AT2021ueyLb

AT2021ueyLb
Photometric data and fitted light curve of the event AT2021uey
Discovery
Discovered byMakiko Ban et al.
Discovery dateMarch 28, 2025
Microlensing
Orbital characteristics
4.01+1.68
−1.34
 AU
4170+2910
−1710
 d
StarAT2021ueyL
Physical characteristics
1.22 RJ (estimate)[1]
Mass1.34+0.45
−0.50
 MJ

AT2021ueyLb is an exoplanet orbiting the star AT2021ueyL, located 3392 light-years away from Earth in the constellation Pegasus.[2] The planet was discovered in 2021 using the gravitational microlensing method.[2]

The microlensing event was initially detected by the Gaia space telescope as part of its transient monitoring program. The initial event was given the internal designation Gaia21dnc. Subsequently, ground-based observatories, including the Molėtai Astronomical Observatory in Lithuania and the KMTNet telescope network, joined the observations. Analysis of anomalies in the light curve confirmed the presence of a planetary companion to the lensing star.[2] After thorough verification and data analysis, scientists were finally able to determine that it is a gas giant located at a distance of 3392 light-years, with a mass 1.34 times that of Jupiter.[2] The NASA Exoplanet Archive estimates the planet's radius at 1.22 Rj.[1] It orbits a low-mass M1V type red dwarf star, with a mass of 0.49 Solar masses and an effective temperature of 3680 K.[2] The planet completes one orbit around its star in 4170 days, with a projected distance to the star of 4.01 astronomical units.[2]

It is one of the few planets found by Gaia using microlensing in the galactic halo, rather than its central bulge.[2]

See also

References

  1. 1 2 "AT2021ueyL b - NASA Science". science.nasa.gov. 28 March 2025. Retrieved 2025-06-25.
  2. 1 2 3 4 5 6 7 Ban, M.; et al. (45) (31 March 2025). "AT2021uey: A planetary microlensing event outside the Galactic bulge". Astronomy & Astrophysics. 697: A57. arXiv:2503.22331. Bibcode:2025A&A...697A..57B. doi:10.1051/0004-6361/202554236.