Berkeley 24

(MWSC 937; OCL 539; FSR 1070)

Click to load Aladin Lite
0.82 UTI
0.88
CN
1.0
Cdens
0.75
CC3
0.74
Clit
1.0
Cdup
Core radius and density 1.6 [pc], 6.6 [pc-2]
  • CN 0.88 Rich
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.74 Moderately studied
  • Cdup 1.0 Unique

Overview

ℹ️
Berkeley 24 is a rich, very dense object of high C3 quality. Its parallax locates it at a large distance, below the mid-plane, affected by moderate extinction. It is catalogued as a massive, near-solar metallicity, old cluster (see Parameters). It is moderately studied in the literature.

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

Note: This object shares a very 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.

Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.93 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.93 (50th percentile).

Hu et al. (2021)
Ellipticities (core, all): e_core=0.0514, e_all=0.0637.

Data

ℹ️
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 99.448 -0.879 0.178 0.33 1.261 76.143
Hu & Soubiran 2025 99.453 -0.871 – – – –
Almeida et al. 2025 99.455 -0.871 – – – –
Hunt & Reffert 2024 99.445 -0.877 0.187 0.326 1.266 64.848
Cavallo et al. 2024 99.453 -0.871 0.185 – – –
Hunt & Reffert 2023 99.445 -0.877 0.187 0.326 1.266 64.848
Just et al. 2023 99.443 -0.865 – – – –
Jadhav & Subramaniam 2021 99.452 -0.874 – – – –
Dias et al. 2021 99.455 -0.871 0.164 0.411 1.31 73.72
Cantat-Gaudin et al. 2020 99.452 -0.874 0.156 0.382 1.279 –
SΓ‘nchez et al. 2020 99.446 -0.872 – 0.44 1.392 –
Zhong et al. 2020 99.452 -0.874 – 0.382 1.279 51.392
Cantat-Gaudin & Anders 2020 99.452 -0.874 0.156 0.382 1.279 –
Soubiran et al. 2018 99.452 -0.874 – – – 73.84
Bica et al. 2019 99.45 -0.868 – – – –
Cantat-Gaudin et al. 2018 99.452 -0.874 0.156 0.382 1.279 –
Dias et al. 2018 – – – -1.67 -0.63 –
Loktin & Popova 2017 99.45 -0.872 – 0.565 0.412 –
Sampedro et al. 2017 99.446 -0.872 – 0.9 1.86 –
Kharchenko et al. 2016 99.443 -0.865 – – – –
Dias et al. 2014 99.446 -0.872 – -0.85 1.18 –
Kharchenko et al. 2013 99.45 -0.867 – 2.07 1.35 –
Bukowiecki et al. 2011 99.442 0.877 – – – –
Dias et al. 2002 99.446 -0.872 – -0.85 1.18 –
Lynga 1987 99.437 -0.909 – – – –

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– 4.9 1.84 1.76 1622 -0.306 2764 – 2
Hu & Soubiran 2025 – – – – -0.290(5) – – –
Almeida et al. 2025 4.72 2.34 – 1400 – 2577 – –
Hunt & Reffert 2024 4.53 1.85 1.76 1427 – 2664(1) – –
Cavallo et al. 2024 4.53 1.92 – 1778 -0.140 – – –
Hunt & Reffert 2023 4.53 1.85 1.76 1426 – – – –
Just et al. 2023 – – – 1622 – 2864 – –
Jadhav & Subramaniam 2021 4.90 1.74 – 1413 – 4843 – 2(1)
Dias et al. 2021 4.72 2.34 – 1400 -0.323 – – –
Cantat-Gaudin et al. 2020 4.90 1.74 – 1413 – – – –
Kounkel et al. 2020 4.23 1.69 – 1479 – – – –
Zhong et al. 2020 5.39(1) 1.84 – 9210 -0.427 – – –
Cantat-Gaudin & Anders 2020 5.39 – – – – – – –
Soubiran et al. 2018 5.39 – – – – – – –
Cantat-Gaudin et al. 2018 5.39 – – – – – – –
Loktin & Popova 2017 5.07 1.44 – 6310 – – – –
Kharchenko et al. 2016 5.53 1.84 – 1622 – – – –
Kharchenko et al. 2013 5.53 1.84 – 1622 – – – –
Bukowiecki et al. 2011 4.98(1) 1.29 – 1778 – – – –
Dias et al. 2002 4.70 1.26 – 2188 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
S 283 9.8 99.48 -0.83 0.19 0.32 1.24 76.59 0.01

πŸ’‘ Note: The % column shows the percentage of members that Berkeley 24 shares with each listed object.

Visualization

ℹ️