OC 0431

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0.00 UTI
0.0
CN
0.03
Cdens
0.75
CC3
0.06
Clit
0.0
Cdup
Core radius and density 5.4 [pc], 0.1 [pc-2]
  • CN 0.0 Sparse
  • Cdens 0.03 Very loose
  • CC3 0.75 High quality
  • Clit 0.06 Rarely studied
  • Cdup 0.0 Very likely duplicate

Overview

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OC 0431 is a sparse, very loose object of high C3 quality. Its parallax locates it at a large distance, below 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 age and metallicity parameters (see Parameters). It is rarely studied in the literature.

âš ī¸ Warning: This is very likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.14 (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– 117.961 -30.618 0.102 -1.398 1.863 94.718
Hu & Soubiran 2025 117.955 -30.626 – – – –
Cavallo et al. 2024 117.955 -30.626 0.104 – – –
Hunt & Reffert 2023 117.931 -30.639 0.11 -1.404 1.852 114.099
Hao et al. 2022 117.982 -30.61 0.102 -1.413 1.826 78.78

💡 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– 7.77 2.31 2.39 794 -0.200 – – –
Hu & Soubiran 2025 – – – – -0.200(5) – – –
Cavallo et al. 2024 7.76 2.31 – 1230 -0.290 – – –
Hunt & Reffert 2023 7.78 3.14 2.39 277 – – – –
Hao et al. 2022 – 1.37 – 794 0.265 – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Teutsch 62 100.0 117.95 -30.63 0.11 -1.47 1.86 94.72 0.34

💡 Note: The % column shows the percentage of members that OC 0431 shares with each listed object.

Visualization

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