OC 0462

0.00 UTI

0.0

C_N

0.31

C_dens

0.38

C_C3

0.0

C_lit

0.0

C_dup

C3 classification BC

Number of members (P>50%) 12

Radius (P>50% members) 2.5 [arcmin]

C_N 0.0 Sparse
C_dens 0.31 Loose
C_C3 0.38 Low quality
C_lit 0.0 Rarely studied
C_dup 0.0 Very likely duplicate

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

Overview

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OC 0462 is a sparse, loose object of low C3 quality. Its parallax locates it at a moderate distance, well below the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, very old cluster (see Parameters). It is rarely studied in the literature.

⚠️ Warning: This is very likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

High extinction Near-solar metallicity Very old

Data

🔍 Search references for OC 0462 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	–	111.579	-47.71	0.262	-1.421	2.773	22.096
Hao et al.	2022	111.584	-47.713	0.324	-1.418	2.79	–

💡 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
Hao et al.	2022	–	3.38	–	6310	0.112	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Melotte 66	100.0	111.58	-47.68	0.19	-1.43	2.77	21.66	1.0

💡 Note: The % column shows the percentage of members that OC 0462 shares with each listed object.

Visualization

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