Drying of the Martian mesosphere during aphelion induced by lower temperatures

Drying of the Martian mesosphere during aphelion induced by lower temperatures

Abstract The formation of water ice clouds or hazes on Mars imposes substantial limitations on the vertical transport of water into the middle-upper atmosphere, impacting the planet’s hydrogen loss. Recent observations made by the Mars Environmental Dynamics Analyzer instrument onboard Mars 2020 Per...

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Main Authors: Daniel Toledo, Pascal Rannou, Victor Apéstigue, Raul Rodriguez-Veloso, Ignacio Arruego, German Martínez, Leslie Tamppari, Asier Munguira, Ralph Lorenz, Aurélien Stcherbinine, Franck Montmessin, Agustin Sanchez-Lavega, Priya Patel, Michael Smith, Mark Lemmon, Alvaro Vicente-Retortillo, Claire Newman, Daniel Viudez-Moreiras, Ricardo Hueso, Tanguy Bertrand, Jorge Pla-Garcia, Margarita Yela, Manuel de la Torre Juarez, Jose Antonio Rodriguez-Manfredi
Format: Article
Language:English
Published: Nature Portfolio 2024-11-01
Series:Communications Earth & Environment
Online Access:https://doi.org/10.1038/s43247-024-01878-7
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