HSC 2225

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0.08 UTI
0.0
CN
0.14
Cdens
0.25
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 0.7 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.14 Very loose
  • CC3 0.25 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 2225 is a sparse, very loose object of low C3 quality. Its parallax locates it at a very close distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age 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.

Liu et al. (2025)
Classified as tidal capture (resonant trapping binary) 222 along with HSC_2166.

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 99999– 155.698 -37.692 3.351 2.805 -5.787 -5.578
Cavallo et al. 2024 156.381 -37.766 3.365 – – –
Hunt & Reffert 2023 157.039 -38.785 3.378 2.91 -5.891 -4.494

💡 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– 0.3 0.16 0.31 245 0.090 – – –
Liu et al. 2025 0.36 0.12 – 309 – – – –
Cavallo et al. 2024 0.30 0.48 – 245 0.090 – – –
Hunt & Reffert 2023 0.29 0.16 0.31 166 – – – –

Visualization

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