Modeling Pluto’s minimum pressure: Implications for haze production
Author:
Funder
NASA ROSES SSW, United States
NASA’s New Horizons mission to the Pluto system, United States
Publisher
Elsevier BV
Subject
Space and Planetary Science,Astronomy and Astrophysics
Reference51 articles.
1. Evidence for a rapid decrease of Pluto’s atmospheric pressure revealed by a stellar occultation in 2019;Arimatsu;Astron. Astrophys.,2020
2. Pluto’s interaction with its space environment: Solar wind, energetic particles, and dust;Bagenal;Science,2016
3. Observed glacier and volatile distribution on Pluto from atmosphere-topography processes;Bertrand;Nature,2016
4. 3D modeling of organic haze in Pluto’s atmosphere;Bertrand;Icarus,2017
5. The nitrogen cycles on Pluto over seasonal and astronomical timescales;Bertrand;Icarus,2018
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1. How obliquity has differently shaped Pluto’s and Triton’s landscapes and climates;Proceedings of the National Academy of Sciences;2024-08-12
2. Nitrogen Loss from Pluto’s Birth to the Present Day via Atmospheric Escape, Photochemical Destruction, and Impact Erosion;The Planetary Science Journal;2024-08-01
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