Theia 502
0.11
UTI
0.0
CN
0.18
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members)
19.3 [arcmin]
- CN 0.0 Sparse
- Cdens 0.18 Very loose
- CC3 0.38 Low quality
- Clit 0.0 Rarely studied
- Cdup 1.0 Unique
Overview
Theia 502 is a sparse, very loose object of low C3 quality. Its parallax locates it at a close 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: 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.
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 | 219.453 | -59.988 | 1.103 | -3.493 | -4.649 | -6.846 |
| Hu & Soubiran | 2025 | 219.525 | -59.994 | â | â | â | â |
| Cavallo et al. | 2024 | 219.525 | -59.994 | 1.111 | â | â | â |
| Hunt & Reffert | 2023 | 219.186 | -60.028 | 1.103 | -3.508 | -4.615 | -27.866 |
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 |
| Cavallo et al. | 2024 | 0.85 | 0.37 | â | 955 | 0.720 | â | â | â |
| Hunt & Reffert | 2023 | 0.87 | 0.81 | 0.41 | 475 | 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.