UPK 38
0.73
UTI
0.5
CN
1.0
Cdens
0.75
CC3
0.7
Clit
1.0
Cdup
Radius (P>50% members)
6.1 [arcmin]
- CN 0.5 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.7 Moderately studied
- Cdup 1.0 Unique
Overview
UPK 38 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, very young cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is moderately studied in the literature.
Close
Moderate extinction
Near-solar metallicity
Very young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 280.827 | -1.639 | 1.697 | -1.091 | -5.254 | -9.812 |
| Li et al. | 2025 | 280.829 | -1.654 | 1.675 | -1.102 | -5.202 | â |
| Almeida et al. | 2025 | 280.83 | -1.653 | â | â | â | â |
| Alfonso et al. | 2024 | 281.488 | -2.085 | 1.54 | 0.024 | -5.987 | â |
| Celli et al. | 2024 | 280.829 | -1.654 | â | â | â | â |
| Cavallo et al. | 2024 | 280.789 | -1.605 | 1.687 | â | â | â |
| Hunt & Reffert | 2023 | 280.82 | -1.643 | 1.665 | -1.173 | -5.377 | -7.026 |
| Almeida et al. | 2023 | 280.818 | -1.648 | â | â | â | â |
| He et al. | 2022 | 280.839 | -1.647 | 1.706 | -1.073 | -5.333 | â |
| Dias et al. | 2021 | 280.83 | -1.653 | 1.65 | -1.088 | -5.243 | â |
| Cantat-Gaudin et al. | 2020 | 280.829 | -1.654 | 1.675 | -1.102 | -5.202 | â |
| Cantat-Gaudin & Anders | 2020 | 280.829 | -1.654 | 1.676 | -1.179 | -5.134 | â |
| Sim et al. | 2019 | 280.843 | -1.654 | â | -1.11 | -5.27 | 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 | 2.20 | â | 18 | -0.349 | â | â | â |
| Almeida et al. | 2025 | 0.59 | 2.20 | â | 12 | â | 94 | â | â |
| Alfonso et al. | 2024 | 0.60 | 2.09 | â | 14 | -0.025 | â | â | â |
| Celli et al. | 2024 | â | â | â | 14 | â | 58 | â | â |
| Cavallo et al. | 2024 | 0.66 | 2.42 | â | 4 | -0.030 | â | â | â |
| Hunt & Reffert | 2023 | 0.56 | 1.94 | 1.82 | 4 | â | â | â | â |
| Almeida et al. | 2023 | 0.57 | 2.32 | â | 11 | -0.044 | 75* | 0.68 | â |
| He et al. | 2022 | â | 2.35 | â | 6 | â | â | â | â |
| Dias et al. | 2021 | 0.59 | 2.20 | â | 12 | -0.025 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.60 | 2.09 | â | 14 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.59 | â | â | â | â | â | â | â |
| Sim et al. | 2019 | 0.57 | â | â | 3 | 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.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as a moving group.