Theia 4310

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0.00 UTI
0.33
CN
1.0
Cdens
0.5
CC3
0.25
Clit
0.0
Cdup
Radius (P>50% members) 6.1 [arcmin]
  • CN 0.33 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.5 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 0.0 Very likely duplicate

Overview

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Theia 4310 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate 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.

âš ī¸ Warning: This is very likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

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 – 0.547 63.549 0.891 -2.607 -1.417 -43.299
Hu & Soubiran 2025 0.489 63.575 – – – –
Hunt & Reffert 2024 0.425 63.533 0.89 -2.576 -1.419 -45.674
Cavallo et al. 2024 0.489 63.576 0.892 – – –
Hunt & Reffert 2023 0.425 63.533 0.89 -2.576 -1.419 -45.674

💡 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 – – – – -0.120* – – –
Hunt & Reffert 2024 – – – – – 136* – –
Cavallo et al. 2024 1.09 1.36 – 794 0.310 – – –
Hunt & Reffert 2023 1.07 1.30 0.95 441 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
UBC 181 100.0 0.59 63.57 0.88 -2.6 -1.41 -43.1 0.57

💡 Note: The % column shows the percentage of members that Theia 4310 shares with each listed object.

Visualization

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