HSC 1077
Summary
HSC 1077 is a poorly populated, very loose object of very low C3 quality. It is located at a very close distance from the Sun, above the mid-plane. It was recently reported in the literature.
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) | 179.221 | 64.358 | 10.523 | -69.191 | -10.867 | -3.663 |
| Cavallo et al. (2024) | 174.578 | 63.959 | 10.577 | – | – | – |
| Hu & Soubiran (2025) | 174.578 | 63.959 | – | – | – | – |
| UCC | 178.238 | 64.164 | 10.124 | -69.376 | -10.676 | -0.961 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=0.618, diffAV50=0.442, MOD50=4.933, logAge50=9.584 |
| Cavallo et al. (2024) | AV50=0.79, dMod50=4.97, logAge50=9.25, [Fe/H]50=0.25 |
| Hu & Soubiran (2025) | MA23f=-0.49 |
Search coordinates in Bayestar19
