HSC 1487

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0.16 UTI
0.26
CN
0.21
Cdens
0.12
CC3
0.1
Clit
1.0
Cdup
Core radius and density 1.2 [pc], 1.1 [pc-2]
  • CN 0.26 Poorly populated
  • Cdens 0.21 Very loose
  • CC3 0.12 Very low quality
  • Clit 0.1 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 1487 is a poorly populated, very loose object of very low C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age 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.

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.70 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.70 (50th percentile).

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 92.838 23.647 0.227 0.895 -0.264 31.975
Hu & Soubiran 2025 92.847 23.664 – – – –
Zhang et al. 2024 92.846 23.649 – – – –
Hunt & Reffert 2024 92.846 23.649 0.225 0.925 -0.3 40.441
Cavallo et al. 2024 92.847 23.664 0.218 – – –
Hunt & Reffert 2023 92.846 23.649 0.225 0.925 -0.3 40.441

💡 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– 3.99 1.59 1.44 874 -0.229 195 – –
Hu & Soubiran 2025 – – – – -0.250(5) – – –
Zhang et al. 2024 – – – – -0.229(1) – – –
Hunt & Reffert 2024 3.99 1.59 1.44 874 – 195(1) – –
Cavallo et al. 2024 3.65 1.78 – 631 0.140 – – –
Hunt & Reffert 2023 3.99 1.59 1.44 875 – – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Visualization

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