Theia 228

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0.30 UTI
0.5
CN
0.62
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 42.4 [arcmin]
  • CN 0.5 Moderately populated
  • Cdens 0.62 Moderately dense
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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Theia 228 is a moderately populated, moderately dense object of low 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, young cluster (see Parameters). It was recently reported in the literature.
Very close Low extinction Near-solar metallicity Young

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 – 300.629 20.211 3.036 0.32 -5.502 -20.232
Cavallo et al. 2024 301.868 21.024 3.008 – – –
Hunt & Reffert 2023 300.308 19.648 2.981 0.62 -5.343 -22.303

💡 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 0.35 0.44 – 54 0.300 – – –
Hunt & Reffert 2023 0.32 0.12 0.57 98 – – – –

Visualization

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