HSC 242
Summary
HSC 242 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) | 247.846 | 9.216 | 8.719 | -6.528 | 14.357 | -26.593 |
| Cavallo et al. (2024) | 250.124 | 10.031 | 8.792 | – | – | – |
| Hu & Soubiran (2025) | 250.125 | 10.031 | – | – | – | – |
| UCC | 251.968 | 11.039 | 8.429 | -5.795 | 14.838 | -39.116 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=0.04, diffAV50=0.284, MOD50=5.355, logAge50=8.074 |
| Cavallo et al. (2024) | AV50=0.64, dMod50=5.35, logAge50=8.77, [Fe/H]50=0.1 |
| Hu & Soubiran (2025) | MA22=-0.32, MA23f=-0.17, MZ23=0.18, MK24=-0.01, MF24=-0.44 |
Search coordinates in Bayestar19
