Theia 1742
0.41
UTI
0.52
CN
0.54
Cdens
0.62
CC3
0.25
Clit
0.94
Cdup
Stellar density (N50/rad)
2.7 [N/pc2]
- CN 0.52 Moderately populated
- Cdens 0.54 Moderately dense
- CC3 0.62 Intermediate quality
- Clit 0.25 Poorly studied
- Cdup 0.94 Very likely unique
Overview
Theia 1742 is a moderately populated, moderately dense object of intermediate C3 quality. Its parallax locates it at a relatively 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 absorption parameter (see Parameters). It was recently reported in the literature.
Note: This is very likely a unique object, which shares a very small 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 | 133.108 | -47.98 | 0.595 | -6.905 | 5.16 | 26.623 |
| Liu et al. | 2025 | 133.11 | -47.93 | 0.59 | -6.83 | 5.15 | 33.3 |
| Hunt & Reffert | 2024 | 133.115 | -47.933 | 0.594 | -6.827 | 5.154 | 33.303 |
| Cavallo et al. | 2024 | 132.819 | -47.887 | 0.598 | â | â | â |
| Hunt & Reffert | 2023 | 133.115 | -47.933 | 0.594 | -6.827 | 5.154 | 33.303 |
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 | 1.78 | 1.32 | 2.54 | 126 | 0.340 | 247 | â | â |
| Liu et al. | 2025 | 1.91 | 0.37 | â | 89 | â | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 247(1) | â | â |
| Cavallo et al. | 2024 | 1.78 | 1.56 | â | 178 | 0.340 | â | â | â |
| Hunt & Reffert | 2023 | 1.60 | 1.32 | 2.54 | 126 | 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 221 along with HSC_2145, and as primordial binary cluster 386 along with UBC_1621, and of multiple system 63 along with UBC_1621 and HSC_2145.
Palma et al. (2025)
Part of multiple system G139, along with HSC_2145 and UBC_1621.
Cavallo et al. (2024)
Gold sample.