Theia 5431

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0.15 UTI
0.0
CN
0.13
Cdens
0.62
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 11.2 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.13 Very loose
  • CC3 0.62 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
Theia 5431 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a relatively close distance, above 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 object shares a large percentage of members with a later reported entry. See table with shared members information.

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.

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 – 128.42 -34.578 0.568 -4.548 3.291 32.896
Hunt & Reffert 2024 128.431 -34.572 0.569 -4.548 3.282 12.442
Cavallo et al. 2024 128.008 -34.206 0.571 – – –
Hunt & Reffert 2023 128.431 -34.572 0.569 -4.548 3.282 12.442

💡 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
Hunt & Reffert 2024 – – – – – 52* – –
Cavallo et al. 2024 1.70 0.72 – 372 0.260 – – –
Hunt & Reffert 2023 1.64 0.48 1.26 282 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3472 80.0 128.15 -34.41 0.57 -4.53 3.29 9.15 0.23

💡 Note: The % column shows the percentage of members that Theia 5431 shares with each listed object.

Visualization

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