Theia 5015

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0.21 UTI
0.0
CN
0.15
Cdens
0.75
CC3
0.06
Clit
1.0
Cdup
Core radius and density 1.8 [pc], 0.7 [pc-2]
  • CN 0.0 Sparse
  • Cdens 0.15 Very loose
  • CC3 0.75 High quality
  • Clit 0.06 Rarely studied
  • Cdup 1.0 Unique

Overview

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Theia 5015 is a sparse, very loose object of high C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (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: 1.00 (50th percentile), true positive (human-assigned).

Hunt & Reffert (2023)
Classified as open cluster. CMD classes: 1.00 (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– 267.085 -24.185 0.837 -0.3 -0.079 -47.982
Hu & Soubiran 2025 267.229 -23.982 – – – –
Hunt & Reffert 2024 267.059 -24.21 0.843 -0.272 -0.066 -35.627
Cavallo et al. 2024 267.229 -23.982 0.843 – – –
Hunt & Reffert 2023 267.059 -24.21 0.843 -0.272 -0.066 -35.627

💡 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– 1.13 1.75 0.33 224 -0.290 187 – –
Hu & Soubiran 2025 – – – – -0.150(5) – – –
Hunt & Reffert 2024 1.13 1.75 0.33 224 – 187(1) – –
Cavallo et al. 2024 0.99 2.04 – 513 -0.430 – – –
Hunt & Reffert 2023 1.13 1.75 0.33 224 – – – –

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

Visualization

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