Theia 23
0.00
UTI
0.76
CN
1.0
Cdens
1.0
CC3
0.25
Clit
0.0
Cdup
Stellar density (N50/rad)
19.2 [N/pc2]
- CN 0.76 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.25 Poorly studied
- Cdup 0.0 Very likely duplicate
Overview
Theia 23 is a rich, very dense object of very high C3 quality. Its parallax locates it at a very close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, 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 | 277.896 | -3.947 | 2.605 | 2.077 | -8.995 | -8.258 |
| Hunt & Reffert | 2024 | 277.938 | -3.925 | 2.601 | 2.068 | -9.001 | -9.59 |
| Cavallo et al. | 2024 | 277.92 | -3.922 | 2.61 | â | â | â |
| Hunt & Reffert | 2023 | 277.938 | -3.925 | 2.601 | 2.068 | -9.001 | -9.59 |
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 | 0.39 | 2.53 | 2.45 | 21 | 0.240 | 205 | â | â |
| Liu et al. | 2025 | 0.41 | 0.48 | â | 72 | â | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 205(1) | â | â |
| Cavallo et al. | 2024 | 0.39 | 2.53 | â | 15 | 0.240 | â | â | â |
| Hunt & Reffert | 2023 | 0.37 | 2.75 | 2.45 | 21 | 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 tidal capture (resonant trapping binary) 165 along with HSC_238.
Palma et al. (2025)
Classified as tidal capture (resonant trapping pair) P40, along with HSC_238.
Cavallo et al. (2024)
Gold sample.