OC 0302

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0.19 UTI
0.28
CN
0.23
Cdens
0.25
CC3
0.1
Clit
1.0
Cdup
Core radius and density 1.9 [pc], 1.2 [pc-2]
  • CN 0.28 Poorly populated
  • Cdens 0.23 Very loose
  • CC3 0.25 Low quality
  • Clit 0.1 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
OC 0302 is a poorly populated, very loose object of 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, but with a large variance across recent sources for the age and metallicity parameters (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: 0.97 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.97 (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– 88.729 25.089 0.521 0.812 -3.828 –
Zhang et al. 2024 88.712 25.093 – – – –
Hunt & Reffert 2024 88.712 25.093 0.515 0.808 -3.852 –
Cavallo et al. 2024 88.759 25.073 0.513 – – –
Hunt & Reffert 2023 88.712 25.093 0.515 0.808 -3.852 –
Hao et al. 2022 88.741 25.064 0.532 0.799 -3.84 –

💡 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– 1.78 1.94 1.75 98 0.198 256 – –
Zhang et al. 2024 – – – – -0.137(1) – – –
Hunt & Reffert 2024 1.78 1.94 1.75 72 – 256(1) – –
Cavallo et al. 2024 2.07 1.90 – 123 0.750 – – –
Hunt & Reffert 2023 1.78 1.94 1.75 72 – – – –
Hao et al. 2022 – 2.31 – 398 0.198 – – –

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

Visualization

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