Theia 560
0.13
UTI
0.28
CN
0.03
Cdens
0.12
CC3
0.1
Clit
1.0
Cdup
Nm (P>50%)
28
Core radius and density
3.0 [pc], 0.2 [pc-2]
- CN 0.28 Poorly populated
- Cdens 0.03 Very loose
- CC3 0.12 Very low quality
- Clit 0.1 Rarely studied
- Cdup 1.0 Unique
Overview
Theia 560 is a poorly populated, very loose object of very 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 is rarely studied in the literature.
Note: This object shares a significant 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 | 73.665 | 45.926 | 1.493 | -1.293 | -2.968 | -7.69 |
| Yang et al. | 2025 | 73.595 | 45.869 | â | â | â | â |
| Zhang et al. | 2024 | 73.595 | 45.869 | â | â | â | â |
| Cavallo et al. | 2024 | 73.479 | 46.254 | 1.509 | â | â | â |
| Hunt & Reffert | 2023 | 73.595 | 45.869 | 1.51 | -1.283 | -2.93 | -8.822 |
| Kounkel & Covey | 2019 | 71.866 | 47.072 | 1.432 | â | â | -6.373 |
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 | 0.68 | 0.78 | 0.74 | 213 | -0.130 | â | â | â |
| Yang et al. | 2025 | â | â | â | 214 | -0.130(3) | â | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.144(1) | â | â | â |
| Cavallo et al. | 2024 | 0.68 | 0.82 | â | 407 | 0.530 | â | â | â |
| Hunt & Reffert | 2023 | 0.62 | 0.78 | 0.74 | 212 | â | â | â | â |
| Kounkel & Covey | 2019 | 0.70 | 0.72 | â | 211 | 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).