HSC 1892
0.21
UTI
0.33
CN
0.23
Cdens
0.38
CC3
0.06
Clit
1.0
Cdup
Nm (P>50%)
33
Core radius and density
1.1 [pc], 1.2 [pc-2]
- CN 0.33 Poorly populated
- Cdens 0.23 Very loose
- CC3 0.38 Low quality
- Clit 0.06 Rarely studied
- Cdup 1.0 Unique
Overview
HSC 1892 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate 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.
Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.
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.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 110.611 | -23.621 | 0.221 | -1.99 | 2.458 | 105.692 |
| Hu & Soubiran | 2025 | 110.624 | -23.627 | â | â | â | â |
| Hunt & Reffert | 2024 | 110.633 | -23.627 | 0.219 | -1.986 | 2.458 | 105.663 |
| Cavallo et al. | 2024 | 110.624 | -23.627 | 0.222 | â | â | â |
| Hunt & Reffert | 2023 | 110.633 | -23.627 | 0.219 | -1.986 | 2.458 | 105.663 |
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 | 3.95 | 2.24 | 1.84 | 467 | 0.005 | 331 | â | â |
| Hu & Soubiran | 2025 | â | â | â | â | -0.260(5) | â | â | â |
| Hunt & Reffert | 2024 | 3.95 | 2.24 | 1.84 | 467 | â | 331(1) | â | â |
| Cavallo et al. | 2024 | 3.25 | 2.25 | â | 1288 | 0.270 | â | â | â |
| Hunt & Reffert | 2023 | 3.95 | 2.24 | 1.84 | 467 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.16 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.16 (50th percentile).