UBC 247
0.80
UTI
0.7
CN
1.0
Cdens
1.0
CC3
0.65
Clit
1.0
Cdup
Radius (P>50% members)
7.9 [arcmin]
- CN 0.7 Moderately populated
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.65 Moderately studied
- Cdup 1.0 Unique
Overview
UBC 247 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age and metallicity parameters (see Parameters). It is moderately studied in the literature.
Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.
Relatively close
Moderate extinction
Near-solar metallicity
Intermediate age
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 126.674 | -50.727 | 0.876 | -5.052 | 6.167 | 17.871 |
| Li et al. | 2025 | 126.678 | -50.729 | 0.854 | -5.083 | 6.093 | â |
| Hu & Soubiran | 2025 | 126.633 | -50.686 | â | â | â | â |
| Almeida et al. | 2025 | 126.662 | -50.708 | â | â | â | â |
| Hunt & Reffert | 2024 | 126.734 | -50.75 | 0.88 | -5.05 | 6.167 | 18.232 |
| Cavallo et al. | 2024 | 126.633 | -50.686 | 0.879 | â | â | â |
| Hunt & Reffert | 2023 | 126.734 | -50.75 | 0.88 | -5.05 | 6.167 | 18.232 |
| He et al. | 2022 | 126.688 | -50.721 | 0.877 | -5.046 | 6.176 | â |
| Dias et al. | 2021 | 126.662 | -50.708 | 0.87 | -5.068 | 6.107 | â |
| Cantat-Gaudin et al. | 2020 | 126.678 | -50.729 | 0.854 | -5.083 | 6.093 | â |
| Castro-Ginard et al. | 2020 | 126.662 | -50.713 | 0.865 | -5.08 | 6.107 | 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] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Li et al. | 2025 | 1.06 | 1.08 | â | 209 | -0.026 | â | â | â |
| Hu & Soubiran | 2025 | â | â | â | â | -0.170* | â | â | â |
| Almeida et al. | 2025 | 1.10 | 1.09 | â | 191 | â | 208 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 275* | â | â |
| Cavallo et al. | 2024 | 1.13 | 0.92 | â | 550 | 0.510 | â | â | â |
| Hunt & Reffert | 2023 | 1.08 | 1.01 | 1.57 | 124 | â | â | â | â |
| He et al. | 2022 | â | 1.35 | â | 79 | â | â | â | â |
| Tarricq et al. | 2022 | 1.11 | â | â | 60 | â | â | â | â |
| Dias et al. | 2021 | 1.10 | 1.09 | â | 191 | 0.180 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 1.15 | 0.98 | â | 58 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: good fit.
Cavallo et al. (2024)
Gold sample.