Amplifying Resonant Repulsion with Inflated Young Planets, Overlooked Inner Planets, and Nonzero Initial Δ
Most multiplanet systems around mature (∼5 Gyr old) host stars are nonresonant. Even the near-resonant planet pairs still display 1%–2% positive deviation from perfect period commensurabilities (Δ) near first-order mean motion resonances (MMRs). Resonant repulsion due to eccentricity tides was one o...
| Main Authors: | , |
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| 格式: | 文件 |
| 语言: | English |
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IOP Publishing
2025-01-01
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| 丛编: | The Astrophysical Journal |
| 主题: | |
| 在线阅读: | https://doi.org/10.3847/1538-4357/adb281 |