Theia 2822

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0.06 UTI
0.33
CN
0.04
Cdens
0.75
CC3
0.03
Clit
0.24
Cdup
Core radius and density 4.1 [pc], 0.2 [pc-2]
  • CN 0.33 Poorly populated
  • Cdens 0.04 Very loose
  • CC3 0.75 High quality
  • Clit 0.03 Rarely studied
  • Cdup 0.24 Likely duplicate

Overview

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Theia 2822 is a poorly populated, very loose object of high C3 quality. Its parallax locates it at a large distance, above 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: 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.

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.99 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.99 (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– 118.037 -25.494 0.163 -2.153 3.146 89.36
Hunt & Reffert 2024 118.046 -25.491 0.159 -2.159 3.132 89.352
Cavallo et al. 2024 118.04 -25.518 0.158 – – –
Hunt & Reffert 2023 118.046 -25.491 0.159 -2.159 3.132 89.352

💡 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– 6.05 0.63 0.7 282 0.380 168 – –
Hunt & Reffert 2024 6.05 0.63 0.70 282 – 168(1) – –
Cavallo et al. 2024 4.27 0.30 – 339 0.380 – – –
Hunt & Reffert 2023 6.05 0.63 0.70 282 – – – –

(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 1392 75.8 118.05 -25.49 0.16 -2.15 3.15 89.36 0.21

💡 Note: The % column shows the percentage of members that Theia 2822 shares with each listed object.

Visualization

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