FSR 0962

(MWSC 856)

0.23 UTI

0.27

C_N

0.15

C_dens

0.12

C_C3

0.31

C_lit

1.0

C_dup

C3 classification DC

Number of members (P>50%) 27

Radius (P>50% members) 4.5 [arcmin]

C_N 0.27 Poorly populated
C_dens 0.15 Very loose
C_C3 0.12 Very low quality
C_lit 0.31 Poorly studied
C_dup 1.0 Unique

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

Overview

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FSR 0962 is a poorly populated, very loose object of very low C3 quality. Its parallax locates it at a moderate^* distance, above the mid-plane, affected by moderate extinction. It is catalogued as an intermediate-age cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~4.51 kpc) differs significantly from the median photometric distance (~2.67 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 Moderate extinction Intermediate age

Data

🔍 Search references for FSR 0962 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	–	95.964	14.093	0.222	-0.15	-0.699	46.505
Just et al.	2023	95.955	14.102	–	–	–	–
Bica et al.	2019	95.943	14.081	–	–	–	–
Kharchenko et al.	2016	95.955	14.102	–	–	–	–
Kharchenko et al.	2013	95.962	14.1	–	-0.68	-2.41	–
Froebrich et al.	2007	95.958	14.086	–	–	–	–

💡 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	–	–	–	861	–	604	–	–
Kharchenko et al.	2016	2.67	1.62	–	861	–	–	–	–
Kharchenko et al.	2013	2.67	1.62	–	861	–	–	–	–

Visualization

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