Theia 5496

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0.02 UTI
0.27
CN
1.0
Cdens
0.75
CC3
0.25
Clit
0.04
Cdup
Radius (P>50% members) 3.9 [arcmin]
  • CN 0.27 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 0.04 Very likely duplicate

Overview

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Theia 5496 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, near 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.

Relatively close 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 – 211.363 -64.16 0.615 -7.074 -3.539 -47.455
Hu & Soubiran 2025 211.377 -64.16 – – – –
Hunt & Reffert 2024 211.416 -64.159 0.611 -7.083 -3.525 -30.991
Cavallo et al. 2024 211.377 -64.16 0.613 – – –
Hunt & Reffert 2023 211.416 -64.159 0.611 -7.083 -3.525 -30.991

💡 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 – – – – -0.180* – – –
Hunt & Reffert 2024 – – – – – 143* – –
Cavallo et al. 2024 1.22 1.36 – 933 -0.450 – – –
Hunt & Reffert 2023 1.54 1.15 0.65 498 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
OC 0604 96.3 211.36 -64.16 0.63 -7.06 -3.55 -47.46 0.36
CWNU 308 77.8 211.4 -64.16 0.62 -7.05 -3.57 -47.46 0.03

💡 Note: The % column shows the percentage of members that Theia 5496 shares with each listed object.

Visualization

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