Linked from

The 31 pages that link to Atmospheric escape, each with the reason it gives.

• Stellar windRelated: Stellar-wind interactions can strip atmospheric particles, especially from unprotected planets.

• Solar windNarrower topic: Solar-wind interactions can remove particles, especially from bodies with weak magnetic protection.

• Water vaporRelated: In the upper atmosphere, water-derived hydrogen can ultimately escape to space.

• Planetary habitabilityRelated: Atmospheric loss can remove water and climate-regulating gases, narrowing a world's habitable lifetime.

• MagnetosphereRelated: Magnetic shielding may alter escape pathways, but does not guarantee that an atmosphere is retained.

• Escape velocityRelated: A planet's escape speed helps determine whether atmospheric particles can remain gravitationally bound.

• Planetary scienceRelated: Its rates determine whether small worlds retain water and sustain long-lived climates.

• Atmosphere of EarthRelated: Escape gradually removes gases from the upper atmosphere despite Earth’s gravity.

• Habitable zoneRelated: A planet can occupy the zone yet lose the atmosphere needed to retain surface water.

• Gravitational binding energyRelated: A planet's gravity helps determine whether energetic particles can escape.

• Exoplanet atmosphereRelated: Escape can strip an exoplanet’s atmosphere and alter its composition over geological time.

• Planetary atmosphereRelated: Escape determines whether a planet retains light gases over geological time.

• AtmosphereRelated: Escape determines whether a planet can retain gases over time.

• Red dwarfRelated: Flares and energetic radiation from red dwarfs may erode nearby planetary atmospheres.

• Stellar flareRelated: Repeated flare radiation and particles can contribute to atmospheric loss.

• TRAPPIST-1Related: High-energy radiation from the star may have stripped gases from the planets over time.

• Faint young Sun paradoxRelated: Escape may have altered the abundance of hydrogen-bearing greenhouse gases over time.

• Atmospheric absorptionCompared with: Absorption deposits radiation energy in the atmosphere, unlike processes that remove it to space.

• HD 209458 bRelated: The planet’s intense irradiation drives substantial hydrogen loss.

• PhotoevaporationNarrower topic: Photoevaporation is one radiation-driven route by which planetary atmospheres escape.

• OutgassingCompared with: Outgassing supplies atmospheric gases, whereas atmospheric escape removes them from a planet.

• Proxima Centauri bRelated: Radiation and particle activity from the host star may have stripped away some of the planet’s atmosphere.

• Atmosphere of PlutoRelated: Pluto’s weak gravity allows atmospheric molecules to escape, especially from its extended upper atmosphere.

• Volcanic outgassingRelated: Comparing gas supply with escape helps explain whether outgassing can sustain an atmosphere.

• ExosphereNarrower topic: Escape is the broader process that the exosphere makes possible.

• Barometric formulaRelated: The barometric profile describes lower-atmosphere structure, while escape depends on high-altitude particle dynamics.

• Flare starRelated: Repeated high-energy flares can help erode atmospheres, especially around active stars.

• Chthonian planetRelated: It is the process that could strip a close-in gas giant down to its core.

• Future of EarthRelated: Its rate determines how quickly Earth could lose water as the upper atmosphere warms.

• Geological history of MarsRelated: Escape rates help connect Mars’s climate change with its diminishing atmosphere.

• HD 189733 bRelated: Ultraviolet heating drives hydrogen escape from HD 189733 b’s upper atmosphere.