Theia 738

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0.00 UTI
0.0
CN
1.0
Cdens
0.38
CC3
0.0
Clit
0.0
Cdup
Core radius and density 0.6 [pc], 6.7 [pc-2]
  • CN 0.0 Sparse
  • Cdens 1.0 Very dense
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 0.0 Very likely duplicate

Overview

â„šī¸
Theia 738 is a sparse, very dense object of low C3 quality. Its parallax locates it at a close distance, above the mid-plane, affected by moderate extinction. It is catalogued as an old cluster (see Parameters). It is rarely studied in the literature.

âš ī¸ Warning: This is very likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

Palma et al. (2025)
Classified as optical pair P580, along with Theia_38.

Hunt & Reffert (2024)
Classified as moving group. CMD class: 0.97 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.97 (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– 290.77 22.163 1.688 3.774 3.649 -20.657
Hunt & Reffert 2023 290.733 22.155 2.094 3.717 3.742 –
Kounkel & Covey 2019 290.829 22.08 1.708 – – -2.252

💡 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– 0.52 2.145 0.5 2056 – – – –
Hunt & Reffert 2023 0.45 3.33 0.50 3733 – – – –
Kounkel & Covey 2019 0.59 0.96 – 379 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
NGC 6793 100.0 290.81 22.15 1.67 3.8 3.54 -19.66 0.98

💡 Note: The % column shows the percentage of members that Theia 738 shares with each listed object.

Visualization

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