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Energy-Limited Escape: 5 M⊕, 10 TO. Similar to the previous figures but for a super-Earth of mass 5 M⊕ with 10 TO, assuming energy-limited escape. Note the large fraction of the HZ in the lower left portion of the left panel where planets are completely desiccated. Elsewhere, super-Earths lose several TO of water. In the right panel, thousands of bar of O2 are absorbed at the surface of planets throughout most of the HZ of M dwarfs.
