Promotor: Prof.dr. I.A.G. Snellen, C.U. Keller

This thesis describes the implementation and on-sky demonstration of high-resolution integral-field spectroscopy for extreme adaptive optics systems that are used to find and characterize exoplanets.

Over the last three decades, the discovery of exoplanets has revealed the boundless variety of worlds beyond our own Solar System⁠. Majority of planetary systems contain short-period planets that are larger than Earth but smaller than Neptune⁠.

Promotor: I. A. G. Snellen, Co-promotor: M. A. Kenworthy

One of the key discoveries in exoplanet research over the past decade is the abundance of small planets in our Milky Way. Despite their high numbers, our understanding of their atmospheres remains limited, and it is unknown if they possess atmospheres at all.

Diverse types of exoplanets such as gas giants on close-in orbits (hot Jupiters) and young massive giants on wide orbits (super Jupiters), with no analogs in the Solar System, pose challenges but also opportunities to our understanding of planet formation and evolution.

More than 5,000 exoplanets have been found over the past couple of decades. These exoplanets show a tremendous diversity, ranging from scorching hot Jupiters, common super-Earths, to widely separated super-Jupiters on the planet/brown dwarf boundary.

Een groep astronomen heeft onder leiding van de Leidse promovendus Sebastian Zieba met behulp van de James Webb Space Telescope (JWST) ontdekt dat de rotsachtige exoplaneet TRAPPIST-1 c een dunne atmosfeer heeft. Hoewel de planeet qua grootte en temperatuur bijna identiek is aan Venus, en de verwachting…

In de afgelopen 30 jaar zijn er ruim 5000 planeten ontdekt buiten ons zonnestelsel. Een veelvoorkomende exoplaneet is de lavawereld, een hete superaarde met oceanen van vloeibaar lava. Mantas Zilinskas ontwikkelde modellen om mogelijke atmosferen daarvan te simuleren. Die simulaties bieden houvast voor…