HSC 2412
0.40
UTI
0.0
CN
1.0
Cdens
0.38
CC3
0.3
Clit
1.0
Cdup
Stellar density (N50/rad)
5.5 [N/pc2]
- CN 0.0 Sparse
- Cdens 1.0 Very dense
- CC3 0.38 Low quality
- Clit 0.3 Poorly studied
- Cdup 1.0 Unique
Overview
HSC 2412 is a sparse, very dense object of low 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 age and metallicity parameters (see Parameters). It was recently reported in the literature.
Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 170.495 | -58.451 | 1.005 | -11.191 | 1.961 | -4.405 |
| Hu & Soubiran | 2025 | 170.533 | -58.437 | â | â | â | â |
| Hunt & Reffert | 2024 | 170.524 | -58.386 | 0.995 | -11.15 | 1.987 | -6.734 |
| Cavallo et al. | 2024 | 170.533 | -58.437 | 0.999 | â | â | â |
| Hunt & Reffert | 2023 | 170.524 | -58.386 | 0.995 | -11.15 | 1.987 | -6.734 |
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] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999â | 1.03 | 0.12 | 0.6 | 200 | 0.100 | 52 | â | â |
| Liu et al. | 2025 | 1.42 | 0.19 | â | 200 | â | â | â | â |
| Hu & Soubiran | 2025 | â | â | â | â | -0.330(5) | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 52(1) | â | â |
| Cavallo et al. | 2024 | 1.03 | 0.09 | â | 1175 | 0.530 | â | â | â |
| Hunt & Reffert | 2023 | 0.94 | 0.12 | 0.60 | 193 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Liu et al. (2025)
Classified as primordial binary cluster 229 along with HSC_2433.
Palma et al. (2025)
Classified as optical pair P469, along with HSC_2433.
Cavallo et al. (2024)
Gold sample.