IRAS 02484+6022

0.28 UTI

0.8

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

0.56

C_dup

N₅₀ (P>50% members) 227

Stellar density (N₅₀/rad) 12.5 [N/pc²]

C3 classification AB

C_N 0.8 Rich
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.56 Likely unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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IRAS 02484+6022 is a rich, very dense object of high C3 quality. Its parallax locates it at a moderate distance, above 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 23 years.

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.

Relatively close

Lada & Lada (2003)
Embedded cluster within ∼2 Kpc of the Sun.

Data

🔍 Search references for IRAS 02484+6022 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–	43.043	60.562	0.429	-0.205	-0.328	-42.031
Lada & Lada	2003	43.078	60.583	–	–	–	–

💡 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–	2.4	–	–	–	–	55	–	–
Lada & Lada	2003	2.40	–	–	–	–	55	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
IC 1848	44.1	42.83	60.42	0.44	-0.39	-0.37	-22.34	0.93
LP 10	11.9	43.53	60.65	0.44	-0.08	-0.25	-43.05	0.1
SAI 23	9.7	43.53	60.66	0.45	-0.1	-0.24	-43.05	0.37
LP 09	4.8	42.8	60.44	0.45	-0.55	-0.45	-27.92	0.05
FSR 0608	1.3	42.82	60.6	0.46	-0.53	-0.39	-16.76	0.07

💡 Note: The % column shows the percentage of members that IRAS 02484+6022 shares with each listed object.

Visualization

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