UPK 540
(OCSN 313)
0.74
UTI
0.75
CN
0.63
Cdens
1.0
CC3
0.65
Clit
1.0
Cdup
Radius (P>50% members)
53.9 [arcmin]
- CN 0.75 Rich
- Cdens 0.63 Moderately dense
- CC3 1.0 Very high quality
- Clit 0.65 Moderately studied
- Cdup 1.0 Unique
Overview
UPK 540 is a rich, moderately dense object of very high C3 quality. Its parallax locates it at a very close distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is moderately studied in the literature.
Note: This object shares a very small percentage of members with a later reported entry. See table with shared members information.
Very close
Low extinction
Near-solar metallicity
Young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 114.668 | -58.722 | 2.727 | -4.857 | 7.754 | 6.804 |
| Li et al. | 2025 | 114.567 | -58.609 | 2.688 | -4.827 | 7.67 | â |
| Almeida et al. | 2025 | 114.535 | -58.435 | â | â | â | â |
| Alfonso et al. | 2024 | 114.649 | -58.711 | 2.71 | -4.81 | 7.77 | â |
| Cavallo et al. | 2024 | 114.839 | -58.81 | 2.719 | â | â | â |
| Hunt & Reffert | 2023 | 115.516 | -58.662 | 2.718 | -4.841 | 7.689 | 7.935 |
| Qin et al. | 2023 | 115.07 | -58.65 | 2.71 | -4.8 | 7.71 | 6.71 |
| He et al. | 2022 | 114.801 | -58.752 | 2.743 | -4.769 | 7.759 | â |
| Dias et al. | 2021 | 114.535 | -58.435 | 2.663 | -4.815 | 7.661 | 14.456 |
| Cantat-Gaudin et al. | 2020 | 114.567 | -58.609 | 2.688 | -4.827 | 7.67 | â |
| Cantat-Gaudin & Anders | 2020 | 114.614 | -58.613 | 2.693 | -4.921 | 7.663 | â |
| Sim et al. | 2019 | 114.693 | -58.54 | â | -4.82 | 7.66 | 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 | 0.36 | 0.44 | â | 29 | 0.049 | â | â | â |
| Almeida et al. | 2025 | 0.36 | 0.45 | â | 33 | â | 55 | â | â |
| Alfonso et al. | 2024 | 0.36 | 0.32 | â | 31 | -0.008 | â | â | â |
| Cavallo et al. | 2024 | 0.38 | 0.68 | â | 9 | -0.250 | â | â | â |
| Hunt & Reffert | 2023 | 0.36 | 0.25 | 0.47 | 20 | â | â | â | â |
| Qin et al. | 2023 | 0.43 | 0.43 | â | 28 | â | â | â | â |
| He et al. | 2022 | â | 0.50 | â | 28 | â | â | â | â |
| Dias et al. | 2021 | 0.36 | 0.45 | â | 33 | -0.008 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.36 | 0.32 | â | 37 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.37 | â | â | â | â | â | â | â |
| Sim et al. | 2019 | 0.37 | â | â | 32 | â | â | â | â |


Almeida et al. (2025)
Mass determination: good fit. Isochrone match: good fit.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as a moving group.