FSR 0702

0.34 UTI

0.61

C_N

0.06

C_dens

0.75

C_C3

0.13

C_lit

1.0

C_dup

N_m (P>50%) 72

Core radius and density 1.0 [pc], 0.3 [pc^-2]

C3 classification AB

C_N 0.61 Moderately populated
C_dens 0.06 Very loose
C_C3 0.75 High quality
C_lit 0.13 Rarely studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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FSR 0702 is a moderately populated, very loose object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is rarely studied in the literature.

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

Distant Moderate extinction Near-solar metallicity Young

Cavallo et al. (2024)
Silver sample.

Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.53 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.53 (50th percentile).

Data

🔍 Search references for FSR 0702 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–	72.91	45.748	0.203	0.357	-0.402	-55.284
Hunt & Reffert	2024	72.919	45.776	0.197	0.354	-0.387	-24.018
Cavallo et al.	2024	72.907	45.743	0.192	–	–	–
Hunt & Reffert	2023	72.919	45.776	0.197	0.354	-0.387	-24.018
Sampedro et al.	2017	72.917	45.765	–	0.65	-2.28	–
Froebrich et al.	2007	72.917	45.765	–	–	–	–
Dias et al.	2002	72.917	45.765	–	-2.75	-4.91	–

💡 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–	4.05	2.97	2.27	28	0.430	993	–	–
Hunt & Reffert	2024	4.26	2.97	2.27	20	–	993⁽¹⁾	–	–
Cavallo et al.	2024	3.84	2.57	–	35	0.430	–	–	–
Hunt & Reffert	2023	4.26	2.97	2.27	20	–	–	–	–
Dias et al.	2002	2.50	3.15	–	794	–	–	–	–

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

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWNU 1688	50.0	72.9	45.72	0.21	0.31	-0.44	–	0.0

💡 Note: The % column shows the percentage of members that FSR 0702 shares with each listed object.

Visualization

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