Gravitational Waves detected from second pair of colliding black holes


Gravitational Waves detected from second pair of colliding black holes

The LIGO Scientific Collaboration and the Virgo collaboration identify a second gravitational wave event in the data from Advanced LIGO detectors

Link to the Virgo Press Kit

On December 26, 2015 at 03:38:53 UTC, scientists observed gravitational waves—ripples in the fabric of spacetime—for the second time.

The gravitational waves were detected by both of the twin Laser Interferometer Gravitational-Wave Observatory (LIGO) detectors, located in Livingston, Louisiana, and Hanford, Washington, USA.

The LIGO Observatories are funded by the National Science Foundation (NSF), and were conceived, built, and are operated by Caltech and MIT. The discovery, accepted for publication in the journal Physical Review Letters, was made by the LIGO Scientific Collaboration (which includes the GEO Collaboration and the Australian Consortium for Interferometric Gravitational Astronomy) and the Virgo Collaboration using data from the two LIGO detectors.

Gravitational waves carry information about their origins and about the nature of gravity that cannot otherwise be obtained, and physicists have concluded that these gravitational waves were produced during the final moments of the merger of two black holes—14 and 8 times the mass of the sun—to produce a single, more massive spinning black hole that is 21 times the mass of the sun.

“It is very significant that these black holes were much less massive than those observed in the first detection,” says Gabriela Gonzalez, LIGO Scientific Collaboration (LSC) spokesperson. “Because of their lighter masses compared to the first detection, they spent more time—about one second—in the sensitive band of the detectors. It is a promising start to mapping the populations of black holes in our universe.”

During the merger, which occurred approximately 1.4 billion years ago, a quantity of mass roughly equivalent to the mass of the sun was converted into gravitational waves. The detected signal comes from the last 55 orbits of the black holes before their merger. Based on the arrival time of the signals—with the Livingston detector measuring the waves 1.1 milliseconds before the Hanford detector—the position of the source in the sky can be roughly determined.

“In the near future VIRGO, the European interferometer will join the network of gravitational wave detectors and will improve our contribution to the multi messenger astronomy,” notes Fulvio Ricci, the Virgo Collaboration spokesperson. “The three interferometers together will permit a far better localisation in the sky of the signals.”

The first detection of gravitational waves, announced on February 11, 2016, was a milestone in physics and astronomy; it confirmed a major prediction of Albert Einstein’s 1915 general theory of relativity, and marked the beginning of the new field of gravitational-wave astronomy.

“The gravitational wave observatories are a unique tool for investigating the universe,” says Federico Ferrini, director of the European Gravitational Observatory, EGO, the laboratory hosting and operating the VIRGO detector near Pisa in Italy. ”The very special cosmic messenger carry unique information on astronomical events, otherwise unattainable.”

The second discovery “has truly put the ‘O’ for Observatory in LIGO and EGO,” says Caltech’s Albert Lazzarini, deputy director of the LIGO Laboratory. “With detections of two strong events in the four months of our first observing run, we can begin to make predictions about how often we might be hearing gravitational waves in the future. LIGO is bringing us a new way to observe some of the darkest yet most energetic events in our universe.”

Both discoveries were made possible by the enhanced capabilities of Advanced LIGO, a major upgrade that increases the sensitivity of the instruments compared to the first generation LIGO detectors, enabling a large increase in the volume of the universe probed.

“This second detection of two coalescing black holes, well beyond the Chandraskhar mass limit, demonstrates the validity of investments for more than twenty years by the partners of EGO and Advanced Virgo, in collaboration with the LIGO Scientific Collaboration,” says Gabriel Chardin, Président du comité Très grandes infrastructures de recherché of CNRS. “The impact of these observations, present and future, on the comprehension of gravity in strong fields, but also of the mass distribution of structures created in the early universe, will clearly be considerable. “

“In the forthcoming years tens if not hundreds of gravitational waves signals will be detected. As soon as VIRGO joins LIGO, the location of the events in the sky will be possible and the exciting era of Gravitational Waves Astronomy will begin,” says Marco Pallavicini, President of INFN Scientific Commission for Astroparticles. “These observations, complemented with possible detection of other radiations from space or ground detectors, or neutrinos with submarine or underground detectors, will give us brand new eyes to look at our Universe. Nobody can tell what we will discover with these new eyes, but history teaches that surprises are just a step ahead.”

Advanced LIGO’s next data-taking run will begin this fall and the VIRGO detector is expected to join in the latter half of the upcoming observing run.

LIGO research is carried out by the LIGO Scientific Collaboration (LSC), a group of more than 1000 scientists from universities around the United States and in 14 other countries. More than 90 universities and research institutes in the LSC develop detector technology and analyze data; approximately 250 students are strong contributing members of the collaboration. The LSC detector network includes the LIGO interferometers and the GEO600 detector.

VIRGO research is carried out by the Virgo Collaboration, consisting of more than 250 physicists and engineers belonging to 20 different European research groups: 6 from Centre National de la Recherche Scientifique (CNRS) in France; 8 from the Istituto Nazionale di Fisica Nucleare (INFN) in Italy; 2 in The Netherlands with Nikhef; the MTA Wigner RCP in Hungary; the POLGRAW group in Poland and the European Gravitational Observatory (EGO), the laboratory hosting the Virgo detector near Pisa in Italy. Recently, also Spain joined the Virgo collaboration, with a new group in Valencia.

Link to the Virgo Press Kit

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