File:Planets of Red Dwarf Stars May Face Oxygen Loss in Habitable Zones.gif
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Planets_of_Red_Dwarf_Stars_May_Face_Oxygen_Loss_in_Habitable_Zones.gif (673 × 379 pixels, file size: 1.52 MB, MIME type: image/gif, looped, 61 frames, 1.2 s)
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Date/Time | Thumbnail | Dimensions | User | Comment | |
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current | 14:02, 25 April 2020 | ![]() | 673 × 379 (1.52 MB) | commons>Killarnee | {{Information |description ={{en|1=In this artist’s concept, X-ray and extreme ultraviolet light from a young red dwarf star cause ions to escape from an exoplanet’s atmosphere. Scientists have developed a model that estimates the oxygen ion escape rate on planets around red dwarfs, which plays an important role in determining an exoplanet’s habitability. To determine a star’s habitable zone, scientists have traditionally considered how much heat the star emits. Stars more massive than our... |
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