Pōniuāʻena
Third most distant quasar known with a redshift of 7.52 / From Wikipedia, the free encyclopedia
Pōniuāʻena (/ˌpoʊniuːɑːˈɛnə/), also named J100758.264+211529.207 or J1007+2115, is the third most-distant quasar known, with a measured redshift of z = 7.515 or a lookback time of 13.02 billion years.[2] Its 1.5 billion–solar mass black hole is the most distant known black hole with a mass of over one billion solar masses, and models indicate that it must have formed not later than 100 million years after the Big Bang, before reionization.[3] Its discovery was announced in June 2020.[4] Only the quasars ULAS J1342+0928 (z = 7.54) and J0313–1806 (z = 7.64) are known to be more distant.[3][5]
Pōniuāʻena J1007+2115 | |
---|---|
Observation data (Epoch J2000.0) | |
Constellation | Leo |
Right ascension | 10h 07m 58.264s |
Declination | +21° 15′ 29.207″ |
Redshift | 7.52[1] |
Distance | 1.302×1010 light-years (3.99×109 parsecs) (light-travel distance) |
Other designations | |
J100758.264+211529.207, WISEA J100758.33+211529.4 | |
See also: Quasar, List of quasars |
The quasar was primarily observed at the Mauna Kea Observatories on the island of Hawaiʻi; it was first discovered at the Gemini Observatory and was further identified using data from the W. M. Keck Observatory, UKIRT, Magellan Telescopes, and ALMA.[6] Hawaiian language experts at ʻImiloa Astronomy Center gave it the name Pōniuāʻena [ˌpoːnijuwaːˈʔɛnə], which "evokes the unseen spinning source of creation, surrounded by brilliance."[7]