Theia 865

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0.07 UTI
0.0
CN
0.05
Cdens
0.25
CC3
0.03
Clit
1.0
Cdup
Core radius and density 1.1 [pc], 0.2 [pc-2]
  • CN 0.0 Sparse
  • Cdens 0.05 Very loose
  • CC3 0.25 Low quality
  • Clit 0.03 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
Theia 865 is a sparse, very loose object of low C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is rarely studied in the literature.

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.

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– 214.921 -66.716 1.448 -11.284 -9.48 -17.009
Cavallo et al. 2024 211.952 -66.996 1.433 – – –
Hunt & Reffert 2023 215.46 -66.627 1.424 -11.268 -9.308 -15.15
Kounkel & Covey 2019 213.583 -67.048 1.347 – – -20.184

💡 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– 0.67 0.64 0.47 136 -0.090 – – –
Cavallo et al. 2024 0.67 0.74 – 129 -0.090 – – –
Hunt & Reffert 2023 0.67 0.29 0.47 136 – – – –
Kounkel & Covey 2019 0.74 0.64 – 399 – – – –

Visualization

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