Theia 8068

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0.00 UTI
0.35
CN
1.0
Cdens
1.0
CC3
0.25
Clit
0.0
Cdup
Radius (P>50% members) 1.4 [arcmin]
  • CN 0.35 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.25 Poorly studied
  • Cdup 0.0 Very likely duplicate

Overview

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Theia 8068 is a poorly populated, very dense object of very high C3 quality. Its parallax locates it at a large distance, above the mid-plane, affected by moderate 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 very likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

Very distant Moderate extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Gold sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 297.243 34.086 0.162 -2.725 -5.501 -6.87
Hu & Soubiran 2025 297.243 34.077 – – – –
Hunt & Reffert 2024 297.241 34.086 0.16 -2.73 -5.505 -6.839
Cavallo et al. 2024 297.243 34.077 0.156 – – –
Hunt & Reffert 2023 297.241 34.086 0.16 -2.73 -5.505 -6.839

💡 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 – – – – -0.110* – – –
Hunt & Reffert 2024 – – – – – 629* – –
Cavallo et al. 2024 4.29 1.25 – 513 0.100 – – –
Hunt & Reffert 2023 5.86 1.50 0.76 270 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
UBC 1082 100.0 297.24 34.08 0.16 -2.73 -5.5 -6.87 0.5

💡 Note: The % column shows the percentage of members that Theia 8068 shares with each listed object.

Visualization

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