Berkeley 13
(MWSC 439; OCL 402)
0.86
UTI
0.83
CN
1.0
Cdens
0.75
CC3
0.87
Clit
1.0
Cdup
Nm (P>50%)
302
Core radius and density
2.0 [pc], 5.8 [pc-2]
- CN 0.83 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.87 Well-studied
- Cdup 1.0 Unique
Overview
Berkeley 13 is a rich, very dense object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the mass parameter (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 | 99999β | 73.948 | 52.803 | 0.22 | -0.126 | 0.536 | -29.895 |
| Otto et al. | 2026 | 73.953 | 52.81 | β | -0.08 | 0.56 | -30.5 |
| Li et al. | 2025 | 73.943 | 52.809 | 0.208 | -0.078 | 0.558 | β |
| Hu & Soubiran | 2025 | 73.94 | 52.798 | β | β | β | β |
| Almeida et al. | 2025 | 73.944 | 52.802 | β | β | β | β |
| Zhang et al. | 2024 | 73.953 | 52.81 | β | β | β | β |
| Hunt & Reffert | 2024 | 73.953 | 52.81 | 0.223 | -0.143 | 0.528 | -30.019 |
| Cavallo et al. | 2024 | 73.94 | 52.799 | 0.23 | β | β | β |
| Hunt & Reffert | 2023 | 73.953 | 52.81 | 0.223 | -0.143 | 0.528 | -30.019 |
| Just et al. | 2023 | 73.931 | 52.815 | β | β | β | β |
| Jadhav & Subramaniam | 2021 | 73.943 | 52.809 | β | β | β | β |
| Dias et al. | 2021 | 73.944 | 52.802 | 0.218 | -0.091 | 0.569 | -28.558 |
| Cantat-Gaudin et al. | 2020 | 73.943 | 52.809 | 0.208 | -0.078 | 0.558 | β |
| SΓ‘nchez et al. | 2020 | 73.967 | 52.8 | β | -0.336 | 0.488 | β |
| Zhong et al. | 2020 | 73.943 | 52.809 | β | -0.078 | 0.558 | -41.954 |
| Cantat-Gaudin & Anders | 2020 | 73.943 | 52.809 | 0.208 | -0.078 | 0.558 | β |
| Soubiran et al. | 2018 | 73.943 | 52.809 | β | β | β | -28.6 |
| Bica et al. | 2019 | 73.935 | 52.817 | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 73.943 | 52.809 | 0.208 | -0.078 | 0.558 | β |
| Loktin & Popova | 2017 | 73.965 | 52.801 | β | 0.151 | 0.565 | β |
| Sampedro et al. | 2017 | 73.967 | 52.8 | β | -5.52 | 3.71 | β |
| Kharchenko et al. | 2016 | 73.931 | 52.815 | β | β | β | β |
| Dias et al. | 2014 | 73.967 | 52.8 | β | -5.56 | 3.25 | β |
| Kharchenko et al. | 2013 | 73.942 | 52.815 | β | 0.23 | 1.51 | β |
| Kharchenko et al. | 2012 | 73.942 | 52.815 | β | 0.23 | 1.51 | β |
| Bukowiecki et al. | 2011 | 73.95 | 52.814 | β | β | β | β |
| Dias et al. | 2002 | 73.967 | 52.8 | β | -5.56 | 3.25 | β |
| Lynga | 1987 | 73.901 | 52.762 | β | β | β | 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] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999β | 3.52 | 2.335 | 1.79 | 741 | -0.265 | 1140 | β | 0 |
| Otto et al. | 2026 | β | β | β | 490 | -0.220(15) | β | β | β |
| Li et al. | 2025 | 3.39 | 2.42 | β | 733 | -0.339 | β | β | β |
| Hu & Soubiran | 2025 | β | β | β | β | -0.050(5) | β | β | β |
| Almeida et al. | 2025 | 3.26 | 2.32 | β | 769 | β | 1140 | β | β |
| Zhang et al. | 2024 | β | β | β | β | -0.265(1) | β | β | β |
| Hunt & Reffert | 2024 | 3.92 | 2.35 | 1.79 | 454 | β | 1926(1) | β | β |
| Cavallo et al. | 2024 | 3.28 | 2.48 | β | 724 | -0.350 | β | β | β |
| Hunt & Reffert | 2023 | 3.92 | 2.35 | 1.79 | 454 | β | β | β | β |
| Just et al. | 2023 | β | β | β | 741 | β | 122 | β | β |
| Jadhav & Subramaniam | 2021 | 3.96 | 2.09 | β | 490 | β | 2026 | β | 0(1) |
| Dias et al. | 2021 | 3.26 | 2.32 | β | 769 | -0.238 | β | β | β |
| Cantat-Gaudin et al. | 2020 | 3.96 | 2.09 | β | 490 | β | β | β | β |
| Kounkel et al. | 2020 | 3.76 | 1.89 | β | 1047 | β | β | β | β |
| Zhong et al. | 2020 | 4.22(1) | 2.68 | β | 8870 | -0.297 | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 4.22 | β | β | β | β | β | β | β |
| Soubiran et al. | 2018 | 4.22 | β | β | β | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 4.22 | β | β | β | β | β | β | β |
| Loktin & Popova | 2017 | 1.50 | 2.25 | β | 398 | β | β | β | β |
| Kharchenko et al. | 2016 | 2.80 | 2.68 | β | 741 | β | β | β | β |
| Kharchenko et al. | 2013 | 2.80 | 2.68 | β | 741 | β | β | β | β |
| Bukowiecki et al. | 2012 | β | β | β | β | β | 1040 | β | β |
| Kharchenko et al. | 2012 | 2.80 | 2.68 | β | 741 | β | β | β | β |
| Bukowiecki et al. | 2011 | 3.52(1) | 1.55 | β | 1122 | β | β | β | β |
| Dias et al. | 2002 | 2.47 | 2.08 | β | 1000 | β | β | β | β |
(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.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.90 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.90 (50th percentile).
Hu et al. (2021)
Ellipticities (core, all): e_core=0.1375, e_all=0.055.