Theia 2118

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0.18 UTI
0.0
CN
0.28
Cdens
0.12
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 7.7 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.28 Loose
  • CC3 0.12 Very low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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Theia 2118 is a sparse, loose object of very low C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It was recently reported in the literature.

Note: This object shares a small percentage of members with a later reported entry. See table with shared members information.

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

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 – 101.736 7.365 0.638 -1.54 0.207 -4.665
Zhang et al. 2024 101.739 7.387 – – – –
Hunt & Reffert 2024 101.739 7.387 0.679 -1.644 0.186 48.972
Cavallo et al. 2024 101.113 7.793 0.678 – – –
Hunt & Reffert 2023 101.739 7.387 0.679 -1.644 0.186 48.972

💡 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
Zhang et al. 2024 – – – – -0.184* – – –
Hunt & Reffert 2024 – – – – – 66* – –
Cavallo et al. 2024 1.67 1.25 – 123 0.400 – – –
Hunt & Reffert 2023 1.38 1.08 2.40 157 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 4106 20.0 101.68 7.54 0.65 -1.54 0.53 – 0.12

💡 Note: The % column shows the percentage of members that Theia 2118 shares with each listed object.

Visualization

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