Saloranta 10

0.63 UTI

0.72

C_N

1.0

C_dens

0.75

C_C3

0.35

C_lit

1.0

C_dup

N₅₀ (P>50% members) 93

Stellar density (N₅₀/rad) 16.3 [N/pc²]

C3 classification AB

C_N 0.72 Moderately populated
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.35 Poorly studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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Saloranta 10 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is poorly studied in the literature.

Note: This object shares a large percentage of members with 2 later reported entries. See table with shared members information.

Relatively close Moderate extinction Near-solar metallicity Intermediate age

Liu et al. (2025)
Classified as tidal capture (resonant trapping binary) 336 along with NGC_1912.

Palma et al. (2025)
Classified as optical pair P423, along with HSC_1333.

Cavallo et al. (2024)
Gold sample.

Data

🔍 Search references for Saloranta 10 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–	81.227	37.576	0.9	0.28	-4.309	14.411
Zhang et al.	2024	81.215	37.566	–	–	–	–
Hunt & Reffert	2024	81.215	37.566	0.896	0.301	-4.312	4.217
Cavallo et al.	2024	81.216	37.547	0.895	–	–	–
Hunt & Reffert	2023	81.215	37.566	0.896	0.301	-4.312	4.217
Bica et al.	2019	81.22	37.542	–	–	–	–

💡 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–	1.1	1.11	0.76	144	-0.009	382	–	–
Liu et al.	2025	2.12	0.49	–	89	–	–	–	–
Zhang et al.	2024	–	–	–	–	-0.127⁽¹⁾	–	–	–
Hunt & Reffert	2024	–	–	–	–	–	382⁽¹⁾	–	–
Cavallo et al.	2024	1.10	1.22	–	316	0.110	–	–	–
Hunt & Reffert	2023	1.05	1.11	0.76	144	–	–	–	–

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

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
COIN-Gaia 17	98.9	81.23	37.57	0.89	0.29	-4.31	8.92	0.07
UBC 89	96.8	81.23	37.57	0.9	0.29	-4.3	14.41	0.01

💡 Note: The % column shows the percentage of members that Saloranta 10 shares with each listed object.

Visualization

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