HSC 1202

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0.22 UTI
0.0
CN
0.37
Cdens
0.12
CC3
0.3
Clit
1.0
Cdup
Stellar density (N50/rad) 1.8 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.37 Loose
  • CC3 0.12 Very low quality
  • Clit 0.3 Poorly studied
  • Cdup 1.0 Unique

Overview

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HSC 1202 is a sparse, loose object of very low 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, young cluster (see Parameters). It was recently reported in the literature.

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Liu et al. (2025)
Classified as tidal capture (resonant trapping binary) 186 along with UBC_51.

Palma et al. (2025)
Part of multiple system G105, along with HSC_1193 and UBC_51.

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 99999– 61.467 50.935 0.907 -0.082 -2.158 -13.466
Zhang et al. 2024 61.495 50.934 – – – –
Hunt & Reffert 2024 61.495 50.934 0.918 -0.058 -2.158 -1.333
Cavallo et al. 2024 61.583 50.942 0.923 – – –
Hunt & Reffert 2023 61.495 50.934 0.918 -0.058 -2.158 -1.333

💡 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] Bfrac BSS
UCC 99999– 1.16 1.6 0.54 95 -0.148 67 – –
Liu et al. 2025 2.32 0.56 – 95 – – – –
Zhang et al. 2024 – – – – -0.216(1) – – –
Hunt & Reffert 2024 – – – – – 67(1) – –
Cavallo et al. 2024 1.16 1.83 – 69 -0.080 – – –
Hunt & Reffert 2023 1.05 1.60 0.54 115 – – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Visualization

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