Berkeley 69

(FSR 0793; MWSC 532; OCL 444)

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0.91 UTI
0.81
CN
1.0
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad) 19.7 [N/pc2]
  • CN 0.81 Rich
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 1.0 Very well-studied
  • Cdup 1.0 Unique

Overview

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Berkeley 69 is a rich, very dense object of high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is very well-studied in the literature.

Note: This object contains blue stragglers according to at least one source.

Note: This object shares a small percentage of members with a later reported entry. See table with shared members information.

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

Cavallo et al. (2024)
Gold sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 81.09 32.608 0.275 0.756 -1.948 39.014
Li et al. 2025 81.09 32.607 0.259 0.806 -1.937 –
Hu & Soubiran 2025 81.104 32.61 – – – –
Almeida et al. 2025 81.088 32.603 – – – –
Zhang et al. 2024 81.091 32.608 – – – –
Hunt & Reffert 2024 81.091 32.608 0.273 0.739 -1.954 31.679
Cavallo et al. 2024 81.104 32.61 0.275 – – –
Hunt & Reffert 2023 81.091 32.608 0.273 0.739 -1.954 31.679
Almeida et al. 2023 81.087 32.605 – – – –
Just et al. 2023 81.088 32.609 – – – –
Jaehnig et al. 2021 81.096 32.613 0.284 0.822 -1.933 –
Rain et al. 2021 81.09 32.607 0.259 0.806 -1.937 –
Dias et al. 2021 81.088 32.603 0.248 0.791 -1.951 40.227
Cantat-Gaudin et al. 2020 81.09 32.607 0.259 0.806 -1.937 –
Cantat-Gaudin & Anders 2020 81.09 32.607 0.259 0.806 -1.937 –
Soubiran et al. 2018 81.09 32.607 – – – 39.92
Bica et al. 2019 81.091 32.61 – – – –
Cantat-Gaudin et al. 2018 81.09 32.607 0.259 0.806 -1.937 –
Loktin & Popova 2017 81.09 32.608 – 0.7 -1.18 5.2
Kharchenko et al. 2016 81.088 32.609 – – – –
Kharchenko et al. 2013 81.097 32.608 – 2.69 -5.82 5.2
Gozha et al. 2012 81.15 32.65 – – – –
Kharchenko et al. 2012 81.097 32.608 – 2.43 -5.73 5.2
Kharchenko et al. 2007 81.15 32.65 – 0.03 – –
Froebrich et al. 2007 81.088 32.604 – – – –
van den Bergh 2006 81.15 32.65 – – – –
Dias et al. 2002 81.15 32.65 – 5.9 -12.51 5.2

💡 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– 3.11 2.08 2.06 891 -0.223 952 0.72 1.0
Li et al. 2025 3.12 2.09 – 932 -0.134 – – –
Hu & Soubiran 2025 – – – – -0.280(5) – – –
Almeida et al. 2025 3.11 2.10 – 863 – 891 – –
Zhang et al. 2024 – – – – -0.234(1) – – –
Hunt & Reffert 2024 – – – – – 1604(1) – –
Cavallo et al. 2024 2.75 2.23 – 1096 -0.360 – – –
Hunt & Reffert 2023 3.28 2.01 2.06 413 – – – –
Almeida et al. 2023 2.86 2.10 – 971 -0.212 508(1) 0.72 –
Just et al. 2023 – – – 1023 – 1012 – –
Jaehnig et al. 2021 3.48(1) – – – – – – –
Rain et al. 2021 3.47 2.02 – 891 – – – 1
Dias et al. 2021 3.11 2.10 – 863 -0.175 – – –
Cantat-Gaudin et al. 2020 3.40 1.61 – 794 – – – –
Cantat-Gaudin & Anders 2020 3.47 – – – – – – –
Soubiran et al. 2018 3.47 – – – – – – –
Cantat-Gaudin et al. 2018 3.47 – – – – – – –
Loktin & Popova 2017 4.34 2.04 – 618 – – – –
Kharchenko et al. 2016 2.80 2.08 – 1023 – – – –
Kharchenko et al. 2013 2.80 2.08 – 1023 – – – –
Gozha et al. 2012 2.86 – – 891 – – – –
Kharchenko et al. 2012 2.80 2.08 – 1026 – – – –
van den Bergh 2006 1.68 2.08 – 245 – – – –
Dias et al. 2002 2.86 2.02 – 891 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
OC 0294 17.1 81.09 32.61 0.3 0.76 -1.95 39.74 0.0

💡 Note: The % column shows the percentage of members that Berkeley 69 shares with each listed object.

Visualization

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