Theia 4930

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0.21 UTI
0.29
CN
0.09
Cdens
0.62
CC3
0.03
Clit
1.0
Cdup
Core radius and density 1.8 [pc], 0.5 [pc-2]
  • CN 0.29 Poorly populated
  • Cdens 0.09 Very loose
  • CC3 0.62 Intermediate quality
  • Clit 0.03 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
Theia 4930 is a poorly populated, very loose object of intermediate C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by low extinction. It is catalogued as a low-mass, near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the absorption and age parameters (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.

Palma et al. (2025)
Classified as optical pair P547, along with NGC_2546.

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.92 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.92 (50th percentile).

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 124.372 -36.733 1.071 -6.08 4.881 32.682
Hunt & Reffert 2024 124.383 -36.676 1.067 -6.102 4.893 35.423
Cavallo et al. 2024 124.403 -36.739 1.074 – – –
Hunt & Reffert 2023 124.383 -36.676 1.067 -6.102 4.893 35.423

💡 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– 0.9 0.21 0.83 250 -0.120 40 – –
Hunt & Reffert 2024 0.90 0.21 0.83 250 – 40(1) – –
Cavallo et al. 2024 0.94 1.04 – 62 -0.120 – – –
Hunt & Reffert 2023 0.90 0.21 0.83 250 – – – –

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

Visualization

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