Juchert 20
(SAI 35; DSH J0410.8+4652; FSR 0676; MWSC 348)
0.84
UTI
0.76
CN
1.0
Cdens
0.75
CC3
0.84
Clit
1.0
Cdup
Stellar density (N50/rad)
42.9 [N/pc2]
- CN 0.76 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.84 Well-studied
- Cdup 1.0 Unique
Overview
Juchert 20 is a rich, very dense object of high C3 quality. Its parallax locates it at a moderate 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 age and metallicity parameters (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 | 62.701 | 46.868 | 0.342 | 1.116 | -1.684 | -32.383 |
| Almeida et al. | 2025 | 62.695 | 46.868 | â | â | â | â |
| Zhang et al. | 2024 | 62.703 | 46.874 | â | â | â | â |
| Hunt & Reffert | 2024 | 62.703 | 46.874 | 0.314 | 1.094 | -1.662 | -29.739 |
| Cavallo et al. | 2024 | 62.712 | 46.877 | 0.319 | â | â | â |
| Hunt & Reffert | 2023 | 62.703 | 46.874 | 0.314 | 1.094 | -1.662 | -29.739 |
| Almeida et al. | 2023 | 62.698 | 46.866 | â | â | â | â |
| Dias et al. | 2021 | 62.695 | 46.868 | 0.327 | 1.182 | -1.67 | â |
| Cantat-Gaudin et al. | 2020 | 62.703 | 46.874 | 0.331 | 1.103 | -1.643 | â |
| Cantat-Gaudin & Anders | 2020 | 62.703 | 46.874 | 0.331 | 1.103 | -1.643 | â |
| Bica et al. | 2019 | 62.704 | 46.878 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 62.703 | 46.874 | 0.331 | 1.103 | -1.643 | â |
| Loktin & Popova | 2017 | 62.7 | 46.867 | â | -2.052 | -5.9 | â |
| Dias et al. | 2014 | 62.696 | 46.867 | â | -0.11 | -0.9 | â |
| Glushkova et al. | 2010 | 62.696 | 46.867 | â | â | â | â |
| Kronberger et al. | 2006 | 62.701 | 46.874 | â | â | â | â |
| Dias et al. | 2002 | 62.696 | 46.867 | â | -0.09 | -0.92 | 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 | 2.65 | 2.21 | 2.28 | 213 | -0.153 | 707 | 0.71 | â |
| Almeida et al. | 2025 | 2.65 | 2.38 | â | 18 | â | 330 | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.166(1) | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 1036(1) | â | â |
| Cavallo et al. | 2024 | 2.98 | 2.33 | â | 316 | 0.190 | â | â | â |
| Hunt & Reffert | 2023 | 2.77 | 2.21 | 2.28 | 213 | â | â | â | â |
| Almeida et al. | 2023 | 2.60 | 2.41 | â | 101 | -0.188 | 707(1) | 0.71 | â |
| Dias et al. | 2021 | 2.65 | 2.38 | â | 18 | -0.141 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 3.12 | 1.74 | â | 302 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 2.78 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 2.78 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 2.45 | 1.92 | â | 50 | â | â | â | â |
| Glushkova et al. | 2010 | 2.42 | 2.17 | â | 355 | â | â | â | â |
| Dias et al. | 2002 | 2.42 | 2.17 | â | 355 | 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: good fit. Isochrone match: intermediate fit. Silver sample.
Cavallo et al. (2024)
Gold sample.