Theia 5280

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0.22 UTI
0.0
CN
0.46
Cdens
0.62
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 7.1 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.46 Loose
  • CC3 0.62 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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Theia 5280 is a sparse, 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 (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 – 336.502 52.168 0.639 0.992 -2.384 -34.519
Hunt & Reffert 2024 336.504 52.186 0.642 0.983 -2.334 -32.957
Cavallo et al. 2024 336.282 51.947 0.641 – – –
Hunt & Reffert 2023 336.504 52.186 0.642 0.983 -2.334 -32.957

💡 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 – – – – – 66* – –
Cavallo et al. 2024 1.53 0.56 – 417 0.140 – – –
Hunt & Reffert 2023 1.47 0.30 0.39 551 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3253 92.0 336.49 52.16 0.64 0.99 -2.37 -34.52 0.03

💡 Note: The % column shows the percentage of members that Theia 5280 shares with each listed object.

Visualization

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