CWNU 2180
0.21
UTI
0.0
CN
0.24
Cdens
0.12
CC3
0.35
Clit
1.0
Cdup
Stellar density (N50/rad)
1.2 [N/pc2]
- CN 0.0 Sparse
- Cdens 0.24 Very loose
- CC3 0.12 Very low quality
- Clit 0.35 Poorly studied
- Cdup 1.0 Unique
Overview
CWNU 2180 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a relatively close distance, near 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.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 83.138 | 30.578 | 0.775 | -1.262 | -4.217 | -21.013 |
| Zhang et al. | 2024 | 83.15 | 30.602 | â | â | â | â |
| Hunt & Reffert | 2024 | 83.15 | 30.602 | 0.773 | -1.22 | -4.235 | -20.94 |
| Cavallo et al. | 2024 | 83.078 | 30.655 | 0.773 | â | â | â |
| Hunt & Reffert | 2023 | 83.15 | 30.602 | 0.773 | -1.22 | -4.235 | -20.94 |
| He et al. | 2023 | 83.117 | 30.565 | 0.777 | -1.264 | -4.225 | â |
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 | 1.335 | 1.795 | 0.64 | 212 | -0.080 | 72 | â | â |
| Liu et al. | 2025 | 3.10 | 0.67 | â | 200 | â | â | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.399(1) | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 72(1) | â | â |
| Cavallo et al. | 2024 | 1.32 | 1.89 | â | 224 | 0.240 | â | â | â |
| Hunt & Reffert | 2023 | 1.26 | 1.70 | 0.64 | 136 | â | â | â | â |
| He et al. | 2023 | 1.35 | 2.00 | â | 251 | 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 tidal capture (resonant trapping binary) 112 along with HSC_1387.
Palma et al. (2025)
Classified as optical pair P343, along with HSC_1387.
Cavallo et al. (2024)
Gold sample.