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This whitepaper discusses the diversity of exoplanets that could be detectedby future observations, so that comparative exoplanetology can be performed inthe upcoming era of large space-based flagship missions. The primary focus willbe on characterizing Earth-like worlds around Sun-like stars. However, we willalso be able to characterize companion planets in the system simultaneously.This will not only provide a contextual picture with regards to our Solarsystem, but also presents a unique opportunity to observe size dependentplanetary atmospheres at different orbital distances. We propose a preliminaryscheme based on chemical behavior of gases and condensates in a planet'satmosphere that classifies them with respect to planetary radius and incidentstellar flux.

Exoplanet Diversity in the Era of Space-based Direct Imaging Missions