MWSC 5022

0.19 UTI

0.0

C_N

0.07

C_dens

0.38

C_C3

0.25

C_lit

1.0

C_dup

N₅₀ (P>50% members) 24

Stellar density (N₅₀/rad) 0.3 [N/pc²]

C3 classification BC

C_N 0.0 Sparse
C_dens 0.07 Very loose
C_C3 0.38 Low quality
C_lit 0.25 Poorly studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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MWSC 5022 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate^* distance, well above the mid-plane, affected by low extinction. It is catalogued as a low-mass, old cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~4.01 kpc) differs significantly from the median photometric distance (~1.31 kpc).

⚠️ Warning: the low UTI value and no obvious signs of duplication (C_dup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Relatively close Low extinction Low mass Old

Data

🔍 Search references for MWSC 5022 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–	124.114	0.489	0.249	-1.932	-0.392	–
Just et al.	2023	124.093	0.453	–	–	–	–
Bica et al.	2019	124.092	0.451	–	–	–	–
Kharchenko et al.	2016	124.093	0.453	–	–	–	–
Schmeja et al.	2014	124.099	0.45	–	3.36	-2.5	–

💡 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–	1.31	0.64	–	1479	–	26	–	–
Just et al.	2023	–	–	–	1479	–	26	–	–
Kharchenko et al.	2016	1.31	0.64	–	1479	–	–	–	–
Schmeja et al.	2014	1.31	0.64	–	1479	–	–	–	–

Visualization

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