The Dynamics of Planetary Ejection
astro-ph.EP, astro-ph.SR
Submitted: 2026-07-31
Updated: 2026-08-26
Comments: invited review; accepted to PASP
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- The Wide Field Infrared Survey Telescope: 100 Hubbles for the 2020s
- Laser Interferometer Space Antenna
- Suppression of giant planet formation in stellar clusters
- Orbital Parameters of the PSR B1620-26 Triple System
- Two-stage disruption of resonant chains
- Planet-Planet Scattering Explains the Mass-Eccentricity Relation of Warm Jupiters
- Unified Formation Channel of Hot and Warm Jupiters via Planet-Planet Scattering
- ET White Paper: To Find the First Earth 2.0
- Hot Jupiters in Old Wide-Binary Systems
- Formation of Free-Floating Planets via Ejection: Population Synthesis with a Realistic IMF and Comparison to Microlensing Observations
- Free Floating or Merely Detached?
- The MOA 1.8-metre alt-az wide-field survey telescope and the MOA project
- Gravitational Scattering
- KMT-2024-BLG-3237: Another Free-Floating Planet Candidate with Angular Einstein Radius Measurement
- Interstellar Interloper 1I/2017 U1: Observations from the NOT and WIYN Telescopes
- Planetesimal-Driven Instabilities in Resonant Chains of Cold Neptunes and Their Dynamical Outcomes
- The Architecture of the 14 Herculis System Suggests Primordial Ejection of a Massive Planet
- The HARPS search for southern extra-solar planets XXXIV. Occurrence, mass distribution and orbital properties of super-Earths and Neptune-mass planets
- The Origin and Evolution of Multiple Star Systems
- White dwarf planets in star clusters: gravitational scattering versus mass-loss effects
Related papers
- PDS 70 c and SR 12 c: Observational Constraints on Giant-Planet and Satellite Formation
- Two-stage disruption of resonant chains
- Detectability of resolved hydrogen lines from the accretion shock at gas giants and their CPDs
- Binary-lens Microlensing Degeneracy: Impact on Planetary Sensitivity and Mass-ratio Function
- Atmospheric escape fractionates secondary but not primary atmospheres
- The Occurrence Rate of Nearby Planetary Companions to Hot Jupiters