Sculpting the valley in the radius distribution of small exoplanets as a by-product of planet formation: the core-powered mass-loss mechanism
Recent observations revealed a bimodal radius distribution of small, short-period exoplanets with a paucity in their occurrence, a radius ‘valley’, around 1.5–2.0 R⊕. In this work, we investigate the effect of a planet’s own cooling luminosity on its thermal evolution and atmospheric mass loss (core...
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Published in | Monthly notices of the Royal Astronomical Society Vol. 487; no. 1; pp. 24 - 33 |
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Main Authors | , |
Format | Journal Article |
Language | English |
Published |
England
01.07.2019
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Subjects | |
Online Access | Get full text |
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