Theia 569
0.21
UTI
0.0
CN
0.13
Cdens
0.75
CC3
0.1
Clit
1.0
Cdup
Nm (P>50%)
24
Core radius and density
2.1 [pc], 0.6 [pc-2]
- CN 0.0 Sparse
- Cdens 0.13 Very loose
- CC3 0.75 High quality
- Clit 0.1 Rarely studied
- Cdup 1.0 Unique
Overview
Theia 569 is a sparse, very loose object of high C3 quality. Its parallax locates it at a 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 is rarely studied in the literature.
Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.
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.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 72.555 | 44.822 | 1.327 | 2.039 | -6.361 | 3.863 |
| Yang et al. | 2025 | 72.402 | 44.833 | â | â | â | â |
| Zhang et al. | 2024 | 72.402 | 44.833 | â | â | â | â |
| Cavallo et al. | 2024 | 72.558 | 44.692 | 1.328 | â | â | â |
| Hunt & Reffert | 2023 | 72.402 | 44.833 | 1.319 | 2.072 | -6.377 | 0.714 |
| Kounkel & Covey | 2019 | 72.762 | 44.873 | 1.303 | â | â | -12.482 |
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] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999â | 0.75 | 1.06 | 0.61 | 235 | -0.180 | â | â | â |
| Yang et al. | 2025 | â | â | â | 234 | -0.180(3) | â | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.316(1) | â | â | â |
| Cavallo et al. | 2024 | 0.75 | 0.89 | â | 275 | 0.320 | â | â | â |
| Hunt & Reffert | 2023 | 0.70 | 1.06 | 0.61 | 236 | â | â | â | â |
| Kounkel & Covey | 2019 | 0.77 | 1.21 | â | 201 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as moving group. CMD class: 1.00 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 1.00 (50th percentile).