Theia 4310
0.00
UTI
0.33
CN
1.0
Cdens
0.5
CC3
0.25
Clit
0.0
Cdup
Radius (P>50% members)
6.1 [arcmin]
- CN 0.33 Poorly populated
- Cdens 1.0 Very dense
- CC3 0.5 Intermediate quality
- Clit 0.25 Poorly studied
- Cdup 0.0 Very likely duplicate
Overview
Theia 4310 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a relatively close distance, near 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.
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 | 0.547 | 63.549 | 0.891 | -2.607 | -1.417 | -43.299 |
| Hu & Soubiran | 2025 | 0.489 | 63.575 | â | â | â | â |
| Hunt & Reffert | 2024 | 0.425 | 63.533 | 0.89 | -2.576 | -1.419 | -45.674 |
| Cavallo et al. | 2024 | 0.489 | 63.576 | 0.892 | â | â | â |
| Hunt & Reffert | 2023 | 0.425 | 63.533 | 0.89 | -2.576 | -1.419 | -45.674 |
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 | -0.120* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 136* | â | â |
| Cavallo et al. | 2024 | 1.09 | 1.36 | â | 794 | 0.310 | â | â | â |
| Hunt & Reffert | 2023 | 1.07 | 1.30 | 0.95 | 441 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.