?? GRB, short-duration[1] | |
Date | 1 January 2015[1] 15:23 UT by the Burst Alert Telescope (BAT);[1] 15:23:35 UT by the Gamma-ray Burst Monitor (GBM)[1] |
---|---|
Constellation | Virgo[2][3] |
Right ascension | 12h 32m 04.96s[2] |
Declination | −10° 56′ 00.7″[2] |
Epoch | J2000[1] |
Galactic coordinates | 295.26103 +51.64971 [ 1800 1800 0 ][4] |
Distance | 1.7 billion light-years (0.52 Gpc)[1] z=0.13437;[1] 0.1341[2] |
Redshift | ?? 0.093[4] |
Total energy output | ~1.3 ×1049 ergs[1] |
GRB 150101B is a gamma-ray burst (GRB) that was detected on 1 January 2015 at 15:23 UT by the Burst Alert Telescope (BAT) on board the Swift Observatory Satellite, and at 15:23:35 UT by the Gamma-ray Burst Monitor (GBM) on board the Fermi Gamma-ray Space Telescope.[1] The GRB was determined to be 1.7 billion light-years (0.52 Gpc) from Earth near the host galaxy 2MASX J12320498-1056010 [4] in the constellation Virgo.[2][3] The characteristics of GRB 150101B are remarkably similar to the historic event GW170817, a merger of neutron stars.[2][5][6][7]
HRV-20181016
was invoked but never defined (see the help page).EA-20181016
was invoked but never defined (see the help page).NC-20181016
was invoked but never defined (see the help page).NASA-20181016
was invoked but never defined (see the help page).