HSC 485

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0.43 UTI
0.25
CN
0.67
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 5.9 [arcmin]
  • CN 0.25 Poorly populated
  • Cdens 0.67 Moderately dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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HSC 485 is a poorly populated, moderately dense object of high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.
Relatively close Moderate 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 – 296.745 23.071 0.629 -0.29 -0.611 -4.031
Hu & Soubiran 2025 296.768 23.103 – – – –
Hunt & Reffert 2024 296.74 23.066 0.647 -0.314 -0.593 -4.715
Cavallo et al. 2024 296.768 23.103 0.647 – – –
Hunt & Reffert 2023 296.74 23.066 0.647 -0.314 -0.593 -4.715

💡 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 – – – – 0.040* – – –
Hunt & Reffert 2024 – – – – – 180* – –
Cavallo et al. 2024 1.34 2.28 – 617 -0.260 – – –
Hunt & Reffert 2023 1.50 1.95 1.02 480 – – – –

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

Visualization

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