Theia 569

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0.25 UTI
0.0
CN
0.49
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 14.3 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.49 Loose
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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Theia 569 is a sparse, loose object of high C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by low 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.

Note: This object shares a large percentage of members with a later 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 – 72.555 44.822 1.327 2.039 -6.361 3.863
Zhang et al. 2024 72.402 44.833 – – – –
Cavallo et al. 2024 72.558 44.692 1.328 – – –
Hunt & Reffert 2023 72.402 44.833 1.319 2.072 -6.377 0.714

💡 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
Zhang et al. 2024 – – – – -0.316* – – –
Cavallo et al. 2024 0.75 0.89 – 275 0.320 – – –
Hunt & Reffert 2023 0.70 1.06 0.61 236 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 4066 92.0 72.56 44.84 1.35 2.04 -6.36 3.69 0.02

💡 Note: The % column shows the percentage of members that Theia 569 shares with each listed object.

Visualization

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