Cmg 902

0.29 UTI

0.68

C_N

0.14

C_dens

0.62

C_C3

0.0

C_lit

1.0

C_dup

N₅₀ (P>50% members) 87

Stellar density (N₅₀/rad) 0.7 [N/pc²]

C3 classification AC

C_N 0.68 Moderately populated
C_dens 0.14 Very loose
C_C3 0.62 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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Cmg 902 is a moderately populated, very loose object of intermediate C3 quality. Its parallax locates it at a moderate distance, well below 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.

Note: This object shares a small percentage of members with at least one entry reported in the same catalogue. See table with shared members information.

No fundamental parameters

Data

🔍 Search references for Cmg 902 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–	63.784	32.254	0.205	-0.053	-0.461	-17.913
Bica et al.	2019	63.785	32.24	–	–	–	–

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

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 1293	21.8	63.79	32.27	0.19	0.26	-0.66	-12.1	0.04
Cmg 903	11.5	63.98	32.29	0.16	-0.1	-0.96	-19.15	0.03

💡 Note: The % column shows the percentage of members that Cmg 902 shares with each listed object.

Visualization

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