OCSN 54
0.52
UTI
0.57
CN
0.66
Cdens
0.75
CC3
0.3
Clit
1.0
Cdup
Stellar density (N50/rad)
3.3 [N/pc2]
- CN 0.57 Moderately populated
- Cdens 0.66 Moderately dense
- CC3 0.75 High quality
- Clit 0.3 Poorly studied
- Cdup 1.0 Unique
Overview
OCSN 54 is a moderately populated, moderately dense object of high 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 (see Parameters). It was recently reported in the literature.
Note: This object shares a very small percentage of members with at least one entry reported in the same catalogue. 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 | 77.572 | 17.522 | 2.325 | 0.597 | -5.46 | 15.205 |
| Zhang et al. | 2024 | 77.622 | 17.431 | â | â | â | â |
| Cavallo et al. | 2024 | 77.567 | 18.111 | 2.266 | â | â | â |
| Hunt & Reffert | 2023 | 77.622 | 17.431 | 2.267 | 0.632 | -5.448 | 14.302 |
| Qin et al. | 2023 | 77.62 | 17.42 | 2.36 | 0.59 | -5.52 | 12.5 |
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 | 0.535 | 0.715 | 0.66 | 31 | -0.013 | â | â | â |
| Liu et al. | 2025 | 0.60 | 0.27 | â | 30 | â | â | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.095(1) | â | â | â |
| Cavallo et al. | 2024 | 0.49 | 0.98 | â | 9 | 0.070 | â | â | â |
| Hunt & Reffert | 2023 | 0.42 | 0.62 | 0.66 | 35 | â | â | â | â |
| Qin et al. | 2023 | 0.58 | 0.81 | â | 32 | 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 318 along with Theia_818.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as a moving group.