Theia 222

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0.12 UTI
0.62
CN
0.77
Cdens
0.62
CC3
0.0
Clit
0.29
Cdup
Radius (P>50% members) 60.4 [arcmin]
  • CN 0.62 Moderately populated
  • Cdens 0.77 Dense
  • CC3 0.62 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 0.29 Possibly duplicate

Overview

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Theia 222 is a moderately populated, dense object of intermediate C3 quality. Its parallax locates it at a very close distance, near 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.

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

Very 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 – 286.448 -16.074 4.034 0.767 -11.099 -23.969
Cavallo et al. 2024 285.998 -16.478 4.011 – – –
Hunt & Reffert 2023 286.569 -15.608 4.022 0.668 -11.246 -25.718

💡 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 0.26 0.73 – 105 0.220 – – –
Hunt & Reffert 2023 0.25 0.19 0.55 142 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
OCSN 5 71.2 286.45 -16.6 4.08 0.85 -11.52 -24.13 0.41

💡 Note: The % column shows the percentage of members that Theia 222 shares with each listed object.

Visualization

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