J1144–4308
Appearance
Coordinates:
11h 44m 47.77s, −43° 08′ 59.3″

SMSS J114447.77–430859.3 | |
---|---|
Approximate location of SMSS J114447.77–430859.3 in the sky (circled) | |
Observation data (Epoch J2000) | |
Constellation | Centaurus |
Right ascension | 11h 44m 47.76096s[1] |
Declination | −43° 08′ 59.4276″[1] |
Redshift | 0.83[2] |
Other designations | |
2MASS J11444776-4308594[1] | |
See also: Quasar, List of quasars |
SMSS J114447.77–430859.3 or J1144 or J1144–4308 is a very bright (unbeamed)
Southern Cross (Crux). The SkyMapper Southern Survey (SMSS) was used to ascertain its spectral properties.[2]
J1144 was identified during a search for
binary stars.[2][3] Despite being relatively bright, it had escaped classification as a quasar in earlier searches, which avoided the crowded fields near the galactic equator.[4]
After examining various data sets, the study group determined that J1144 is the most intrinsically luminous quasar known over the last ~9 Gyr of cosmic history, having a luminosity 8 times greater than 3C 273 in Virgo.[2]
According to the lead researcher Dr Christofer Onken, of the Australian National University: While black holes are themselves not visible; their gravity is so great that not even light can escape them, they are observable because of the matter that swirls around them.
References
- ^ a b c "SMSS J114447.77-430859.3". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2022-11-03.
- ^ S2CID 249538461.
- ABC News Online, 2022-06-15
- ^ "Fastest-growing black hole of the last 9 billion years". cosmosmagazine.com. 2022-06-15. Retrieved 2022-06-15.