HSC 1789
0.15
UTI
0.0
CN
0.14
Cdens
0.5
CC3
0.06
Clit
1.0
Cdup
Nm (P>50%)
21
Core radius and density
2.2 [pc], 0.7 [pc-2]
- CN 0.0 Sparse
- Cdens 0.14 Very loose
- CC3 0.5 Intermediate quality
- Clit 0.06 Rarely studied
- Cdup 1.0 Unique
Overview
HSC 1789 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a large distance, above 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 | 110.085 | -12.137 | 0.197 | -0.946 | 0.636 | 111.348 |
| Hu & Soubiran | 2025 | 110.073 | -12.11 | â | â | â | â |
| Hunt & Reffert | 2024 | 110.082 | -12.129 | 0.194 | -0.911 | 0.659 | 99.163 |
| Cavallo et al. | 2024 | 110.073 | -12.11 | 0.193 | â | â | â |
| Hunt & Reffert | 2023 | 110.082 | -12.129 | 0.194 | -0.911 | 0.659 | 99.163 |
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 | 4.34 | 1.4 | 1.94 | 539 | -0.455 | 251 | â | â |
| Hu & Soubiran | 2025 | â | â | â | â | -0.290(5) | â | â | â |
| Hunt & Reffert | 2024 | 4.34 | 1.40 | 1.94 | 539 | â | 251(1) | â | â |
| Cavallo et al. | 2024 | 3.08 | 2.14 | â | 617 | -0.620 | â | â | â |
| Hunt & Reffert | 2023 | 4.34 | 1.40 | 1.94 | 538 | 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: 0.35 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.35 (50th percentile).