Berkeley 55

(MWSC 3490)

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0.90 UTI
0.82
CN
1.0
Cdens
1.0
CC3
0.84
Clit
1.0
Cdup
Stellar density (N50/rad) 88.3 [N/pc2]
  • CN 0.82 Rich
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.84 Well-studied
  • Cdup 1.0 Unique

Overview

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Berkeley 55 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 high extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age, metallicity, and mass parameters (see Parameters). It is well-studied in the literature.

Almeida et al. (2025)
Mass determination: invalid due to poor quality CMD. Isochrone match: worst fit.

Cavallo et al. (2024)
Silver 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– 319.236 51.765 0.312 -4.085 -4.653 -45.45
Almeida et al. 2025 319.227 51.763 – – – –
Hunt & Reffert 2024 319.235 51.761 0.325 -4.086 -4.68 -32.001
Cavallo et al. 2024 319.23 51.764 0.325 – – –
Hunt & Reffert 2023 319.235 51.761 0.325 -4.086 -4.68 -32.001
Just et al. 2023 319.245 51.761 – – – –
Dias et al. 2021 319.227 51.763 0.304 -4.026 -4.627 -42.456
Cantat-Gaudin et al. 2020 319.232 51.762 0.309 -4.05 -4.618 –
SΓ‘nchez et al. 2020 319.242 51.759 – -3.976 -4.546 –
Cantat-Gaudin & Anders 2020 319.232 51.762 0.309 -4.05 -4.618 –
Soubiran et al. 2018 319.232 51.762 – – – -43.58
Cantat-Gaudin et al. 2018 319.232 51.762 0.309 -4.05 -4.618 –
Loktin & Popova 2017 319.245 51.761 – -1.135 -2.297 –
Kharchenko et al. 2016 319.245 51.761 – – – –
Kharchenko et al. 2013 319.249 51.765 – -3.02 -7.83 –
Kharchenko et al. 2012 319.249 51.765 – -3.02 -7.83 –
Dias et al. 2002 319.242 51.759 – -5.93 -12.57 –

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– 2.85 4.96 3.07 200 0.175 863 – –
Almeida et al. 2025 2.58 4.16 – 130 – 863 – –
Hunt & Reffert 2024 – – – – – 3609(1) – –
Cavallo et al. 2024 2.96 5.17 – 47 0.010 – – –
Hunt & Reffert 2023 2.85 5.56 3.07 63 – – – –
Just et al. 2023 – – – 372 – 10 – –
Dias et al. 2021 2.58 4.16 – 130 0.341 – – –
Cantat-Gaudin et al. 2020 2.75 4.80 – 200 – – – –
Cantat-Gaudin & Anders 2020 2.96 – – – – – – –
Soubiran et al. 2018 2.96 – – – – – – –
Cantat-Gaudin et al. 2018 2.96 – – – – – – –
Loktin & Popova 2017 3.66 4.39 – 380 – – – –
Kharchenko et al. 2016 1.70 4.96 – 372 – – – –
Kharchenko et al. 2013 1.70 4.96 – 372 – – – –
Kharchenko et al. 2012 1.70 4.96 – 372 – – – –
Dias et al. 2002 3.98 5.74 – 50 – – – –

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

Visualization

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