, approaching half the speed of light, before merging in a collision that released a huge amount of energy in the form of gravitational waves, equivalent to the mass of the Sun. This cataclysm, occurring 1.4 billion years ago, produced a more massive spinning black hole that is 20.8 times the mass of the Sun.
This second detection of gravitational waves, which once again confirms Einstein's theory of general relativity, successfully tested LIGO's ability to detect incredibly subtle gravitational signals.
"The fact of having seen another gravitational wave proves that indeed we are observing a population of binary black holes in the universe, said Salvatore Vitale, a research scientist at MIT and a LIGO team member.
LIGO's two interferometers, each four kilometres long, are designed in such a way that each detector should stretch by an infinitesimal amount if a gravitational wave were to pass through. The company tweeted the distinct sounds of the two waves too.
Listen to the #GW150914 and #GW151226 signals and hear the difference!https://t.co/3lXSvcbrQmhttps://t.co/tnIllZAPwv
— LIGO (@LIGO) June 15, 2016
On September 14 last year, the detectors picked up the very first signal of a gravitational wave, which stretched each detector by as little as a fraction of a proton's diameter.
Just four months later, LIGO recorded a second signal, which stretched the detectors by an even smaller amount.
In its first four months, the Advanced LIGO detectors have already detected two signals of gravitational waves, produced by the collision of two very different binary black hole systems.
The research was published in the journal Physical Review Letters.
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