NGC 4993 | |
---|---|
Observation data (J2000 epoch) | |
Constellation | Hydra |
Right ascension | 13h 09m 47.7s[2] |
Declination | −23° 23′ 02″[2] |
Redshift | 0.009727[2] |
Heliocentric radial velocity | 2916 km/s[2] |
Distance | 44.1 Mpc (144 Mly)[2] |
Group or cluster | NGC 4993 Group[3] |
Apparent magnitude (V) | 13.32[2] |
Characteristics | |
Type | (R')SAB0^-(rs)[2] |
Size | ~55,000 ly (17 kpc) (estimated)[2] |
Apparent size (V) | 1.3 x 1.1[2] |
Notable features | Host of neutron star merger detected as gravitational wave GW170817 and gamma-ray burst GRB 170817A |
Other designations | |
NGC 4994, ESO 508-18, AM 1307-230, MCG -4-31-39, PGC 45657, WH III 766[4] |
NGC 4993 (also catalogued as NGC 4994 in the New General Catalogue) is a lenticular galaxy[5] located about 140 million light-years away[2] in the constellation Hydra.[6] It was discovered on 26 March 1789[7] by William Herschel[6][7] and is a member of the NGC 4993 Group.[3]
NGC 4993 was the site of GW170817, a collision of two neutron stars, the first astronomical event detected in both electromagnetic and gravitational radiation, a discovery given the Breakthrough of the Year award for 2017 by the journal Science.[8][9] Detecting a gravitational wave event associated with the gamma-ray burst provided direct confirmation that binary neutron star collisions produce short gamma-ray bursts.[10]
NASA-20171016a
was invoked but never defined (see the help page).:2
was invoked but never defined (see the help page).