Theia 295

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0.25 UTI
0.0
CN
0.14
Cdens
0.62
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 11.9 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.14 Very loose
  • CC3 0.62 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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Theia 295 is a sparse, very loose object of intermediate 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, intermediate-age 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 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 – 152.586 -61.541 0.666 -7.289 3.851 21.129
Hu & Soubiran 2025 152.751 -61.553 – – – –
Hunt & Reffert 2024 152.541 -61.477 0.664 -7.267 3.84 13.814
Cavallo et al. 2024 152.751 -61.553 0.665 – – –
Hunt & Reffert 2023 152.541 -61.477 0.664 -7.267 3.84 13.814

💡 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 – – – – -0.260* – – –
Hunt & Reffert 2024 – – – – – 54* – –
Cavallo et al. 2024 1.42 0.30 – 537 0.330 – – –
Hunt & Reffert 2023 1.45 0.54 0.43 169 – – – –

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

Visualization

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