Theia 833

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0.13 UTI
0.0
CN
0.25
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 21.0 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.25 Loose
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
Theia 833 is a sparse, loose object of low C3 quality. Its parallax locates it at a close distance, above the mid-plane, affected by low 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: 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.

Close Low extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as a moving group.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 297.323 38.593 1.428 1.132 -0.012 -18.952
Hu & Soubiran 2025 297.324 38.644 – – – –
Cavallo et al. 2024 297.324 38.644 1.445 – – –
Hunt & Reffert 2023 297.39 38.569 1.43 1.094 0.005 -21.067

💡 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 – – – – -0.130* – – –
Cavallo et al. 2024 0.68 0.19 – 933 0.370 – – –
Hunt & Reffert 2023 0.68 0.15 0.46 169 – – – –

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

Visualization

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