LP 10

0.10 UTI

0.75

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

0.2

C_dup

C3 classification AB

Number of members (P>50%) 110

Radius (P>50% members) 3.2 [arcmin]

C_N 0.75 Rich
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.2 Likely duplicate

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

Overview

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LP 10 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 an intermediate-age cluster (see Parameters). It is rarely studied in the literature, with no articles listed in the last 9 years.

⚠️ Warning: This is likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

Relatively close Moderate extinction Intermediate age

Data

🔍 Search references for LP 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	–	43.534	60.654	0.442	-0.084	-0.253	-43.049
Loktin & Popova	2017	43.515	60.66	–	0.076	-1.523	–

💡 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
Loktin & Popova	2017	2.03	1.33	–	550	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
SAI 23	80.0	43.53	60.66	0.45	-0.1	-0.24	-43.05	0.48
OC 0255	22.7	43.54	60.66	0.47	-0.08	-0.23	–	0.0

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

Visualization

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