Scattering cold Jupiters disrupt inner mean-motion resonances via secular perturbations from their orbital history, driving resonance circulation in most 2:1 and 3:2 configurations and explaining the Kepler period ratio distribution.
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In multi-planet systems, the innermost planet's orbit preferentially ends near the protoplanetary disk corotation radius, implying disk-driven migration halts there, with subsequent dynamical evolution scattering a subset inward.
The mutual orbit of Typhon-Echidna is precessing rapidly, revealing Typhon's J2, a 24 degree spin-orbit misalignment, and a triaxial shape consistent with a recently excited binary.
In Kepler multi-planet systems, inner planets tend to be smaller than outer planets, a trend the authors argue is not solely an observational artifact.
Two migrating super-Earths in low-viscosity disks trigger narrow and broad dust substructures with high dust-to-gas ratios favorable for planetesimal formation.
citing papers explorer
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Impact of Cold Jupiter Scattering on the Mean-Motion Resonance of Inner Small Planets
Scattering cold Jupiters disrupt inner mean-motion resonances via secular perturbations from their orbital history, driving resonance circulation in most 2:1 and 3:2 configurations and explaining the Kepler period ratio distribution.
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Exoplanet System Architecture: Sculpting the Inner Regions
In multi-planet systems, the innermost planet's orbit preferentially ends near the protoplanetary disk corotation radius, implying disk-driven migration halts there, with subsequent dynamical evolution scattering a subset inward.
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Beyond Point Masses. VI. Spin-Orbit Evolution of the Centaur Binary Typhon-Echidna
The mutual orbit of Typhon-Echidna is precessing rapidly, revealing Typhon's J2, a 24 degree spin-orbit misalignment, and a triaxial shape consistent with a recently excited binary.
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On the Ordering of Exoplanet Systems
In Kepler multi-planet systems, inner planets tend to be smaller than outer planets, a trend the authors argue is not solely an observational artifact.
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On the Dust Substructures Triggered by Two Super-Earths Migrating in Low-viscosity Disks
Two migrating super-Earths in low-viscosity disks trigger narrow and broad dust substructures with high dust-to-gas ratios favorable for planetesimal formation.