UPK 53
0.79
UTI
0.79
CN
1.0
Cdens
0.75
CC3
0.7
Clit
1.0
Cdup
Radius (P>50% members)
22.6 [arcmin]
- CN 0.79 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.7 Moderately studied
- Cdup 1.0 Unique
Overview
UPK 53 is a rich, 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 age and metallicity parameters (see Parameters). It is moderately studied in the literature.
Note: This object shares a small percentage of members with 2 later reported entries. See table with shared members information.
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 | 288.52 | 14.369 | 1.682 | 2.454 | 1.021 | -5.703 |
| Li et al. | 2025 | 288.544 | 14.392 | 1.661 | 2.441 | 1.086 | â |
| Almeida et al. | 2025 | 288.576 | 14.414 | â | â | â | â |
| Alfonso et al. | 2024 | 288.48 | 14.33 | 1.642 | 2.409 | 1.012 | â |
| Hunt & Reffert | 2024 | 288.529 | 14.269 | 1.678 | 2.465 | 1.032 | -5.224 |
| Cavallo et al. | 2024 | 288.519 | 14.353 | 1.675 | â | â | â |
| Hunt & Reffert | 2023 | 288.529 | 14.269 | 1.678 | 2.465 | 1.032 | -5.224 |
| He et al. | 2022 | 288.575 | 14.434 | 1.679 | 2.467 | 1.03 | â |
| Tarricq et al. | 2022 | 288.508 | 14.273 | 1.687 | 2.45 | 1.038 | â |
| Dias et al. | 2021 | 288.576 | 14.414 | 1.665 | 2.457 | 1.07 | -4.203 |
| Cantat-Gaudin et al. | 2020 | 288.544 | 14.392 | 1.661 | 2.441 | 1.086 | â |
| Cantat-Gaudin & Anders | 2020 | 288.553 | 14.396 | 1.659 | 2.449 | 1.084 | â |
| Sim et al. | 2019 | 288.59 | 14.388 | â | 2.44 | 1.08 | 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 | 0.48 | 1.22 | â | 605 | -0.338 | â | â | â |
| Almeida et al. | 2025 | 0.58 | 1.39 | â | 194 | â | 245 | â | â |
| Alfonso et al. | 2024 | 0.62 | 0.98 | â | 486 | 0.119 | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 434* | â | â |
| Cavallo et al. | 2024 | 0.60 | 1.37 | â | 214 | 0.300 | â | â | â |
| Hunt & Reffert | 2023 | 0.56 | 1.31 | 1.28 | 188 | â | â | â | â |
| He et al. | 2022 | â | 1.55 | â | 71 | â | â | â | â |
| Tarricq et al. | 2022 | 0.61 | â | â | 490 | â | â | â | â |
| Dias et al. | 2021 | 0.58 | 1.39 | â | 194 | 0.119 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.62 | 0.98 | â | 457 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.59 | â | â | â | â | â | â | â |
| Sim et al. | 2019 | 0.59 | â | â | 794 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


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