Theia 248
0.20
UTI
0.25
CN
0.08
Cdens
0.5
CC3
0.1
Clit
1.0
Cdup
Nm (P>50%)
25
Core radius and density
2.5 [pc], 0.4 [pc-2]
- CN 0.25 Poorly populated
- Cdens 0.08 Very loose
- CC3 0.5 Intermediate quality
- Clit 0.1 Rarely studied
- Cdup 1.0 Unique
Overview
Theia 248 is a poorly populated, very loose object of intermediate 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, intermediate-age cluster (see Parameters). It is rarely studied in the literature.
Note: This object shares a large percentage of members with a later reported entry. 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 | 324.03 | 53.3 | 2.086 | 8.983 | 6.471 | -14.958 |
| Zhang et al. | 2024 | 324.696 | 53.669 | â | â | â | â |
| Cavallo et al. | 2024 | 323.937 | 53.124 | 2.073 | â | â | â |
| Hunt & Reffert | 2023 | 324.696 | 53.669 | 2.077 | 8.837 | 6.29 | -16.834 |
| He et al. | 2022 | 323.597 | 53.179 | 2.079 | 8.729 | 6.471 | â |
| Kounkel & Covey | 2019 | 323.355 | 52.764 | 2.172 | â | â | -5.187 |
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 | 0.46 | 0.78 | 1.35 | 102 | 0.181 | â | â | â |
| Zhang et al. | 2024 | â | â | â | â | 0.182(1) | â | â | â |
| Cavallo et al. | 2024 | 0.49 | 0.95 | â | 120 | 0.180 | â | â | â |
| Hunt & Reffert | 2023 | 0.46 | 0.61 | 1.35 | 112 | â | â | â | â |
| He et al. | 2022 | â | 1.05 | â | 63 | â | â | â | â |
| Kounkel & Covey | 2019 | 0.45 | 0.51 | â | 93 | 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 G239, along with Theia_101, OCSN_28 and OCSN_27.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as moving group. CMD class: 0.97 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.97 (50th percentile).