Theia 1140

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0.13 UTI
0.0
CN
0.15
Cdens
0.38
CC3
0.06
Clit
1.0
Cdup
Core radius and density 1.6 [pc], 0.7 [pc-2]
  • CN 0.0 Sparse
  • Cdens 0.15 Very loose
  • CC3 0.38 Low quality
  • Clit 0.06 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
Theia 1140 is a sparse, very 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 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.

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.92 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.92 (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– 280.887 5.642 1.449 3.743 0.247 -14.161
Hunt & Reffert 2024 280.919 5.627 1.451 3.732 0.18 -11.628
Cavallo et al. 2024 280.956 5.602 1.453 – – –
Hunt & Reffert 2023 280.919 5.627 1.451 3.732 0.18 -11.628
Kounkel & Covey 2019 281.13 5.155 1.478 – – -19.915

💡 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– 0.665 0.88 0.99 108 0.390 46 – –
Hunt & Reffert 2024 0.65 0.88 0.99 92 – 46(1) – –
Cavallo et al. 2024 0.74 0.64 – 123 0.390 – – –
Hunt & Reffert 2023 0.65 0.88 0.99 92 – – – –
Kounkel & Covey 2019 0.68 1.17 – 951 – – – –

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

Visualization

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