HSC 1897

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0.32 UTI
0.57
CN
0.28
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 1.4 [N/pc2]
  • CN 0.57 Moderately populated
  • Cdens 0.28 Loose
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 1897 is a moderately populated, loose object of high C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, 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 primordial binary cluster 213 along with HSC_1911.

Palma et al. (2025)
Classified as genetic pair P221, along with HSC_1911.

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– 115.129 -21.343 1.518 -5.988 4.222 36.126
Cavallo et al. 2024 114.693 -21.029 1.525 – – –
Hunt & Reffert 2023 115.148 -21.553 1.516 -5.989 4.184 36.515

💡 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– 0.63 0.12 0.59 51 0.190 – – –
Liu et al. 2025 0.62 0.01 – 51 – – – –
Cavallo et al. 2024 0.69 0.27 – 23 0.190 – – –
Hunt & Reffert 2023 0.63 0.12 0.59 89 – – – –

Visualization

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