Collinder 385

(NGC 6664; MWSC 2962; OCL 68; Alessi 153)

1.0 UTI

1.0

C_N

1.0

C_dens

1.0

C_C3

1.0

C_lit

1.0

C_dup

N₅₀ (P>50% members) 522

Stellar density (N₅₀/rad) 33.4 [N/pc²]

C3 classification AA

C_N 1.0 Very rich
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 1.0 Very well-studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

MOCA 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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Collinder 385 is a very rich, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a massive, near-solar metallicity, young cluster, but with a large variance across recent sources for the age, metallicity, and mass parameters (see Parameters). It is very well-studied in the literature.

Note: This object shares a very small percentage of members with a later reported entry. See table with shared members information.

Relatively close Moderate extinction Massive Near-solar metallicity Young

Almeida et al. (2025)
Mass determination: good fit. Isochrone match: good fit. Gold sample.

Cavallo et al. (2024)
Gold sample.

Data

🔍 Search references for Collinder 385 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	99999–	279.121	-8.184	0.464	-0.075	-2.591	16.065
Li et al.	2025	279.125	-8.194	0.468	-0.089	-2.561	–
Almeida et al.	2025	279.125	-8.188	–	–	–	–
Hunt & Reffert	2024	279.118	-8.206	0.455	-0.099	-2.593	17.343
Cavallo et al.	2024	279.119	-8.185	0.456	–	–	–
Hunt & Reffert	2023	279.118	-8.206	0.455	-0.099	-2.593	17.343
Just et al.	2023	279.125	-8.212	–	–	–	–
Jaehnig et al.	2021	279.131	-8.199	0.509	-0.091	-2.552	–
Rain et al.	2021	279.125	-8.194	0.468	-0.089	-2.561	–
Dias et al.	2021	279.125	-8.188	0.473	-0.094	-2.55	2.007
Cantat-Gaudin et al.	2020	279.125	-8.194	0.468	-0.089	-2.561	–
Cantat-Gaudin & Anders	2020	279.125	-8.194	0.468	-0.089	-2.561	–
Dias et al.	2019	279.125	-8.194	0.468	-0.089	-2.561	-4.44
Soubiran et al.	2018	279.125	-8.194	–	–	–	-4.44
Bica et al.	2019	279.14	-8.216	–	–	–	–
Cantat-Gaudin et al.	2018	279.125	-8.194	0.468	-0.089	-2.561	–
Loktin & Popova	2017	279.15	-7.814	–	-2.729	-3.562	17.8
Kharchenko et al.	2016	279.125	-8.212	–	–	–	–
Dias et al.	2014	279.154	-7.813	–	0.54	4.18	–
Kharchenko et al.	2013	279.132	-8.21	–	-2.52	-2.0	17.8
Gozha et al.	2012	279.154	-7.813	–	–	–	–
Kharchenko et al.	2007	279.15	-7.81	–	0.1	–	–
van den Bergh	2006	279.175	-8.217	–	–	–	–
Kharchenko et al.	2003	279.18	-8.22	–	0.47	-1.02	–
Chen et al.	2003	279.209	-8.173	–	-0.31	-2.31	17.8
Dias et al.	2002	279.154	-7.813	–	-0.31	-2.31	18.58
Dambis	1999	279.154	-7.813	–	–	–	–

💡 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]	B_frac	BSS
UCC	99999–	1.76	2.2	2.42	24	-0.299	1545	–	0.0
Li et al.	2025	1.55	1.73	–	652	0.150	–	–	–
Almeida et al.	2025	1.94	2.44	–	13	–	1545	–	–
Hunt & Reffert	2024	–	–	–	–	–	3177⁽¹⁾	–	–
Cavallo et al.	2024	1.76	2.95	–	50	-0.460	–	–	–
Hunt & Reffert	2023	1.96	2.54	2.42	69	–	–	–	–
Just et al.	2023	–	–	–	79	–	147	–	–
Jaehnig et al.	2021	1.95⁽¹⁾	–	–	–	–	–	–	–
Rain et al.	2021	2.01	2.17	–	14	–	–	–	0
Dias et al.	2021	1.94	2.44	–	13	-0.138	–	–	–
Cantat-Gaudin et al.	2020	2.11	1.94	–	224	–	–	–	–
Cantat-Gaudin & Anders	2020	2.01	–	–	–	–	–	–	–
Dias et al.	2019	1.90	2.17	–	24	-2.028	–	–	–
Soubiran et al.	2018	2.01	–	–	–	–	–	–	–
Cantat-Gaudin et al.	2018	2.01	–	–	–	–	–	–	–
Loktin & Popova	2017	1.18	2.19	–	16	–	–	–	–
Kharchenko et al.	2016	1.71	2.29	–	79	–	–	–	–
Kharchenko et al.	2013	1.71	2.29	–	79	–	–	–	–
Gozha et al.	2012	1.16	–	–	15	–	–	–	–
van den Bergh	2006	1.16	2.20	–	14	–	–	–	–
Kharchenko et al.	2003	1.16	1.86	–	–	–	–	–	–
Chen et al.	2003	1.16	–	–	10	–	–	–	–
Dias et al.	2002	1.16	2.20	–	15	–	–	–	–
Dambis	1999	1.26	2.26	–	79	–	–	–	–

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

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
OC 0042	4.8	279.15	-8.13	0.5	-0.1	-2.6	-8.18	0.0

💡 Note: The % column shows the percentage of members that Collinder 385 shares with each listed object.

Visualization

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