Theia 652

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0.12 UTI
0.0
CN
0.06
Cdens
0.5
CC3
0.03
Clit
1.0
Cdup
Core radius and density 2.6 [pc], 0.3 [pc-2]
  • CN 0.0 Sparse
  • Cdens 0.06 Very loose
  • CC3 0.5 Intermediate quality
  • Clit 0.03 Rarely studied
  • Cdup 1.0 Unique

Overview

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Theia 652 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is rarely studied in the literature.

Note: This object shares a large 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.

Palma et al. (2025)
Classified as optical pair P585, along with UPK_294.

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as moving group. CMD class: 1.00 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 1.00 (50th percentile).

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 56.588 68.947 1.302 0.327 -1.263 -27.749
Cavallo et al. 2024 56.712 68.963 1.302 – – –
Hunt & Reffert 2023 57.497 68.713 1.303 0.192 -1.229 -24.115
Kounkel & Covey 2019 55.187 68.888 1.426 – – -17.952

💡 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– 0.73 1.19 0.45 99 0.300 – – –
Cavallo et al. 2024 0.78 1.42 – 93 0.300 – – –
Hunt & Reffert 2023 0.73 1.19 0.45 99 – – – –
Kounkel & Covey 2019 0.70 0.61 – 263 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 438 76.0 56.16 68.95 1.29 0.4 -1.25 -28.26 0.02

💡 Note: The % column shows the percentage of members that Theia 652 shares with each listed object.

Visualization

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