Theia 651
0.22
UTI
0.0
CN
0.22
Cdens
0.75
CC3
0.06
Clit
1.0
Cdup
Nm (P>50%)
24
Core radius and density
1.5 [pc], 1.1 [pc-2]
- CN 0.0 Sparse
- Cdens 0.22 Very loose
- CC3 0.75 High quality
- Clit 0.06 Rarely studied
- Cdup 1.0 Unique
Overview
Theia 651 is a sparse, very loose object of high C3 quality. Its parallax locates it at a 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 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 | 130.945 | -30.721 | 1.361 | -2.537 | -0.606 | 3.222 |
| Hu & Soubiran | 2025 | 130.833 | -30.747 | â | â | â | â |
| Cavallo et al. | 2024 | 130.833 | -30.747 | 1.36 | â | â | â |
| Hunt & Reffert | 2023 | 130.957 | -30.737 | 1.356 | -2.59 | -0.554 | 3.95 |
| Kounkel & Covey | 2019 | 131.321 | -31.41 | 1.467 | â | â | -3.803 |
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 | 0.69 | 0.19 | 0.3 | 575 | -0.065 | â | â | â |
| Hu & Soubiran | 2025 | â | â | â | â | -0.270(5) | â | â | â |
| Cavallo et al. | 2024 | 0.69 | 0.19 | â | 575 | 0.140 | â | â | â |
| Hunt & Reffert | 2023 | 0.69 | 0.09 | 0.30 | 689 | â | â | â | â |
| Kounkel & Covey | 2019 | 0.68 | 0.27 | â | 282 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Palma et al. (2025)
Classified as optical pair P373, along with CWNU_384.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as moving group. CMD class: 0.99 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.99 (50th percentile).