HSC 1697

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0.32 UTI
0.3
CN
0.44
Cdens
0.38
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 3.8 [arcmin]
  • CN 0.3 Poorly populated
  • Cdens 0.44 Loose
  • CC3 0.38 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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HSC 1697 is a poorly populated, loose object of low C3 quality. Its parallax locates it at a moderate distance, near 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.

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 – 103.988 -2.291 0.299 -0.696 -0.713 –
Hu & Soubiran 2025 103.981 -2.29 – – – –
Hunt & Reffert 2024 103.995 -2.272 0.286 -0.691 -0.727 –
Cavallo et al. 2024 103.981 -2.29 0.29 – – –
Hunt & Reffert 2023 103.995 -2.272 0.286 -0.691 -0.727 –

💡 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 – – – – -0.200* – – –
Hunt & Reffert 2024 – – – – – 281* – –
Cavallo et al. 2024 2.99 1.98 – 603 0.350 – – –
Hunt & Reffert 2023 3.09 1.98 1.97 210 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3270 86.7 103.99 -2.29 0.29 -0.7 -0.71 – 0.02

💡 Note: The % column shows the percentage of members that HSC 1697 shares with each listed object.

Visualization

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