Theia 7593

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0.00 UTI
0.25
CN
0.21
Cdens
0.5
CC3
0.25
Clit
0.0
Cdup
Radius (P>50% members) 16.2 [arcmin]
  • CN 0.25 Poorly populated
  • Cdens 0.21 Very loose
  • CC3 0.5 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 0.0 Very likely duplicate

Overview

â„šī¸
Theia 7593 is a poorly populated, very loose object of intermediate C3 quality. Its parallax locates it at a relatively close distance, below 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.

Close 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 – 124.322 -55.64 0.957 -1.237 1.532 -2.55
Hu & Soubiran 2025 124.761 -55.681 – – – –
Hunt & Reffert 2024 124.434 -55.632 0.967 -1.251 1.555 -6.271
Cavallo et al. 2024 124.761 -55.682 0.965 – – –
Hunt & Reffert 2023 124.434 -55.632 0.967 -1.251 1.555 -6.271

💡 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 – – – – -0.240* – – –
Hunt & Reffert 2024 – – – – – 51* – –
Cavallo et al. 2024 1.00 1.23 – 1122 -0.230 – – –
Hunt & Reffert 2023 0.97 0.84 0.82 933 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 323 100.0 124.45 -55.64 0.96 -1.24 1.53 -3.0 0.21

💡 Note: The % column shows the percentage of members that Theia 7593 shares with each listed object.

Visualization

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