Theia 6042

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0.00 UTI
0.0
CN
0.75
Cdens
0.12
CC3
0.0
Clit
0.0
Cdup
Stellar density (N50/rad) 3.8 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.75 Dense
  • CC3 0.12 Very low quality
  • Clit 0.0 Rarely studied
  • Cdup 0.0 Very likely duplicate

Overview

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Theia 6042 is a sparse, dense object of very low C3 quality. Its parallax locates it at a moderate* distance, well above the mid-plane, affected by moderate extinction. It is catalogued as a very old cluster (see Parameters). It was recently reported 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.

(*): The parallax distance estimate (~2.13 kpc) differs significantly from the median photometric distance (~1.38 kpc).

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 114.619 21.569 0.47 -1.125 -2.069 72.683
Hunt & Reffert 2024 114.628 21.543 0.719 -1.084 -2.024 –
Hunt & Reffert 2023 114.628 21.543 0.719 -1.084 -2.024 –

💡 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– 1.38 1.88 0.58 6252 – 528 – –
Hunt & Reffert 2024 – – – – – 528(1) – –
Hunt & Reffert 2023 1.38 1.88 0.58 6252 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Melotte 69 100.0 114.6 21.58 0.38 -1.21 -2.04 73.59 1.0

💡 Note: The % column shows the percentage of members that Theia 6042 shares with each listed object.

Visualization

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