HSC 1417
Summary
HSC 1417 is a sparse, very loose object of very low C3 quality. It is located at a relatively close distance from the Sun, near 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) | 87.347 | 29.711 | 0.758 | -0.843 | -6.887 | 24.0 |
| Cavallo et al. (2024) | 86.88 | 29.749 | 0.758 | – | – | – |
| Hu & Soubiran (2025) | 86.88 | 29.749 | – | – | – | – |
| UCC | 87.287 | 29.712 | 0.777 | -0.866 | -6.852 | -2.306 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=0.917, diffAV50=0.791, MOD50=10.521, logAge50=8.672 |
| Cavallo et al. (2024) | AV50=1.03, dMod50=10.4, logAge50=9.77, [Fe/H]50=-0.23 |
| Hu & Soubiran (2025) | MA22=-0.18, MA23f=-0.25, MZ23=-0.02, MK24=-0.05, MF24=-0.11 |
Search coordinates in Bayestar19