Theia 332

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0.18 UTI
0.3
CN
0.1
Cdens
0.38
CC3
0.06
Clit
1.0
Cdup
Core radius and density 2.3 [pc], 0.5 [pc-2]
  • CN 0.3 Poorly populated
  • Cdens 0.1 Very loose
  • CC3 0.38 Low quality
  • Clit 0.06 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
Theia 332 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by low extinction. It is catalogued as a low-mass, near-solar metallicity, intermediate-age cluster (see Parameters). It is rarely studied 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.

Palma et al. (2025)
Part of multiple system G245, along with Theia_470 and Theia_73.

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as open cluster. CMD class: 1.00 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 1.00 (50th percentile).

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 299.174 32.884 1.494 3.746 1.381 -11.185
Hunt & Reffert 2024 299.032 32.903 1.473 3.781 1.395 -10.296
Cavallo et al. 2024 299.217 32.901 1.48 – – –
Hunt & Reffert 2023 299.032 32.903 1.473 3.781 1.395 -10.296
Kounkel & Covey 2019 298.979 32.9 1.529 – – 1.197

💡 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– 0.645 0.285 0.7 102 0.040 45 – –
Hunt & Reffert 2024 0.64 0.20 0.70 102 – 45(1) – –
Cavallo et al. 2024 0.70 0.52 – 54 0.040 – – –
Hunt & Reffert 2023 0.64 0.20 0.70 102 – – – –
Kounkel & Covey 2019 0.65 0.37 – 111 – – – –

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

Visualization

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