Dzeta Scul

0.12 UTI

0.0

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

0.29

C_dup

C3 classification AA

Number of members (P>50%) 24

Radius (P>50% members) 6.0 [arcmin]

C_N 0.0 Sparse
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.29 Possibly duplicate

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

Overview

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Dzeta Scul is a sparse, very dense object of very high C3 quality. Its parallax locates it at a very close distance, below the mid-plane, affected by low extinction. It is catalogued as a young cluster (see Parameters). It is rarely studied in the literature, with no articles listed in the last 9 years.

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

Very close Low extinction Young

Data

🔍 Search references for Dzeta Scul 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	–	0.425	-30.204	4.214	18.721	2.39	6.901
Loktin & Popova	2017	0.42	-30.217	–	–	–	–

💡 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
Loktin & Popova	2017	0.27	0.03	–	63	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Blanco 1	70.8	1.22	-29.95	4.23	18.75	2.6	5.19	1.0
CWWDL 14677	62.5	1.03	-30.01	4.23	18.75	2.61	5.52	0.0

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

Visualization

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