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.
, archivePrefix = "arXiv", eprint =
5 Pith papers cite this work, alongside 120 external citations. Polarity classification is still indexing.
5
Pith papers citing it
120
external citations · Crossref
fields
astro-ph.EP 5representative citing papers
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
-
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.
-
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.
-
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.
-
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.