Theia 31

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0.64 UTI
0.69
CN
1.0
Cdens
1.0
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 16.4 [N/pc2]
  • CN 0.69 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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Theia 31 is a moderately populated, very dense object of very high 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, very young cluster, but with a large variance across recent sources for the absorption 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.

Liu et al. (2025)
Classified as primordial binary cluster 93 along with CWNU_1096, and of multiple system 30 along with CWNU_1096 and CWNU_1083.

Palma et al. (2025)
Classified as optical pair P89, along with CWNU_1096.

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 99999– 126.956 -34.757 2.803 -6.94 10.853 21.016
Liu et al. 2025 127.0 -34.91 2.8 -7.01 10.85 11.62
Cavallo et al. 2024 126.857 -34.898 2.803 – – –
Hunt & Reffert 2023 127.002 -34.911 2.804 -7.006 10.853 11.621
He et al. 2022 126.887 -34.8 2.803 -6.978 10.874 –

💡 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] Bfrac BSS
UCC 99999– 0.36 0.23 0.88 7 -0.150 – – –
Liu et al. 2025 0.37 0.04 – 7 – – – –
Cavallo et al. 2024 0.36 0.78 – 5 -0.150 – – –
Hunt & Reffert 2023 0.35 0.31 0.88 7 – – – –
He et al. 2022 – 0.15 – 7 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
OCSN 202 100.0 126.93 -34.74 2.81 -6.96 10.9 13.13 0.09

💡 Note: The % column shows the percentage of members that Theia 31 shares with each listed object.

Visualization

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