Theia 5705

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0.27 UTI
0.0
CN
0.1
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 15.1 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.1 Very loose
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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Theia 5705 is a sparse, very loose object of high C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, old cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It was recently reported in the literature.
Relatively close Low extinction Near-solar metallicity Old

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 – 266.804 -42.434 0.688 3.256 -4.851 -28.899
Hu & Soubiran 2025 266.771 -42.416 – – – –
Hunt & Reffert 2024 266.822 -42.394 0.677 3.237 -4.934 -30.108
Cavallo et al. 2024 266.771 -42.416 0.681 – – –
Hunt & Reffert 2023 266.822 -42.394 0.677 3.237 -4.934 -30.108

💡 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 – – – – -0.140* – – –
Hunt & Reffert 2024 – – – – – 57* – –
Cavallo et al. 2024 1.60 1.14 – 955 0.300 – – –
Hunt & Reffert 2023 1.43 0.63 0.39 1667 – – – –

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

Visualization

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