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
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
GW170817
Artistic concept: two neutron stars merge
Artistic concept: two neutron stars merge
Light curves at various wavelengths of kilonova in NGC 4993
Light curves at various wavelengths of kilonova in NGC 4993
Artist's impression of strontium emerging from a neutron star merger.
Artist's impression of strontium emerging from a neutron star merger.
PIA21423 Surface of TRAPPIST 1f
PIA21423 Surface of TRAPPIST 1f