Theia 458

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0.11 UTI
0.26
CN
0.1
Cdens
0.12
CC3
0.03
Clit
1.0
Cdup
Core radius and density 3.0 [pc], 0.5 [pc-2]
  • CN 0.26 Poorly populated
  • Cdens 0.1 Very loose
  • CC3 0.12 Very low quality
  • Clit 0.03 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
Theia 458 is a poorly populated, very loose object of very low C3 quality. Its parallax locates it at a close distance, near 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.

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as moving group. CMD class: 0.99 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.99 (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– 106.275 -16.997 1.68 -6.552 0.075 22.904
Cavallo et al. 2024 106.41 -17.094 1.687 – – –
Hunt & Reffert 2023 106.24 -16.827 1.663 -6.452 0.027 20.652
Kounkel & Covey 2019 106.275 -16.53 1.885 – – 4.921

💡 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– 0.57 0.23 0.95 138 -0.050 – – –
Cavallo et al. 2024 0.60 0.43 – 63 -0.050 – – –
Hunt & Reffert 2023 0.57 0.21 0.95 138 – – – –
Kounkel & Covey 2019 0.53 0.23 – 193 – – – –

Visualization

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