Theia 2812

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0.08 UTI
0.47
CN
1.0
Cdens
0.75
CC3
0.25
Clit
0.15
Cdup
Stellar density (N50/rad) 6.4 [N/pc2]
  • CN 0.47 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 0.15 Likely duplicate

Overview

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Theia 2812 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (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) P170, along with Theia_2118.

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– 101.95 7.654 0.689 -0.608 -2.206 9.533
Zhang et al. 2024 101.987 7.664 – – – –
Hunt & Reffert 2024 101.988 7.664 0.697 -0.596 -2.2 10.297
Cavallo et al. 2024 101.921 7.657 0.696 – – –
Hunt & Reffert 2023 101.988 7.664 0.697 -0.596 -2.2 10.297

💡 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– 1.42 0.87 1.73 136 0.101 262 – –
Zhang et al. 2024 – – – – -0.109(1) – – –
Hunt & Reffert 2024 – – – – – 262(1) – –
Cavallo et al. 2024 1.48 0.99 – 132 0.310 – – –
Hunt & Reffert 2023 1.36 0.75 1.73 141 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
OC 0342 85.1 101.96 7.66 0.69 -0.61 -2.2 9.53 0.43

💡 Note: The % column shows the percentage of members that Theia 2812 shares with each listed object.

Visualization

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