Astrophysics (Index)About

Virgo

(Virgo Detector)
(ground-based gravitational-wave detector in Italy)

Virgo is a gravitational-wave detector in Italy, the primary detector of the European Gravitational Observatory (EGO). It is a large laser Michelson interferometer sending two beams back and forth through 3 km vacuum chambers, reflected multiple times to travel 100 km each, designed to detect minute changes in distances due to gravitational waves. It aims at the 10-10000 hertz frequency range, to detect mergers of compact objects.

The detector began operation in 2007 with no detections during its first years. Following an upgrade completed in 2017 (aka Advanced Virgo), it was in operation at the same time as LIGO, resulting (as intended) in two 2017 detections seen by Virgo and both LIGO detectors: GW170814 and GW170817. In the latter, Virgo detected "something" but the detection wasn't clear. Given that these detectors' sensitivity depends upon the direction of the source of the signal, this fact helped localize the source and contributed to its discovery in visible light. Following another upgrade completed in 2019, more than 20 additional candidate GW detections have been reported by both Virgo and LIGO. The next Virgo operating run has been planned to coincide with those of LIGO and KAGRA beginning on May 24, 2023, but Virgo's participation was delayed by equipment problems. Both LIGO and Virgo resumed operation on April 10, 2024, with plans to continue until February 2025.


Virgo is a constellation, which also lends its name to astronomical objects such as the Virgo Cluster.


(observatory,interferometer,gravitational waves,Italy,ground)
Further reading:
https://en.wikipedia.org/wiki/Virgo_interferometer
http://www.virgo-gw.eu/
http://hyperphysics.phy-astr.gsu.edu/hbase/Forces/ligo.html#c3
https://ui.adsabs.harvard.edu/abs/2005CQGra..22S.869A/abstract
https://ui.adsabs.harvard.edu/abs/2013ASPC..467..151D/abstract
https://ui.adsabs.harvard.edu/abs/2018mgm..conf.3183A/abstract
https://ui.adsabs.harvard.edu/abs/2019ehep.confE..33B/abstract

Referenced by pages:
binary black hole (BBH)
black hole merger
BlackGEM
Chinese Pulsar Timing Array (CPTA)
common envelope (CE)
European Gravitational Observatory (EGO)
European Pulsar Timing Array (EPTA)
GEO600
GOTO
gravitational wave (GW)
gravitational wave spectrum
Gravitational Wave Transient Catalog (GWTC)
gravitational-wave detector
GW detection (GW)
GW170817
Indian Pulsar Timing Array (InPTA)
intermediate-mass black hole (IMBH)
International Pulsar Timing Array (IPTA)
KAGRA
LIGO
localization
MeerKAT Pulsar Timing Array (MPTA)
NANOGrav
neutron star merger
neutron-star black-hole merger (NSBH merger)
observatory (obs.)
Parkes Pulsar Timing Array (PPTA)
pulsar timing array (PTA)
TAMA 300

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