HSC 1667

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0.28 UTI
0.0
CN
0.42
Cdens
1.0
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 2.1 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.42 Loose
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 1667 is a sparse, loose object of very high C3 quality. Its parallax locates it at a very close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, very young cluster, but with a large variance across recent sources for the absorption parameter (see Parameters). It was recently reported in the literature.

Liu et al. (2025)
Classified as tidal capture (resonant trapping binary) 84 along with CWNU_1015.

Palma et al. (2025)
Classified as optical pair P289, along with CWNU_1057.

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– 80.765 -8.55 6.405 8.646 -12.356 24.046
Cavallo et al. 2024 80.539 -7.671 6.412 – – –
Hunt & Reffert 2023 81.034 -8.667 6.403 8.583 -12.714 24.75

💡 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– 0.15 0.92 0.63 11 0.360 – – –
Liu et al. 2025 0.18 0.02 – 8 – – – –
Cavallo et al. 2024 0.15 0.92 – 25 0.360 – – –
Hunt & Reffert 2023 0.15 1.39 0.63 11 – – – –

Visualization

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