G3CC 17

0.08 UTI

0.0

C_N

0.05

C_dens

0.38

C_C3

0.0

C_lit

0.96

C_dup

N₅₀ (P>50% members) 11

Stellar density (N₅₀/rad) 0.2 [N/pc²]

C3 classification BC

C_N 0.0 Sparse
C_dens 0.05 Very loose
C_C3 0.38 Low quality
C_lit 0.0 Rarely studied
C_dup 0.96 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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G3CC 17 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate^* distance, near the mid-plane. It is catalogued as a cluster (see Parameters). It is rarely studied in the literature, with no articles listed in the last 13 years.

(*): The parallax distance estimate (~2.97 kpc) differs significantly from the median photometric distance (~5.74 kpc).

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

⚠️ Warning: the low UTI value and no obvious signs of duplication (C_dup=0.96) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Very distant

Morales et al. (2013)
Classified as morphological type 'EC2' (partially embedded cluster). Morphological flag: cluster partially embedded.

Data

🔍 Search references for G3CC 17 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–	216.336	-60.587	0.337	-6.492	-2.612	-20.087
Morales et al.	2013	216.314	-60.589	–	–	–	–

💡 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–	5.74	–	–	–	–	–	–	–
Morales et al.	2013	5.74	–	–	–	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
MCM 52	4.0	216.21	-60.45	0.33	-6.5	-2.3	-27.24	0.07

💡 Note: The % column shows the percentage of members that G3CC 17 shares with each listed object.

Visualization

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