Theia 13
0.00
UTI
0.74
CN
1.0
Cdens
1.0
CC3
0.3
Clit
0.0
Cdup
Stellar density (N50/rad)
34.2 [N/pc2]
- CN 0.74 Moderately populated
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.3 Poorly studied
- Cdup 0.0 Very likely duplicate
Overview
Theia 13 is a moderately populated, very dense object of very high 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, very young cluster, but with a large variance across recent sources for the absorption parameter (see Parameters). It was recently reported in the literature.
â ī¸ Warning: This is very likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 83.138 | -1.758 | 2.404 | 0.076 | -0.219 | 25.773 |
| Liu et al. | 2025 | 83.13 | -1.75 | 2.41 | 0.1 | -0.22 | 25.83 |
| Zhang et al. | 2024 | 83.132 | -1.753 | â | â | â | â |
| Hunt & Reffert | 2024 | 83.132 | -1.753 | 2.41 | 0.104 | -0.222 | 25.828 |
| Cavallo et al. | 2024 | 83.197 | -1.691 | 2.409 | â | â | â |
| Hunt & Reffert | 2023 | 83.132 | -1.753 | 2.41 | 0.104 | -0.222 | 25.828 |
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 | 0.41 | 0.3 | 0.98 | 6 | -0.057 | 201 | â | â |
| Liu et al. | 2025 | 0.43 | 0.09 | â | 13 | â | â | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.003(1) | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 201(1) | â | â |
| Cavallo et al. | 2024 | 0.41 | 0.85 | â | 5 | -0.110 | â | â | â |
| Hunt & Reffert | 2023 | 0.40 | 0.30 | 0.98 | 6 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Liu et al. (2025)
Classified as primordial binary cluster 4 along with ASCC_18, and as primordial binary cluster 321 along with OCSN_65, and as primordial binary cluster 337 along with Sigma_Orionis, and of multiple system 3 along with ASCC_18, Sigma_Orionis, OCSN_65 and CWNU_1054.
Palma et al. (2025)
Part of multiple system G229, along with OCSN_56, OCSN_65, CWNU_1072, Sigma_Orionis, CWNU_1088, ASCC_18 and OCSN_68.
Cavallo et al. (2024)
Gold sample.