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NatureClose-in transiting sub-Neptunes are abundant in our Galaxy1. Planetary interior models based on their observed radius–mass relationship suggest that sub-Neptunes contain a discernible amount of either hydrogen (dry planets) or water (wet planets) blanketing a core composed of rocks and metal2. Water-rich sub-Neptunes have been believed to form farther from the star and then migrate inwards to their present orbits3. Here we report experimental e…See the Story
Building Wet Planets Through High-Pressure Magma–Hydrogen Reactions
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