HSC 969
Summary
HSC 969 is a sparse, very loose object of very 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) | 9.99 | 58.338 | 0.705 | -7.69 | -1.785 | -75.096 |
| Cavallo et al. (2024) | 8.721 | 58.507 | 0.706 | – | – | – |
| Hu & Soubiran (2025) | 8.721 | 58.508 | – | – | – | – |
| UCC | 9.943 | 58.457 | 0.7 | -7.632 | -1.692 | -71.812 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=1.284, diffAV50=2.164, MOD50=10.702, logAge50=9.14 |
| Cavallo et al. (2024) | AV50=0.93, dMod50=10.82, logAge50=9.2, [Fe/H]50=0.28 |
| Hu & Soubiran (2025) | MA22=-0.06, MA23f=-0.16, MA23g=-0.24, MZ23=-0.18, MK24=-0.18, MF24=-0.25 |
Search coordinates in Bayestar19