UPK 24
(OCSN 290)
0.45
UTI
0.34
CN
0.13
Cdens
0.38
CC3
0.7
Clit
1.0
Cdup
Radius (P>50% members)
48.2 [arcmin]
- CN 0.34 Poorly populated
- Cdens 0.13 Very loose
- CC3 0.38 Low quality
- Clit 0.7 Moderately studied
- Cdup 1.0 Unique
Overview
UPK 24 is a poorly populated, very loose object of low 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.
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 | 282.717 | -10.717 | 1.963 | -3.774 | -9.906 | -0.328 |
| Li et al. | 2025 | 282.646 | -10.788 | 1.945 | -3.751 | -9.838 | â |
| Almeida et al. | 2025 | 282.565 | -10.897 | â | â | â | â |
| Alfonso et al. | 2024 | 282.815 | -10.846 | 1.921 | -3.779 | -9.817 | â |
| Cavallo et al. | 2024 | 282.604 | -10.899 | 1.979 | â | â | â |
| Hunt & Reffert | 2023 | 281.879 | -11.701 | 1.979 | -3.798 | -9.855 | 2.281 |
| Almeida et al. | 2023 | 282.549 | -10.823 | â | â | â | â |
| Qin et al. | 2023 | 282.79 | -10.62 | 1.97 | -3.76 | -9.91 | -0.63 |
| Tarricq et al. | 2022 | 282.892 | -12.085 | 1.964 | -3.776 | -9.811 | â |
| Dias et al. | 2021 | 282.565 | -10.897 | 1.959 | -3.764 | -9.776 | -0.798 |
| Cantat-Gaudin et al. | 2020 | 282.646 | -10.788 | 1.945 | -3.751 | -9.838 | â |
| Cantat-Gaudin & Anders | 2020 | 282.673 | -10.728 | 1.963 | -3.755 | -9.775 | â |
| Sim et al. | 2019 | 282.728 | -10.697 | â | -3.75 | -9.79 | 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 | 0.90 | â | 841 | -0.035 | â | â | â |
| Almeida et al. | 2025 | 0.50 | 1.12 | â | 1038 | â | 112 | â | â |
| Alfonso et al. | 2024 | 0.50 | 0.95 | â | 212 | -0.007 | â | â | â |
| Cavallo et al. | 2024 | 0.52 | 1.56 | â | 380 | 0.120 | â | â | â |
| Hunt & Reffert | 2023 | 0.48 | 1.36 | 2.11 | 471 | â | â | â | â |
| Almeida et al. | 2023 | 0.50 | 1.35 | â | 545 | -0.373 | 105* | 0.88 | â |
| Qin et al. | 2023 | 0.79 | 1.12 | â | 1122 | â | â | â | â |
| Tarricq et al. | 2022 | 0.50 | â | â | 282 | â | â | â | â |
| Dias et al. | 2021 | 0.50 | 1.12 | â | 1038 | -0.007 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.50 | 0.95 | â | 269 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.50 | â | â | â | â | â | â | â |
| Sim et al. | 2019 | 0.50 | 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: intermediate fit. Isochrone match: good fit. Silver sample.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as a moving group.