Czernik 5
(FSR 0570; MWSC 150; OCL 338)
0.91
UTI
0.78
CN
1.0
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
Radius (P>50% members)
2.2 [arcmin]
- CN 0.78 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
Czernik 5 is a rich, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age and mass parameters (see Parameters). It is very well-studied in the literature.
Distant
High 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 | β | 28.923 | 61.354 | 0.254 | -2.03 | 0.376 | -125.495 |
| Almeida et al. | 2025 | 28.921 | 61.354 | β | β | β | β |
| Hunt & Reffert | 2024 | 28.919 | 61.354 | 0.272 | -2.01 | 0.366 | β |
| Cavallo et al. | 2024 | 28.971 | 61.348 | 0.27 | β | β | β |
| Hunt & Reffert | 2023 | 28.919 | 61.354 | 0.272 | -2.01 | 0.366 | β |
| Almeida et al. | 2023 | 28.923 | 61.361 | β | β | β | β |
| Just et al. | 2023 | 28.915 | 61.351 | β | β | β | β |
| Dias et al. | 2021 | 28.921 | 61.354 | 0.215 | -2.031 | 0.461 | β |
| Cantat-Gaudin et al. | 2020 | 28.927 | 61.355 | 0.229 | -2.02 | 0.476 | β |
| SΓ‘nchez et al. | 2020 | 28.929 | 61.356 | β | -1.99 | 0.401 | β |
| Cantat-Gaudin & Anders | 2020 | 28.927 | 61.355 | 0.229 | -2.02 | 0.476 | β |
| Cantat-Gaudin et al. | 2019 | 28.927 | 61.355 | 0.23 | -2.02 | 0.45 | β |
| Bica et al. | 2019 | 28.914 | 61.358 | β | β | β | β |
| Loktin & Popova | 2017 | 28.935 | 61.356 | β | -2.35 | 0.06 | β |
| Kharchenko et al. | 2016 | 28.915 | 61.351 | β | β | β | β |
| Kharchenko et al. | 2013 | 28.927 | 61.354 | β | -3.13 | -3.18 | β |
| Kharchenko et al. | 2012 | 28.927 | 61.354 | β | -3.13 | -3.18 | β |
| Froebrich et al. | 2007 | 28.938 | 61.355 | β | β | β | β |
| Dias et al. | 2002 | 28.929 | 61.356 | β | -2.35 | 0.06 | β |
π‘ 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 | 3.26 | 3.02 | β | 402 | β | 632 | β | β |
| Hunt & Reffert | 2024 | β | β | β | β | β | 1281* | β | β |
| Cavallo et al. | 2024 | 3.25 | 3.46 | β | 309 | 0.110 | β | β | β |
| Hunt & Reffert | 2023 | 3.30 | 3.42 | 1.77 | 64 | β | β | β | β |
| Almeida et al. | 2023 | 3.21 | 3.18 | β | 224 | -0.174 | 919* | 0.64 | β |
| Just et al. | 2023 | β | β | β | 412 | β | 68 | β | β |
| Dias et al. | 2021 | 3.26 | 3.02 | β | 402 | -0.174 | β | β | β |
| Cantat-Gaudin et al. | 2020 | 4.15 | 3.22 | β | 135 | β | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 3.88 | β | β | β | β | β | β | β |
| Cantat-Gaudin et al. | 2019 | 3.88 | β | β | β | β | β | β | β |
| Loktin & Popova | 2017 | 2.59 | 2.42 | β | 468 | β | β | β | β |
| Kharchenko et al. | 2016 | 2.40 | 3.41 | β | 412 | β | β | β | β |
| Kharchenko et al. | 2013 | 2.40 | 3.41 | β | 412 | β | β | β | β |
| Kharchenko et al. | 2012 | 2.40 | 3.41 | β | 412 | β | β | β | β |
| Dias et al. | 2002 | 2.75 | 3.72 | β | 282 | β | β | β | β |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


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