Theia 1976

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0.00 UTI
0.63
CN
1.0
Cdens
1.0
CC3
0.25
Clit
0.0
Cdup
Radius (P>50% members) 3.6 [arcmin]
  • CN 0.63 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.25 Poorly studied
  • Cdup 0.0 Very likely duplicate

Overview

â„šī¸
Theia 1976 is a moderately populated, very dense object of very high 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 (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.

Relatively close 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 – 278.32 -13.062 0.39 -0.926 -0.246 1.269
Hu & Soubiran 2025 278.305 -13.062 – – – –
Hunt & Reffert 2024 278.32 -13.053 0.388 -0.915 -0.258 -4.098
Cavallo et al. 2024 278.305 -13.062 0.389 – – –
Hunt & Reffert 2023 278.32 -13.053 0.388 -0.915 -0.258 -4.098

💡 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 – – – – -0.220* – – –
Hunt & Reffert 2024 – – – – – 819* – –
Cavallo et al. 2024 1.71 2.62 – 794 -0.420 – – –
Hunt & Reffert 2023 2.30 2.45 1.79 356 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 397 100.0 278.32 -13.06 0.39 -0.93 -0.25 1.27 0.16
UBC 1022 77.6 278.32 -13.06 0.39 -0.93 -0.24 1.27 0.51

💡 Note: The % column shows the percentage of members that Theia 1976 shares with each listed object.

Visualization

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