Theia 1170

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0.32 UTI
0.37
CN
0.72
Cdens
0.5
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 16.1 [arcmin]
  • CN 0.37 Poorly populated
  • Cdens 0.72 Moderately dense
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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Theia 1170 is a poorly populated, moderately dense object of intermediate 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 (see Parameters). It was recently reported in the literature.
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 – 137.804 -54.475 1.463 -10.68 8.215 4.691
Cavallo et al. 2024 137.338 -54.249 1.491 – – –
Hunt & Reffert 2023 137.639 -54.555 1.493 -10.746 8.289 8.269

💡 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 0.68 0.36 – 71 0.370 – – –
Hunt & Reffert 2023 0.64 0.17 0.84 161 – – – –

Visualization

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