Theia 2395

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0.35 UTI
0.0
CN
0.7
Cdens
1.0
CC3
0.03
Clit
1.0
Cdup
Stellar density (N50/rad) 3.5 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.7 Moderately dense
  • CC3 1.0 Very high quality
  • Clit 0.03 Rarely studied
  • Cdup 1.0 Unique

Overview

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Theia 2395 is a sparse, moderately dense object of very high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by high extinction. It is catalogued as a metal-rich, young cluster (see Parameters). It was recently reported in the literature.

Note: This object shares a large percentage of members with at least one entry reported in the same catalogue. See table with shared members information.

Palma et al. (2025)
Part of multiple system G179, along with CWNU_2364 and HSC_486.

Cavallo et al. (2024)
Bronze sample.

Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.70 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.70 (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– 295.105 24.238 0.237 -2.345 -5.584 36.367
Hunt & Reffert 2024 295.109 24.244 0.224 -2.37 -5.516 21.327
Cavallo et al. 2024 295.157 24.122 0.226 – – –
Hunt & Reffert 2023 295.109 24.244 0.224 -2.37 -5.516 21.327

💡 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– 4.12 3.085 2.77 53 0.740 614 – –
Hunt & Reffert 2024 – – – – – 614(1) – –
Cavallo et al. 2024 4.21 2.73 – 89 0.740 – – –
Hunt & Reffert 2023 4.03 3.44 2.77 17 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
HSC 486 76.0 295.1 24.24 0.24 -2.32 -5.6 36.37 0.35

💡 Note: The % column shows the percentage of members that Theia 2395 shares with each listed object.

Visualization

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