Theia 117
0.00
UTI
0.49
CN
0.69
Cdens
1.0
CC3
0.08
Clit
0.0
Cdup
Stellar density (N50/rad)
3.5 [N/pc2]
- CN 0.49 Poorly populated
- Cdens 0.69 Moderately dense
- CC3 1.0 Very high quality
- Clit 0.08 Rarely studied
- Cdup 0.0 Very likely duplicate
Overview
Theia 117 is a poorly populated, moderately dense object of very high C3 quality. Its parallax locates it at a very close distance, near 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: 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 | 340.808 | 53.942 | 4.322 | 12.328 | -1.627 | -4.293 |
| Liu et al. | 2025 | 341.12 | 53.92 | 4.32 | 12.28 | -1.53 | -8.62 |
| Cavallo et al. | 2024 | 340.524 | 54.165 | 4.312 | â | â | â |
| Hunt & Reffert | 2023 | 341.115 | 53.925 | 4.32 | 12.282 | -1.528 | -8.619 |
| Kounkel & Covey | 2019 | 340.434 | 53.97 | 4.187 | â | â | 4.259 |
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 | 0.24 | 0.3 | 0.45 | 55 | 0.260 | â | â | â |
| Liu et al. | 2025 | 0.27 | 0.12 | â | 55 | â | â | â | â |
| Cavallo et al. | 2024 | 0.24 | 0.72 | â | 55 | 0.260 | â | â | â |
| Hunt & Reffert | 2023 | 0.23 | 0.18 | 0.45 | 89 | â | â | â | â |
| Kounkel & Covey | 2019 | 0.24 | 0.42 | â | 43 | â | â | â | â |
MOCA


Liu et al. (2025)
Classified as primordial binary cluster 1 along with ADS_16795, and as primordial binary cluster 134 along with Delta_Cephei_Cluster, and of multiple system 4 along with ADS_16795 and Delta_Cephei_Cluster.
Palma et al. (2025)
Part of multiple system G69, along with ADS_16795 and Delta_Cephei_Cluster.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as moving group. CMD class: 1.00 (50th percentile).