MACS J1149 Lensed Star 1

MACS J1149 Lensed Star 1

Detection of MACS J1149 Lensed Star 1
A galactic cluster (left) magnified a distant star (now named Icarus) more than 2,000 times, making it visible in 2016 from Earth (lower right), 9.34 billion light-years away—although visible in 2016, the star was not visible in 2011 (upper right).
Observation data
Epoch J2000      Equinox J2000
Constellation Leo
Right ascension 11h 49m 35.59s
Declination 22° 23 47.4
Astrometry
DistanceRedshift of 1.49 yields comoving distances of 14.4 billion ly
Characteristics
Spectral type B
Apparent magnitude (V) ≈28.4 (normally 29.9)
Apparent magnitude (R) ≈28.2 (normally 29.7)
Apparent magnitude (Z) ≈27.9 (normally 29.4)
Apparent magnitude (J) 27.3 (normally 28.8)
Apparent magnitude (H) 27.4 (normally 28.9)
Details
Surface gravity (log g)2 - 4 cgs
Temperature11,000 – 14,000 K
Metallicity≈0.006
Age~8 Myr
Other designations
Icarus, LS1, MACS J1149 LS1, MACS J1149 Lensed Star 1 (LS1), MACS J1149+2223 Lensed Star 1

MACS J1149 Lensed Star 1, also known as Icarus, is a blue supergiant star observed through a gravitational lens. It is the seventh most distant individual star to have been detected so far (after Earendel, Godzilla, Mothra, Quyllur, star-1 and star-2), at approximately 14 billion light-years from Earth (redshift z=1.49; comoving distance of 14.4 billion light-years; lookback time of 9.34 billion years). Light from the star was emitted 4.4 billion years after the Big Bang. According to co-discoverer Patrick Kelly, the star is at least a hundred times more distant than the next-farthest non-supernova star observed, SDSS J1229+1122, and is the first magnified individual star seen.