Theia 1188

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0.38 UTI
0.28
CN
0.5
Cdens
0.5
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members) 36.0 [arcmin]
  • CN 0.28 Poorly populated
  • Cdens 0.5 Moderately dense
  • CC3 0.5 Intermediate quality
  • Clit 0.31 Poorly studied
  • Cdup 1.0 Unique

Overview

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Theia 1188 is a poorly populated, moderately dense object of intermediate C3 quality. Its parallax locates it at a very close distance, below 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 is poorly studied in the literature.

Note: This object shares a large percentage of members with a later 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 – 338.708 29.919 3.115 -7.865 -4.35 4.995
Hu & Soubiran 2025 338.195 29.939 – – – –
Zhang et al. 2024 338.742 29.991 – – – –
Cavallo et al. 2024 338.195 29.939 3.036 – – –
Hunt & Reffert 2023 338.742 29.991 3.027 -7.847 -4.536 4.219
He et al. 2022 338.673 29.937 3.116 -7.852 -4.356 –

💡 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
Hu & Soubiran 2025 – – – – -0.190* – – –
Zhang et al. 2024 – – – – 0.141* – – –
Cavallo et al. 2024 0.33 0.36 – 575 0.410 – – –
Hunt & Reffert 2023 0.31 0.23 0.66 570 – – – –
He et al. 2022 – 0.50 – 891 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
OCSN 26 85.7 338.71 29.95 3.12 -7.91 -4.35 4.99 0.02

💡 Note: The % column shows the percentage of members that Theia 1188 shares with each listed object.

Visualization

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