NGC 2202

0.25 UTI

0.0

C_N

0.21

C_dens

0.25

C_C3

0.4

C_lit

1.0

C_dup

N₅₀ (P>50% members) 19

Stellar density (N₅₀/rad) 1.0 [N/pc²]

C3 classification CC

C_N 0.0 Sparse
C_dens 0.21 Very loose
C_C3 0.25 Low quality
C_lit 0.4 Poorly studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

ℹ️

NGC 2202 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate^* distance, below the mid-plane, affected by low extinction. It is catalogued as a low-mass, near-solar metallicity, intermediate-age cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~3.27 kpc) differs significantly from the median photometric distance (~0.90 kpc).

Close Low extinction Low mass Near-solar metallicity Intermediate age

Data

🔍 Search references for NGC 2202 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	99999–	94.237	6.0	0.306	-0.052	-0.97	-0.461
Zhang et al.	2024	94.207	5.985	–	–	–	–
Hunt & Reffert	2024	94.207	5.985	1.162	-0.909	-3.778	14.179
He et al.	2023	94.268	5.985	0.366	-0.051	-1.016	-0.46
Donor et al.	2020	94.215	6.027	–	-0.97	0.53	52.8
Dias et al.	2014	94.208	5.997	–	0.36	-0.08	–
Piskunov et al.	2008	94.212	6.0	–	–	–	–
Kharchenko et al.	2005	94.21	6.0	–	0.42	1.52	–

💡 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–	0.9	0.0	–	550	-0.058	41	–	–
Zhang et al.	2024	–	–	–	–	0.025⁽¹⁾	–	–	–
Hunt & Reffert	2024	–	–	–	–	–	41⁽¹⁾	–	–
He et al.	2023	3.63	1.50	–	63	–	–	–	–
Donor et al.	2020	–	–	–	–	-0.140	–	–	–
Piskunov et al.	2008	0.90	0.00	–	550	–	–	–	–
Kharchenko et al.	2005	0.90	0.00	–	550	–	–	–	–

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

Visualization

ℹ️