The entire wiki reimagined as a visual magazine with video discovery · Watch your interests come alive
The entire wiki reimagined as a visual magazine with video discovery · Watch your interests come alive
LIGO
The LIGO Livingston control room as it was during Advanced LIGO's first observing run (O1)
The LIGO Livingston control room as it was during Advanced LIGO's first observing run (O1)
LIGO Hanford Observatory
LIGO Hanford Observatory
LIGO Louisiana Observatory
LIGO Louisiana Observatory
Western leg of LIGO interferometer on Hanford Reservation
Western leg of LIGO interferometer on Hanford Reservation
Aerial view of Virgo
Aerial view of Virgo
Computer simulation of gravitational waves emitted by the orbital decay and merger of two black holes
Computer simulation of gravitational waves emitted by the orbital decay and merger of two black holes
Typical "chirp" of a gravitational-wave signal from the GW170817 event. The x axis represents time, and the y axis the frequency. The frequency increa
Typical "chirp" of a gravitational-wave signal from the GW170817 event. The x axis represents time, and the y axis the frequency. The frequency increase over time is typical of gravitational waves from binary compact objects, and its shape is primarily determined by the objects' mass.
Mirror from the initial Virgo detector, now an exposition model at the Virgo site
Mirror from the initial Virgo detector, now an exposition model at the Virgo site