The far future of exoplanet direct characterization
Jean Schneider, Alain Leger, Malcolm Fridlund, Glenn White, Carlos, Eiroa, Thomas Henning, Tom Herbst, Helmut Lammer, Rene Liseau, Francesco, Paresce, Alan Penny, Andreas Quirrenbach, Huub Roettgering, Franck Selsis,, Charles Beichman, William Danchi, Lisa Kaltenegger

TL;DR
This paper discusses the future prospects and challenges of directly characterizing habitable exoplanets over the next century, emphasizing technological advancements and the long timeline before visualizing extraterrestrial life forms.
Contribution
It provides an outlook on the technological and scientific steps needed for exoplanet characterization beyond current missions, highlighting future mission generations and their potential.
Findings
Long timeline before direct imaging of extraterrestrial organisms
Advancements in spectroscopic and imaging techniques are crucial
Future missions will extend over the next 100 years
Abstract
In this outlook we describe what could be the next steps of the direct characterization of habitable exoplanets after first the medium and large mission projects and investigate the benefits of the spectroscopic and direct imaging approaches. We show that after third and fourth generation missions foreseeable for the next 100 years, we will face a very long era before being able to see directly the morphology of extrasolar organisms.
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