Theia 1822

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0.10 UTI
0.64
CN
1.0
Cdens
0.75
CC3
0.0
Clit
0.22
Cdup
Stellar density (N50/rad) 6.1 [N/pc2]
  • CN 0.64 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 0.22 Likely duplicate

Overview

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Theia 1822 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.

âš ī¸ Warning: This is 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 (not dynamically associated) P83, along with BH_200.

Cavallo et al. (2024)
Gold sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 252.881 -44.493 0.414 -0.597 -2.528 -80.971
Hunt & Reffert 2024 252.894 -44.496 0.419 -0.605 -2.523 -48.574
Cavallo et al. 2024 252.891 -44.496 0.419 – – –
Hunt & Reffert 2023 252.894 -44.496 0.419 -0.605 -2.523 -48.574

💡 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– 2.075 2.09 2.64 92 0.410 719 – –
Hunt & Reffert 2024 – – – – – 719(1) – –
Cavallo et al. 2024 2.01 2.04 – 98 0.410 – – –
Hunt & Reffert 2023 2.14 2.14 2.64 85 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
UBC 1559 78.2 252.87 -44.49 0.41 -0.61 -2.54 -82.92 0.46

💡 Note: The % column shows the percentage of members that Theia 1822 shares with each listed object.

Visualization

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