Pickard 80

0.07 UTI

0.0

C_N

0.05

C_dens

0.38

C_C3

0.0

C_lit

0.84

C_dup

N₅₀ (P>50% members) 17

Stellar density (N₅₀/rad) 0.2 [N/pc²]

C3 classification BC

C_N 0.0 Sparse
C_dens 0.05 Very loose
C_C3 0.38 Low quality
C_lit 0.0 Rarely studied
C_dup 0.84 Very likely unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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Pickard 80 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It was recently reported in the literature.

Note: This is very likely a unique object, which shares a small percentage of members with at least one previously reported entry. See table with shared members information.

⚠️ Warning: the low UTI value and no obvious signs of duplication (C_dup=0.84) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Relatively close Moderate extinction Near-solar metallicity Very young

Data

🔍 Search references for Pickard 80 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–	24.337	61.007	0.324	-1.351	-0.437	–
Dias et al.	2026	24.295	61.013	0.302	-1.376	-0.423	–

💡 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–	2.98	1.38	–	14	-0.046	–	–	–
Dias et al.	2026	2.98	1.38	–	14	-0.046	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWWDL 8467	16.0	24.7	61.08	0.33	-1.29	-0.51	–	0.15
UBC 602	12.0	24.6	60.67	0.34	-1.21	-0.51	300.88	0.37
Trumpler 1	4.0	23.91	61.29	0.35	-1.63	-0.58	–	0.96

💡 Note: The % column shows the percentage of members that Pickard 80 shares with each listed object.

Visualization

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