UPK 152

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0.34 UTI
0.31
CN
0.25
Cdens
0.25
CC3
0.45
Clit
1.0
Cdup
Stellar density (N50/rad) 1.3 [N/pc2]
  • CN 0.31 Poorly populated
  • Cdens 0.25 Loose
  • CC3 0.25 Low quality
  • Clit 0.45 Poorly studied
  • Cdup 1.0 Unique

Overview

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UPK 152 is a poorly populated, loose object of low C3 quality. Its parallax locates it at a close 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 is poorly studied in the literature.

Cavallo et al. (2024)
Gold sample.

Almeida et al. (2025)
Mass determination: worst fit. Isochrone match: intermediate fit.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 319.24 56.375 1.356 3.707 -1.256 -11.398
Almeida et al. 2025 319.244 56.199 – – – –
Hunt & Reffert 2024 319.341 56.287 1.339 3.685 -1.297 -10.559
Cavallo et al. 2024 319.191 56.307 1.343 – – –
Hunt & Reffert 2023 319.341 56.287 1.339 3.685 -1.297 -10.559
Dias et al. 2021 319.244 56.199 1.325 3.707 -1.25 –
Cantat-Gaudin et al. 2020 319.315 56.25 1.324 3.655 -1.208 –
Cantat-Gaudin & Anders 2020 319.301 56.258 1.326 3.72 -1.224 –
Sim et al. 2019 319.126 56.206 – 3.73 -1.17 –

💡 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– 0.745 2.31 1.48 148 0.146 64 – –
Almeida et al. 2025 0.75 2.31 – 148 – 67 – –
Hunt & Reffert 2024 – – – – – 60(1) – –
Cavallo et al. 2024 0.87 2.58 – 46 0.320 – – –
Hunt & Reffert 2023 0.71 2.17 1.48 192 – – – –
Dias et al. 2021 0.75 2.31 – 148 -0.028 – – –
Cantat-Gaudin & Anders 2020 0.74 – – – – – – –
Sim et al. 2019 0.74 – – 1000 – – – –

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

Visualization

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