Theia 1024
Summary
Theia 1024 is a sparse, dense object of low C3 quality. It is located at a close distance from the Sun, above the mid-plane. It was recently reported in the literature.
Warning: contains less than 25 stars with P>0.5 estimated.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| He et al. (2022) | 134.097 | -38.085 | 2.001 | -5.317 | 5.341 | – |
| Hunt & Reffert (2023) | 134.102 | -38.08 | 1.95 | -5.388 | 5.418 | 22.91 |
| Cavallo et al. (2024) | 133.937 | -38.332 | 1.958 | – | – | – |
| UCC | 134.126 | -38.145 | 1.988 | -5.39 | 5.399 | 21.342 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2022) | A0=0.2, logAge=8.65 |
| Hunt & Reffert (2023) | AV50=0.077, diffAV50=0.476, MOD50=8.438, logAge50=8.721 |
| Cavallo et al. (2024) | AV50=0.57, dMod50=8.55, logAge50=8.09, [Fe/H]50=-0.33 |
Search coordinates in Bayestar19
