HSC 2380

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0.11 UTI
0.0
CN
0.28
Cdens
0.25
CC3
0.0
Clit
1.0
Cdup
Core radius and density 1.0 [pc], 1.4 [pc-2]
  • CN 0.0 Sparse
  • Cdens 0.28 Loose
  • CC3 0.25 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 2380 is a sparse, loose object of low C3 quality. Its parallax locates it at a very close distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Palma et al. (2025)
Classified as optical pair (not dynamically associated) P142, along with HSC_2336.

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as moving group. CMD class: 0.90 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.90 (50th percentile).

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 131.395 -74.256 3.354 -3.006 12.843 12.844
Cavallo et al. 2024 132.089 -73.681 3.315 – – –
Hunt & Reffert 2023 130.964 -74.375 3.317 -3.301 12.513 6.977

💡 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] Bfrac BSS
UCC 99999– 0.31 0.45 0.6 78 0.420 – – –
Cavallo et al. 2024 0.32 0.68 – 63 0.420 – – –
Hunt & Reffert 2023 0.30 0.22 0.60 94 – – – –

Visualization

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