CKCWDM 47285

0.08 UTI

0.33

C_N

0.08

C_dens

0.25

C_C3

0.0

C_lit

0.61

C_dup

N₅₀ (P>50% members) 33

Stellar density (N₅₀/rad) 0.4 [N/pc²]

C3 classification DB

C_N 0.33 Poorly populated
C_dens 0.08 Very loose
C_C3 0.25 Low quality
C_lit 0.0 Rarely studied
C_dup 0.61 Likely unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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CKCWDM 47285 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a large distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age 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 Moderate extinction Near-solar metallicity Intermediate age

Data

🔍 Search references for CKCWDM 47285 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–	147.997	-52.149	0.163	-4.764	3.227	21.232
Chi et al.	2025	148.184	-52.056	0.149	-4.76	3.25	–

💡 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–	6.73	2.92	–	821	-0.289	–	–	–
Chi et al.	2025	6.73	2.92	–	821	-0.289	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
OC 0522	39.4	147.91	-52.21	0.14	-4.75	3.21	89.19	0.13

💡 Note: The % column shows the percentage of members that CKCWDM 47285 shares with each listed object.

Visualization

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