UPK 131
0.73
UTI
0.52
CN
1.0
Cdens
0.75
CC3
0.7
Clit
1.0
Cdup
Stellar density (N50/rad)
5.1 [N/pc2]
- CN 0.52 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.7 Moderately studied
- Cdup 1.0 Unique
Overview
UPK 131 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a close distance, near 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 metallicity parameter (see Parameters). It is moderately studied in the literature.
Note: This object shares a significant percentage of members with a later 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 | 315.508 | 45.422 | 1.016 | 2.832 | -1.121 | -7.468 |
| Li et al. | 2025 | 315.517 | 45.391 | 1.013 | 2.833 | -1.08 | â |
| Almeida et al. | 2025 | 315.489 | 45.388 | â | â | â | â |
| Alfonso et al. | 2024 | 315.46 | 45.404 | 0.988 | 2.799 | -1.192 | â |
| Zhang et al. | 2024 | 315.477 | 45.448 | â | â | â | â |
| Hunt & Reffert | 2024 | 315.477 | 45.448 | 1.015 | 2.723 | -1.249 | -13.52 |
| Cavallo et al. | 2024 | 315.542 | 45.319 | 1.019 | â | â | â |
| Hunt & Reffert | 2023 | 315.477 | 45.448 | 1.015 | 2.723 | -1.249 | -13.52 |
| He et al. | 2022 | 315.57 | 45.385 | 1.011 | 2.829 | -1.133 | â |
| Tarricq et al. | 2022 | 315.448 | 45.407 | 0.999 | 2.837 | -1.124 | â |
| Dias et al. | 2021 | 315.489 | 45.388 | 1.018 | 2.793 | -1.129 | â |
| Cantat-Gaudin et al. | 2020 | 315.517 | 45.391 | 1.013 | 2.833 | -1.08 | â |
| Cantat-Gaudin & Anders | 2020 | 315.499 | 45.375 | 1.014 | 2.784 | -1.138 | â |
| Sim et al. | 2019 | 315.501 | 45.37 | â | 2.83 | -1.09 | 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 | 0.96 | 1.835 | 1.97 | 463 | 0.011 | 188 | â | â |
| Li et al. | 2025 | 1.06 | 2.11 | â | 465 | 0.054 | â | â | â |
| Almeida et al. | 2025 | 0.96 | 1.84 | â | 461 | â | 162 | â | â |
| Alfonso et al. | 2024 | 0.96 | 1.11 | â | 716 | 0.011 | â | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.014(1) | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 213(1) | â | â |
| Cavallo et al. | 2024 | 0.99 | 1.83 | â | 447 | 0.440 | â | â | â |
| Hunt & Reffert | 2023 | 0.94 | 1.78 | 1.97 | 348 | â | â | â | â |
| He et al. | 2022 | â | 2.00 | â | 447 | â | â | â | â |
| Tarricq et al. | 2022 | 0.94 | â | â | 562 | â | â | â | â |
| Dias et al. | 2021 | 0.96 | 1.84 | â | 461 | 0.011 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.96 | 1.11 | â | 537 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.96 | â | â | â | â | â | â | â |
| Sim et al. | 2019 | 0.98 | â | â | 562 | 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 P518, along with HSC_687.
Cavallo et al. (2024)
Gold sample.
Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: intermediate fit. Silver sample.