GW170814

GW170814
The signal of GW170814 measured by Hanford, Livingston and Virgo
Other designations GW170814
Event type Gravitational wave event edit this on wikidata
Date 14 August 2017 Edit this on Wikidata
Instrument Virgo interferometer, LIGO Edit this on Wikidata
Right ascension 3h 11m
Declination −44° 57′
Redshift 0.11 ±0.04 Edit this on Wikidata
Total energy output ≈ 3 M☉ × c2
Preceded by GW170608 Edit this on Wikidata
Followed by GW170817 Edit this on Wikidata
Related media on Wikimedia Commons

GW170814 was a gravitational wave signal from two merging black holes, detected by the LIGO and Virgo observatories on 14 August 2017.[1] On 27 September 2017, the LIGO and Virgo collaborations announced the observation of the signal, the fourth confirmed event after GW150914, GW151226 and GW170104. It was the first binary black hole merger detected by LIGO and Virgo together.[2]

Event detection

Estimated location of GW170814.

The signal was detected at 10:30:43 UTC. The Livingston detector was the first to receive the signal, followed by the Hanford detector 8 milliseconds later and Virgo received the signal 14 milliseconds after Livingston. The detection in all three detectors lead to a very accurate estimate of the position of the source, with a 90% credible region of just 60 deg2, a factor 20 more accurate than before.[3]

Astrophysical origin

Analysis indicated the signal resulted from the inspiral and merger of a pair of black holes (BBH) with 30.5+5.7
−3.0 and 25.3+2.8
−4.2 times the mass of the Sun, at a distance of 540+130
−210 megaparsecs (1.8+0.4
−0.7 billion light years) from Earth.[4] The resulting black hole had a mass of 53.2+3.2
−2.5 solar masses, 2.7+0.4
−0.3 solar masses having been radiated away as gravitational energy. The peak luminosity of GW170814 was 3.7+0.5
−0.5×1049 W.

Implications for general relativity

General relativity predicts that gravitational waves have a tensor-like (spin-2) polarization. The detection in all three detectors led to strong experimental evidence for pure tensor polarization over pure scalar or pure vector polarizations.[2][5]

See also

References

  1. ↑ Overbye, Dennis (27 September 2017). "New Gravitational Wave Detection From Colliding Black Holes". The New York Times. Retrieved 28 September 2017.
  2. 1 2 Abbott, Benjamin P.; et al. (LIGO Scientific Collaboration and Virgo Collaboration) (2017). "GW170814: A three-detector observation of gravitational waves from a binary black hole coalescence". Phys. Rev. Lett. 119 (14): 141101. arXiv:1709.09660. Bibcode:2017PhRvL.119n1101A. doi:10.1103/PhysRevLett.119.141101. Lay summary (PDF).
  3. ↑ Update on Gravitational Wave Science from the LIGO-Virgo Scientific Collaborations (Video of the press conference), retrieved 27 September 2017
  4. ↑ New detectors reveal a cosmic calamity. Don Lincoln, CNN News, 1 October 2017
  5. ↑ "European detector spots its first gravitational wave". Elizabeth Gibney & Davide Castelvecchi. Nature. 27 September 2017. Retrieved 27 September 2017.
This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.