Theia 2175

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0.04 UTI
0.0
CN
0.38
Cdens
0.5
CC3
0.0
Clit
0.2
Cdup
Stellar density (N50/rad) 1.9 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.38 Loose
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 0.2 Likely duplicate

Overview

â„šī¸
Theia 2175 is a sparse, loose object of intermediate C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a metal-rich, young 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.

Palma et al. (2025)
Part of multiple system G205, along with UPK_241 and HSC_974.

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 99999– 8.723 68.844 0.981 -1.531 -0.652 -18.208
Hunt & Reffert 2024 8.571 68.864 0.98 -1.566 -0.663 -17.41
Cavallo et al. 2024 8.926 68.847 0.987 – – –
Hunt & Reffert 2023 8.571 68.864 0.98 -1.566 -0.663 -17.41

💡 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– 1.065 1.985 0.72 74 0.880 113 – –
Hunt & Reffert 2024 – – – – – 113(1) – –
Cavallo et al. 2024 1.16 1.87 – 59 0.880 – – –
Hunt & Reffert 2023 0.97 2.10 0.72 89 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 14487 80.0 9.19 68.83 0.99 -1.51 -0.63 -16.4 0.01
HXHWL 39 80.0 9.19 68.83 0.98 -1.51 -0.63 -16.4 0.13

💡 Note: The % column shows the percentage of members that Theia 2175 shares with each listed object.

Visualization

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