HSC 1438
0.21
UTI
0.41
CN
0.17
Cdens
0.5
CC3
0.25
Clit
0.66
Cdup
Stellar density (N50/rad)
0.9 [N/pc2]
- CN 0.41 Poorly populated
- Cdens 0.17 Very loose
- CC3 0.5 Intermediate quality
- Clit 0.25 Poorly studied
- Cdup 0.66 Likely unique
Overview
HSC 1438 is a poorly populated, very loose object of intermediate C3 quality. Its parallax locates it at a very close distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the absorption parameter (see Parameters). It was recently reported in the literature.
Note: This is likely a unique object, which shares a moderate percentage of members with at least one previously 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 | 57.711 | 9.737 | 6.632 | 24.149 | -23.82 | 16.543 |
| Liu et al. | 2025 | 60.27 | 8.34 | 6.69 | 24.0 | -23.57 | 15.94 |
| Zhang et al. | 2024 | 60.266 | 8.339 | â | â | â | â |
| Cavallo et al. | 2024 | 58.648 | 9.643 | 6.657 | â | â | â |
| Hunt & Reffert | 2023 | 60.266 | 8.339 | 6.69 | 24.0 | -23.566 | 15.942 |
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 | 0.15 | 0.2 | 0.7 | 57 | 0.140 | â | â | â |
| Liu et al. | 2025 | 0.16 | 0.10 | â | 59 | â | â | â | â |
| Zhang et al. | 2024 | â | â | â | â | 0.120(1) | â | â | â |
| Cavallo et al. | 2024 | 0.15 | 0.73 | â | 38 | 0.160 | â | â | â |
| Hunt & Reffert | 2023 | 0.14 | 0.20 | 0.70 | 57 | 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 193 along with HSC_1426, and as tidal capture (resonant trapping binary) 195 along with Theia_66, and of multiple system 35 along with Theia_71, CWNU_1129, Theia_54, HSC_1426 and Theia_66.
Palma et al. (2025)
Part of multiple system G115, along with HSC_1373 and HSC_1426.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as a moving group.