Theia 1450

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0.20 UTI
0.38
CN
0.07
Cdens
0.38
CC3
0.1
Clit
1.0
Cdup
Core radius and density 3.7 [pc], 0.4 [pc-2]
  • CN 0.38 Poorly populated
  • Cdens 0.07 Very loose
  • CC3 0.38 Low quality
  • Clit 0.1 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
Theia 1450 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a close distance, above the mid-plane, affected by moderate 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 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)
Silver sample.

Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.01 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.01 (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– 315.201 49.778 1.259 5.91 2.998 -49.982
Yang et al. 2025 315.494 49.824 – – – –
Hunt & Reffert 2024 315.494 49.824 1.26 5.887 3.127 -49.531
Cavallo et al. 2024 314.338 49.449 1.262 – – –
Hunt & Reffert 2023 315.494 49.824 1.26 5.887 3.127 -49.531
Kounkel & Covey 2019 314.431 49.039 1.375 – – -24.628

💡 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– 0.75 2.865 2.78 224 0.190 74 – –
Yang et al. 2025 – – – 224 -0.080(3) – – –
Hunt & Reffert 2024 0.75 3.14 2.78 223 – 74(1) – –
Cavallo et al. 2024 0.91 2.59 – 263 0.460 – – –
Hunt & Reffert 2023 0.75 3.14 2.78 223 – – – –
Kounkel & Covey 2019 0.73 1.09 – 1760 – – – –

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

Visualization

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