A Resonant Beginning for the Solar System’s Terrestrial Planets
In the past two decades, transit surveys have revealed a class of planets with thick atmospheres—sub-Neptunes—that must have completed their accretion in protoplanet disks. When planets form in the gaseous disk, the gravitational interaction with the disk gas drives their migration and results in th...
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| Huvudupphov: | , , , , |
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| Materialtyp: | Artigo |
| Språk: | Inglês |
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IOP Publishing
2025-01-01
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| Serie: | The Astrophysical Journal |
| Ämnen: | |
| Länkar: | https://doi.org/10.3847/1538-4357/ade25a |
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