Sister_facilities_collage

Top: GEO600 near Hannover, Germany (Harald Lück/AEI). Bottom left: KAGRA cutaway showing the interferometer's location underground (KAGRA). Bottom right: VIRGO in the Italian countryside (EGO).

Our Sister Facilities

LIGO may be the biggest gravitational wave observatory on Earth, but it is not the only one. Since the best way to learn about gravitational waves and their sources is by having many detectors observing simultaneously, LIGO and other observatories plan to share their data. At present, three other gravitational wave observatories are in operation or under construction in other parts of the world. These are LIGO's sister facilities.

Virgo

Sister Facilities Virgo

Aerial view of the Virgo gravitational wave interferometer in Italy (Credit: EGO/Virgo)

Located outside of Pisa, Italy is a 3 km interferometer called Virgo. This detector is funded by the European Gravitational Observatory (EGO) a collaboration between the Italian and French governments. Virgo is undergoing its own upgrades to increase its sensitivity much like the upgrades LIGO has now completed. Virgo expects to begin full-scale operation in 2016.

GEO600

Sister Facilities GEO600

The GEO600 gravitational wave interferometer in Germany (Credit: Harald Lück/AEI)

GEO600 is a 0.6 km (600 m) interferometer located near Hannover, Germany, funded by both the German and British governments. This working gravitational wave detector also serves as a test site to develop advanced interferometer and optical suspension systems for use in future detectors. An agreement between the GEO collaboration and the LIGO Scientific Collaboration ensures the joint analysis of data, and makes all members of the GEO collaboration members of the LIGO Scientific Collaboration (LSC).

KAGRA

Sister Facilities KAGRA Yarm

KAGRA's Y-arm under construction (Credit: KAGRA)

Japan is currently building a 3 km interferometer inside of the Kamioka mine (also home to the Super Kamiokande neutrino detector). Being underground, the detector will be exposed to much less seismic vibration than surface instruments like LIGO, Virgo and GEO600. KAGRA will also use cryogenic systems, meaning that the optics will be cooled to such a degree that molecular vibrations within the material itself will be brought almost to a stop (the key to detecting gravitational waves is to isolate the detector from any and all Earthly vibrations that might mimic or mask a gravitational wave vibration). Full-scale operation of this observatory is expected to commence later in this decade.