UPK 300

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0.18 UTI
0.26
CN
0.06
Cdens
0.38
CC3
0.1
Clit
1.0
Cdup
Core radius and density 2.8 [pc], 0.3 [pc-2]
  • CN 0.26 Poorly populated
  • Cdens 0.06 Very loose
  • CC3 0.38 Low quality
  • Clit 0.1 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
UPK 300 is a poorly populated, very 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, young cluster, but with a large variance across recent sources for the metallicity parameter (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.

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.91 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.91 (50th percentile).

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 57.759 60.121 1.052 0.185 -0.824 -9.115
Yang et al. 2025 57.408 60.146 – – – –
Hunt & Reffert 2024 57.408 60.146 1.059 0.207 -0.768 -8.096
Cavallo et al. 2024 57.94 60.06 1.054 – – –
Hunt & Reffert 2023 57.408 60.146 1.059 0.207 -0.768 -8.096
Sim et al. 2019 58.02 59.983 – 0.25 -0.75 –

💡 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– 0.93 2.46 1.23 62 -0.365 87 – –
Yang et al. 2025 – – – 63 -0.110(3) – – –
Hunt & Reffert 2024 0.91 2.46 1.23 62 – 87(1) – –
Cavallo et al. 2024 0.95 2.81 – 21 -0.620 – – –
Hunt & Reffert 2023 0.91 2.46 1.23 62 – – – –
Sim et al. 2019 0.96 – – 398 – – – –

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

Visualization

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