Theia 1424
0.03
UTI
0.25
CN
0.28
Cdens
0.62
CC3
0.31
Clit
0.08
Cdup
Radius (P>50% members)
10.1 [arcmin]
- CN 0.25 Poorly populated
- Cdens 0.28 Loose
- CC3 0.62 Intermediate quality
- Clit 0.31 Poorly studied
- Cdup 0.08 Very likely duplicate
Overview
Theia 1424 is a poorly populated, loose object of intermediate C3 quality. Its parallax locates it at a relatively close distance, above 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 | 81.195 | 38.242 | 0.701 | 2.332 | -5.825 | -9.953 |
| Hu & Soubiran | 2025 | 81.235 | 38.242 | â | â | â | â |
| Zhang et al. | 2024 | 81.155 | 38.246 | â | â | â | â |
| Hunt & Reffert | 2024 | 81.155 | 38.246 | 0.693 | 2.316 | -5.81 | -5.013 |
| Cavallo et al. | 2024 | 81.235 | 38.242 | 0.696 | â | â | â |
| Hunt & Reffert | 2023 | 81.155 | 38.246 | 0.693 | 2.316 | -5.81 | -5.013 |
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 | -0.130* | â | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.041* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 65* | â | â |
| Cavallo et al. | 2024 | 1.38 | 0.68 | â | 513 | 0.590 | â | â | â |
| Hunt & Reffert | 2023 | 1.35 | 0.86 | 1.66 | 395 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.