MWSC 5010

0.23 UTI

0.25

C_N

0.16

C_dens

0.25

C_C3

0.25

C_lit

1.0

C_dup

C3 classification BD

Number of members (P>50%) 25

Radius (P>50% members) 11.6 [arcmin]

C_N 0.25 Poorly populated
C_dens 0.16 Very loose
C_C3 0.25 Low quality
C_lit 0.25 Poorly studied
C_dup 1.0 Unique

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

Overview

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MWSC 5010 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a relatively close^* distance, well above the mid-plane, affected by low extinction. It is catalogued as an old cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~1.68 kpc) differs significantly from the median photometric distance (~3.55 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.

Distant Low extinction Old

Data

🔍 Search references for MWSC 5010 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	–	94.603	86.024	0.596	-0.598	-1.158	-33.08
Just et al.	2023	94.513	86.037	–	–	–	–
Bica et al.	2019	94.575	86.041	–	–	–	–
Kharchenko et al.	2016	94.513	86.037	–	–	–	–
Schmeja et al.	2014	94.575	86.035	–	2.68	-2.38	–

💡 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
Just et al.	2023	–	–	–	2818	–	741	–	–
Kharchenko et al.	2016	3.55	0.45	–	2818	–	–	–	–
Schmeja et al.	2014	3.55	0.45	–	2818	–	–	–	–

Visualization

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