Theia 5015

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0.34 UTI
0.0
CN
0.46
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 9.1 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.46 Loose
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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Theia 5015 is a sparse, 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.
Relatively close Moderate extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Gold sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 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] Bfr BSS
Hu & Soubiran 2025 – – – – -0.150* – – –
Hunt & Reffert 2024 – – – – – 187* – –
Cavallo et al. 2024 0.99 2.04 – 513 -0.430 – – –
Hunt & Reffert 2023 1.13 1.75 0.33 224 – – – –

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Visualization

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