Theia 200
0.18
UTI
0.25
CN
0.02
Cdens
0.5
CC3
0.06
Clit
1.0
Cdup
Nm (P>50%)
25
Core radius and density
3.3 [pc], 0.1 [pc-2]
- CN 0.25 Poorly populated
- Cdens 0.02 Very loose
- CC3 0.5 Intermediate quality
- Clit 0.06 Rarely studied
- Cdup 1.0 Unique
Overview
Theia 200 is a poorly populated, very loose object of intermediate C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is rarely studied in the literature.
Note: This object shares a large percentage of members with 2 later reported entries. See table with shared members information.
â ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 18.877 | 60.756 | 1.155 | 2.947 | -1.691 | -15.76 |
| Hunt & Reffert | 2024 | 18.701 | 60.75 | 1.148 | 2.959 | -1.672 | -14.795 |
| Cavallo et al. | 2024 | 19.113 | 60.914 | 1.148 | â | â | â |
| Hunt & Reffert | 2023 | 18.701 | 60.75 | 1.148 | 2.959 | -1.672 | -14.795 |
| Kounkel & Covey | 2019 | 24.386 | 58.529 | 1.192 | â | â | â |
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 | 0.835 | 0.89 | 0.27 | 155 | 0.270 | 75 | â | â |
| Hunt & Reffert | 2024 | 0.83 | 0.89 | 0.27 | 155 | â | 75(1) | â | â |
| Cavallo et al. | 2024 | 0.89 | 1.07 | â | 214 | 0.270 | â | â | â |
| Hunt & Reffert | 2023 | 0.83 | 0.89 | 0.27 | 155 | â | â | â | â |
| Kounkel & Covey | 2019 | 0.84 | 0.78 | â | 70 | 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)
Classified as optical pair P404, along with HSC_1022.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 1.00 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 1.00 (50th percentile).