Theia 202

Click to load Aladin Lite
0.22 UTI
0.0
CN
0.1
Cdens
0.5
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 0.5 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.1 Very loose
  • CC3 0.5 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
Theia 202 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a close distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the absorption parameter (see Parameters). It was recently reported 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.

Liu et al. (2025)
Classified as tidal capture (resonant trapping binary) 167 along with HSC_330.

Palma et al. (2025)
Classified as tidal capture (resonant trapping pair) P48, along with HSC_330.

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as a moving group.

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 290.964 -2.74 1.18 -0.553 -2.279 0.356
Zhang et al. 2024 290.978 -2.988 – – – –
Cavallo et al. 2024 291.02 -2.414 1.189 – – –
Hunt & Reffert 2023 290.978 -2.988 1.178 -0.523 -2.256 -1.512

💡 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– 0.82 1.14 1.37 63 -0.172 – – –
Liu et al. 2025 1.04 0.31 – 63 – – – –
Zhang et al. 2024 – – – – -0.124(1) – – –
Cavallo et al. 2024 0.82 1.48 – 56 -0.220 – – –
Hunt & Reffert 2023 0.81 1.14 1.37 112 – – – –

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

Visualization

â„šī¸