Patchick 90
(SAI 68; MWSC 974; DSH J0644.7-0031)
0.76
UTI
0.59
CN
1.0
Cdens
0.5
CC3
0.86
Clit
1.0
Cdup
Radius (P>50% members)
1.3 [arcmin]
- CN 0.59 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.5 Intermediate quality
- Clit 0.86 Well-studied
- Cdup 1.0 Unique
Overview
Patchick 90 is a moderately populated, very dense object of intermediate C3 quality. Its parallax locates it at a large distance, below 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.
Very distant
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 | 101.18 | -0.526 | 0.169 | -0.188 | 1.076 | 78.12 |
| Hu & Soubiran | 2025 | 101.173 | -0.527 | â | â | â | â |
| Almeida et al. | 2025 | 101.179 | -0.532 | â | â | â | â |
| Hunt & Reffert | 2024 | 101.181 | -0.524 | 0.191 | -0.166 | 1.079 | 78.122 |
| Cavallo et al. | 2024 | 101.173 | -0.528 | 0.179 | â | â | â |
| Hunt & Reffert | 2023 | 101.181 | -0.524 | 0.191 | -0.166 | 1.079 | 78.122 |
| Just et al. | 2023 | 101.15 | -0.558 | â | â | â | â |
| Dias et al. | 2021 | 101.179 | -0.532 | 0.1 | -0.204 | 1.038 | â |
| Cantat-Gaudin et al. | 2020 | 101.181 | -0.532 | 0.126 | -0.15 | 1.063 | â |
| Cantat-Gaudin & Anders | 2020 | 101.181 | -0.532 | 0.126 | -0.15 | 1.063 | â |
| Bica et al. | 2019 | 101.182 | -0.52 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 101.181 | -0.532 | 0.126 | -0.15 | 1.063 | â |
| Kharchenko et al. | 2016 | 101.15 | -0.558 | â | â | â | â |
| Kharchenko et al. | 2013 | 101.157 | -0.56 | â | -0.44 | -2.28 | â |
| Glushkova et al. | 2010 | 101.178 | -0.539 | â | â | â | â |
| Kronberger et al. | 2006 | 101.179 | -0.518 | â | â | â | â |
| Dias et al. | 2002 | 101.179 | -0.539 | â | 9.39 | 1.43 | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Hu & Soubiran | 2025 | â | â | â | â | -0.300* | â | â | â |
| Almeida et al. | 2025 | 7.25 | 1.94 | â | 676 | â | 286 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 508* | â | â |
| Cavallo et al. | 2024 | 4.35 | 2.67 | â | 832 | -1.070 | â | â | â |
| Hunt & Reffert | 2023 | 4.81 | 1.74 | 1.79 | 859 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 891 | â | 287 | â | â |
| Dias et al. | 2021 | 7.25 | 1.94 | â | 676 | -0.129 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 6.79 | 1.57 | â | 1096 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 6.46 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 6.46 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 6.37 | 1.74 | â | 891 | â | â | â | â |
| Kharchenko et al. | 2013 | 6.37 | 1.74 | â | 891 | â | â | â | â |
| Glushkova et al. | 2010 | 6.31 | 1.27 | â | 891 | â | â | â | â |
| Dias et al. | 2002 | 6.31 | 1.27 | â | 891 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


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