FSR 0902

(MWSC 832)

0.72 UTI

0.67

C_N

1.0

C_dens

0.75

C_C3

0.6

C_lit

1.0

C_dup

C3 classification AB

Number of members (P>50%) 84

Radius (P>50% members) 5.5 [arcmin]

C_N 0.67 Moderately populated
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.6 Moderately studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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FSR 0902 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a relatively close^* distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It is moderately studied in the literature.

(*): The parallax distance estimate (~1.96 kpc) differs significantly from the median photometric distance (~1.24 kpc).

Note: This object shares a moderate percentage of members with a later reported entry. See table with shared members information.

Relatively close Moderate extinction Near-solar metallicity Very young

Cavallo et al. (2024)
Gold sample.

Data

🔍 Search references for FSR 0902 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	–	94.578	20.549	0.509	0.45	-2.649	18.882
Zhang et al.	2024	94.578	20.562	–	–	–	–
Hunt & Reffert	2024	94.578	20.562	0.513	0.443	-2.625	8.103
Cavallo et al.	2024	94.617	20.556	0.514	–	–	–
Hunt & Reffert	2023	94.578	20.562	0.513	0.443	-2.625	8.103
Just et al.	2023	94.567	20.542	–	–	–	–
Bica et al.	2019	94.586	20.528	–	–	–	–
Kharchenko et al.	2016	94.567	20.542	–	–	–	–
Kharchenko et al.	2013	94.575	20.54	–	-0.51	-5.5	–
Froebrich et al.	2007	94.579	20.528	–	–	–	–
Dias et al.	2002	94.579	20.528	–	2.28	-5.23	–

💡 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]	Bfr	BSS
Zhang et al.	2024	–	–	–	–	-0.182*	–	–	–
Hunt & Reffert	2024	–	–	–	–	–	346*	–	–
Cavallo et al.	2024	1.62	1.43	–	11	-0.080	–	–	–
Hunt & Reffert	2023	1.81	1.31	1.54	5	–	–	–	–
Just et al.	2023	–	–	–	14	–	86	–	–
Kharchenko et al.	2016	1.24	1.23	–	14	–	–	–	–
Kharchenko et al.	2013	1.24	1.23	–	14	–	–	–	–
Dias et al.	2002	1.24	1.23	–	14	–	–	–	–

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 1308	29.8	94.57	20.56	0.51	0.36	-2.62	2.98	0.0

💡 Note: The % column shows the percentage of members that FSR 0902 shares with each listed object.

Visualization

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