Berkeley 67

(MWSC 404; OCL 400; FSR 0677; FoF 577)

0.91 UTI

0.8

C_N

1.0

C_dens

0.75

C_C3

1.0

C_lit

1.0

C_dup

C3 classification AB

Number of members (P>50%) 233

Radius (P>50% members) 4.4 [arcmin]

C_N 0.8 Rich
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 1.0 Very well-studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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Berkeley 67 is a rich, very dense object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a massive, near-solar metallicity, old cluster, but with a large variance across recent sources for the metallicity and mass parameters (see Parameters). It is very well-studied in the literature.

Relatively close Moderate extinction Massive Near-solar metallicity Old

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

Cavallo et al. (2024)
Gold sample.

Data

🔍 Search references for Berkeley 67 in: SciX Simbad

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Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	69.465	50.758	0.459	2.285	-1.416	-0.245
Li et al.	2025	69.472	50.755	0.415	2.316	-1.374	–
Hu & Soubiran	2025	69.486	50.737	–	–	–	–
Almeida et al.	2025	69.493	50.746	–	–	–	–
Zhang et al.	2024	69.459	50.776	–	–	–	–
Hunt & Reffert	2024	69.459	50.776	0.463	2.255	-1.411	-2.049
Cavallo et al.	2024	69.486	50.737	0.464	–	–	–
Hunt & Reffert	2023	69.459	50.776	0.463	2.255	-1.411	-2.049
Just et al.	2023	69.439	50.775	–	–	–	–
Dias et al.	2021	69.493	50.746	0.41	2.338	-1.376	-0.092
Cantat-Gaudin et al.	2020	69.472	50.755	0.415	2.316	-1.374	–
Sánchez et al.	2020	69.525	50.75	–	2.223	-1.473	–
Cantat-Gaudin & Anders	2020	69.472	50.755	0.415	2.316	-1.374	–
Liu & Pang	2019	69.478	50.753	0.412	2.334	-1.393	–
Soubiran et al.	2018	69.472	50.755	–	–	–	-0.28
Bica et al.	2019	69.458	50.763	–	–	–	–
Cantat-Gaudin et al.	2018	69.472	50.755	0.415	2.316	-1.374	–
Kharchenko et al.	2016	69.439	50.775	–	–	–	–
Dias et al.	2014	69.525	50.75	–	-0.25	-1.07	–
Kharchenko et al.	2013	69.45	50.775	–	0.09	-1.49	–
Kharchenko et al.	2012	69.45	50.775	–	0.09	-1.49	–

💡 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]	Bfr	BSS
Li et al.	2025	1.98	2.93	–	1214	-0.268	–	–	–
Hu & Soubiran	2025	–	–	–	–	0.020*	–	–	–
Almeida et al.	2025	2.18	2.93	–	796	–	1013	–	–
Zhang et al.	2024	–	–	–	–	-0.221*	–	–	–
Hunt & Reffert	2024	–	–	–	–	–	1527*	–	–
Cavallo et al.	2024	2.04	2.98	–	832	0.170	–	–	–
Hunt & Reffert	2023	1.99	3.02	2.38	655	–	–	–	–
Just et al.	2023	–	–	–	1746	–	200	–	–
Dias et al.	2021	2.18	2.93	–	796	-0.197	–	–	–
Cantat-Gaudin et al.	2020	2.22	2.03	–	1259	–	–	–	–
Cantat-Gaudin & Anders	2020	2.25	–	–	–	–	–	–	–
Liu & Pang	2019	–	–	–	813	0.250	–	–	–
Soubiran et al.	2018	2.25	–	–	–	–	–	–	–
Cantat-Gaudin et al.	2018	2.25	–	–	–	–	–	–	–
Kharchenko et al.	2016	2.00	2.17	–	1746	–	–	–	–
Kharchenko et al.	2013	2.00	2.17	–	1746	–	–	–	–
Kharchenko et al.	2012	2.00	2.17	–	1746	–	–	–	–

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Visualization

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