UPK 17
0.79
UTI
0.68
CN
1.0
Cdens
0.75
CC3
0.75
Clit
1.0
Cdup
Stellar density (N50/rad)
10.6 [N/pc2]
- CN 0.68 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.75 Well-studied
- Cdup 1.0 Unique
Overview
UPK 17 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 well-studied in the literature.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 279.745 | -15.024 | 1.49 | 0.929 | -7.933 | -23.022 |
| Li et al. | 2025 | 279.741 | -15.034 | 1.479 | 0.894 | -7.856 | â |
| Almeida et al. | 2025 | 279.749 | -15.046 | â | â | â | â |
| Alfonso et al. | 2024 | 279.678 | -15.019 | 1.428 | 0.912 | -7.909 | â |
| Hunt & Reffert | 2024 | 279.716 | -15.042 | 1.481 | 0.96 | -7.891 | -21.111 |
| Cavallo et al. | 2024 | 279.794 | -14.942 | 1.48 | â | â | â |
| Hunt & Reffert | 2023 | 279.716 | -15.042 | 1.481 | 0.96 | -7.891 | -21.111 |
| Almeida et al. | 2023 | 279.745 | -15.036 | â | â | â | â |
| He et al. | 2022 | 279.732 | -15.065 | 1.467 | 0.947 | -7.951 | â |
| Tarricq et al. | 2022 | 279.69 | -15.025 | 1.501 | 0.931 | -7.922 | â |
| Dias et al. | 2021 | 279.749 | -15.046 | 1.483 | 0.904 | -7.855 | â |
| Cantat-Gaudin et al. | 2020 | 279.741 | -15.034 | 1.479 | 0.894 | -7.856 | â |
| Cantat-Gaudin & Anders | 2020 | 279.745 | -15.024 | 1.479 | 0.927 | -7.852 | â |
| Sim et al. | 2019 | 279.739 | -15.056 | â | 0.9 | -7.92 | 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 | 0.66 | 1.63 | 1.66 | 472 | 0.073 | 294 | 0.5 | â |
| Li et al. | 2025 | 0.65 | 1.23 | â | 648 | 0.241 | â | â | â |
| Almeida et al. | 2025 | 0.66 | 1.73 | â | 248 | â | 200 | â | â |
| Alfonso et al. | 2024 | 0.73 | 1.38 | â | 409 | 0.073 | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 321(1) | â | â |
| Cavallo et al. | 2024 | 0.68 | 1.63 | â | 407 | 0.350 | â | â | â |
| Hunt & Reffert | 2023 | 0.64 | 1.68 | 1.66 | 251 | â | â | â | â |
| Almeida et al. | 2023 | 0.66 | 1.72 | â | 472 | -0.060 | 294(1) | 0.50 | â |
| He et al. | 2022 | â | 1.60 | â | 562 | â | â | â | â |
| Tarricq et al. | 2022 | 0.71 | â | â | 550 | â | â | â | â |
| Dias et al. | 2021 | 0.66 | 1.73 | â | 248 | 0.073 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.73 | 1.38 | â | 537 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.66 | â | â | â | â | â | â | â |
| Sim et al. | 2019 | 0.66 | â | â | 794 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


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