Theia 710
0.09
UTI
0.26
CN
0.06
Cdens
0.12
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members)
81.4 [arcmin]
- CN 0.26 Poorly populated
- Cdens 0.06 Very loose
- CC3 0.12 Very low quality
- Clit 0.0 Rarely studied
- Cdup 1.0 Unique
Overview
Theia 710 is a poorly populated, very loose object of very low C3 quality. Its parallax locates it at a very close distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, old 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: 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.
Very close
Low extinction
Near-solar metallicity
Old
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 339.843 | 64.112 | 2.508 | 7.12 | -4.65 | -10.257 |
| Hu & Soubiran | 2025 | 339.908 | 64.174 | â | â | â | â |
| Cavallo et al. | 2024 | 339.908 | 64.174 | 2.489 | â | â | â |
| Hunt & Reffert | 2023 | 339.21 | 63.568 | 2.472 | 7.103 | -4.654 | -10.016 |
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 | -0.220* | â | â | â |
| Cavallo et al. | 2024 | 0.42 | 0.81 | â | 3020 | 0.610 | â | â | â |
| Hunt & Reffert | 2023 | 0.39 | 0.50 | 0.78 | 1023 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as a moving group.