Melotte 96

(Collinder 206; VDBH 59; NGC 2818A; OCL 743; vdBergh-Hagen 59; ESO 372 14; FSR 1408; MWSC 1644)

0.06 UTI

0.89

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

0.11

C_dup

N₅₀ (P>50% members) 476

Stellar density (N₅₀/rad) 17.8 [N/pc²]

C3 classification AA

C_N 0.89 Rich
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.11 Likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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Melotte 96 is a rich, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane. No fundamental parameter values are available for this object. It is rarely studied in the literature, with no articles listed in the last 7 years.

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

No fundamental parameters

Data

🔍 Search references for Melotte 96 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–	139.044	-36.625	0.303	-4.423	4.543	20.624
Bica et al.	2019	139.036	-36.629	–	–	–	–

💡 Note: The UCC values are estimated from its identified members.

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
NGC 2818	89.3	139.04	-36.62	0.3	-4.42	4.54	20.62	0.98

💡 Note: The % column shows the percentage of members that Melotte 96 shares with each listed object.

Visualization

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