Theia 5779
Summary
Theia 5779 is a sparse, very loose object of low C3 quality. It is located at a relatively close distance from the Sun, below the mid-plane. It was recently reported in the literature.
Warning: contains less than 25 stars with P>0.5 estimated.
Warning: the low UTI value and no obvious signs of duplication (C_dup=1.0) indicates that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Hunt & Reffert (2023) | 115.702 | -39.175 | 0.924 | -7.649 | 2.079 | 14.856 |
| Cavallo et al. (2024) | 115.652 | -39.122 | 0.925 | – | – | – |
| Hu & Soubiran (2025) | 115.651 | -39.122 | – | – | – | – |
| UCC | 115.628 | -39.126 | 0.939 | -7.68 | 1.966 | 18.293 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=0.356, diffAV50=1.166, MOD50=10.096, logAge50=9.135 |
| Cavallo et al. (2024) | AV50=0.5, dMod50=10.04, logAge50=9.35, [Fe/H]50=-0.07 |
| Hu & Soubiran (2025) | MA22=-0.22, MA23f=-0.3, MA23g=-0.18, MZ23=-0.32, MK24=-0.17, MF24=-0.24 |
Search coordinates in Bayestar19