But #RV searches continued, aiming to reach the next level: going to lower masses + higher precision. And our advances are still ongoing, with plenty of new #spectrographs to play with.
Look at the development in the precision. From 50 m/s down to 0.4 m/s 🙌🏻
So what‘s next? We need a couple of years more to reach our goal precision, but the community is working on it!
Another emblematic system is beta Pic! - it will be covered in some talks later this week.
A sub-solar C/O ratio should give us a hint of the formation scenario but the stellar C/O ratio is a tricky one. Tbh, this showcases again that there is lots to do in the quest to understand formation pathways and locations of giant planets.
Beta Pic was observed by GRAVITY, giving us constraints on mass and orbit. #ExSSV
The two previous systems are around A stars, but since recently we also have extreme solar systems around other stellar types. Exciting!
An example are young systems or FGK stars.
I love that I spot so many familiar names, Bohn et al. Alex studied at ETH in his master’s when I did my bachelor’s, and we’ve been friends ever since. Insane! #ExSSV
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