Theia 1062

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0.11 UTI
0.0
CN
0.05
Cdens
0.38
CC3
0.06
Clit
1.0
Cdup
Core radius and density 2.5 [pc], 0.3 [pc-2]
  • CN 0.0 Sparse
  • Cdens 0.05 Very loose
  • CC3 0.38 Low quality
  • Clit 0.06 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
Theia 1062 is a sparse, very loose object of low C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate 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.

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– 135.113 -49.274 0.641 -7.084 4.903 –
Hunt & Reffert 2024 135.111 -49.277 0.623 -7.092 4.904 –
Cavallo et al. 2024 135.131 -49.286 0.634 – – –
Hunt & Reffert 2023 135.111 -49.277 0.623 -7.092 4.904 –
Kounkel & Covey 2019 135.53 -49.562 1.374 – – –

💡 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– 1.53 1.53 1.3 173 0.210 50 – –
Hunt & Reffert 2024 1.53 1.64 1.30 168 – 50(1) – –
Cavallo et al. 2024 1.56 1.42 – 178 0.210 – – –
Hunt & Reffert 2023 1.53 1.64 1.30 168 – – – –
Kounkel & Covey 2019 0.73 0.45 – 778 – – – –

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

Visualization

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