Exoplanet atmospheres and demographics in the 2040s

Fuente: arXiv
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Main Authors: Kammerer, Jens, Vach, Sydney, Lacour, Sylvestre, Nowak, Mathias, Winterhalder, Thomas, Mérand, Antoine, Corporaal, Akke, Bourdarot, Guillaume, Kraus, Stefan, Hinkley, Sasha
Format: Preprint
Published: 2026
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author Kammerer, Jens
Vach, Sydney
Lacour, Sylvestre
Nowak, Mathias
Winterhalder, Thomas
Mérand, Antoine
Corporaal, Akke
Bourdarot, Guillaume
Kraus, Stefan
Hinkley, Sasha
author_facet Kammerer, Jens
Vach, Sydney
Lacour, Sylvestre
Nowak, Mathias
Winterhalder, Thomas
Mérand, Antoine
Corporaal, Akke
Bourdarot, Guillaume
Kraus, Stefan
Hinkley, Sasha
contents Direct observations of exoplanets probe the demographics and atmospheric composition of young self-luminous companions, yielding insight into their formation and early evolution history. In the near future, Gaia will reveal hundreds of nearby young exoplanets amenable to direct follow-up observations. Long-baseline interferometry with current and future facilities is best capable of exploiting this unique synergy which is poised to deliver a statistical sample of benchmark planets with precise dynamical masses and in-depth atmospheric characterization. This will enable tackling the longstanding question of how giant planets form from multiple angles simultaneously, shining light on the complex physical processes underlying planet formation.
format Preprint
id arxiv_https___arxiv_org_abs_2601_11695
institution arXiv
publishDate 2026
record_format arxiv
spellingShingle Exoplanet atmospheres and demographics in the 2040s
Kammerer, Jens
Vach, Sydney
Lacour, Sylvestre
Nowak, Mathias
Winterhalder, Thomas
Mérand, Antoine
Corporaal, Akke
Bourdarot, Guillaume
Kraus, Stefan
Hinkley, Sasha
Instrumentation and Methods for Astrophysics
Earth and Planetary Astrophysics
Direct observations of exoplanets probe the demographics and atmospheric composition of young self-luminous companions, yielding insight into their formation and early evolution history. In the near future, Gaia will reveal hundreds of nearby young exoplanets amenable to direct follow-up observations. Long-baseline interferometry with current and future facilities is best capable of exploiting this unique synergy which is poised to deliver a statistical sample of benchmark planets with precise dynamical masses and in-depth atmospheric characterization. This will enable tackling the longstanding question of how giant planets form from multiple angles simultaneously, shining light on the complex physical processes underlying planet formation.
title Exoplanet atmospheres and demographics in the 2040s
topic Instrumentation and Methods for Astrophysics
Earth and Planetary Astrophysics
url https://arxiv.org/abs/2601.11695