We use both ground based high-resolution spectroscopy and space-based secondary eclipse measurements to study the chemical compositions, physical structures, and dynamical processes of the atmospheres of extreme Neptune-like exoplanets. By identifying the metallic structure of clouds in the atmosphere of planets like LTT9779b for example, we can better understand the formation histories and evolutionary pathways for such worlds.
Type of project: Research – actively recruiting new young researchers
Status: Ongoing
Researchers: James Jenkins, Suman Saha
Funding source: FONDECYT Regular, Basal CATA2, ESO-Chile