Theia 455

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0.09 UTI
0.0
CN
0.09
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 0.4 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.09 Very loose
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
Theia 455 is a sparse, very loose object of low C3 quality. Its parallax locates it at a very close distance, near the mid-plane, affected by low 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 was recently reported 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 a moving group.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 138.644 -44.187 2.208 -7.042 -0.21 30.042
Hu & Soubiran 2025 138.833 -44.083 – – – –
Cavallo et al. 2024 138.833 -44.083 2.198 – – –
Hunt & Reffert 2023 138.306 -44.186 2.198 -7.17 -0.049 28.667

💡 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– 0.455 0.255 0.56 493 0.025 – – –
Hu & Soubiran 2025 – – – – -0.340(5) – – –
Cavallo et al. 2024 0.47 0.40 – 813 0.390 – – –
Hunt & Reffert 2023 0.44 0.11 0.56 173 – – – –

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

Visualization

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