Theia 1769
Summary
Theia 1769 is a sparse, very loose object of intermediate C3 quality. It is located at a relatively close distance from the Sun, below the mid-plane. It was recently reported in the literature.
This is likely a unique object, which shares a moderate percentage of members with at least one previously reported entry.
Warning: contains less than 25 stars with P>0.5 estimated.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Hunt & Reffert (2023) | 101.969 | -12.836 | 0.707 | -2.915 | 2.125 | 49.243 |
| Cavallo et al. (2024) | 101.851 | -13.597 | 0.709 | – | – | – |
| UCC | 101.907 | -12.979 | 0.712 | -2.926 | 2.062 | 42.342 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=0.785, diffAV50=1.064, MOD50=10.608, logAge50=7.677 |
| Cavallo et al. (2024) | AV50=1.09, dMod50=10.74, logAge50=7.54, [Fe/H]50=-0.08 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| CWNU 1778 | 44.0 | 101.85 | -13.33 | 0.71 | -2.91 | 2.08 | 89.53 | 0.15 |
