Hydrodynamic escape
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- Early Hydrodynamic Escape Limits Rocky Planets to ~1.6 Earth Radii Owen Lehmer and David Catling ESS Gala 3/30/2017
- Origin and Evolution of the Atmospheres of Early Venus, Earth and Mars
- Evolution and Properties of Planetary Systems
- Magma Ocean Outgassing and Hydrogen Isotopic Constraints on the Hadean Earth
- A More Comprehensive Habitable Zone for Finding Life on Other Planets
- Energy-Limited Escape Revised the Transition from Strong Planetary Winds to Stable Thermospheres
- Hydrodynamic Escape from H2 Rich Atmospheres
- Watson Et Al. 1981
- Xenon Fractionation and Archean Hydrogen Escape K
- 1 Thermally-Driven Atmospheric Escape: Transition From
- Arxiv:1801.00748V1 [Astro-Ph.EP] 2 Jan 2018 Amplitude Perturbations (Due to Tectonics, Stellar Evolu- Tion, E.T.C.) Through a Negative Feedback
- D. Atri, MNRAS Letters, 465, L34 (2017) D
- The Escape of Planetary Atmospheres
- Escape from Titan's Atmosphere: Kinetic Monte Carlo Simulations
- Atmospheric Escape and Evolution of Terrestrial Planets and Satellites
- The Early Evolution of Venus Controlled by Hydrodynamic Escape
- Effective Hydrodynamic Hydrogen Escape from an Early Earth
- The Planetary Air Leak As Earth’S Atmosphere Slowly Trickles Away Into Space, Will Our Planet Come to Look Like Venus? by David C