Theia 4482

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0.04 UTI
0.39
CN
0.06
Cdens
0.5
CC3
0.06
Clit
0.2
Cdup
Core radius and density 2.8 [pc], 0.3 [pc-2]
  • CN 0.39 Poorly populated
  • Cdens 0.06 Very loose
  • CC3 0.5 Intermediate quality
  • Clit 0.06 Rarely studied
  • Cdup 0.2 Likely duplicate

Overview

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Theia 4482 is a poorly populated, very loose object of intermediate C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.

âš ī¸ Warning: This is 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 (2024)
Classified as open cluster. CMD class: 0.08 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.08 (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– 234.782 -58.54 0.294 -3.502 -4.638 -23.824
Hu & Soubiran 2025 234.771 -58.546 – – – –
Hunt & Reffert 2024 234.832 -58.538 0.301 -3.504 -4.628 -19.851
Cavallo et al. 2024 234.771 -58.546 0.302 – – –
Hunt & Reffert 2023 234.832 -58.538 0.301 -3.504 -4.628 -19.851

💡 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– 3.09 2.72 1.31 563 -0.180 517 – –
Hu & Soubiran 2025 – – – – -0.100(5) – – –
Hunt & Reffert 2024 3.09 2.72 1.31 563 – 517(1) – –
Cavallo et al. 2024 2.31 2.94 – 1096 -0.260 – – –
Hunt & Reffert 2023 3.09 2.72 1.31 562 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 2650 79.5 234.79 -58.54 0.29 -3.5 -4.63 -23.02 0.18

💡 Note: The % column shows the percentage of members that Theia 4482 shares with each listed object.

Visualization

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