Theia 3227
0.02
UTI
0.49
CN
1.0
Cdens
0.5
CC3
0.25
Clit
0.04
Cdup
Radius (P>50% members)
2.3 [arcmin]
- CN 0.49 Poorly populated
- Cdens 1.0 Very dense
- CC3 0.5 Intermediate quality
- Clit 0.25 Poorly studied
- Cdup 0.04 Very likely duplicate
Overview
Theia 3227 is a poorly populated, very dense 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 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.
Distant
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 | 156.331 | -59.084 | 0.27 | -5.746 | 3.884 | 7.174 |
| Hu & Soubiran | 2025 | 156.332 | -59.081 | â | â | â | â |
| Hunt & Reffert | 2024 | 156.339 | -59.08 | 0.261 | -5.762 | 3.885 | -5.967 |
| Cavallo et al. | 2024 | 156.332 | -59.082 | 0.262 | â | â | â |
| Hunt & Reffert | 2023 | 156.339 | -59.08 | 0.261 | -5.762 | 3.885 | -5.967 |
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 |
|---|---|---|---|---|---|---|---|---|---|
| Hu & Soubiran | 2025 | â | â | â | â | -0.350* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 498* | â | â |
| Cavallo et al. | 2024 | 2.87 | 1.47 | â | 1096 | 0.360 | â | â | â |
| Hunt & Reffert | 2023 | 3.68 | 2.11 | 2.25 | 291 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.