Theia 2505

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0.30 UTI
0.0
CN
0.23
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 1.1 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.23 Very loose
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
Theia 2505 is a sparse, very loose object of high C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a metal-poor, young cluster, but with a large variance across recent sources for the absorption parameter (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.

Liu et al. (2025)
Classified as primordial binary cluster 364 along with Theia_2803, and as tidal capture (resonant trapping binary) 371 along with Trumpler_26, and of multiple system 82 along with Theia_2803 and Trumpler_26.

Palma et al. (2025)
Part of multiple system G240, along with Theia_2803 and Trumpler_26.

Cavallo et al. (2024)
Silver sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 263.275 -30.007 0.646 -0.735 -2.651 -8.231
Liu et al. 2025 263.25 -30.02 0.64 -0.76 -2.66 -18.22
Hunt & Reffert 2024 263.246 -30.024 0.636 -0.761 -2.663 -18.217
Cavallo et al. 2024 263.268 -30.01 0.635 – – –
Hunt & Reffert 2023 263.246 -30.024 0.636 -0.761 -2.663 -18.217

💡 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– 1.48 1.76 2.15 32 -0.760 285 – –
Liu et al. 2025 2.33 0.58 – 32 – – – –
Hunt & Reffert 2024 – – – – – 285(1) – –
Cavallo et al. 2024 1.48 2.47 – 81 -0.760 – – –
Hunt & Reffert 2023 1.48 1.76 2.15 24 – – – –

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

Visualization

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