HSC 2022
0.17
UTI
0.0
CN
0.23
Cdens
0.62
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members)
15.4 [arcmin]
- CN 0.0 Sparse
- Cdens 0.23 Very loose
- CC3 0.62 Intermediate quality
- Clit 0.0 Rarely studied
- Cdup 1.0 Unique
Overview
HSC 2022 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a close distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It was recently reported in the literature.
â ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.
Relatively close
Low extinction
Near-solar metallicity
Intermediate age
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 127.567 | -30.909 | 1.022 | -5.275 | 4.521 | 28.583 |
| Hu & Soubiran | 2025 | 127.611 | -30.948 | â | â | â | â |
| Cavallo et al. | 2024 | 127.611 | -30.948 | 1.03 | â | â | â |
| Hunt & Reffert | 2023 | 127.497 | -30.846 | 1.031 | -5.23 | 4.496 | 26.687 |
đĄ Note: The UCC values are estimated from its identified members.
| Reference | Year | Dist [kpc] | Av [mag] | DAv [mag] | Age [Myr] | [Fe/H] [dex] | Mass [Msun] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Hu & Soubiran | 2025 | â | â | â | â | -0.170* | â | â | â |
| Cavallo et al. | 2024 | 1.07 | 0.80 | â | 575 | -0.490 | â | â | â |
| Hunt & Reffert | 2023 | 0.94 | 0.10 | 0.61 | 959 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as a moving group.