Theia 625

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0.10 UTI
0.0
CN
0.17
Cdens
0.25
CC3
0.03
Clit
1.0
Cdup
Core radius and density 1.5 [pc], 0.9 [pc-2]
  • CN 0.0 Sparse
  • Cdens 0.17 Very loose
  • CC3 0.25 Low quality
  • Clit 0.03 Rarely studied
  • Cdup 1.0 Unique

Overview

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Theia 625 is a sparse, very loose object of low C3 quality. Its parallax locates it at a close distance, below 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.

Palma et al. (2025)
Classified as optical pair P475, along with HSC_255.

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as moving group. 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– 289.445 -13.779 1.892 5.821 0.491 -24.004
Cavallo et al. 2024 289.247 -14.213 1.908 – – –
Hunt & Reffert 2023 289.447 -13.775 1.9 5.84 0.281 -14.966
Kounkel & Covey 2019 288.064 -12.756 2.109 – – 4.082

💡 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– 0.5 0.61 0.98 166 -0.160 – – –
Cavallo et al. 2024 0.52 0.76 – 120 -0.160 – – –
Hunt & Reffert 2023 0.50 0.32 0.98 166 – – – –
Kounkel & Covey 2019 0.47 0.61 – 288 – – – –

Visualization

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