HSC 1442

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0.37 UTI
0.27
CN
0.7
Cdens
0.25
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members) 7.2 [arcmin]
  • CN 0.27 Poorly populated
  • Cdens 0.7 Moderately dense
  • CC3 0.25 Low quality
  • Clit 0.31 Poorly studied
  • Cdup 1.0 Unique

Overview

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HSC 1442 is a poorly populated, moderately dense object of low C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by moderate 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.

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

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 – 81.11 22.725 0.752 -0.435 1.08 26.39
Hu & Soubiran 2025 81.152 22.666 – – – –
Zhang et al. 2024 81.138 22.698 – – – –
Hunt & Reffert 2024 81.138 22.698 0.729 -0.453 1.116 26.381
Cavallo et al. 2024 81.152 22.666 0.734 – – –
Hunt & Reffert 2023 81.138 22.698 0.729 -0.453 1.116 26.381

💡 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 – – – – -0.050* – – –
Zhang et al. 2024 – – – – -0.251* – – –
Hunt & Reffert 2024 – – – – – 199* – –
Cavallo et al. 2024 1.41 1.99 – 891 0.520 – – –
Hunt & Reffert 2023 1.29 1.86 1.88 630 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 2936 96.3 81.1 22.73 0.75 -0.43 1.08 26.39 0.04

💡 Note: The % column shows the percentage of members that HSC 1442 shares with each listed object.

Visualization

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