HSC 1021

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0.37 UTI
0.28
CN
0.19
Cdens
0.75
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members) 4.8 [arcmin]
  • CN 0.28 Poorly populated
  • Cdens 0.19 Very loose
  • CC3 0.75 High quality
  • Clit 0.31 Poorly studied
  • Cdup 1.0 Unique

Overview

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HSC 1021 is a poorly populated, very loose object of high C3 quality. Its parallax locates it at a moderate distance, below 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.

Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.

Distant 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 – 20.544 57.237 0.256 -2.117 -1.091 -62.619
Hu & Soubiran 2025 20.546 57.249 – – – –
Zhang et al. 2024 20.674 57.221 – – – –
Hunt & Reffert 2024 20.674 57.221 0.258 -2.08 -1.097 -55.353
Cavallo et al. 2024 20.546 57.249 0.255 – – –
Hunt & Reffert 2023 20.674 57.221 0.258 -2.08 -1.097 -55.353

💡 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 – – – – -0.170* – – –
Zhang et al. 2024 – – – – -0.254* – – –
Hunt & Reffert 2024 – – – – – 130* – –
Cavallo et al. 2024 3.08 1.19 – 617 0.030 – – –
Hunt & Reffert 2023 3.43 1.25 1.68 469 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3279 85.7 20.44 57.25 0.25 -2.12 -1.11 -62.62 0.06

💡 Note: The % column shows the percentage of members that HSC 1021 shares with each listed object.

Visualization

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