Theia 2460

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0.10 UTI
0.71
CN
1.0
Cdens
0.75
CC3
0.25
Clit
0.16
Cdup
Stellar density (N50/rad) 15.7 [N/pc2]
  • CN 0.71 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 0.16 Likely duplicate

Overview

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Theia 2460 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by low 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.

Liu et al. (2025)
Classified as tidal capture (resonant trapping binary) 133 along with DBSB_104.

Palma et al. (2025)
Classified as optical pair P383, along with DBSB_104.

Cavallo et al. (2024)
Gold 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– 256.154 -51.388 0.888 -0.682 -1.246 1.932
Hunt & Reffert 2024 256.158 -51.401 0.879 -0.693 -1.267 9.52
Cavallo et al. 2024 256.144 -51.387 0.883 – – –
Hunt & Reffert 2023 256.158 -51.401 0.879 -0.693 -1.267 9.52

💡 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– 1.16 0.82 0.48 158 0.460 315 – –
Liu et al. 2025 1.49 0.31 – 158 – – – –
Hunt & Reffert 2024 – – – – – 315(1) – –
Cavallo et al. 2024 1.16 0.94 – 162 0.460 – – –
Hunt & Reffert 2023 1.07 0.82 0.48 157 – – – –

(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 1151 83.7 256.16 -51.39 0.89 -0.68 -1.24 1.93 0.48

💡 Note: The % column shows the percentage of members that Theia 2460 shares with each listed object.

Visualization

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