Theia 2118
0.18
UTI
0.0
CN
0.28
Cdens
0.12
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members)
7.7 [arcmin]
- CN 0.0 Sparse
- Cdens 0.28 Loose
- CC3 0.12 Very low quality
- Clit 0.25 Poorly studied
- Cdup 1.0 Unique
Overview
Theia 2118 is a sparse, loose object of very low C3 quality. Its parallax locates it at a relatively close distance, above 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.
Note: This object shares a small 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.
Relatively close
Moderate extinction
Near-solar metallicity
Intermediate age
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 101.736 | 7.365 | 0.638 | -1.54 | 0.207 | -4.665 |
| Zhang et al. | 2024 | 101.739 | 7.387 | â | â | â | â |
| Hunt & Reffert | 2024 | 101.739 | 7.387 | 0.679 | -1.644 | 0.186 | 48.972 |
| Cavallo et al. | 2024 | 101.113 | 7.793 | 0.678 | â | â | â |
| Hunt & Reffert | 2023 | 101.739 | 7.387 | 0.679 | -1.644 | 0.186 | 48.972 |
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] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Zhang et al. | 2024 | â | â | â | â | -0.184* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 66* | â | â |
| Cavallo et al. | 2024 | 1.67 | 1.25 | â | 123 | 0.400 | â | â | â |
| Hunt & Reffert | 2023 | 1.38 | 1.08 | 2.40 | 157 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.