This study examines the effects of M-dwarf stellar wind and photoevaporation on the atmospheric evolution of small planets. M-dwarfs are the most common type of star in the universe, and they are known to host many exoplanets.
To study this, the researchers use models that simulate stellar activity and photoevaporative mass loss. They apply these models to the atmospheres of 34 exoplanets in the habitable zone and 4 planets that are very close to their host stars.
Publisher: CityLife
Date: 2023-09-27T21:01:25 00:00
Author: Mampho Brescia
Reference: (Read more) Visit Source
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