Berkeley 90

(MWSC 3377)

0.78 UTI

0.78

C_N

1.0

C_dens

0.75

C_C3

0.69

C_lit

1.0

C_dup

C3 classification AB

Number of members (P>50%) 189

Radius (P>50% members) 4.3 [arcmin]

C_N 0.78 Rich
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.69 Moderately studied
C_dup 1.0 Unique

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

Overview

Berkeley 90 is a rich, very dense object of 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 parameter (see Parameters). It is moderately studied in the literature.

Relatively close High extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024): Silver sample.

Data

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	308.818	46.843	0.333	-2.869	-4.364	-45.116
Hunt & Reffert	2024	308.812	46.844	0.343	-2.875	-4.367	-19.413
Celli et al.	2024	308.819	46.843	–	–	–	–
Cavallo et al.	2024	308.823	46.841	0.342	–	–	–
Hunt & Reffert	2023	308.812	46.844	0.343	-2.875	-4.367	-19.413
Just et al.	2023	308.807	46.838	–	–	–	–
Cantat-Gaudin et al.	2020	308.819	46.843	0.302	-2.829	-4.369	–
Cantat-Gaudin et al.	2018	308.819	46.843	0.302	-2.829	-4.369	–
Loktin & Popova	2017	308.805	46.841	–	-0.267	-0.155	–
Kharchenko et al.	2016	308.807	46.838	–	–	–	–
Kharchenko et al.	2013	308.812	46.841	–	-2.09	-0.63	–
Dias et al.	2002	308.825	46.833	–	-2.13	-0.52	–

💡 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
Hunt & Reffert	2024	–	–	–	–	–	1923*	–	–
Celli et al.	2024	–	–	–	5	–	817	–	–
Cavallo et al.	2024	2.50	3.85	–	45	0.420	–	–	–
Hunt & Reffert	2023	2.76	3.90	2.82	8	–	–	–	–
Just et al.	2023	–	–	–	200	–	385	–	–
Cantat-Gaudin et al.	2020	3.02	3.60	–	5	–	–	–	–
Cantat-Gaudin et al.	2018	3.02	–	–	–	–	–	–	–
Loktin & Popova	2017	1.63	2.03	–	1047	–	–	–	–
Kharchenko et al.	2016	2.65	3.68	–	200	–	–	–	–
Kharchenko et al.	2013	2.65	3.68	–	200	–	–	–	–
Dias et al.	2002	2.07	3.69	–	112	–	–	–	–

💡 Note: The parameters are sometimes transformed from their original values to match the format of the columns shown here, see FAQ. The columns DAv, Bfr, BSS correspond to differential extinction, binary fraction, and blue stragglers, respectively. BSS values can be listed as fractions or integers.
(*): indicates that this parameter is assigned more than one value in the corresponding reference.

Visualization

1 2 3

💡 Note: How are the galactocentric plots generated? See FAQ.