Theia 3227

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0.02 UTI
0.49
CN
1.0
Cdens
0.5
CC3
0.25
Clit
0.04
Cdup
Radius (P>50% members) 2.3 [arcmin]
  • CN 0.49 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.5 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 0.04 Very likely duplicate

Overview

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Theia 3227 is a poorly populated, very dense 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, 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.

Distant Moderate extinction Near-solar metallicity Intermediate age

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 – 156.331 -59.084 0.27 -5.746 3.884 7.174
Hu & Soubiran 2025 156.332 -59.081 – – – –
Hunt & Reffert 2024 156.339 -59.08 0.261 -5.762 3.885 -5.967
Cavallo et al. 2024 156.332 -59.082 0.262 – – –
Hunt & Reffert 2023 156.339 -59.08 0.261 -5.762 3.885 -5.967

💡 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] Bfr BSS
Hu & Soubiran 2025 – – – – -0.350* – – –
Hunt & Reffert 2024 – – – – – 498* – –
Cavallo et al. 2024 2.87 1.47 – 1096 0.360 – – –
Hunt & Reffert 2023 3.68 2.11 2.25 291 – – – –

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
UBC 1478 95.9 156.33 -59.08 0.27 -5.75 3.89 -5.95 0.38

💡 Note: The % column shows the percentage of members that Theia 3227 shares with each listed object.

Visualization

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