Theia 4725
0.04
UTI
0.3
CN
0.23
Cdens
0.62
CC3
0.03
Clit
0.17
Cdup
Nm (P>50%)
30
Core radius and density
1.8 [pc], 1.1 [pc-2]
- CN 0.3 Poorly populated
- Cdens 0.23 Very loose
- CC3 0.62 Intermediate quality
- Clit 0.03 Rarely studied
- Cdup 0.17 Likely duplicate
Overview
Theia 4725 is a poorly populated, very loose object of intermediate C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.
â ī¸ Warning: This is 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 | 301.609 | 36.418 | 0.339 | -2.542 | -5.103 | â |
| Hunt & Reffert | 2024 | 301.612 | 36.431 | 0.313 | -2.547 | -5.089 | â |
| Cavallo et al. | 2024 | 301.532 | 36.281 | 0.319 | â | â | â |
| Hunt & Reffert | 2023 | 301.612 | 36.431 | 0.313 | -2.547 | -5.089 | 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 | 2.81 | 2.17 | 2.345 | 45 | 0.090 | 234 | â | â |
| Hunt & Reffert | 2024 | 2.81 | 2.17 | 2.34 | 45 | â | 234(1) | â | â |
| Cavallo et al. | 2024 | 2.98 | 2.43 | â | 60 | 0.090 | â | â | â |
| Hunt & Reffert | 2023 | 2.81 | 2.17 | 2.35 | 45 | 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 P510, along with HSC_584.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.54 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.54 (50th percentile).