Berkeley 85

(OCL 160; Dolidze 41; OCL 163; FSR 0208; MWSC 3311; MWSC 3309)

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C3
N_50
r_50
AA 687 3.3
Summary

Berkeley 85 is a very rich, very dense object of very high C3 quality. It is located at a moderate distance from the Sun, above the mid-plane. It is well-studied in the literature.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
Dias et al. (2002) 304.729 37.759 -1.45 -1.52
Kharchenko et al. (2012) 304.688 37.73 -3.52 -2.78
Loktin & Popova (2017) 304.725 37.758 -0.945 -0.945 -1.0
Cantat-Gaudin et al. (2018) 304.692 37.744 0.22 -2.94 -4.677
Bica et al. (2019) 304.712 37.737
Soubiran et al. (2018) 304.692 37.744 -33.72
Cantat-Gaudin et al. (2020) 304.692 37.744 0.22 -2.94 -4.677
Dias et al. (2021) 304.694 37.75 0.216 -2.947 -4.677 -33.478
Hunt & Reffert (2023) 304.699 37.731 0.249 -2.953 -4.673 -26.033
Cavallo et al. (2024) 304.701 37.746 0.244
Hunt & Reffert (2024) 304.699 37.731 0.249 -2.953 -4.673 -26.033
Almeida et al. (2025) 304.694 37.75
           
UCC 304.697 37.744 0.243 -2.937 -4.678 -34.091
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

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Estimated members

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Fundamental parameters

Reference Values
Dias et al. (2002) E(B-V)=0.77, Dist=1760.0, Age=9.0
Kharchenko et al. (2012) e_bv=0.77, distance=1760, log_age=9.065
Loktin & Popova (2017) E(B-V)=0.833, Dist=3073, logt=8.88
Cantat-Gaudin et al. (2018) dmode=4017.8
Soubiran et al. (2018) dmode=4017.8
Cantat-Gaudin et al. (2020) AVNN=2.77, DistPc=3526.0, AgeNN=8.62
Dias et al. (2021) Av=3.07, Dist=3005, logage=8.383, [Fe/H]=0.424
Hunt & Reffert (2023) AV50=3.827, diffAV50=2.476, MOD50=12.845, logAge50=7.901
Cavallo et al. (2024) AV50=3.75, dMod50=12.55, logAge50=8.26, [Fe/H]50=0.24
Hunt & Reffert (2024) MassJ=8390.39, MassTot=8390.39
Almeida et al. (2025) AV=3.07, Dist=3005, logAge=8.383, MassRk=3236.6

Search coordinates in Bayestar19

Cluster region map