Theia 1232

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0.11 UTI
0.0
CN
0.03
Cdens
0.5
CC3
0.0
Clit
1.0
Cdup
Core radius and density 2.9 [pc], 0.1 [pc-2]
  • CN 0.0 Sparse
  • Cdens 0.03 Very loose
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
Theia 1232 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a very close distance, near the mid-plane, affected by low extinction. It is catalogued as an 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.

Palma et al. (2025)
Classified as optical pair P531, along with HSC_873.

Hunt & Reffert (2024)
Classified as moving group. CMD class: 0.93 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.93 (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– 350.412 60.566 2.744 7.892 -3.404 -11.296
Hunt & Reffert 2023 350.433 60.561 2.72 7.987 -3.488 -19.652
Kounkel & Covey 2019 352.031 60.301 1.754 – – -4.755

💡 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– 0.46 0.82 0.69 631 – – – –
Hunt & Reffert 2023 0.35 1.02 0.69 15 – – – –
Kounkel & Covey 2019 0.57 0.62 – 1247 – – – –

Visualization

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