HSC 2055

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0.17 UTI
0.0
CN
0.12
Cdens
0.25
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 2.9 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.12 Very loose
  • CC3 0.25 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 2055 is a sparse, very loose object of low C3 quality. Its parallax locates it at a large distance, above 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.

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

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.

Very distant Moderate extinction Near-solar metallicity Old

Cavallo et al. (2024)
Gold sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 130.21 -35.641 0.14 -2.862 4.083 92.254
Hu & Soubiran 2025 130.19 -35.636 – – – –
Hunt & Reffert 2024 130.197 -35.64 0.136 -2.874 4.08 92.247
Cavallo et al. 2024 130.19 -35.636 0.136 – – –
Hunt & Reffert 2023 130.197 -35.64 0.136 -2.874 4.08 92.247

💡 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 – – – – -0.120* – – –
Hunt & Reffert 2024 – – – – – 354* – –
Cavallo et al. 2024 5.32 1.62 – 1349 -0.770 – – –
Hunt & Reffert 2023 6.21 1.59 1.47 946 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3395 80.0 130.21 -35.64 0.14 -2.85 4.08 92.25 0.05

💡 Note: The % column shows the percentage of members that HSC 2055 shares with each listed object.

Visualization

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