IC 1848

(MWSC 236)

0.93 UTI

0.88

C_N

1.0

C_dens

0.75

C_C3

1.0

C_lit

1.0

C_dup

N₅₀ (P>50% members) 456

Stellar density (N₅₀/rad) 46.3 [N/pc²]

C3 classification AB

C_N 0.88 Rich
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 1.0 Very well-studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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IC 1848 is a rich, very dense object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a massive, near-solar metallicity, very young cluster, but with a large variance across recent sources for the mass parameter (see Parameters). It is very well-studied in the literature.

Note: This object shares a small percentage of members with 3 later reported entries. See table with shared members information.

Relatively close Moderate extinction Massive Near-solar metallicity Very young

Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: intermediate fit. Silver sample.

Cavallo et al. (2024)
Gold sample.

Data

🔍 Search references for IC 1848 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–	42.825	60.417	0.436	-0.393	-0.37	-22.34
Almeida et al.	2025	42.909	60.417	–	–	–	–
Hunt & Reffert	2024	42.791	60.408	0.443	-0.399	-0.415	-14.888
Celli et al.	2024	42.855	60.419	–	–	–	–
Cavallo et al.	2024	42.838	60.44	0.448	–	–	–
Hunt & Reffert	2023	42.791	60.408	0.443	-0.399	-0.415	-14.888
Just et al.	2023	42.764	60.408	–	–	–	–
Jaehnig et al.	2021	42.839	60.426	0.464	-0.327	-0.32	–
Rain et al.	2021	42.855	60.419	0.415	-0.372	-0.315	–
Dias et al.	2021	42.909	60.417	0.401	-0.374	-0.321	-57.452
Cantat-Gaudin et al.	2020	42.855	60.419	0.415	-0.372	-0.315	–
Cantat-Gaudin & Anders	2020	42.855	60.419	0.415	-0.372	-0.315	–
Soubiran et al.	2018	42.855	60.419	–	–	–	-53.36
Cantat-Gaudin et al.	2018	42.855	60.419	0.415	-0.372	-0.315	–
Loktin & Popova	2017	42.795	60.434	–	-0.731	-1.67	-47.4
Kharchenko et al.	2016	42.764	60.408	–	–	–	–
Dias et al.	2014	42.8	60.433	–	-1.39	-0.34	–
Kharchenko et al.	2013	42.777	60.41	–	-0.79	-0.89	-47.4
Gozha et al.	2012	42.8	60.434	–	–	–	–
Kharchenko et al.	2012	42.777	60.41	–	-0.72	-0.84	-47.38
Piskunov et al.	2008	42.789	60.425	–	–	–	–
Kharchenko et al.	2007	42.79	60.43	–	0.34	–	-29.24
Piskunov et al.	2007	42.789	60.425	–	–	–	–
van den Bergh	2006	42.337	60.634	–	–	–	–
Kharchenko et al.	2005	42.79	60.43	–	-2.51	-0.7	-29.24
Kharchenko et al.	2003	42.78	60.41	–	-3.78	-1.32	–
Chen et al.	2003	42.888	60.501	–	-5.15	0.35	-22.0
Dias et al.	2002	42.8	60.433	–	-5.15	0.35	-33.76
Dambis	1999	42.337	60.634	–	–	–	–

💡 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–	2.0	1.88	2.44	7	-0.150	1847	–	0.0
Almeida et al.	2025	2.00	1.88	–	12	–	1880	–	–
Hunt & Reffert	2024	–	–	–	–	–	1541⁽¹⁾	–	–
Celli et al.	2024	–	–	–	16	–	1847	–	–
Cavallo et al.	2024	1.96	1.97	–	6	-0.200	–	–	–
Hunt & Reffert	2023	2.07	1.86	2.44	9	–	–	–	–
Just et al.	2023	–	–	–	7	–	220	–	–
Jaehnig et al.	2021	2.14⁽¹⁾	–	–	–	–	–	–	–
Rain et al.	2021	2.25	2.05	–	5	–	–	–	0
Dias et al.	2021	2.00	1.88	–	12	-0.100	–	–	–
Cantat-Gaudin et al.	2020	2.40	1.75	–	16	–	–	–	–
Cantat-Gaudin & Anders	2020	2.25	–	–	–	–	–	–	–
Soubiran et al.	2018	2.25	–	–	–	–	–	–	–
Cantat-Gaudin et al.	2018	2.25	–	–	–	–	–	–	–
Loktin & Popova	2017	1.96	1.88	–	7	–	–	–	–
Kharchenko et al.	2016	1.50	2.08	–	7	–	–	–	–
Kharchenko et al.	2013	1.50	2.08	–	7	–	–	–	–
Gozha et al.	2012	2.00	–	–	7	–	9333	–	–
Kharchenko et al.	2012	1.50	2.08	–	7	–	–	–	–
Piskunov et al.	2008	2.00	1.86	–	4	–	4236⁽¹⁾	–	–
Piskunov et al.	2007	2.00	1.86	–	4	–	658	–	–
van den Bergh	2006	2.00	1.86	–	7	–	–	–	–
Kharchenko et al.	2005	2.00	1.86	–	4	–	–	–	–
Kharchenko et al.	2003	2.00	1.86	–	–	–	–	–	–
Chen et al.	2003	2.00	–	–	0	–	–	–	–
Dias et al.	2002	2.20	2.05	–	5	–	–	–	–
Dambis	1999	1.90	1.91	–	6	–	–	–	–

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
IRAS 02484+6022	21.9	43.04	60.56	0.43	-0.21	-0.33	-42.03	0.28
LP 09	15.1	42.8	60.44	0.45	-0.55	-0.45	-27.92	0.05
FSR 0608	3.3	42.82	60.6	0.46	-0.53	-0.39	-16.76	0.07

💡 Note: The % column shows the percentage of members that IC 1848 shares with each listed object.

Visualization

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