Theia 1802

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0.08 UTI
0.0
CN
0.04
Cdens
0.25
CC3
0.06
Clit
1.0
Cdup
Core radius and density 4.2 [pc], 0.2 [pc-2]
  • CN 0.0 Sparse
  • Cdens 0.04 Very loose
  • CC3 0.25 Low quality
  • Clit 0.06 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
Theia 1802 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It was recently reported 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 classes: 0.16 (50th percentile), true positive? (human-assigned).

Hunt & Reffert (2023)
Classified as open cluster. CMD classes: 0.16 (50th percentile), true positive? (human-assigned).

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 89.836 20.746 0.304 -0.083 -1.477 –
Zhang et al. 2024 89.863 20.716 – – – –
Hunt & Reffert 2024 89.863 20.716 0.29 -0.138 -1.469 89.276
Cavallo et al. 2024 89.663 20.935 0.292 – – –
Hunt & Reffert 2023 89.863 20.716 0.29 -0.138 -1.469 89.276

💡 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– 2.94 3.27 2.82 22 0.409 241 – –
Zhang et al. 2024 – – – – 0.088(1) – – –
Hunt & Reffert 2024 2.94 3.28 2.82 22 – 241(1) – –
Cavallo et al. 2024 4.15 2.99 – 35 0.730 – – –
Hunt & Reffert 2023 2.94 3.27 2.82 22 – – – –

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

Visualization

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