UPK 110

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0.20 UTI
0.37
CN
0.11
Cdens
0.38
CC3
0.06
Clit
1.0
Cdup
Core radius and density 1.3 [pc], 0.6 [pc-2]
  • CN 0.37 Poorly populated
  • Cdens 0.11 Very loose
  • CC3 0.38 Low quality
  • Clit 0.06 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
UPK 110 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is rarely studied 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.

Palma et al. (2025)
Classified as optical pair (not dynamically associated) P79, along with ASCC_111.

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.20 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.20 (50th percentile).

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 305.752 38.025 1.12 2.911 -1.202 -10.252
Hunt & Reffert 2024 305.774 38.006 1.127 2.828 -1.161 -8.226
Cavallo et al. 2024 305.615 37.887 1.124 – – –
Hunt & Reffert 2023 305.774 38.006 1.127 2.828 -1.161 -8.226
Sim et al. 2019 305.702 38.024 – 2.9 -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– 0.87 1.27 1.63 98 0.230 67 – –
Hunt & Reffert 2024 0.87 1.27 1.63 70 – 67(1) – –
Cavallo et al. 2024 0.90 1.06 – 126 0.230 – – –
Hunt & Reffert 2023 0.87 1.27 1.63 70 – – – –
Sim et al. 2019 0.86 – – 447 – – – –

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

Visualization

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