Theia 2018
0.30
UTI
0.39
CN
0.1
Cdens
0.5
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad)
0.5 [N/pc2]
- CN 0.39 Poorly populated
- Cdens 0.1 Very loose
- CC3 0.5 Intermediate quality
- Clit 0.25 Poorly studied
- Cdup 1.0 Unique
Overview
Theia 2018 is a poorly populated, very loose object of intermediate C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a metal-rich, young cluster (see Parameters). It was recently reported in the literature.
Note: This object shares a significant percentage of members with a later reported entry. See table with shared members information.
â ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 116.087 | -26.914 | 0.311 | -1.855 | 2.485 | â |
| Hunt & Reffert | 2024 | 116.087 | -26.871 | 0.319 | -1.839 | 2.476 | â |
| Cavallo et al. | 2024 | 116.074 | -26.898 | 0.319 | â | â | â |
| Hunt & Reffert | 2023 | 116.087 | -26.871 | 0.319 | -1.839 | 2.476 | 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 | 3.6 | 1.06 | 1.0 | 68 | 0.640 | 273 | â | â |
| Liu et al. | 2025 | 4.15 | 0.38 | â | 59 | â | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 273(1) | â | â |
| Cavallo et al. | 2024 | 3.60 | 1.06 | â | 100 | 0.640 | â | â | â |
| Hunt & Reffert | 2023 | 2.80 | 1.12 | 1.00 | 68 | 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) 360 along with UBC_231.
Palma et al. (2025)
Classified as optical pair P573, along with UBC_231.
Cavallo et al. (2024)
Gold sample.