Pickard 247

0.09 UTI

0.0

C_N

0.08

C_dens

0.75

C_C3

0.0

C_lit

0.52

C_dup

N₅₀ (P>50% members) 18

Stellar density (N₅₀/rad) 0.4 [N/pc²]

C3 classification AB

C_N 0.0 Sparse
C_dens 0.08 Very loose
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.52 Likely unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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Pickard 247 is a sparse, very loose object of high C3 quality. Its parallax locates it at a large distance, below the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It was recently reported in the literature.

Note: This is likely a unique object, which shares a moderate percentage of members with at least one previously reported entry. See table with shared members information.

Very distant High extinction Near-solar metallicity Very young

Data

🔍 Search references for Pickard 247 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–	167.687	-61.202	0.109	-5.737	2.052	–
Dias et al.	2026	167.653	-61.199	0.104	-5.752	2.042	–

💡 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–	8.64	3.18	–	13	0.025	–	–	–
Dias et al.	2026	8.64	3.18	–	13	0.025	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWNU 3568	48.0	167.69	-61.25	0.11	-5.69	2.09	–	0.16

💡 Note: The % column shows the percentage of members that Pickard 247 shares with each listed object.

Visualization

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