Czernik 1
(MWSC 17; OCL 283)
0.79
UTI
0.45
CN
1.0
Cdens
0.5
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad)
36.3 [N/pc2]
- CN 0.45 Poorly populated
- Cdens 1.0 Very dense
- CC3 0.5 Intermediate quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
Czernik 1 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the metallicity and mass parameters (see Parameters). It is very 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 | 1.904 | 61.483 | 0.313 | -2.953 | -1.449 | â |
| Li et al. | 2025 | 1.906 | 61.476 | 0.31 | -2.964 | -1.395 | â |
| Almeida et al. | 2025 | 1.907 | 61.477 | â | â | â | â |
| Hunt & Reffert | 2024 | 1.907 | 61.479 | 0.321 | -2.949 | -1.465 | â |
| Cavallo et al. | 2024 | 1.909 | 61.486 | 0.32 | â | â | â |
| Hunt & Reffert | 2023 | 1.907 | 61.479 | 0.321 | -2.949 | -1.465 | â |
| Almeida et al. | 2023 | 1.908 | 61.481 | â | â | â | â |
| Just et al. | 2023 | 1.893 | 61.486 | â | â | â | â |
| Dias et al. | 2021 | 1.907 | 61.477 | 0.308 | -2.956 | -1.379 | â |
| Cantat-Gaudin et al. | 2020 | 1.906 | 61.476 | 0.31 | -2.964 | -1.395 | â |
| Cantat-Gaudin & Anders | 2020 | 1.906 | 61.476 | 0.31 | -2.964 | -1.395 | â |
| Bica et al. | 2019 | 1.915 | 61.479 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 1.906 | 61.476 | 0.31 | -2.964 | -1.395 | â |
| Loktin & Popova | 2017 | 1.905 | 61.475 | â | -1.073 | -0.342 | â |
| Kharchenko et al. | 2016 | 1.893 | 61.486 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.902 | 61.49 | â | -3.83 | 1.66 | â |
| Kharchenko et al. | 2012 | 1.902 | 61.49 | â | -3.83 | 1.66 | â |
| Bukowiecki et al. | 2011 | 1.933 | 61.473 | â | â | â | â |
| Dias et al. | 2002 | 1.908 | 61.475 | â | -3.83 | 1.66 | 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 | 2.62 | 2.35 | 0.8 | 31 | -0.072 | 201 | 0.44 | â |
| Li et al. | 2025 | 2.58 | 2.48 | â | 25 | -0.065 | â | â | â |
| Almeida et al. | 2025 | 2.62 | 2.34 | â | 22 | â | 228 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 510(1) | â | â |
| Cavallo et al. | 2024 | 2.90 | 2.23 | â | 62 | 0.630 | â | â | â |
| Hunt & Reffert | 2023 | 2.88 | 2.35 | 0.80 | 68 | â | â | â | â |
| Almeida et al. | 2023 | 2.69 | 2.39 | â | 17 | -0.079 | 201(1) | 0.44 | â |
| Just et al. | 2023 | â | â | â | 58 | â | 22 | â | â |
| Dias et al. | 2021 | 2.62 | 2.34 | â | 22 | -0.087 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 3.12 | 2.17 | â | 37 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 2.95 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 2.95 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 2.17 | 2.27 | â | 14 | â | â | â | â |
| Kharchenko et al. | 2016 | 2.61 | 2.58 | â | 58 | â | â | â | â |
| Kharchenko et al. | 2013 | 2.61 | 2.58 | â | 58 | â | â | â | â |
| Bukowiecki et al. | 2012 | â | â | â | â | â | 125 | â | â |
| Kharchenko et al. | 2012 | 2.61 | 2.58 | â | 58 | â | â | â | â |
| Bukowiecki et al. | 2011 | 2.28(1) | 1.86 | â | 18 | â | â | â | â |
| Dias et al. | 2002 | 2.53 | 3.81 | â | 5 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


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