Theia 776

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0.12 UTI
0.0
CN
0.14
Cdens
0.38
CC3
0.03
Clit
1.0
Cdup
Core radius and density 1.8 [pc], 0.7 [pc-2]
  • CN 0.0 Sparse
  • Cdens 0.14 Very loose
  • CC3 0.38 Low quality
  • Clit 0.03 Rarely studied
  • Cdup 1.0 Unique

Overview

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Theia 776 is a sparse, very loose object of low C3 quality. Its parallax locates it at a close distance, below the mid-plane, affected by low extinction. It is catalogued as a 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)
Classified as optical pair P173, along with Theia_280.

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as moving group. CMD class: 0.93 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.93 (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– 338.605 49.279 1.183 -3.225 -3.859 -19.136
Cavallo et al. 2024 338.669 49.242 1.177 – – –
Hunt & Reffert 2023 338.582 49.334 1.175 -3.2 -3.86 -8.247
Kounkel & Covey 2019 338.444 49.509 1.225 – – -1.336

💡 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– 0.81 0.36 0.49 263 -0.020 – – –
Cavallo et al. 2024 0.81 0.36 – 263 -0.020 – – –
Hunt & Reffert 2023 0.81 0.32 0.49 114 – – – –
Kounkel & Covey 2019 0.82 0.50 – 329 – – – –

Visualization

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