HSC 1222
Summary
HSC 1222 is a sparse, very loose object of low C3 quality. It is located at a moderate 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) | 62.348 | 46.533 | 0.393 | -1.102 | -0.97 | – |
| Cavallo et al. (2024) | 62.53 | 46.398 | 0.398 | – | – | – |
| Hu & Soubiran (2025) | 62.53 | 46.398 | – | – | – | – |
| UCC | 62.482 | 46.499 | 0.382 | -1.108 | -0.986 | -11.012 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=1.313, diffAV50=0.751, MOD50=11.819, logAge50=9.351 |
| Cavallo et al. (2024) | AV50=2.0, dMod50=12.2, logAge50=8.86, [Fe/H]50=0.07 |
| Hu & Soubiran (2025) | MA22=-0.11, MA23f=-0.36, MF24=-0.25 |
Search coordinates in Bayestar19