HSC 1057

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0.53 UTI
0.52
CN
1.0
Cdens
0.62
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 1.7 [arcmin]
  • CN 0.52 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 0.62 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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HSC 1057 is a moderately populated, very dense object of intermediate C3 quality. Its parallax locates it at a large* distance, above 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.

(*): The parallax distance estimate (~6.57 kpc) differs significantly from the median photometric distance (~4.71 kpc).

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 – 30.722 64.42 0.152 -0.748 -0.018 -63.033
Hu & Soubiran 2025 30.774 64.437 – – – –
Hunt & Reffert 2024 30.72 64.42 0.141 -0.764 -0.009 -63.334
Cavallo et al. 2024 30.774 64.437 0.148 – – –
Hunt & Reffert 2023 30.72 64.42 0.141 -0.764 -0.009 -63.334

💡 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 – – – – -0.160* – – –
Hunt & Reffert 2024 – – – – – 746* – –
Cavallo et al. 2024 3.96 2.33 – 661 -0.800 – – –
Hunt & Reffert 2023 5.45 2.23 1.49 329 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3163 98.1 30.73 64.42 0.15 -0.74 -0.04 -63.03 0.13

💡 Note: The % column shows the percentage of members that HSC 1057 shares with each listed object.

Visualization

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