Theia 1432
Summary
Theia 1432 is a sparse, very loose object of intermediate C3 quality. It is located at a 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) | 35.673 | 54.257 | 1.429 | -0.476 | 1.117 | 17.13 |
| Cavallo et al. (2024) | 36.32 | 54.108 | 1.435 | – | – | – |
| Hu & Soubiran (2025) | 36.32 | 54.108 | – | – | – | – |
| UCC | 35.944 | 54.163 | 1.449 | -0.487 | 1.155 | 21.053 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=0.201, diffAV50=0.268, MOD50=9.064, logAge50=9.242 |
| Cavallo et al. (2024) | AV50=0.7, dMod50=9.29, logAge50=9.19, [Fe/H]50=-0.13 |
| Hu & Soubiran (2025) | MA22=-0.23, MA23f=-0.18, MA23g=-0.18, MZ23=-0.12, MK24=-0.15, MF24=-0.09 |
Search coordinates in Bayestar19
