Theia 5731

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0.07 UTI
0.0
CN
0.11
Cdens
0.38
CC3
0.0
Clit
0.72
Cdup
Radius (P>50% members) 39.5 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.11 Very loose
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 0.72 Likely unique

Overview

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Theia 5731 is a sparse, very loose object of low C3 quality. Its parallax locates it at a close distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.

Note: This is likely a unique object, which shares a moderate percentage of members with at least one previously reported entry. See table with shared members information.

Close Low extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as a moving group.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 272.27 -60.358 1.758 -0.364 -9.431 -12.649
Cavallo et al. 2024 273.398 -60.165 1.77 – – –
Hunt & Reffert 2023 272.091 -60.29 1.762 -0.336 -9.47 -10.732

💡 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
Cavallo et al. 2024 0.57 0.46 – 138 0.020 – – –
Hunt & Reffert 2023 0.53 0.22 0.68 341 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
LISC-III 3629 28.0 272.27 -60.52 1.77 -0.31 -8.79 2.64 0.04

💡 Note: The % column shows the percentage of members that Theia 5731 shares with each listed object.

Visualization

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