Berkeley 80

(OCL 87; MWSC 3019)

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C3
N_50
r_50
AA 86 2.1
Summary

Berkeley 80 is a moderately populated, very dense object of very high C3 quality. It is located at a moderate distance from the Sun, near 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) 283.592 -1.217 0.91 0.26
Kharchenko et al. (2012) 283.582 -1.217 -1.08 -5.11
Loktin & Popova (2017) 283.59 -1.213 -0.075 -7.738
Cantat-Gaudin et al. (2018) 283.591 -1.214 0.39 -0.755 -2.667
Bica et al. (2019) 283.585 -1.216
Soubiran et al. (2018) 283.591 -1.214 43.95
Cantat-Gaudin et al. (2020) 283.591 -1.214 0.39 -0.755 -2.667
Dias et al. (2021) 283.588 -1.21 0.396 -0.767 -2.675
Hunt & Reffert (2023) 283.59 -1.216 0.401 -0.765 -2.712 189.075
Cavallo et al. (2024) 283.59 -1.213 0.402
Hunt & Reffert (2024) 283.59 -1.216 0.401 -0.765 -2.712 189.075
Almeida et al. (2025) 283.588 -1.21
           
UCC 283.591 -1.215 0.401 -0.743 -2.697 153.853
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)=1.31, Dist=1413.0, Age=8.6, [Fe/H]=0.0
Kharchenko et al. (2012) e_bv=1.041, distance=1791, log_age=8.35, metallicity=0.0
Loktin & Popova (2017) E(B-V)=0.965, Dist=2913, logt=8.55
Cantat-Gaudin et al. (2018) dmode=2388.9
Soubiran et al. (2018) dmode=2388.9
Cantat-Gaudin et al. (2020) AVNN=3.5, DistPc=2270.0, AgeNN=8.2
Dias et al. (2021) Av=3.344, Dist=1833, logage=8.646, [Fe/H]=0.098
Hunt & Reffert (2023) AV50=4.203, diffAV50=1.839, MOD50=11.837, logAge50=7.86
Cavallo et al. (2024) AV50=4.22, dMod50=12.28, logAge50=7.76, [Fe/H]50=0.36
Hunt & Reffert (2024) MassJ=1188.23, MassTot=1188.23
Almeida et al. (2025) AV=3.344, Dist=1833, logAge=8.646, MassRk=567.7

Search coordinates in Bayestar19

Cluster region map