HSC 2643

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

Overview

â„šī¸
HSC 2643 is a poorly populated, very 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, intermediate-age cluster, but with a large variance across recent sources for the age 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.

Palma et al. (2025)
Classified as optical pair P145, along with HSC_2638.

Cavallo et al. (2024)
Silver 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– 305.628 -81.005 3.98 8.752 -11.739 24.514
Cavallo et al. 2024 306.585 -80.959 4.028 – – –
Hunt & Reffert 2023 301.484 -80.997 4.034 9.033 -11.729 26.346

💡 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– 0.265 0.715 0.46 163 -0.060 – – –
Cavallo et al. 2024 0.28 1.00 – 62 -0.060 – – –
Hunt & Reffert 2023 0.25 0.43 0.46 264 – – – –

Visualization

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