this post was submitted on 16 Jul 2025
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A critical part of understanding and identifying habitable worlds is understanding how their atmospheres evolve, including atmospheric escape. Atmospheric escape is a natural part of planetary evolution, and it has occurred throughout Earth's history. However, it was much more pronounced in Earth's early history, due to the Sun's energetic output and more frequent impacts from asteroids and comets. In current times, the escape is minimal, though steady.

Since atmospheric escape is much more pronounced in a planet's early years, it can shape its future habitability.

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