Theia 5422

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0.04 UTI
0.77
CN
0.84
Cdens
1.0
CC3
0.25
Clit
0.06
Cdup
Stellar density (N50/rad) 4.2 [N/pc2]
  • CN 0.77 Rich
  • Cdens 0.84 Dense
  • CC3 1.0 Very high quality
  • Clit 0.25 Poorly studied
  • Cdup 0.06 Very likely duplicate

Overview

â„šī¸
Theia 5422 is a rich, dense object of very high C3 quality. Its parallax locates it at a large distance, above the mid-plane, affected by high extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It was recently reported 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.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 314.313 46.451 0.184 -2.942 -3.592 -35.479
Hu & Soubiran 2025 314.289 46.439 – – – –
Hunt & Reffert 2024 314.336 46.48 0.174 -2.941 -3.601 -45.883
Cavallo et al. 2024 314.289 46.439 0.175 – – –
Hunt & Reffert 2023 314.336 46.48 0.174 -2.941 -3.601 -45.883

💡 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– 4.68 3.565 2.59 465 -0.210 3336 – –
Hu & Soubiran 2025 – – – – -0.380(5) – – –
Hunt & Reffert 2024 – – – – – 3336(1) – –
Cavallo et al. 2024 4.53 3.40 – 631 -0.040 – – –
Hunt & Reffert 2023 4.83 3.73 2.59 299 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
UBC 1571 93.5 314.29 46.44 0.19 -2.94 -3.59 -36.27 0.55

💡 Note: The % column shows the percentage of members that Theia 5422 shares with each listed object.

Visualization

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