Theia 711
0.13
UTI
0.0
CN
0.06
Cdens
0.38
CC3
0.1
Clit
1.0
Cdup
Nm (P>50%)
22
Core radius and density
2.1 [pc], 0.3 [pc-2]
- CN 0.0 Sparse
- Cdens 0.06 Very loose
- CC3 0.38 Low quality
- Clit 0.1 Rarely studied
- Cdup 1.0 Unique
Overview
Theia 711 is a sparse, very loose object of low 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.
Note: This object shares a significant 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 | 282.208 | -7.559 | 2.296 | 1.128 | -11.4 | -10.747 |
| Swiggum et al. | 2024 | 282.094 | -7.744 | 2.305 | 1.065 | -11.383 | -10.146 |
| Hunt & Reffert | 2024 | 282.094 | -7.744 | 2.305 | 1.065 | -11.383 | -9.119 |
| Cavallo et al. | 2024 | 281.992 | -7.4 | 2.299 | â | â | â |
| Hunt & Reffert | 2023 | 282.094 | -7.744 | 2.305 | 1.065 | -11.383 | -9.119 |
| Kounkel & Covey | 2019 | 282.181 | -7.177 | 2.252 | â | â | 0.169 |
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 | 0.43 | 0.855 | 1.92 | 62 | -0.030 | 154 | â | â |
| Swiggum et al. | 2024 | 0.43 | â | â | 62 | â | 254 | â | â |
| Hunt & Reffert | 2024 | 0.41 | 0.86 | 1.92 | 62 | â | 53(1) | â | â |
| Cavallo et al. | 2024 | 0.45 | 1.43 | â | 30 | -0.030 | â | â | â |
| Hunt & Reffert | 2023 | 0.41 | 0.85 | 1.92 | 62 | â | â | â | â |
| Kounkel & Covey | 2019 | 0.44 | 0.61 | â | 354 | 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 G152, along with HSC_236 and OCSN_6.
Cavallo et al. (2024)
Silver sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.72 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.72 (50th percentile).