Theia 139
0.21
UTI
0.31
CN
0.19
Cdens
0.38
CC3
0.1
Clit
1.0
Cdup
Nm (P>50%)
31
Core radius and density
1.6 [pc], 0.9 [pc-2]
- CN 0.31 Poorly populated
- Cdens 0.19 Very loose
- CC3 0.38 Low quality
- Clit 0.1 Rarely studied
- Cdup 1.0 Unique
Overview
Theia 139 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a very close distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is rarely studied 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.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 82.511 | -2.114 | 3.114 | -2.783 | -4.261 | 14.731 |
| Yang et al. | 2025 | 82.51 | -2.11 | â | â | â | â |
| Zhang et al. | 2024 | 82.51 | -2.11 | â | â | â | â |
| Cavallo et al. | 2024 | 83.403 | -1.296 | 3.056 | â | â | â |
| Hunt & Reffert | 2023 | 82.51 | -2.11 | 3.054 | -2.902 | -4.27 | 16.194 |
| Kounkel & Covey | 2019 | 82.658 | -0.662 | 2.514 | â | â | 1.136 |
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 | 0.34 | 0.41 | 0.88 | 74 | 0.020 | â | â | â |
| Yang et al. | 2025 | â | â | â | 96 | -0.050(3) | â | â | â |
| Zhang et al. | 2024 | â | â | â | â | 0.037(1) | â | â | â |
| Cavallo et al. | 2024 | 0.34 | 0.46 | â | 35 | 0.020 | â | â | â |
| Hunt & Reffert | 2023 | 0.32 | 0.18 | 0.88 | 95 | â | â | â | â |
| Kounkel & Covey | 2019 | 0.44 | 0.41 | â | 52 | 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 P607, along with OCSN_64.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as moving group. CMD class: 0.98 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.98 (50th percentile).