Theia 322
Summary
Theia 322 is a sparse, loose object of low C3 quality. It is located at a very 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 |
|---|---|---|---|---|---|---|
| He et al. (2022) | 12.435 | 50.219 | 2.186 | 7.351 | -3.107 | – |
| Hunt & Reffert (2023) | 12.263 | 50.773 | 2.773 | 4.993 | -1.587 | -24.905 |
| Cavallo et al. (2024) | 12.462 | 50.942 | 2.783 | – | – | – |
| UCC | 12.229 | 50.809 | 2.681 | 4.981 | -1.57 | -20.211 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2022) | A0=0.4, logAge=7.9 |
| Hunt & Reffert (2023) | AV50=0.992, diffAV50=0.526, MOD50=7.688, logAge50=6.735 |
| Cavallo et al. (2024) | AV50=1.13, dMod50=7.98, logAge50=7.72, [Fe/H]50=0.53 |
Search coordinates in Bayestar19
