Theia 5094

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0.04 UTI
0.0
CN
0.1
Cdens
0.75
CC3
0.03
Clit
0.24
Cdup
Core radius and density 2.7 [pc], 0.5 [pc-2]
  • CN 0.0 Sparse
  • Cdens 0.1 Very loose
  • CC3 0.75 High quality
  • Clit 0.03 Rarely studied
  • Cdup 0.24 Likely duplicate

Overview

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Theia 5094 is a sparse, very loose object of high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by low 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 likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as open cluster. CMD classes: 0.99 (50th percentile), true positive (human-assigned).

Hunt & Reffert (2023)
Classified as open cluster. CMD classes: 0.99 (50th percentile), true positive (human-assigned).

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 146.282 -56.562 0.611 -5.586 3.344 –
Hunt & Reffert 2024 146.264 -56.602 0.611 -5.619 3.393 8.425
Cavallo et al. 2024 146.261 -56.521 0.61 – – –
Hunt & Reffert 2023 146.264 -56.602 0.611 -5.619 3.393 8.425

💡 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– 1.58 0.7 0.88 111 0.040 178 – –
Hunt & Reffert 2024 1.58 0.70 0.88 111 – 178(1) – –
Cavallo et al. 2024 1.47 0.79 – 182 0.040 – – –
Hunt & Reffert 2023 1.58 0.70 0.88 111 – – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 2757 76.0 146.26 -56.5 0.62 -5.57 3.36 – 0.23

💡 Note: The % column shows the percentage of members that Theia 5094 shares with each listed object.

Visualization

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