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Thanks to the James Webb Space Telescope and other upcoming missions, we are capturing high-quality data from distant worlds at an unprecedented rate. Our ability to interpret those data reliably is lagging, however. Many atmospheric “retrieval” and climate/chemistry models rest on incomplete laboratory measurements, simplified physics/chemistry, and coarse-grained assumptions – different models can reach conflicting conclusions from the same set of observations. This initiative aims to close the ground truth gap by building a cross-disciplinary community linking observations, laboratory experiments, and theory to create more realistic, process-based atmospheric models for both Earth and other worlds. It will bring together astrophysicists and exoplanet observers, planetary scientists, terrestrial atmospheric observers and modelers, astro-statisticians, and physical/analytical chemists and experimentalists to create an integrated community to advance characterization and modeling of terrestrial and extraterrestrial atmospheres and build validated, cross-checked tools to expand what atmospheres can teach us about planetary evolution and deepen insight into our own planet.

Applications will open on July 1, 2026 and should be submitted by April 15, 2027 for full consideration.