Loden 466

0.03 UTI

0.0

C_N

0.16

C_dens

0.0

C_C3

0.0

C_lit

1.0

C_dup

N₅₀ (P>50% members) 24

Stellar density (N₅₀/rad) 0.8 [N/pc²]

C3 classification DD

C_N 0.0 Sparse
C_dens 0.16 Very loose
C_C3 0.0 Very low quality
C_lit 0.0 Rarely studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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Loden 466 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It is rarely studied in the literature, with no articles listed in the last 7 years.

⚠️ 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 Near-solar metallicity Very young

Data

🔍 Search references for Loden 466 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–	175.882	-62.549	0.452	-5.214	-5.527	–
Monteiro & Dias	2019	175.925	-62.537	–	-6.365	0.751	2.41
Dias et al.	2014	175.925	-62.517	–	-5.41	-6.01	-12.91
Dias et al.	2002	175.925	-62.517	–	-5.42	-6.02	-12.91

💡 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–	2.93	0.94	–	14	0.041	–	–	–
Monteiro & Dias	2019	2.93	0.94	–	14	0.041	–	–	–

Visualization

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