Theia 2185
0.01
UTI
0.27
CN
0.23
Cdens
0.38
CC3
0.25
Clit
0.04
Cdup
Stellar density (N50/rad)
1.1 [N/pc2]
- CN 0.27 Poorly populated
- Cdens 0.23 Very loose
- CC3 0.38 Low quality
- Clit 0.25 Poorly studied
- Cdup 0.04 Very likely duplicate
Overview
Theia 2185 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by low 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.
â ī¸ Warning: This is very likely a duplicate object, which shares a large 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 | 160.579 | -57.147 | 0.37 | -8.992 | 2.707 | -18.528 |
| Hu & Soubiran | 2025 | 160.596 | -57.165 | â | â | â | â |
| Hunt & Reffert | 2024 | 160.581 | -57.154 | 0.368 | -9.0 | 2.705 | -14.046 |
| Cavallo et al. | 2024 | 160.596 | -57.165 | 0.37 | â | â | â |
| Hunt & Reffert | 2023 | 160.581 | -57.154 | 0.368 | -9.0 | 2.705 | -14.046 |
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 | 2.41 | 0.8 | 0.95 | 966 | -0.110 | 67 | â | â |
| Hu & Soubiran | 2025 | â | â | â | â | -0.290(5) | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 67(1) | â | â |
| Cavallo et al. | 2024 | 2.37 | 0.95 | â | 1023 | 0.070 | â | â | â |
| Hunt & Reffert | 2023 | 2.45 | 0.65 | 0.95 | 908 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Palma et al. (2025)
Part of multiple system G78, along with LP_403 and HSC_2368.
Cavallo et al. (2024)
Gold sample.