GW170817

E734728

GW170817 is the first observed gravitational-wave signal from a binary neutron star merger, famously accompanied by electromagnetic counterparts across the spectrum.

All labels observed (1)

Label Occurrences
GW170817 canonical 1

How this entity was disambiguated

Statements (50)

Predicate Object
instanceOf astronomical event
binary neutron star merger
gravitational-wave event
announcementDate 2017-10-16
binaryComponentType neutron star
componentMassRange about 1.1 to 1.6 solar masses
detectedBy LIGO NERFINISHED
Virgo NERFINISHED
distanceFromEarth about 130 million light-years
about 40 megaparsecs
enabledMeasurement Hubble constant
eventDate 2017-08-17
gravitationalWaveFrequencyRange about 30 to 3000 hertz
hasDiscoveryMethod electromagnetic observation
gravitational-wave detection
hasElectromagneticCounterpart AT 2017gfo NERFINISHED
GRB 170817A NERFINISHED
X-ray afterglow
infrared transient
kilonova
optical transient
radio afterglow
short gamma-ray burst
hasHostGalaxy NGC 4993 NERFINISHED
hasSignificance first gravitational-wave detection from a binary neutron star merger
first multi-messenger observation combining gravitational waves and light from the same source
hostGalaxyConstellation Hydra NERFINISHED
hostGalaxyType lenticular galaxy
numberOfComponents 2
observedBy Chandra X-ray Observatory NERFINISHED
Fermi Gamma-ray Space Telescope NERFINISHED
Hubble Space Telescope NERFINISHED
INTEGRAL NERFINISHED
many ground-based telescopes worldwide
observedIn X-rays
gamma rays
gravitational waves
infrared
optical
radio
ultraviolet
produced gold
platinum
r-process heavy elements
providedEvidenceFor kilonova emission from r-process nucleosynthesis
origin of short gamma-ray bursts in binary neutron star mergers
signalDuration about 100 seconds
tested general relativity NERFINISHED
totalMass about 2.7 solar masses
usedAs standard siren

How these facts were elicited

Referenced by (1)

Full triples — surface form annotated when it differs from this entity's canonical label.