Theia 295

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0.18 UTI
0.0
CN
0.06
Cdens
0.62
CC3
0.1
Clit
1.0
Cdup
Core radius and density 3.0 [pc], 0.3 [pc-2]
  • CN 0.0 Sparse
  • Cdens 0.06 Very loose
  • CC3 0.62 Intermediate quality
  • Clit 0.1 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
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 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.

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as open cluster. 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– 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
Kounkel & Covey 2019 152.598 -61.3 1.129 – – 10.261

💡 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– 1.435 0.435 0.43 169 0.035 54 – –
Hu & Soubiran 2025 – – – – -0.260(5) – – –
Hunt & Reffert 2024 1.45 0.54 0.43 169 – 54(1) – –
Cavallo et al. 2024 1.42 0.30 – 537 0.330 – – –
Hunt & Reffert 2023 1.45 0.54 0.43 169 – – – –
Kounkel & Covey 2019 0.89 0.33 – 86 – – – –

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

Visualization

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