HSC 2054

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0.03 UTI
0.0
CN
0.05
Cdens
0.12
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 7.2 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.05 Very loose
  • CC3 0.12 Very low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 2054 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, old cluster, but with a large variance across recent sources for the metallicity parameter (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.

Distant Moderate extinction Near-solar metallicity Old

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as a moving group.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 120.672 -40.576 0.243 -3.329 5.195 58.813
Hu & Soubiran 2025 120.684 -40.565 – – – –
Cavallo et al. 2024 120.684 -40.565 0.244 – – –
Hunt & Reffert 2023 120.7 -40.534 0.246 -3.318 5.177 –

💡 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
Hu & Soubiran 2025 – – – – -0.310* – – –
Cavallo et al. 2024 3.36 1.37 – 1862 0.020 – – –
Hunt & Reffert 2023 3.63 1.55 1.63 238 – – – –

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Visualization

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