HSC 831

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0.30 UTI
0.25
CN
0.38
Cdens
0.38
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 2.2 [arcmin]
  • CN 0.25 Poorly populated
  • Cdens 0.38 Loose
  • CC3 0.38 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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HSC 831 is a poorly populated, loose object of low C3 quality. Its parallax locates it at a large* distance, above the mid-plane, affected by high 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.

(*): The parallax distance estimate (~5.64 kpc) differs significantly from the median photometric distance (~4.12 kpc).

Distant High extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Gold sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 339.913 58.979 0.177 -3.562 -1.335 –
Hu & Soubiran 2025 339.885 58.976 – – – –
Hunt & Reffert 2024 339.916 58.986 0.191 -3.532 -1.314 –
Cavallo et al. 2024 339.885 58.976 0.189 – – –
Hunt & Reffert 2023 339.916 58.986 0.191 -3.532 -1.314 –

💡 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] Bfr BSS
Hu & Soubiran 2025 – – – – -0.140* – – –
Hunt & Reffert 2024 – – – – – 466* – –
Cavallo et al. 2024 3.77 3.15 – 1072 0.330 – – –
Hunt & Reffert 2023 4.46 3.57 1.34 419 – – – –

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Visualization

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