Theia 618

Click to load Aladin Lite
0.10 UTI
0.0
CN
0.24
Cdens
0.25
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 1.2 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.24 Very loose
  • CC3 0.25 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
Theia 618 is a sparse, very loose object of low C3 quality. Its parallax locates it at a close distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (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.

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– 4.97 55.705 1.386 0.187 -4.939 -12.884
Hu & Soubiran 2025 4.992 55.58 – – – –
Cavallo et al. 2024 4.992 55.58 1.389 – – –
Hunt & Reffert 2023 5.286 55.784 1.382 0.192 -5.079 -7.607

💡 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– 0.695 0.645 0.24 540 -0.050 – – –
Hu & Soubiran 2025 – – – – -0.100(5) – – –
Cavallo et al. 2024 0.70 0.64 – 813 0.000 – – –
Hunt & Reffert 2023 0.69 0.65 0.24 266 – – – –

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

Visualization

â„šī¸