Theia 5292
0.03
UTI
0.26
CN
0.31
Cdens
0.62
CC3
0.31
Clit
0.08
Cdup
Radius (P>50% members)
13.4 [arcmin]
- CN 0.26 Poorly populated
- Cdens 0.31 Loose
- CC3 0.62 Intermediate quality
- Clit 0.31 Poorly studied
- Cdup 0.08 Very likely duplicate
Overview
Theia 5292 is a poorly populated, loose object of intermediate C3 quality. Its parallax locates it at a relatively close distance, below 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.
Relatively close
Low 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 | 39.998 | 48.794 | 0.951 | 2.62 | -4.822 | -17.069 |
| Hu & Soubiran | 2025 | 40.03 | 48.805 | â | â | â | â |
| Zhang et al. | 2024 | 40.021 | 48.792 | â | â | â | â |
| Hunt & Reffert | 2024 | 40.021 | 48.792 | 0.95 | 2.643 | -4.764 | -14.926 |
| Cavallo et al. | 2024 | 40.03 | 48.805 | 0.95 | â | â | â |
| Hunt & Reffert | 2023 | 40.021 | 48.792 | 0.95 | 2.643 | -4.764 | -14.926 |
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 |
| Zhang et al. | 2024 | â | â | â | â | -0.260* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 101* | â | â |
| Cavallo et al. | 2024 | 1.07 | 0.48 | â | 562 | 0.420 | â | â | â |
| Hunt & Reffert | 2023 | 1.00 | 0.42 | 1.22 | 265 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.