OCSN 89
0.41
UTI
0.7
CN
0.88
Cdens
0.75
CC3
0.25
Clit
0.72
Cdup
Stellar density (N50/rad)
4.4 [N/pc2]
- CN 0.7 Moderately populated
- Cdens 0.88 Dense
- CC3 0.75 High quality
- Clit 0.25 Poorly studied
- Cdup 0.72 Likely unique
Overview
OCSN 89 is a moderately populated, dense object of high C3 quality. Its parallax locates it at a very close distance, near 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 and age parameters (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 | 187.912 | -66.011 | 2.447 | -13.577 | -2.654 | 2.59 |
| Liu et al. | 2025 | 186.45 | -65.88 | 2.41 | -13.75 | -2.68 | 1.39 |
| Cavallo et al. | 2024 | 188.14 | -66.162 | 2.407 | â | â | â |
| Hunt & Reffert | 2023 | 186.45 | -65.883 | 2.41 | -13.751 | -2.685 | 1.392 |
| Qin et al. | 2023 | 188.06 | -66.04 | 2.48 | -13.49 | -2.96 | 3.72 |
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 | 0.485 | 0.87 | 1.62 | 42 | 0.300 | â | â | â |
| Liu et al. | 2025 | 0.55 | 0.26 | â | 47 | â | â | â | â |
| Cavallo et al. | 2024 | 0.42 | 1.01 | â | 22 | 0.300 | â | â | â |
| Hunt & Reffert | 2023 | 0.40 | 0.73 | 1.62 | 37 | â | â | â | â |
| Qin et al. | 2023 | 0.66 | 1.27 | â | 141 | â | â | â | â |
MOCA


Liu et al. (2025)
Classified as primordial binary cluster 323 along with CWNU_1173, and of multiple system 36 along with CWNU_1173 and CWNU_1256.
Palma et al. (2025)
Classified as optical pair P561, along with Theia_246.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as a moving group.