GW170817

E734728

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

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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

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