Theia 100
0.39
UTI
0.68
CN
0.06
Cdens
1.0
CC3
0.1
Clit
1.0
Cdup
Nm (P>50%)
87
Core radius and density
5.0 [pc], 0.3 [pc-2]
- CN 0.68 Moderately populated
- Cdens 0.06 Very loose
- CC3 1.0 Very high quality
- Clit 0.1 Rarely studied
- Cdup 1.0 Unique
Overview
Theia 100 is a moderately populated, very loose 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 (see Parameters). It is rarely studied in the literature.
Note: This object shares a significant percentage of members with at least one entry reported in the same catalogue. 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 | 346.904 | 45.932 | 2.036 | -0.806 | -3.026 | -12.975 |
| Zhang et al. | 2024 | 346.888 | 46.068 | â | â | â | â |
| Swiggum et al. | 2024 | 346.888 | 46.068 | 2.066 | -0.826 | -3.143 | -13.615 |
| Cavallo et al. | 2024 | 346.969 | 45.567 | 2.062 | â | â | â |
| Hunt & Reffert | 2023 | 346.888 | 46.068 | 2.066 | -0.826 | -3.143 | -13.655 |
| Kounkel & Covey | 2019 | 347.008 | 45.171 | 2.084 | â | â | -3.826 |
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 | 0.48 | 0.52 | 0.68 | 16 | -0.083 | 195 | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.036(1) | â | â | â |
| Swiggum et al. | 2024 | 0.48 | â | â | 16 | â | 195 | â | â |
| Cavallo et al. | 2024 | 0.50 | 0.74 | â | 7 | -0.130 | â | â | â |
| Hunt & Reffert | 2023 | 0.46 | 0.33 | 0.68 | 16 | â | â | â | â |
| Kounkel & Covey | 2019 | 0.48 | 0.52 | â | 35 | 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)
Part of multiple system G195, along with OCSN_36 and HSC_825.
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).