UPK 178
0.74
UTI
0.55
CN
1.0
Cdens
0.75
CC3
0.7
Clit
1.0
Cdup
Radius (P>50% members)
6.2 [arcmin]
- CN 0.55 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.7 Moderately studied
- Cdup 1.0 Unique
Overview
UPK 178 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a close distance, above 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 | 334.469 | 60.086 | 1.045 | -4.279 | -3.386 | -24.756 |
| Almeida et al. | 2025 | 334.438 | 60.084 | â | â | â | â |
| Alfonso et al. | 2024 | 334.479 | 60.071 | 1.015 | -4.274 | -3.413 | â |
| Hunt & Reffert | 2024 | 334.45 | 60.08 | 1.048 | -4.288 | -3.394 | -20.199 |
| Cavallo et al. | 2024 | 334.431 | 60.097 | 1.042 | â | â | â |
| Hunt & Reffert | 2023 | 334.45 | 60.08 | 1.048 | -4.288 | -3.394 | -20.199 |
| Almeida et al. | 2023 | 334.45 | 60.071 | â | â | â | â |
| He et al. | 2022 | 334.433 | 60.079 | 1.042 | -4.294 | -3.421 | â |
| Tarricq et al. | 2022 | 334.507 | 60.065 | 1.053 | -4.298 | -3.422 | â |
| Dias et al. | 2021 | 334.438 | 60.084 | 1.04 | -4.314 | -3.372 | â |
| Cantat-Gaudin et al. | 2020 | 334.479 | 60.071 | 1.039 | -4.297 | -3.322 | â |
| Cantat-Gaudin & Anders | 2020 | 334.462 | 60.069 | 1.035 | -4.356 | -3.314 | â |
| Sim et al. | 2019 | 334.458 | 60.077 | â | -4.34 | -3.36 | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Almeida et al. | 2025 | 0.91 | 2.33 | â | 148 | â | 74 | â | â |
| Alfonso et al. | 2024 | 0.96 | 1.80 | â | 225 | 0.019 | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 232* | â | â |
| Cavallo et al. | 2024 | 1.01 | 2.49 | â | 110 | 0.350 | â | â | â |
| Hunt & Reffert | 2023 | 0.92 | 2.42 | 1.30 | 125 | â | â | â | â |
| Almeida et al. | 2023 | 0.92 | 2.27 | â | 151 | 0.120 | 132* | 0.76 | â |
| He et al. | 2022 | â | 2.75 | â | 40 | â | â | â | â |
| Tarricq et al. | 2022 | 0.94 | â | â | 224 | â | â | â | â |
| Dias et al. | 2021 | 0.91 | 2.33 | â | 148 | 0.019 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.96 | 1.80 | â | 204 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.94 | â | â | â | â | â | â | â |
| Sim et al. | 2019 | 0.95 | â | â | 316 | 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.