Berkeley 10

(FSR 0623; MWSC 290; OCL 370; FoF 630)

Click to load Aladin Lite
0.97 UTI
0.84
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
N50 (P>50% members) 349
Stellar density (N50/rad) 27.9 [N/pc2]
C3 classification AA
  • CN 0.84 Rich
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 1.0 Very well-studied
  • Cdup 1.0 Unique
πŸ“₯ Members πŸ“Š Colab πŸ”¬ Bayestar19 MOCAMOCA πŸ” CDS πŸ” Simbad πŸ” CDS (Ξ±, Ξ΄) πŸ” Simbad (Ξ±, Ξ΄)

Overview
ℹ️
Berkeley 10 is a rich, very dense object of very 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 very well-studied in the literature.

Almeida et al. (2025)
Mass determination: good fit. Isochrone match: intermediate fit.

Cavallo et al. (2024)
Gold sample.

Data
πŸ” Search references for Berkeley 10 in: SciX Simbad
ℹ️
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 54.895 66.484 0.387 -1.497 1.01 -36.462
Li et al. 2025 54.894 66.486 0.372 -1.47 1.047 –
Almeida et al. 2025 54.888 66.49 – – – –
Hunt & Reffert 2024 54.885 66.489 0.398 -1.497 1.005 -32.448
Cavallo et al. 2024 54.895 66.488 0.396 – – –
Hunt & Reffert 2023 54.885 66.489 0.398 -1.497 1.005 -32.448
Almeida et al. 2023 54.899 66.481 – – – –
Just et al. 2023 54.886 66.488 – – – –
Dias et al. 2021 54.888 66.49 0.368 -1.464 1.053 -36.134
Cantat-Gaudin et al. 2020 54.894 66.486 0.372 -1.47 1.047 –
SΓ‘nchez et al. 2020 54.883 66.486 – -1.545 1.057 –
Cantat-Gaudin & Anders 2020 54.894 66.486 0.372 -1.47 1.047 –
Liu & Pang 2019 54.89 66.486 0.368 -1.426 1.036 –
Soubiran et al. 2018 54.894 66.486 – – – -36.29
Bica et al. 2019 54.874 66.49 – – – –
Cantat-Gaudin et al. 2018 54.894 66.486 0.372 -1.47 1.047 –
Loktin & Popova 2017 54.885 66.486 – -2.837 -2.97 –
Kharchenko et al. 2016 54.886 66.488 – – – –
Dias et al. 2014 54.883 66.486 – -2.11 -0.5 –
Kharchenko et al. 2013 54.9 66.49 – -1.72 -1.22 –
Gozha et al. 2012 54.883 66.486 – – – –
Kharchenko et al. 2012 54.9 66.49 – -1.93 -0.96 –
Froebrich et al. 2007 54.925 66.495 – – – –
Dias et al. 2002 54.883 66.486 – -2.11 -0.5 –

πŸ’‘ 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 99999– 2.2 2.54 1.2 692 -0.116 1019 0.66 –
Li et al. 2025 2.15 2.37 – 1047 0.039 – – –
Almeida et al. 2025 2.00 2.60 – 798 – 1156 – –
Hunt & Reffert 2024 – – – – – 2288(1) – –
Cavallo et al. 2024 2.50 3.14 – 355 0.040 – – –
Hunt & Reffert 2023 2.36 2.80 1.20 340 – – – –
Almeida et al. 2023 2.09 2.65 – 785 -0.116 882(1) 0.66 –
Just et al. 2023 – – – 646 – 542 – –
Dias et al. 2021 2.00 2.60 – 798 -0.100 – – –
Cantat-Gaudin et al. 2020 2.37 1.94 – 1202 – – – –
Cantat-Gaudin & Anders 2020 2.50 – – – – – – –
Liu & Pang 2019 – – – 692 0.500 – – –
Soubiran et al. 2018 2.50 – – – – – – –
Cantat-Gaudin et al. 2018 2.50 – – – – – – –
Loktin & Popova 2017 2.54 2.61 – 468 – – – –
Kharchenko et al. 2016 2.20 2.48 – 646 – – – –
Kharchenko et al. 2013 2.20 2.48 – 646 -0.490 – – –
Gozha et al. 2012 1.70 – – 1148 -0.490 – – –
Kharchenko et al. 2012 2.20 2.48 – 668 -0.490 – – –
Dias et al. 2002 1.70 2.33 – 1148 -0.490 – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Visualization
ℹ️
Berkeley 10 UCC
Berkeley 10 HUNT23
Berkeley 10 CANTAT20
Galactocentric position diagram