Theia 2249
0.00
UTI
0.41
CN
0.46
Cdens
0.5
CC3
0.3
Clit
0.0
Cdup
Stellar density (N50/rad)
2.3 [N/pc2]
- CN 0.41 Poorly populated
- Cdens 0.46 Loose
- CC3 0.5 Intermediate quality
- Clit 0.3 Poorly studied
- Cdup 0.0 Very likely duplicate
Overview
Theia 2249 is a poorly populated, loose object of intermediate C3 quality. Its parallax locates it at a moderate distance, near 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 | 94.387 | 14.655 | 0.425 | -0.198 | -1.277 | â |
| Zhang et al. | 2024 | 94.375 | 14.594 | â | â | â | â |
| Hunt & Reffert | 2024 | 94.375 | 14.594 | 0.428 | -0.203 | -1.277 | â |
| Cavallo et al. | 2024 | 94.383 | 14.642 | 0.427 | â | â | â |
| Hunt & Reffert | 2023 | 94.375 | 14.594 | 0.428 | -0.203 | -1.277 | 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 | 2.2 | 0.79 | 0.4 | 309 | 0.264 | 265 | â | â |
| Liu et al. | 2025 | 2.68 | 0.30 | â | 468 | â | â | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.072(1) | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 265(1) | â | â |
| Cavallo et al. | 2024 | 2.20 | 0.79 | â | 309 | 0.600 | â | â | â |
| Hunt & Reffert | 2023 | 2.13 | 0.93 | 0.40 | 188 | 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) 48 along with CWNU_26.
Palma et al. (2025)
Classified as optical pair P360, along with CWNU_26.
Cavallo et al. (2024)
Gold sample.