Theia 2902

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0.21 UTI
0.55
CN
0.58
Cdens
0.75
CC3
0.25
Clit
0.44
Cdup
Radius (P>50% members) 10.1 [arcmin]
  • CN 0.55 Moderately populated
  • Cdens 0.58 Moderately dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 0.44 Possibly duplicate

Overview

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Theia 2902 is a moderately populated, moderately 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 possibly a duplicate object, which shares a significant 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 – 346.857 58.902 0.654 -1.812 -1.498 -17.615
Zhang et al. 2024 346.892 58.886 – – – –
Hunt & Reffert 2024 346.892 58.886 0.646 -1.819 -1.5 -17.587
Cavallo et al. 2024 346.885 58.923 0.651 – – –
Hunt & Reffert 2023 346.892 58.886 0.646 -1.819 -1.5 -17.587

💡 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 – – – – 0.021* – – –
Hunt & Reffert 2024 – – – – – 229* – –
Cavallo et al. 2024 1.47 1.27 – 269 0.100 – – –
Hunt & Reffert 2023 1.44 1.15 1.80 89 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 419 55.9 346.9 58.92 0.66 -1.81 -1.5 -17.61 0.04
UBC 1574 50.8 346.9 58.91 0.66 -1.8 -1.5 -17.61 0.29
CWWDL 14151 47.5 346.94 58.95 0.66 -1.8 -1.5 -17.61 0.02

💡 Note: The % column shows the percentage of members that Theia 2902 shares with each listed object.

Visualization

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