Kronberger 69
(SAI 133; MWSC 3227; DSH J2001.9+3126; FSR 0181)
0.86
UTI
0.53
CN
1.0
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
Radius (P>50% members)
3.0 [arcmin]
- CN 0.53 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
Kronberger 69 is a moderately populated, very dense object of high 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 mass parameter (see Parameters). It is very well-studied in the literature.
Relatively close
Moderate extinction
Near-solar metallicity
Young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 300.509 | 31.413 | 0.356 | -2.791 | -5.245 | -13.203 |
| Almeida et al. | 2025 | 300.49 | 31.423 | â | â | â | â |
| Hunt & Reffert | 2024 | 300.509 | 31.42 | 0.37 | -2.776 | -5.235 | -44.436 |
| Cavallo et al. | 2024 | 300.507 | 31.403 | 0.371 | â | â | â |
| Hunt & Reffert | 2023 | 300.509 | 31.42 | 0.37 | -2.776 | -5.235 | -44.436 |
| Just et al. | 2023 | 300.483 | 31.442 | â | â | â | â |
| Dias et al. | 2021 | 300.49 | 31.423 | 0.355 | -2.719 | -5.206 | â |
| Cantat-Gaudin et al. | 2020 | 300.499 | 31.42 | 0.351 | -2.741 | -5.246 | â |
| Cantat-Gaudin & Anders | 2020 | 300.499 | 31.42 | 0.351 | -2.741 | -5.246 | â |
| Bica et al. | 2019 | 300.491 | 31.441 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 300.499 | 31.42 | 0.351 | -2.741 | -5.246 | â |
| Loktin & Popova | 2017 | 300.48 | 31.445 | â | -2.044 | -4.582 | â |
| Kharchenko et al. | 2016 | 300.483 | 31.442 | â | â | â | â |
| Dias et al. | 2014 | 300.496 | 31.438 | â | -2.63 | -2.75 | â |
| Kharchenko et al. | 2013 | 300.487 | 31.445 | â | -2.78 | -3.63 | â |
| Glushkova et al. | 2010 | 300.495 | 31.438 | â | â | â | â |
| Kronberger et al. | 2006 | 300.488 | 31.44 | â | â | â | â |
| Dias et al. | 2002 | 300.496 | 31.438 | â | -2.63 | -2.75 | 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 | 2.65 | 2.83 | â | 12 | â | 312 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 596* | â | â |
| Cavallo et al. | 2024 | 3.30 | 3.06 | â | 43 | 0.640 | â | â | â |
| Hunt & Reffert | 2023 | 2.55 | 2.91 | 1.60 | 57 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 79 | â | 3639 | â | â |
| Dias et al. | 2021 | 2.65 | 2.83 | â | 12 | -0.111 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 2.68 | 2.46 | â | 41 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 2.63 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 2.63 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 2.33 | 1.73 | â | 589 | â | â | â | â |
| Kharchenko et al. | 2016 | 8.49 | 6.32 | â | 79 | â | â | â | â |
| Kharchenko et al. | 2013 | 8.49 | 6.32 | â | 79 | â | â | â | â |
| Glushkova et al. | 2010 | 6.14 | 5.58 | â | 71 | â | â | â | â |
| Dias et al. | 2002 | 6.14 | 5.58 | â | 71 | â | â | â | â |
(*): 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.