Theia 6978

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0.00 UTI
0.77
CN
1.0
Cdens
0.75
CC3
0.25
Clit
0.0
Cdup
Radius (P>50% members) 2.6 [arcmin]
  • CN 0.77 Rich
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 0.0 Very likely duplicate

Overview

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Theia 6978 is a rich, very dense object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, old 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.

Distant Moderate extinction Near-solar metallicity Old

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 – 133.924 -38.568 0.236 -5.008 3.848 51.673
Hu & Soubiran 2025 133.918 -38.564 – – – –
Hunt & Reffert 2024 133.924 -38.567 0.245 -4.992 3.866 54.0
Cavallo et al. 2024 133.918 -38.564 0.237 – – –
Hunt & Reffert 2023 133.924 -38.567 0.245 -4.992 3.866 54.0

💡 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* – – –
Hunt & Reffert 2024 – – – – – 847* – –
Cavallo et al. 2024 3.02 1.61 – 1288 -0.410 – – –
Hunt & Reffert 2023 3.67 1.35 1.13 767 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
LISC 0901 100.0 133.92 -38.57 0.24 -4.98 3.86 53.53 0.52
UBC 1438 87.7 133.92 -38.57 0.23 -5.01 3.84 51.67 0.0
CWWDL 3104 50.6 133.93 -38.57 0.23 -5.01 3.84 49.16 0.0

💡 Note: The % column shows the percentage of members that Theia 6978 shares with each listed object.

Visualization

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